Meade Telescope LXD55 User Manual

Instruction Manual  
LXD55-Series Telescopes  
Meade Instruments Corporation  
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CONTENTS  
Telescope Features ...................................................... 4  
Autostar Features .......................................................... 9  
Getting Started ..............................................................11  
Unpacking and Assembly..........................................11  
How to Assemble Your Telescope ............................11  
Balancing the Telescope ..........................................13  
Aligning the Viewfinder..............................................14  
Choosing an Eyepiece..............................................14  
Observing By Moving the Telescope Manually ........15  
Activate the Arrow Keys............................................16  
Slew Speeds ............................................................16  
Observe the Moon ....................................................17  
Tracking Objects ......................................................17  
Setting the Polar Home Position ........................17  
Observe a Star Using Automatic Tracking ..........18  
Using Autostar's GO TO Capabilities ..................18  
Moving Through Autostar’s Menus......................19  
Initializing Autostar ..............................................19  
Training the Drive ................................................20  
Easy Alignment ........................................................21  
Go To Saturn ............................................................21  
Using the Guided Tour ..............................................22  
Basic Autostar Operation................................................23  
Autostar Navigation Exercise....................................23  
Entering Data into Autostar ......................................24  
Navigating Autostar ..................................................24  
Autostar's Menus............................................................25  
Object Menu..............................................................26  
Event Menu ..............................................................27  
Glossary Menu..........................................................27  
Utilities Menu ............................................................27  
Setup Menu ..............................................................28  
Useful Autostar Features................................................32  
Adding Observing Sites ............................................32  
Using Autostar to Find Objects Not in the Libraries....33  
Observing Satellites..................................................34  
Landmarks ................................................................34  
To Check on Available Memory ................................35  
Photography ..................................................................36  
Optional Accessories......................................................37  
Maintenance ..................................................................39  
Specifications ................................................................45  
Appendix A: Celestial Coordinates ................................48  
Setting Circles ....................................................48  
Locating the Celestial Pole..................................49  
One- And Two-Star Polar Alignment....................49  
Appendix B: Enhancing Pointing Precision....................50  
The Polar Alignment Viewfinder ..........................50  
Axis Alignment Method 1 ....................................50  
Axis Alignment Method 2 ....................................53  
Appendix C: Latitude Chart ............................................54  
Appendix D: EC Handbox ..............................................55  
Appendix E: Mounting the Model SC-8 Optical Tube ....59  
Appendix F: Basic Astronomy ........................................60  
WARNING!  
®
Never use  
a
Meade  
LXD55-Series  
Telescope to look at the Sun! Looking at or  
near the Sun will cause instant and irre-  
versible damage to your eye. Eye damage is  
often painless, so there is no warning to the  
observer that damage has occurred until it is  
too late. Do not point the telescope or its  
viewfinder at or near the Sun. Do not look  
through the telescope or its viewfinder as it is  
moving. Children should always have adult  
supervision while observing.  
CAUTION: Use care to install batteries in  
the orientation indicated by the illustration in  
the battery slots of the battery holder. Follow  
battery manufacturer's precautions. Do not  
install batteries backwards or mix new and  
used batteries. Do not mix battery types. If  
these precautions are not followed, batteries  
may explode, catch fire, or leak. Improperly  
installed batteries void your Meade warranty.  
® The name "Meade" and the Meade logo are trademarks  
registered with the U.S. Patent Office and in principal coun-  
tries throughout the world. "LXD55" and "Autostar" are  
trademarks of Meade Instruments Corporation.  
"Easy Align" U.S. patent 6,392,799 and other patents pend-  
ing.  
Intelligent Network Architecture to Facilitate Parallel Task  
Management U.S. patent 6,304,376  
© 2003 Meade Instruments Corporation.  
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T E L E S C O P E F E A T U R E S  
d
I H g e C B  
f
1$  
J
1#  
1#  
1)  
1!  
1@  
Fig. 1a: The LXD55-Series Telescope Optical Assembly (Schmidt-Newtonian model with Autostar handbox shown;  
Electronic Controller model users, see Appendix D, page 55).  
d
B 1^ 1% g f e  
3%  
3(  
4)  
3^  
C
I
H
3&  
3*  
Fig. 1b: Close up of Focuser and Viewfinder Assembly,  
Scmidt-Newtonian shown. (See Fig. 1a for overview.) For  
a close up of the refractor focuser assembly, see Fig. 10b,  
page 13.  
Fig. 1c: The LXD55-Series Tripod  
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1&  
1*  
3$  
3#  
3@  
3!  
3)  
1(  
ƿ
2(  
2*  
2!  
2@  
2#  
2^  
2$ 2^  
2%  
2&  
Fig. 1d: The LXD55-Series Mount.  
Fig. 1e: The LXD55-Series Computer Control Panel (see 2$ above).  
5
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L X D 5 5 -S e r ie s : Y o u r P e r s o n a l  
W in d o w t o t h e U n iv e r s e  
The Meade LXD55-Series models are versatile, high-resolution telescopes. Supplied  
with either an Electronic Controller or an Autostar handbox, the LXD55-Series models  
offer unmatched mechanical and electronic performance.  
Caution: Using products  
other than standard Meade  
accessories may cause dam-  
age to the telescope’s inter-  
nal electronics and may void  
the Meade warranty.  
The LXD55-Series telescopes reveal nature in an ever-expanding level of detail.  
Observe the feather structure of an eagle from 50 yards or study the rings of the plan-  
et Saturn from a distance of 800 million miles. Focus beyond the Solar System and  
observe majestic nebulae, ancient star clusters, and remote galaxies. Meade LXD55-  
Series telescopes are instruments fully capable of growing with your interest and can  
meet the requirements of the most demanding advanced observer.  
Refer to Figures 1a through 1e for the following features:  
B Eyepiece Thumbscrew: Tightens the eyepiece (see d) in place. Tighten to a  
firm feel only.  
C Eyepiece Holder: Holds eyepiece in place. Holders supplied for both 1.25" and  
2" eyepieces.  
d
Want to learn more  
about the eyepieces  
available for your  
LXD55-Series tele-  
scope?  
Diagonal (not shown, achromatic refractor models only): Provides a more  
comfortable right-angle viewing position. Slide the diagonal directly into the eye-  
piece holder (see c) and tighten the thumbscrew on the eyepiece holder to a  
firm feel only. See page 13 for a photo and more information.  
See OPTIONAL  
ACCESSORIES, page  
37.  
D Eyepiece: Place the supplied Super Plössl 26mm eyepiece into the eyepiece  
holder or the diagonal and tighten in place with the eyepiece thumbscrew (see  
b). The eyepiece magnifies the image collected in the optical tube.  
¿ 8 x 50mm (achromatic refractors models) or 6 x 30mm (Schmidt-Newtonian  
models) Viewfinder: A low-power, wide-field sighting scope with crosshairs that  
enables easy centering of objects in the telescope eyepiece (see d).  
e
h
Want to learn more  
about aligning the  
viewfinder? See page  
14.  
´ Viewfinder Collimation Screws (6): Use these screws to adjust the alignment of  
the viewfinder.  
² Viewfinder Front Cell and Locking Ring: Adjust the front cell to focus the  
viewfinder. See step 3, page 14 for more details. The viewfinder is supplied with  
a small dust cover placed over the front cell.  
Want to learn more  
about attaching the  
viewfinder? See page  
12.  
Viewfinder Bracket: Holds the viewfinder in place.  
º Focus Knobs: Moves the telescope’s focuser drawtube in a finely-controlled  
motion to achieve precise image focus. The LXD55-Series telescopes can be  
focused on objects from a distance of about 75 ft. to infinity. Rotate the focus  
knobs to focus on objects.  
¾ Corrector/Dust Cover: Place the dust cover (not visible in photo) over the cor-  
rector when storing the telescope.  
Note: The dust cover should be replaced after each observing session  
and the power turned off to the telescope. Allow time for any dew that  
might have collected during the observing session to evaporate prior to  
replacing the dust cover.  
1!  
1@  
Want to learn more  
about assembling your  
telescope?  
See ASSEMBLING  
YOUR TELESCOPE,  
page 11.  
1) Optical Tube: The main optical component that gathers the light from distant  
objects and brings this light to a focus for examination through the eyepiece.  
1! Cradle Assembly: Attaches to mount base. See 1# and 1$.  
1@ Autostar: See pages 9 and 10 for a description of features.  
EC Handbox users,  
see Appendix D, page  
55, for more informa-  
tion.  
1# Cradle Ring Lock Knobs (2) and Washers (2): Slide washers onto lock knobs  
before inserting. Tighten to a firm feel to secure the optical tube in place.  
1$ Cradle Rings (2): Part of the cradle assembly (see 1!); hold the optical tube firm-  
ly in place.  
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1% Viewfinder Bracket Screws (2): Tighten to a firm feel to hold viewfinder secure-  
ly in place (see E). See page 12 for more information.  
1^ Focus Lock Knob: Designed to prevent the focuser drawtube from moving when  
a heavy accessory, such as a camera, is attached to the focuser assembly. For  
normal observing with an eyepiece and diagonal, it is not necessary to use the  
lock knob.  
Caution When loosening  
the Dec. lock, be sure to  
support the optical tube  
(18, Fig. 1a). The weight of  
the tube could cause the  
tube to swing suddenly.  
1& Dec. Lock: Controls the manual movement of the telescope. Turning the Dec.  
lock counterclockwise unlocks the telescope enabling it to be freely rotated by  
hand about the Dec. axis. Turning the Dec. lock clockwise (to a firm feel only)  
tightens the lock and prevents the telescope from being moved manually, but  
engages the Dec. motor drive (see 3$) for Autostar operation.  
1* PolarViewfinder Cap: Remove this cap when using the polar viewfinder (see 2().  
1( Declination (Dec.) Setting Circle: See APPENDIX A, page 48, for more informa-  
tion.  
2) Counterweight Shaft Base: Thread, along with the shaft, to the mount. See  
page 11 for more information.  
2! Counterweight and Counterweight Lock Knob: Counterbalances the weight of  
the optical tube, and adds stability to the mount. Tighten the lock knob on the side  
of the counterweight to a firm feel to prevent the weight from sliding on the shaft.  
2@ Counterweight Shaft: Slide the counterweight onto this shaft (see 2!).  
2# Counterweight Safety Cap: Prevents the counterweight from accidentally slip-  
ping off the end of the counterweight shaft.  
2$ Computer Control Panel (see Fig. 1e):  
A. Handbox (HBX) Port: Plug the Autostar or EC handbox coil cord (10,  
Fig. 2) into this port.  
B. 12v DC Power Connector: Plug the battery pack into this connector.  
The telescope assembly also may be powered from either a 12v DC  
auto cigarette lighter plug using the optional #607 Cigarette Lighter  
Adaptor or from a standard 115v AC home outlet using the optional  
#547 Power Adapter with Cable or #547F Power Adapter for 220v out-  
lets. See OPTIONAL ACCESSORIES, page 38.  
C. LED: Illuminates when power is supplied to the Autostar or EC hand-  
box and the telescope’s motor drive.  
D. ON/OFF Switch: Turns the Computer Control Panel and Autostar ON  
or OFF.  
E. AUX Port: Provides connection for current and future Meade accessories.  
See OPTIONAL ACCESSORIES, page 38.  
F. Dec Port: Plug the coil cord from the Dec. motor assembly into this port  
for Autostar to control the motor drive.  
2% R.A. Motor Drive Assembly: Controlled by Autostar or EC handbox. Moves the  
optical tube along the R.A. axis. The R.A. Lock (see 3#) must be tightened to a  
firm feel in order for the R.A. motor to operate.  
2^ Latitude Adjustment (2): Sets the latitude of your observing location. The two T-  
handle screws work in a "push - pull" operation—as you tighten one, loosen the  
other. The T-handle above the star marking on top of one of the tripod legs is the  
North T-handle screw (South in the Southern Hemisphere). The leg marked with  
a star must be pointed North (South in the Southern hemisphere) during the polar  
alignment procedure.  
2& Fine Azimuth Control Knobs: Fine tune the side-to-side movement of the tele-  
scope when centering Polaris in the telescope eyepiece or when using the polar  
alignment viewfinder (see 2().  
2*  
Want to learn more  
about setting the lati-  
tude dials?  
2* Latitude Dial: Set the latitude of the observing site on this dial using the latitude  
See STEP 6, page 12.  
T-handle screws. For more information see Step 6, page 12.  
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2( Polar Alignment Viewfinder: Allows you to precisely polar align the telescope.  
Useful when performing astrophotography. See page 50.  
2(  
Want to learn more  
about the polar align-  
ment viewfinder?  
3) Polar Alignment Viewfinder Reticle and LED Knob: Rotate the knob to switch  
on or off the LED that illuminates the reticle within the polar alignment finder. Be  
sure to turn off the LED when finished with the polar viewfinder. Powered by (fac-  
tory-supplied) batteries contained within.  
See the The Polar  
Alignment Viewfinder,  
page 50.  
3! Right Ascension (R.A.) Setting Circle: See APPENDIX A, page 48, for more  
information.  
3@ R.A. Setting Circle Lock Knob: Rotate the knob to lock the R.A. Setting Circle  
(see 3!) in place.  
3# R.A. Lock: Controls the manual movement of the telescope. Turning the R.A.  
lock counterclockwise unlocks the telescope enabling it to be freely rotated by  
hand about the R.A. axis. Turning the R.A. lock clockwise (to a firm feel only)  
tightens the lock and prevents the telescope from being moved manually, but  
engages the R.A. motor drive (see 2%) for Autostar or EC handbox operation.  
3$ Dec. Motor Drive Assembly: Controlled by Autostar or the EC handbox. Moves  
the optical tube along the Dec. axis. The Dec. Lock (see 1&) must be tightened to  
a firm feel in order for the Dec. motor to operate.  
4!  
3% Tripod Leg Adjustment Knobs (3): Tighten to a firm feel to secure tripod legs.  
3^ Variable Height Tripod Legs (3): Supports the telescope mount. Note that one  
legs has a star stamped on top of it. This leg must be pointed North (South in the  
Southern hemisphere) during the alignment procedure. The mount attaches to  
the top of the tripod.  
3& Accessory tray: Set extra eyepieces and other accessory on this convenient  
tray.  
3* Tripod Leg Braces (3): Make the tripod more secure and stable. See Fig. 3.  
Fig. 1f: The LXD55-Series Battery  
Pack and holder.  
3( Accessory Tray Thumbscrew: Attach on the top side of the tray and tighten to a  
firm feel to secure the tray to the tripod and keep the tripod stable. See HOW TO  
ASSEMBLE YOUR TELESCOPE, page 11 for more information.  
4) Tripod Leg Lock Knobs (one on each leg): Loosen these knobs to slide the  
inner leg extension. Tighten the knobs to a firm feel to lock in the height of the tri-  
pod.  
4!  
Want to learn how to  
install the batteries?  
See step 12, page 13.  
4! Battery Pack and holder (see Fig. 1f): Plug into the 12v DC power connector  
(B, Fig. 1e) of the computer control panel. Insert 8 (user-supplied) D-cell batter-  
ies to power motor drives and Autostar handbox.  
Caution: Use care to  
install batteries as indicat-  
ed by the battery com-  
partment. Follow battery  
manufacturer's precau-  
tions. Do not install batter-  
ies backwards or mix new  
and used batteries. Do  
not mix battery types. If  
these precautions are not  
followed, batteries may  
explode, catch fire, or  
leak. Improperly installed  
batteries void your Meade  
warranty. Always remove  
the batteries if they are  
not to be used for a long  
period of time.  
LXD55 TIPS  
J o in a n A s t r o n o m y C lu b , A t t e n d  
a
S t a r P a r t y  
One of the best ways to increase your knowledge of astronomy is to join an astronomy  
club. Check your local newspaper, school, library, or telescope dealer/store to find out if  
there’s a club in your area.  
At club meetings, you will meet other astronomy and Meade enthusiasts with whom you  
will be able to share your discoveries. Clubs are an excellent way to learn more about  
observing the sky, to find out where the best observing sites are, and to compare notes  
about telescopes, eyepieces, filters, tripods, and so forth.  
Often, club members are excellent astrophotographers. Not only will you be able to see  
examples of their art, but you may even be able to pick up some “tricks of the trade” to  
try out on your LXD55-Series telescope. See page 36 for more information about pho-  
tography with the LXD55-Series.  
Many groups also hold regularly scheduled Star Parties at which you can check out and  
observe with many different telescopes and other pieces of astronomical equipment.  
Magazines such as Sky & Telescope and Astronomy print schedules for many popular  
Star Parties around the United States and Canada.  
8
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A U T O S T A R F E A T U R E S  
¹
Important Note: The  
model SN-6EC, model  
SN-8EC, and model AR-  
5EC are equipped with an  
Electronic Controller  
handbox, rather than the  
Autostar Handbox.  
Several of the following  
procedures, such as  
Tracking Objects and  
Initializing Autostar (to  
name but a few), are rele-  
vant only to models  
·
¿
´
»
º
²
equipped with the  
Autostar handbox and do  
not apply to the EC mod-  
els. For more information  
about the EC handbox,  
see APPENDIX D: EC  
HANDBOX, page 55.  
¾
µ
¸
Fig. 2: The Autostar Handbox.  
Tour the Cosmos with Just the Push of a Button  
Note: Autostar does not  
require batteries; the tele-  
scope’s batteries supply  
power to Autostar.  
Control of most LXD55-Series telescope models (excluding the EC models; see mar-  
gin note) is through the operation of Autostar. Nearly all functions of the telescope are  
accomplished with just a few pushes of Autostar’s buttons. Some of the major fea-  
tures of Autostar are:  
I
I
I
Automatic GO TO capability: Automatically move the telescope to any of the  
more than 30,000 objects stored in the object library.  
Take a guided tour of the best celestial objects to view on any given night of the  
year.  
Download the latest satellite data and software revisions directly from the Meade  
website (www.meade.com) and share software with other Autostar enthusiasts.  
Requires optional #505 AstroFinder™ Software and Cable Connector Kit. See  
OPTIONAL ACCESSORIES, page 38.  
I
I
Access a glossary of astronomical terms.  
Fully automatic tracking of celestial objects.  
Features  
The Autostar Computer Controller provides control of virtually every telescope func-  
tion within a compact handbox. Autostar has soft-touch keys designed to have a pos-  
itive feel. The LCD (Liquid Crystal Display) is backlit with a red LED (Light Emitting  
Diode) for easy viewing in the dark. The backlit display, key arrangement, and  
sequential menu structure make Autostar extremely user friendly.  
B 2-Line LCD Display: This screen displays Autostar's menus and other informa-  
tion about the telescope.  
I
I
Top line: Lists the primary menu.  
Bottom line: Contains other menus that may be selected, menu options, tele-  
scope status, or information about a function that is currently being performed.  
C ENTER Key: Press to go to the next menu level or to choose an option in a  
menu. The ENTER key is similar to the RETURN or ENTER key on a computer.  
See MOVING THROUGH AUTOSTAR'S MENUS, page 19 and AUTOSTAR’S MENUS,  
page 25.  
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Note: If ENTER is pressed for two seconds or more and then released,  
Autostar emits a beep and “ENTER to Sync” is displayed. "ENTER to  
Sync" may be used only after your telescope has been aligned and is  
pointing at an object. See page 30 for more details.  
Tip:  
If the "ENTER to Sync"  
feature is accessed by  
mistake, press MODE  
to return to the previous  
screen.  
MODE Key: Press to return to the previous menu level. The top menu level is  
“Select Item." The MODE key is similar to the ESCAPE key on a computer.  
Note: Pressing MODE repeatedly while in the “Select Item” level moves  
Autostar to the topmost screen: “Select Item: Object.”  
Note: If MODE is pressed and held for two seconds or more, information  
about the telescope's status displays. When the status displays, press the  
Scroll keys (7, Fig. 2) to display the following information and more:  
I
Right Ascension and Declination (astronomical) coordinates  
E
Want to learn more  
about using the GO TO  
function? See page  
21.  
IIAltitude (vertical) and Azimuth (horizontal) coordinates  
I Local Time and Local Sidereal Time (LST)  
I Timer and Alarm Status  
Press MODE again to return to the previous menu.  
Want to learn how to  
perform a spiral  
search? See page 21.  
E GO TO Key: Press to slew (move) the telescope to the coordinates of the cur-  
rently selected object. While the telescope is slewing, the operation may be  
aborted at any time by pressing any key except GO TO. Pressing GO TO again  
resumes the slew to the object. Also, press GO TO after a slew is completed to  
activate a "spiral search."  
Definitions:  
"Slew" means to move the  
telescope's optical tube to  
a selected object.  
F Arrow Keys: Press to slew the telescope in a specific direction (up, down, left,  
and right), at any one of nine different speeds. See SLEW SPEEDS, page 16.  
G Number Keys: Press to input digits 0 to 9. When data is not being entered, the  
Number keys can be used to change the slew speed. To operate, just press a  
number key (1 is the slowest speed, 9 is the highest speed). Press the Number  
key "0" to turn on and off the red utility light on the top of the handbox.  
H Scroll Keys: Press to access options within a selected menu. The menu is dis-  
played on the first line of the screen. Options in that menu are displayed, one at  
a time, on the second line. Press the Scroll keys to move through the options.  
Press and hold a Scroll key to move quickly through the options.  
I ? Key: Press to access the "Help" function. Help provides on-screen information  
on how to accomplish whatever task is currently active.  
Hold down the ? key and then follow the prompts on the display to access details  
of Autostar functions in the Help feature. The Help system is essentially an on-  
screen instruction manual.  
If you have a question about an Autostar operation, e.g., INITIALIZATION,  
ALIGNMENT, etc., hold down the ? key and follow the directions that scroll on the  
second line. When satisfied with the Help provided, press MODE to return to the  
original screen and continue with the chosen procedure.  
J Coil Cord Port: Plug one end of the Autostar coil cord (see 1)) into this port  
located at the bottom of the Autostar handbox and the other end into the HBX  
port of the computer control panel (A, Fig. 1e).  
1) Coil Cord: Plug one end of the Autostar coil cord into the HBX port (A, Fig. 1e)  
of the computer control panel of the telescope and the other end into the Autostar  
coil cord port (See J).  
1! RS232 Port: Plug in RS232 connections for downloading and connecting to com-  
puter. Useful for downloading the latest satellite data and software revisions  
directly from the Meade website (www.meade.com) Requires optional #505  
AstroFinder™ Software and Cable Connector Kit. See OPTIONAL ACCESSORIES,  
page 38.  
1@ Utility Light: Use this built-in red light to illuminate star charts and accessories  
without disturbing your eye's adaptation to darkness. Press "0" to turn the light  
on and off.  
10  
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G E T T IN G S T A R T E D  
As you unpack your telescope, carefully note the following parts. The assembly is  
shipped in separate boxes.  
Leg  
Braces  
Telescope Assembly  
I
Equatorial mount with polar alignment finder  
I
Heavy duty, adjustable aluminum tripod with leg braces, three tripod leg lock  
knobs, and a captive mount locking knob  
I
Complete optical tube assembly including primary mirror with dust cover and a  
rack-and-pinion focuser and eyepiece holders for both 1.25" and 2" eyepiece  
holders, tube cradle assembly with two rings and two lock knobs  
Super Plössl (SP) 26mm eyepiece  
Counterweight and counterweight shaft. The 8" and 10" models include extra  
counterweights.  
I
I
Fig. 3: Tripod assembly.  
Slot  
over  
Protrusion  
I
8 x 50mm (achromatic refractors models) or 6 x 30mm (Schmidt-Newtonian  
models) viewfinder  
Motor Assembly  
Mounting  
I
I
I
Factory-mounted dual electronic motor drive assembly  
Autostar handbox, detachable coil cord, or Electronic Controller  
Battery pack and holder  
Thumbscrew  
Accessories  
Accessory shelf with mounting knob, hex keys, LXD55-Series T-Adapter (includ-  
ed with Schmidt-Newtonian models only)  
I
How to Assemble Your Telescope  
The giftboxes contain the optical tube assembly and the tripod with the equatorial  
mount. The accessories are located within compartments custom-cut into the styro-  
foam block inserts.  
Fig. 4: Place slots in tray over protru-  
sions on leg braces.  
1. Remove the components from the giftboxes: Remove and identify the tele-  
scope’s equipment. Refer to Figures 1a through 1f for images of the parts and  
the overall assembly of your telescope. When removing the tripod from the gift-  
box, hold the assembly parallel (horizontal) to the ground or the inner tripod leg  
extensions will slide out as they are not locked in place.  
Fine  
Azimuth  
Control  
Knobs  
Protrusion  
Star  
2. Adjust the tripod legs. Spread the tripod legs as far as they will open, so that  
the leg braces are taut. See Fig. 3.  
3. Attach the accessory shelf to the tripod: Remove the mounting knob from the  
center of the leg braces (39, Fig. 1c). Place the triangular accessory shelf on top  
of the leg braces so that each corner of the triangle lies over a leg brace. Notice  
that there is protrusion on each leg brace. There is a corresponding slot for each  
protrusion on the accessory tray. See Fig. 4. Line up the slots with the protrusions  
and slide the protrusions through the slots to hold the tray in place. Next, slide  
the mounting thumbscrew through the hole in the center of the brace and tighten  
to a firm feel.  
Mount  
Locking  
Knob (not  
visible)  
Fig. 5: Attach the mount to the tripod.  
Dec. Setting Circle  
4. Attach mount to tripod base: Place the mount over the base of the tripod with  
the computer control panel positioned above the tripod leg marked with a star and  
with the protrusion on top of the tripod's base positioned between the fine  
azimuth control knobs. See Fig. 5. Back off the azimuth control knobs wide  
enough for protrusion to fit between them. Slide the hole in the center of the  
underside of the mount onto the captive mount locking bolt in the center of the  
base and tighten it by turning the knob below the base. Tighten to a firm feel.  
Shaft  
Base  
Counterweight  
Lock  
Knob  
Shaft  
5. Attach the counterweight(s) to the counterweight shaft: Place the counter-  
weight shaft base (20, Fig. 1d) over the threaded end of the shaft (22, Fig. 1d).  
Thread the shaft and base assembly into the hole beneath the Dec. setting circle  
as depicted in Fig. 6.  
Safety  
Cap  
Look through the hole in the counterweight and note the pin blocking the hole. Tilt  
the counterweight slightly and the pin moves out of position, clearing the hole. If  
the pin does not move, unscrew the counterweight lock knob slightly until the pin  
moves.  
Fig. 6: Attach Counterweight assem-  
bly.  
11  
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Unscrew the safety cap (23, Fig. 1d) from the shaft. Holding the counterweight  
(21, Fig. 1d) firmly in one hand, slip the counterweight to approximately the mid-  
point of the counterweight shaft (22, Fig. 1d). Tighten the counterweight lock  
knob to a firm feel. Replace the safety cap.  
Note: If the counterweight ever slips, the safety cap (23, Fig. 1d) prevents  
the counterweight from sliding entirely off the shaft. Always leave the  
safety cap in place when the counterweight is on the shaft.  
Cradle Assembly  
Slot  
6. Set the latitude: Setting the latitude is easier if it is set before you attach the opti-  
cal tube to the assembly. Locate the latitude dial (28, Fig. 1d); note that there is  
a triangular pointer above the dial located on the mount. The pointer is not fixed;  
it moves as the mount moves.  
Secondary  
Lock Knob  
Cradle Lock Knob  
Determine the latitude of your observing location. See APPENDIX C: LATITUDE  
CHART, page 54, for a list of latitudes, or check an atlas. Move the latitude T-han-  
dle screws in order to move the mount until the pointer points to your latitude. The  
two T-handle screws work in a "push - pull" operation—as you tighten one, loosen  
the other. When the pointer points at your latitude, tighten both screws until they  
make contact with the mount.  
Fig. 7: Attach cradle to base mount-  
ing slot and tighten locking knobs.  
Cradle Rings  
Also note that below the latitude T-handle screw located directly under the com-  
puter control panel is a star on top of the tripod leg. At your observing site, set up  
the telescope assembly so that this leg approximately faces North (or South in  
the Southern Hemisphere). Model SC-8 users, see APPENDIX E, page 59.  
Lock  
Knobs  
7. Attach the cradle assembly to the mount: Remove the optical tube from the  
cradle and slide the cradle assembly (11, Fig. 1a) onto the cradle mounting slot.  
See Fig. 7. The rounded base of the cradle assembly fits into the rounded por-  
tion of the mounting slot. Tighten both the cradle locking knob and the secondary  
locking knob to a firm feel.  
Fig. 8: Place optical tube in rings  
and loosely tighten cradle ring lock  
knobs.  
8. Position optical tube: Unscrew the cradle ring lock knobs (13, Fig. 1a) and open  
the cradle rings. While firmly holding the optical tube (10, Fig. 1a), position it onto  
the cradle rings (14, Fig. 1a) with the mid-point of the optical tube’s length lying  
roughly in the center of the cradle ring assembly. Point the tube so that the front  
end (this end comes shipped with the dust cover (9, Fig. 1a) over it) is oriented  
as depicted in Fig. 1a. Then close the cradle rings (14, Fig. 1a) over the optical  
tube. Loosely tighten the cradle ring lock knobs just to hold the tube securely in  
place until you balance it. See BALANCING THE TELESCOPE, page 13.  
Note: Model SC-8 users:  
After completing step 6,  
refer to APPENDIX E, page  
59, step 1, for information  
on how to attach the SC  
optical tube to the mount.  
9. Attach viewfinder bracket: Schmidt-Newtonian models (Fig. 9a): Locate the  
viewfinder bracket screws (15, Fig. 1b and Fig. 9a) and remove the nuts from the  
screws. Slide the holes in the viewfinder bracket over the viewfinder bracket  
screws. Replace the nuts and tighten to a firm feel only.  
Viewfinder  
Mounting  
Screws and  
Nuts  
Attach viewfinder tube: Back off the viewfinder collimation screws (5, Fig. 1b)  
and slide the viewfinder tube into the bracket. Orient the viewfinder eyepiece as  
depicted in Fig. 1b. Tighten the collimation screws to a firm feel. See ALIGNING  
THE VIEWFINDER, page 14.  
Fig. 9a: Viewfinder assembly,  
Schmidt-Newtonian models.  
Attach viewfinder bracket: Achromatic refractor and Schmidt-Cassegrain  
models (Fig. 9b): Slide the track on the bottom of the viewfinder bracket into the  
slot in the viewfinder mounting assembly (which is already attached to the tube).  
To secure the viewfinder to the mounting assembly, tighten the two thumbscrews  
to a firm feel only.  
Attach viewfinder tube: Back off the viewfinder collimation screws (5, Fig. 1b)  
and slide the viewfinder tube into the bracket. Point the viewfinder eyepiece  
toward the focuser assembly. See Fig. 10b. Tighten the collimation screws to a  
firm feel. See ALIGNING THE VIEWFINDER, page 14.  
10. Insert the eyepiece: Schmidt-Newtonian models (Fig. 10a): Lift to remove the  
dust cap from the eyepiece holder on the focuser assembly. Set the dust cap  
aside in a safe place and replace it when you have finished observing to protect  
the eyepiece assembly. Back off the eyepiece thumbscrews (1, Fig. 1a) and  
insert the supplied SP 26mm eyepiece (3, Fig. 1a) into the the eyepiece holder.  
Tighten the holder thumbscrews to a firm feel to secure the eyepiece.  
Fig. 9b: Viewfinder assembly, refrac-  
tor models. Slide bracket into slot.  
12  
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Insert the eyepiece: Achromatic refractor and Schmidt-Cassegrain models  
(Fig. 10b): Lift to remove the dust cap from the eyepiece holder on the focuser  
assembly. Set the dust cap aside in a safe place and replace it when you have  
finished observing to protect the eyepiece assembly. Back off the eyepiece  
thumbscrews (1, Fig. 1b) and slide the diagonal into the holder and tighten the  
thumbscrews to a firm feel only. Insert the supplied SP 26mm eyepiece (3, Fig.  
1b) into the the diagonal. Tighten the diagonal's thumbscrews to a firm feel to  
secure the eyepiece.  
Eyepiece  
Holder  
Note: Two eyepiece holders are included with your telescope—for both  
1.25" and 2" eyepieces.To change eyepiece holders, unscrew the attached  
holder from the focuser and thread on the other holder.  
Thumbscrew  
11. Adjust the height of the tripod: Adjust the height of the tripod by loosening the  
tripod lock knobs (Fig. 11). Extend the sliding inner section of each tripod leg to  
the desired length; then tighten each knob. Adjust the tripod to a height that is  
comfortable for viewing.  
Fig. 10a: Insert eyepiece into holder  
and tighten thumbscrews.  
Viewfinder  
Eyepiece  
12. Install Batteries: Insert eight (user-supplied) D-size batteries into the battery  
holder, oriented as shown in the diagram on the battery slots of the holder. Plug  
the battery pack into the 12v DC connector (B, Fig. 1e) on the computer control  
panel. See Fig. 12.  
Eyepiece  
Thumbscrews  
Holder  
Caution: Use care to install batteries as indicated by the battery com-  
partment. Follow battery manufacturer's precautions. Do not install bat-  
teries backwards or mix new and used batteries. Do not mix battery types.  
If these precautions are not followed, batteries may explode, catch fire, or  
leak. Improperly installed batteries void your Meade warranty. Always  
remove the batteries if they are not to be used for a long period of time.  
Diagonal  
Fig. 10b: Insert eyepiece into diagonal  
and tighten thumbscrews.  
Leg  
Lock  
Knob  
Fig. 13b: Reticle LED assembly: (A) Reticle Container; (B) LED;  
(C) Batteries; (D) Battery Holder; (E) Threaded Lid; (F) Thumbscrew.  
Fig. 11: Adjust the tripod height  
using the leg lock knobs.  
13. Remove Plastic from Reticle LED: The polar alignment reticle LED (30, Fig. 1d)  
contains two watch batteries. The reticle's LED is shipped with a plastic strip  
between the two batteries to protect battery life. Unthread both the thumbscrew (F)  
and the threaded lid (E). Remove the plastic strip before using. Refer to the reti-  
cle assembly in Fig. 13b and note the orientation of the batteries. Place the bat-  
teries (C) into the battery holder (D) before inserting into the reticle container (A).  
Note: Remember to turn off the LED when you are not using the reticle.  
14. Plug in Autostar or EC Handbox: Plug the Autostar or EC handbox cable into  
the HBX port (A, Fig. 1e).  
Balancing the Telescope  
Fig. 12: Battery holder.  
In order for the telescope to be stable on the tripod and also for it to move smoothly,  
it must be balanced. To balance the telescope, unlock the Right Ascension or R.A.  
lock (33, Fig. 1d). When this axis is unlocked, the telescope pivots on the R.A. axis.  
Later in the procedure, you will also unlock the Declination or Dec. lock (17, Fig. 1d).  
When unlocked, the telescope pivots on the Dec. axis. Most of the motion of the tel-  
escope takes place by moving about these two axes, separately or simultaneously.  
Try to become familiar with these locks and observe how the telescope moves on  
each axis. To obtain a fine balance of the telescope, follow the method below:  
Polar  
Viewfinder  
Reticle LED  
1. Firmly hold the optical tube secure so that it cannot accidentally swing freely.  
Loosen the R.A. lock (33, Fig. 1d). The optical tube now moves freely about the  
R.A. axis. Rotate the telescope so that the counterweight shaft (22, Fig. 1d) is  
parallel (horizontal) to the ground.  
Fig. 13a: Remove plastic from reticle  
batteries  
2. Unlock the counterweight lock knob and slide the counterweight (21, Fig. 1d)  
along the counterweight shaft until the telescope remains in one position without 13  
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tending to drift down in either direction. Then re-tighten the counterweight lock  
knob, locking the counterweight in position.  
3. Achromatic refractor and Schmidt-Newtonian models: Again, hold the optical  
tube so that it cannot accidentally swing freely. Lock the R.A. lock (33, Fig. 1d),  
and unlock the Dec. lock (17, Fig. 1d). The telescope now is able to move freely  
about the Dec. axis. Loosen the cradle ring lock knobs (13, Fig. 1a) so that the  
main tube slides easily back and forth in the cradle rings. Move the main tube in  
the cradle rings until the telescope remains in one position without tending to drift  
down in either direction. Re-lock the Dec. lock (17, Fig. 1d).  
The telescope is now properly balanced on both axes. Next, the viewfinder must be  
aligned.  
Aligning the Viewfinder  
The wide field of view of the telescope's viewfinder (4, Fig. 1a) provides an easier way  
to initially sight objects than the main telescope's eyepiece (3, Fig. 1a), which has a  
much narrower field of view. If you have not already attached the viewfinder to the tel-  
escope tube assembly, follow the procedure described in step 9, page 12.  
Viewfinder  
Eyepiece  
Collimation Screws  
In order for the viewfinder to be useful, it must be aligned to the main telescope, so  
that both the viewfinder and telescope's optical tube (10, Fig. 1a) point at the same  
position in the sky. This alignment makes it easier to find objects: First locate an  
object in the wide-field viewfinder, then look into the eyepiece of the main telescope  
for a detailed view.  
Viewfinder  
Bracket  
To align the viewfinder, perform steps 1 through 4 during the daytime; perform step 5  
at night. Both the 6 x 30mm and the 8 x 50mm viewfinders align in an identical man-  
ner. Refer to Fig. 14.  
Fig. 14: Viewfinder Alignment.  
1. Remove the dust covers from the optical tube (9, Fig. 1a) and the viewfinder.  
2. If you have not already done so, insert the low-power SP 26mm eyepiece (3, Fig.  
Important Note: Objects  
appear upside-down and  
reversed left-for-right when  
observed in the viewfinder.  
With refracting telescope  
models, objects viewed  
through the main telescope  
with the diagonal mirror in  
place are seen right-side-up,  
but reversed left-for-right.  
1b) into the eyepiece holder of the main telescope. See step 10, page 12.  
3. Look through the viewfinder eyepiece at an object at least one-half mile away  
(Tip: Remove the viewfinder tube from the bracket to simplify this operation). If  
the distant object is not in focus, turn the focus lock ring counterclockwise to  
loosen the viewfinder front cell (6, Fig. 1b). Twist the front cell until focus is  
achieved and retighten the focus lock ring.  
4. Unlock the R.A. lock (33, Fig. 1d) and the Dec lock (17, Fig. 1d) so that the tel-  
escope turns freely on both axes. Then point the main telescope at a tall, well-  
defined and stationary land object (e.g., the top of a telephone pole) at least 200  
yards distant and center the object in the telescope's eyepiece. Focus the image  
by turning the focus knobs (8, Fig. 1b). Retighten the R.A. and Dec. locks.  
This image inversion is of no  
consequence when observ-  
ing astronomical objects,  
and in fact all astronomical  
telescopes yield inverted  
images.  
5. Look through the viewfinder and loosen or tighten, as appropriate, one or more  
of the viewfinder collimation thumbscrews (5, Fig. 1b) until the viewfinder’s  
crosshairs are precisely centered on the object you previously centered in the  
main telescope's eyepiece. You are now ready to make your first observations  
with your telescope.  
During terrestrial observing,  
where a fully-correctly-orient-  
ed image (right-side up and  
correct left-for-right) is desir-  
able, an optional Meade  
#928 45° Erect-Image  
Diagonal Prism is available.  
See OPTIONAL ACCES-  
SORIES, page 38.  
NEVER point the telescope directly at or near the Sun at any time!  
Observing the Sun, even for the smallest fraction of a second, will  
result in instant and irreversible eye damage, as well as physical  
damage to the telescope itself.  
5. Check this alignment on a celestial object, such as a bright star or the Moon, and  
make any necessary refinements, using the method outlined above in steps 3 and  
4.  
Note that for Schmidt-  
Newtonian models, no  
With this alignment performed, objects first located in the wide-field viewfinder will  
also appear in the telescope's eyepiece.  
means of image inversion is  
available; while these tele-  
scopes may be used for ter-  
restrial observing, the image  
will not be correctly oriented  
in either right-side-up or left-  
for-right orientations.  
Choosing an Eyepiece  
A telescope’s eyepiece magnifies the image formed by the telescope’s main optics.  
Each eyepiece has a focal length, expressed in millimeters, or “mm.” The smaller the  
focal length, the higher the magnification. For example, an eyepiece with a focal length  
of 9mm has a higher magnification than an eyepiece with a focal length of 26mm.  
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Your telescope comes supplied with a Super Plössl (SP) 26mm eyepiece which gives  
a wide, comfortable field of view with high image resolution.  
Note: Seeing conditions  
vary widely from night-to-  
night and site-to-site.  
Low power eyepieces offer a wide field of view, bright, high-contrast images, and eye  
relief during long observing sessions. To find an object with a telescope, always start  
with a lower power eyepiece such as the Super Plössl 26mm. When the object is  
located and centered in the eyepiece, you may wish to switch to a higher power eye-  
piece to enlarge the image as much as practical for prevailing seeing conditions. For  
information about optional eyepieces for the LXD55-Series models, see OPTIONAL  
ACCESSORIES, page 37.  
Turbulence in the air, even  
on an apparently clear  
night, can distort images. If  
an image appears fuzzy  
and ill-defined, back off to a  
lower power eyepiece for a  
more well-resolved image  
(see Fig. 15a and 15b  
below).  
The power, or magnification of a telescope is determined by the focal length of the tel-  
escope and the focal length of the eyepiece being used. To calculate eyepiece power,  
divide the telescope's focal length by the eyepiece's focal length. For example, a  
26mm eyepiece is supplied with the LXD55-Series. The focal length of the 8" LXD55-  
Series model is 812mm (see SPECIFICATIONS, page 45).  
Note: For a list of magnifi-  
cation ratings of the eye-  
pieces available for the  
LXD55-Series telescopes,  
see OPTIONAL ACCES-  
SORIES, page 37.  
Telescope Focal Length ÷ Eyepiece Focal Length = Eyepiece Power  
Telescope Focal Length = 812mm  
Eyepiece Focal Length  
812 ÷ 26  
= 26mm  
= 31  
The eyepiece power, or magnification is therefore 31X (approximately).  
Observing by Moving the Telescope Manually  
After the telescope is assembled and balanced as described previously, you are ready  
to begin manual observations. View easy-to-find terrestrial objects such as street  
signs or traffic lights to become accustomed to the functions and operations of the tel-  
escope. For the best results during observations, follow the suggestions below:  
I
When you wish to locate an object to observe, first loosen the telescope’s R.A.  
lock (33, Fig. 1d) and Dec. lock (17, Fig. 1d). The telescope can now turn freely  
on its axes. Unlock each axis separately and practice moving your telescope.  
Then practice with two unlocked axes at the same time. It is very important to  
practice this step to understand how your telescope moves, as the movement  
of an equatorial mount is not intuitive.  
I
I
Use the aligned viewfinder to sight-in on the object you wish to observe. When the  
object is centered in the viewfinder’s crosshairs, re-tighten the R.A. and Dec. locks.  
A telescope’s eyepiece magnifies the image formed by the telescope’s main  
optics. Each eyepiece has a focal length, expressed in millimeters, or “mm.” The  
smaller the focal length, the higher the magnification. For example, an eyepiece  
with a focal length of 9mm has a higher magnification than an eyepiece with a  
focal length of 26mm.  
Low-power magnification eyepieces offer a wide field of view, bright, high-contrast  
images, and relief of eye strain during long observing sessions. To observe an object  
with a telescope, always start with a low power eyepiece such as the SP 26mm  
LXD55 TIPS  
T o o M u c h P o w e r ?  
Can you ever have too much power? If the type of power you’re referring to is  
eyepiece magnification, yes, you can! The most common mistake of the begin-  
ning observer is to “overpower” a telescope by using high magnifications which  
the telescope’s aperture and atmospheric conditions cannot reasonably support.  
Keep in mind that a smaller, but bright and well-resolved image is far superior to  
one that is larger, but dim and poorly resolved (see Figs. 15a and 15b). Powers  
above 400X should be employed only under the steadiest atmospheric condi-  
tions.  
Fig. 15a & 15b: Jupiter; examples of  
the right amount of magnification and  
too much magnification.  
Autostar can calculate the best eyepiece for you to use. Try out the “Eyepiece  
Calc” feature in the Utilities menu.  
Most observers should have three or four additional eyepieces to achieve the full  
range of reasonable magnifications possible with the LXD55-Series telescopes.  
See OPTIONAL ACCESSORIES, page 37.  
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supplied with your telescope. When the object is centered and focused in the eye-  
piece, switch to a higher power eyepiece to enlarge the image as much as practi-  
cal for prevailing viewing conditions. For information about other eyepieces avail-  
able for your telescope, see OPTIONAL ACCESSORIES, page 37.  
I
Once centered, an object can be focused by turning one of the knobs of the  
focusing mechanism (8, Fig. 1b). Notice that when observing astronomical  
objects, the field of view begins to slowly drift across the eyepiece field. This  
motion is caused by the rotation of the Earth on its axis. Objects appear to move  
through the field more rapidly at higher powers. See TRACKING OBJECTS, page  
17, for detailed information on how you can counteract the drift in the field of view.  
Activate the Arrow Keys (Autostar Models Only)  
Autostar's Arrow keys allow you to slew (move) the telescope up, down, right, or left.  
The following procedure describes how to activate Autostar's Arrow keys:  
Note: Autostar only  
prompts you to enter  
Country (or State) and  
City as described in steps  
3, 4, and 5, the first time it  
is activated. These  
prompts do not appear  
again, unless you reset  
Autostar (see RESET,  
page 31).  
1. After the batteries are installed and Autostar's cord is plugged into the HBX port  
of computer control panel (A, Fig 1e), a copyright message lights on the Autostar  
LCD display (1, Fig. 2).  
2. A message warning not to look at the Sun scrolls across the display. Press the  
key prompted by Autostar to acknowledge that the Sun warning has been read  
and understood.  
3. Press ENTER (2, Fig. 2) repeatedly until "Country/State" appears on the display.  
(Ignore the prompts requesting Date and Time. See INITIALIZING AUTOSTAR,  
page 19, for more information).  
However, if you need to  
re-enter this information  
(e.g., you change your  
geographic location), you  
can change the location  
information by using the  
Site option of the Setup  
menu. See ADDING  
4. Use the Scroll keys (7, Fig. 2) to cycle through the database of countries, states,  
and provinces. Press ENTER when the correct location displays.  
5. Autostar then prompts you to enter the nearest city (listed alphabetically) to the  
observing site. Use the Scroll keys to cycle through the database of cities. Press  
ENTER when the correct city appears on the display.  
6. Autostar then prompts you to enter the model number of your telescope. Use the  
Scroll keys to cycle through the list of telescope models. Press ENTER when the  
correct model appears on the display.  
OBSERVING SITES, page  
32, for detailed informa-  
tion.  
7. The display then reads "Align: Easy." You now can use Autostar's Arrow keys to  
move the telescope to observe.  
Note: If you go past the "Align: Easy" (or any other menu display you wish  
to select), press MODE to return to the previous display(s).  
8. Press the Arrow keys (5, Fig. 2) to move the telescope up, down, right, or left.  
You can move the telescope at different speeds.  
Slew Speeds (Autostar Models Only)  
Autostar has nine slew speeds that move the optical tube at rates that are directly pro-  
portional to the sidereal rate and have been calculated to accomplish specific func-  
tions. Press a Number key (6, Fig. 2) to change the slew speed, which is shown for  
about two seconds on Autostar’s display.  
The nine available speeds are:  
Number Key 1 =  
Number Key 2 =  
Number Key 3 =  
1x =  
2x =  
8x =  
1 x sidereal (0.25 arc-min/sec or 0.004°/sec)  
2 x sidereal (0.5 arc-min/sec or 0.008°/sec)  
8 x sidereal (2 arc-min/sec or 0.033°/sec)  
16 x sidereal (4 arc-min/sec or 0.067°/sec)  
64 x sidereal (16 arc-min/sec or 0.27°/sec)  
30 arc-min/sec or 0.5°/sec  
Number Key 4 = 16x =  
Number Key 5 = 64x =  
Number Key 6 = 128x =  
Number Key 7 = 1.5° =  
90 arc-min/sec or 1.5°/sec  
Number Key 8 =  
3° = 180 arc-min/sec or 3°/sec  
Number Key 9 = Max = 270 arc-min/sec or 4.5°/sec  
16  
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Speeds 1, 2, or 3: Best used for fine centering of an object in the field of view of a  
higher power eyepiece, such as a 12mm or a 9mm eyepiece.  
Speeds 4, 5, or 6: Enables centering an object in the field of a low-to-moderate power  
eyepiece, such as the standard Super Plössl 26mm.  
Speeds 7 or 8: Best used for rough centering of an object in the viewfinder.  
Note: If you wish to per-  
form a more precise  
polar alignment for the  
purposes of astrophotog-  
raphy, see "Appendix B,"  
page 50.  
Speed 9: Moves the telescope quickly from one point in the sky to another.  
Observe the Moon  
Point your telescope at the Moon (note that the Moon is not visible every night). Use  
your EC handbox or Autostar to practice using the Arrow keys and the slew speeds to  
view different features. The Moon contains many interesting features, including  
craters, mountain ranges, and fault lines. The best time to view the Moon is during its  
crescent or half phase. Sunlight strikes the Moon at an angle during these periods and  
adds a depth to the view. No shadows are seen during a full Moon, making the over-  
ly bright surface to appear flat and rather uninteresting. Consider the use of a neutral  
density Moon filter when observing the Moon. See OPTIONAL ACCESSORIES, page  
38. Not only does it cut down the Moon's bright glare, but it also enhances contrast,  
providing a more dramatic image.  
Point optical  
tube to North  
North  
Point  
counterweight  
shaft straight  
down over  
mount.  
Tracking Objects  
Level  
Mount  
As the Earth rotates beneath the night sky, the stars appear to move from East to  
West. The speed at which the stars move is called the sidereal rate. You can setup  
your telescope to move at the sidereal rate so that it automatically tracks the stars and  
other objects in the night sky. The tracking function automatically keeps an object  
more or less centered in the telescope’s eyepiece.  
To automatically track objects, you first need to learn how to set the polar home position  
of your telescope and then how to select "Targets: Astronomical" from the Autostar  
Setup menu. EC handbox users, see APPENDIX D, page 55, for more information.  
Point leg marked with  
a star to North  
Setting the Polar Home Position  
1. Level the mount, if necessary, by adjusting the length of the three tripod legs.  
2. Unlock the R.A. Lock (33, Fig. 1d). Rotate the Optical Tube Assembly until the  
Fig. 16a: The polar home position,  
side view.  
counterweight shaft is pointing straight down over the mount. See Figs. 16a and  
16b.  
3. If you have not already done so, lift the telescope assembly and turn it so that the  
tripod leg marked with a star faces approximately North (South in the Southern  
Hemisphere). Release the Dec. lock (17, Fig. 1d) of the tripod, so that the opti-  
cal tube (10, Fig. 1a) may be rotated. Rotate the optical tube until it points North  
(or South in the Southern Hemisphere). Then re-tighten the lock. Locate Polaris,  
the North Star, if necessary, to use as an accurate reference for due North (or  
Octantis in the Southern Hemisphere). See LOCATING THE CELESTIAL POLE,  
page 49.  
4. If you have not already done so, determine the latitude of your observing location.  
See APPENDIX C: LATITUDE CHART, page 54, for a list of latitudes of major cities  
around the world. Use the latitude T-handle screws (26, Fig. 1d) to tilt the tele-  
scope mount so that the pointer indicates the correct latitude of your viewing loca-  
tion on the latitude dial (28, Fig. 1d). See step 6, page 12 for more information.  
5. If steps 1 through 4 above were performed with reasonable accuracy, your tele-  
scope is now sufficiently well-aligned to Polaris, the North Star, for you to begin  
making observations.  
Once the mount has been placed in the polar home position as described above, the  
latitude angle need not be adjusted again, unless you move to a different geographi-  
cal location (i.e., a different latitude).  
Important Note: For almost all astronomical observing requirements,  
approximate settings of the telescope’s latitude and other settings are  
acceptable. Do not allow undue attention to precise settings of polar home  
position of the telescope to interfere with your basic enjoyment of the  
instrument.  
Fig. 16b: The polar home position,  
front view.  
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Observe a Star using the Automatic Tracking Feature  
In this example, Autostar's Arrow keys are used to find a star, and then Autostar's  
tracking capability automatically keeps the star centered in your telescope's eyepiece.  
EC handbox users, see APPENDIX D, page 55, for information about tracking with the  
EC handbox.  
Tip:  
You can change the tele-  
scope's slew rate while  
centering an object in the  
eyepiece. See SLEW  
SPEEDS, page 16 for  
more information.  
1. If you have activated the Arrow keys and completed setting the telescope in the  
polar home position, Autostar's display now reads "Align: Easy." Go to Step 2.  
If you have not used Autostar yet or have just plugged it into the HBX port, per-  
form the procedures described in ACTIVATETHE ARROW KEYS, page 16 and SET-  
TING THE POLAR HOME POSITION, page 17. Then go to Step 2 of this procedure.  
If you have been using Autostar to perform other functions and the display does  
not read "Align: Easy," follow these steps:  
a. Press MODE (3, Fig. 2) repeatedly until "Select Item: Object" displays.  
b. Press the Scroll Up key (7, Fig. 2) once. "Select Item: Setup" displays.  
c. Press ENTER (2, Fig. 2). "Setup: Align" displays. Go to Step 3.  
Important Note: While  
performing the automatic  
tracking procedure, you  
may use the Arrow keys  
to move the telescope or  
you may also loosen the  
telescope locks (17 and  
33, Fig. 1d) and move  
the optical tube manually  
to locate another object  
in the sky. The tracking  
function will continue to  
be operational and the  
telescope will track the  
new object.  
2. Press MODE (3, Fig. 2). "Setup: Align" displays.  
3. Press the Scroll Down key repeatedly until "Setup: Targets" displays. Press  
ENTER (2, Fig. 2).  
4. "Targets: Terrestrial" displays. Press one of the Scroll keys once (7, Fig. 2).  
"Targets: Astronomical" now displays.  
5. Use the Arrow keys (5, Fig. 2) to locate a bright star in the night sky. Use the  
viewfinder to help line up on the star. You may choose any unobstructed, bright  
star for the purposes of this example. Use Autostar's Arrow keys to center the star  
in the eyepiece. Once the star is centered, press ENTER to select  
"Astronomical." The telescope's tracking motors then engage. It may take the  
tracking motors several seconds to begin tracking. When they do, it may be nec-  
essary to once again center the star in the eyepiece. The tracking motors will  
then keep any star you choose in the center of the eyepiece.  
6. Press and hold the ENTER key for a few seconds and then release to stop track-  
ing. You may also stop tracking by choosing "Terrestrial" in the Targets menu.  
Using Autostar's GOTO Capabilities (Autostar Models Only)  
Before you can use Autostar's GO TO capabilities, you must first:  
Learn how Autostar's keys move through the menus  
Initialize Autostar  
Place the telescope in the polar home position, if you have not already done so  
(see SETTING THE POLAR HOME POSITION, page 17)  
Select "Align: Easy" from Autostar's menus  
LXD55 TIPS  
W h ic h O n e ’s t h e A lig n m e n t S t a r ?  
If Autostar has chosen an alignment star with which you are unfamiliar, how can  
you be sure if the star in your eyepiece is really the alignment star?  
The rule of thumb is that an alignment star is usually the brightest star in that  
area of the sky. If you perform a GO TO to an alignment star and you're not sure  
if you have located the alignment star or it isn't in the eyepiece, look through your  
viewfinder. When you view an alignment star in the viewfinder, it stands out dra-  
matically from the rest of the stars in that portion of the sky. The viewfinder will  
help you locate a star more quickly than the eyepiece, because it has a much  
wider field of view than the eyepiece. Using Autostar, set the slew speed to 6 or  
higher and use the Arrow keys to center the alignment star in the viewfinder. If  
your viewfinder has been aligned with the telescope, the alignment star should  
now be in the eyepiece. Set the slew speed to 4 or less and center the star in  
the eyepiece. Also see the "Spiral Search" tip on page 21.  
If you have an obstruction, such as a tree or a building blocking your view of the  
alignment star, or if you have any doubts at all about the star that has been cho-  
sen, no problem. Just press the Scroll Down key and Autostar will find another  
star to align upon.  
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Moving Through Autostar’s Menus (Autostar Models Only)  
Autostar's menus are organized for quick and easy navigation.  
Tip:  
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Press ENTER (2, Fig. 2) to go deeper into Autostar menu levels.  
Press MODE (3, Fig. 2) to move back toward the top menu level.  
Press the Scroll keys (7, Fig. 2) to move up and down through the options avail-  
able for each menu level.  
Press the Arrow keys (5, Fig. 2) to enter characters.  
Press the Number keys (6, Fig. 2) to enter digits.  
When multiple choices are  
available within a menu  
option, the current option is  
usually displayed first and  
highlighted by a right point-  
ing arrow (>).  
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Initializing Autostar (Autostar Models Only)  
This exercise describes how to initialize Autostar.  
Note: Normally, you will enter the Time and Date at the beginning of each  
observing session, but you will only perform the full Initialization proce-  
dure (i.e., entering the Location information and selecting the model num-  
ber as well as entering the Time and Date) the first time you use Autostar  
or after performing a Reset.  
Definition:  
Initialization is a proce-  
dure that ensures that  
Autostar operates correctly.  
When you first use  
Autostar, it doesn't yet  
know where the observa-  
tion location site is or the  
time or date of the obser-  
vation session.  
1. Make sure that the telescope is assembled correctly, and that the batteries are  
installed as described previously.  
2. Make sure the On/Off switch (D, Fig. 1e) is in the Off position. Plug Autostar's  
cord into the HBX port (A, Fig. 1e), as previously described. Push the On/Off  
switch to the On position.  
3. A copyright message lights on Autostar’s LCD display and a message warning  
not to look at the Sun scrolls across the display. Press the key prompted by  
Autostar to acknowledge the message has been read and understood.  
You will enter information,  
such as the current time  
and date, and observation  
location.  
Autostar uses this informa-  
tion to precisely calculate  
the location of celestial  
objects (such as stars and  
planets) and to automati-  
cally move your telescope  
correctly for various opera-  
tions.  
4. The Getting Started menu displays a scrolling message with two choices:  
a. Press and hold down the ? key (8, Fig. 2) for about 2 seconds for informa-  
tion on Autostar functions and controls. When finished, press MODE (3, Fig.  
2) to exit Help, or,  
b. Press ENTER (2, Fig. 2) to bypass the Help tutorial and continue with  
Initialization.  
5. Autostar prompts you to enter the current date:  
a. Press the Numbers keys (6, Fig. 2) to enter numbers 0 through 9. After the  
desired number is displayed, use the Right Arrow key (5, Fig. 2) to move the  
cursor from one number to the next in the day display (or use the Left Arrow  
key to move in the other direction across the display, if necessary).  
b. Use the Right Arrow key (5, Fig. 2) to move the cursor to the month. Use the  
Scroll keys (7, Fig. 2) to cycle through the list of months. When the current  
month is displayed, use the Right Arrow (5, Fig. 2) to move the cursor to the  
year.  
c. Use Number keys (6, Fig. 2) to enter all four digits of the current year. Use  
the Right Arrow key (5, Fig. 2) to move the cursor from one number to the  
next.  
d. Press ENTER (2, Fig. 2) when the entire date has been entered.  
6. Autostar then prompts you to enter the current time. Use the Number keys to  
enter digits. The Right and Left Arrow keys move the cursor across the screen  
as described in the previous step. Enter the current time (use a "0" for the first  
digit if less than 10). Use the Up Arrow key (7, Fig. 2) to scroll through "AM,"  
"PM,'" or "blank." The "blank" option (screen displays neither AM nor PM) selects  
the 24-hour (i.e., military time) clock. Then press ENTER to start the clock.  
7. Autostar then prompts you to enter the status of Daylight Savings Time. Press  
one of the Scroll keys to toggle between the YES/NO settings. Select the desired  
setting by pressing ENTER.  
Note: Daylight Savings Time may be referred to by a different name in  
various areas of the world.  
8. If you have previously entered the Country/State and City of your observing site  
(as described in ACTIVATE THE ARROW KEYS, page 16), go to step 9. If you have  
not entered this information, perform the following steps:  
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a. Autostar prompts you to enter the Country or State (listed alphabetically) of  
the observing site. Use the Scroll keys to cycle through the database of  
countries, states, and provinces. Press ENTER when the correct location  
displays.  
b. Autostar then prompts you to enter the nearest city (listed alphabetically) to  
the observing site. Use the Scroll keys to cycle through the database of  
cities. Press ENTER when the correct city appears on screen.  
9. Autostar then prompts you to enter the model number of your telescope. Use the  
Scroll keys to cycle through the list of telescope models. Press ENTER when the  
correct model appears on the display.  
Note: Autostar only prompts you to enter Country/State and City and  
model number the first time it is activated. These prompts do not appear  
again, unless you reset Autostar (see RESET, page 31). However, if you  
need to enter this information (e.g., you change your geographic location),  
you can do so by using the Site option of the Setup menu. See ADDING  
OBSERVING SITES, page 32, for detailed information.  
10. System Initialization is complete and the display reads "Align: Easy." After per-  
forming the Initialization procedure, you MUST train your drive.  
Training the Drive (Autostar Models Only)  
Next, train the drive using Autostar. Perform this procedure the first time you use  
Autostar with your telescope, after a Reset, or if you are experiencing any pointing  
accuracy problems. Training the drive gives your telescope a higher degree of point-  
ing accuracy.  
Note: Use a terrestrial object, such as a telephone pole or lamp post, to  
train the drive. It is best to perform this procedure during the daytime.  
Complete this exercise once every 3 to 6 months to maintain the highest  
level of telescope pointing accuracy.  
1. If you have just performed INITIALIZING AUTOSTAR, go to step 2.  
If you have not yet initialized Autostar, go to page 19 and follow the procedure  
described in INITIALIZING AUTOSTAR.Then go to step 2 of this procedure.  
2. Keep pressing MODE until "Select Item: Object" displays.  
3. Press the Scroll Up key once. "Select: Item: Setup" displays.  
4. Press ENTER to access the Setup menu. "Setup: Align" displays.  
5. Keep pressing the Scroll Up key until "Setup: Telescope" displays.  
6. Press ENTER to access the Telescope menu. "Telescope: Focal Length" dis-  
plays.  
7. Keep pressing the Scroll Down key until "Telescope: Train Drive" displays.  
8. Press ENTER to choose the Train Drive option. "Train Drive: Az/RA Train" dis-  
plays.  
9. Press ENTER to begin Az/R.A. (Right Ascension) training.  
10. "Drive Setup: For this...." begins to scroll across the display. This is a reminder to  
point your telescope at a terrestrial object. Loosen the R.A. and Dec. locks (17  
and 33, Fig. 1d) and point the telescope at an object. Then re-tighten the locks.  
Press ENTER when the telescope is pointing at the desired terrestrial object.  
11. "Center reference object" displays. Center your target object using the Arrow  
keys. When centered, press ENTER.  
12. The telescope slews and "Press > until it is centered" displays. Press the Right  
Arrow key until the target is centered again. Then press ENTER.  
Note: If you pass the object when pressing the Arrow key, you cannot slew  
the telescope back in the other direction. Press MODE until "Train Drive:  
Az/RA Train" displays and begin the procedure over again.  
13. The telescope slews and "Press < until it is centered" displays. Press the Left  
Arrow key until the target is centered again. Then press ENTER.  
14. "Train Drive: Az/RA Train" displays again. Press the Scroll Down key and "Train  
Drive: Alt/Dec Train" displays. Press ENTER to begin Alt/Dec. (Declination) training.  
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15. "Drive Setup: For this...." begins to scroll across the display. This is another  
reminder to point your telescope at a terrestrial object. Loosen the R.A. and Dec.  
locks (17 and 33, Fig. 1d) and point the telescope at an object. Then re-tighten  
the locks. Press ENTER when the telescope is pointing at the desired terrestrial  
object.  
16. "Center reference object" displays. Center your target object using the Arrow  
keys. When centered, press ENTER.  
V
17. The telescope slews and "Press until it is centered" displays. Press the Up  
Arrow key until the target is centered again. Then press ENTER.  
18. The telescope slews and "Press V until it is centered" displays. Press the Down  
Arrow key until the target is centered again. Then press ENTER. "Train Drive:  
Alt/Dec Train" displays again. You have now completed this procedure. Continue  
onto the next procedure, EASY ALIGNMENT.  
Note: Two other alignment  
methods, One-Star and  
Two-Star Polar alignment,  
are available as options in  
the "Setup: Align" menu.  
See page 49 for more  
information.  
Easy Alignment (Autostar Models Only)  
After completing the "Train the Drive" procedure, align your telescope using Autostar.  
The fastest and easiest way to start observing with Autostar's Go To capabilities is to  
align your telescope using the Easy Alignment.  
1. Keep pressing MODE until "Select Item: Setup" is displayed. Press ENTER.  
2. "Setup: Align" displays. Press ENTER. "Align: Easy" displays. Press ENTER.  
Tip:  
The GO TO key also  
allows you to perform a  
"spiral search." A spiral  
search is useful when the  
telescope slews to an  
object, but that object is  
not visible in the eyepiece  
after the telescope finishes  
its search. (This some-  
times occurs during an  
alignment procedure.)  
3. "German North" displays and a scrolling message prompts you to set your tele-  
scope in the polar home position. See SETTINGTHE POLAR HOME POSITION, page  
17, for a description of this procedure. Press ENTER after you finish the proce-  
dure.  
4. Autostar then chooses two stars from its database to align upon. When the tele-  
scope slews to the star for alignment, it may not appear in the field of view in the  
eyepiece. Use the Arrow keys to move the telescope until the star is visible and  
centered in the eyepiece. The alignment star should be easily recognized and be  
the brightest star in the area of the sky where the telescope is pointing. See WHICH  
ONE'STHE ALIGNMENT STAR, page 18, for more information. When the star is cen-  
tered, press ENTER. Repeat the procedure for the second alignment star.  
Press GO TO when the  
telescope stops slewing.  
The telescope begins to  
move in a spiral pattern at  
a very slow speed (you  
may change the slew  
speed if you wish—see  
SLEW SPEEDS, page 16)  
around the search area.  
Look through the eyepiece  
and when the object does  
become visible, press  
MODE to stop the spiral  
search. Then use the  
Arrow keys to center the  
object.  
Note: Autostar locates alignment stars based on the date, time, and loca-  
tion entered. The alignment stars may change from night to night. All that  
is required is for the observer to center the selected star in the eyepiece  
when prompted.  
Go To Saturn (Autostar Models Only)  
After performing the Train the Drive and the Easy Alignment procedures, the motor  
drive begins operating and the telescope is aligned for a night of viewing. Objects in  
the eyepiece should maintain (i.e., track) their position even though the Earth is rotat-  
ing beneath the stars.  
Important Note: Once aligned, only use the Autostar menus or Arrow  
keys to move the telescope. Do not loosen the telescope locks, or move  
the base manually, or alignment will be lost.  
This exercise demonstrates how to select an object for viewing from Autostar’s data-  
base, i.e., Saturn. Note that Saturn is not visible all year long and it may be necessary  
for you to choose another object from Autostar's database. However, the procedure  
will be identical to the one used for observing Saturn.  
1. After the telescope is aligned, “Select Item: Object” displays. Press ENTER. If  
“Select Item: Object” is not currently displayed, press MODE repeatedly until it  
displays, then press ENTER.  
2. “Object: Solar System” displays. Press ENTER.  
3. “Solar System: Mercury” displays. Use the Scroll Down key until “Solar System:  
Saturn” displays.  
4. Press ENTER. “Calculating” displays. Then “Saturn” and a set of coordinates dis-  
plays. Saturn’s (and other planets’) coordinates change throughout the year.  
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5. Press GO TO. “Saturn: Slewing...” displays and the telescope slews until it finds  
Saturn. You may need to use the Arrow keys to center Saturn precisely in the  
eyepiece. Autostar then automatically slews (moves) the telescope so that it  
tracks Saturn (or whatever other object you may have chosen). Saturn remains  
centered in the eyepiece.  
Using the Guided Tour (Autostar Models Only)  
This example demonstrates using “Tonight’s Best” Guided Tour.  
1. After observing Saturn, keep pressing MODE until “Select Item: Object” displays  
again.  
Fig. 17: The planet Saturn  
is over 800 million miles  
from the Earth.  
2. Press the Scroll Down key twice. “Select Item: Guided Tour” displays.  
3. Press ENTER. “Guided Tour: Tonight’s Best” displays. Press ENTER.  
Note: If you wish to try out other Guided Tours, press the Scroll Down key  
to scroll through other tour choices. When the tour you wish to select dis-  
plays, press ENTER.  
4. “Tonight’s Best: Searching...” displays. After calculating, “Tonight’s Best: Jupiter”  
displays.  
Note: Different objects may be displayed on a tour list on any given night.  
Press ENTER to display information about the object. Press GO TO to move the  
telescope to the object.  
5. Press MODE to return to the Tour list. Press the Scroll keys to scroll through the  
list. Press ENTER when you find the next object you wish to observe.  
6. Press and hold down MODE for two seconds to leave the Guided Tour menu.  
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B A S IC A U T O S T A R O P E R A T IO N  
OBJECT MENU  
SETUP MENU  
Easy alignment  
permits all telescope  
operations with only  
a quick setup.  
Select Item:  
Object  
Important Note: The  
model SN-6EC, model  
SN-8EC, and model AR-  
5EC are equipped with an  
Electronic Controller  
Want to see Mars? The Orion nebula?  
The Andromeda galaxy? Select from  
over 30,000 database objects and press  
GO TO to move the telescope  
automatically to an object.  
Select Item:  
Setup  
Select Item:  
Event  
M
E A D  
E
handbox, rather than the  
Autostar Handbox. The  
EVENT MENU  
UTILITIES MENU  
Display the time of  
past, present, and future  
astronomical events,  
such as Moon phases  
or meteor showers.  
Calculate eyepiece  
magnifications;  
set timer alerts;  
create your own  
landmark survey.  
following sections (BASIC  
AUTOSTAR OPERATION,  
AUTOSTAR MENUS, AND  
USEFUL AUTOSTAR  
The Universe of  
Autostar  
PROCEDURES), are rele-  
vant only to models  
Select Item:  
Utilities  
Select Item:  
Guided Tour  
equipped with the  
GUIDED TOUR  
Autostar escorts you  
on a tour of tonight's  
GLOSSARY  
What is an elliptical galaxy?  
How far away is the Sun?  
Expand your knowledge of  
astronomy by displaying terms  
and definitions, and other information.  
Autostar handbox and do  
not apply to the EC mod-  
els. For more information  
about the EC handbox,  
see APPENDIX D: EC  
HANDBOX, page 55.  
best celestial objects  
at your viewing location.  
Select Item:  
Glossary  
Fig. 18: The Autostar Universe.The six primary categories listed in the Select Item menu of  
Autostar.  
It is important to understand that menu selections are set in a loop (Fig. 19). This means  
that pressing the Scroll Down key (7, Fig. 2) cycles down through all the available  
options within a given category, then returns to the first option. The Scroll Up key (7,  
Fig. 2) cycles up through the options in the opposite order. Note that this capability is a  
quick way to get to an option that is near the bottom of the list. The following example  
demonstrates this capability.  
Object  
Event  
Guided Tours  
Glossary  
Utilities  
Setup  
Example:  
To navigate to the “Select Item: Setup” menu option when the “Select Item: Object”  
menu is displayed:  
1. Press the Scroll Down key five times or the Scroll Up key once.  
Fig. 19: Menus set in a  
loop.  
The screen in Fig. 20 displays two lines of information. The top line shows the current  
menu level. The second line displays an option which may be selected within that  
menu level. Some options are choices that select the next menu level down. The  
Scroll keys move up and down within the list of available options, showing one option  
at a time.  
Setup  
Align  
Date  
Time  
Daylight Saving  
Telescope  
Targets  
etc.  
When the desired option is displayed on the second line, press the ENTER key to  
choose that option and move down one menu level.  
Press the MODE key to leave a level; e.g., the wrong menu option is chosen.  
Important Note: No matter how many levels into Autostar are traveled,  
each press of the MODE key moves up a level, until the top level, "Select  
Item," is reached. Once in the Select Item level, press MODE to return to  
the topmost level, "Select Item: Object."  
Fig. 20: Menu options dis-  
play on the second line.  
Use the Scroll keys to  
move up or down through  
the list of options. Press  
ENTER to select the  
desired option.  
Autostar Navigation Exercise  
To demonstrate how the Autostar menu structure works, the following exercise calcu-  
lates Sunset time so an evening observing session can be planned.  
Note: Before proceeding with this exercise, Autostar must be properly ini-  
tialized and aligned (see pages 19 and 21).  
To Calculate Sunset time:  
1. Press the MODE key several times, until “Select Item: Object” is displayed.  
2. Press the Scroll Down key once to display the “Event” option in the “Select Item”  
menu.  
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3. Press the ENTER key to choose the "Event" option and move down a level.  
"Event: Sunrise" is displayed.  
4. Press the Scroll Down key once to display the "Sunset" option in the Event menu.  
5. Press the ENTER key to choose the "Sunset" option and move down another  
level.  
6. Autostar calculates the Sunset time based on the current date, time, and location.  
Autostar then displays the results of the calculation.  
7. Press MODE once to start moving back up through the Autostar levels. The first  
level up is the Event menu.  
8. Press MODE again to move up another level. This is the top level, "Select Item."  
9. Press MODE again to return to the starting point of "Select Item: Object."  
Entering Data into Autostar  
I
Use the Number keys to enter digits.  
Tip:  
When multiple choices are  
available within a menu  
option, the current option is  
usually displayed first and  
highlighted by a right point-  
ing arrow (>).  
I
Use the Arrow keys to scroll through numbers 0 through 9 and the alphabet. The  
Down Arrow key begins with the letter "A;" the Up Arrow key begins with digit "9."  
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To move the cursor across the display:  
Use the Right or Left Arrow key (5, Fig. 2) to move the cursor from one number  
to the next in the display.  
Press ENTER when the desired information has been entered.  
Navigating Autostar  
Autostar's menus are organized for quick and easy navigation:  
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Press ENTER (2, Fig. 2) to go deeper into Autostar's menu levels.  
Press MODE (3, Fig. 2) to move back toward the top menu level.  
Press the Scroll keys (7, Fig. 2) to move up and down through the options or lists.  
Press the Arrow keys (5, Fig. 2) to move the cursor across the display.  
Press the Help (?) key (8, Fig. 2) to access on-line help.  
LXD55 TIPS  
Look into the Future  
The Autostar Date option in the Setup menu is much more than just an entry  
of today's date; with it you can look far into the future or learn about past  
events. Autostar can calculate the date and times of future events and, except  
for eclipses, past events as well (based on the current calendar system). E.g.,  
a Sunrise on March 6, 2043 A.D. or the Vernal Equinox in 1776 A.D. To use this  
feature, enter the desired date in the Setup: Date menu and select an option in  
the Event menu.  
Autostar can calculate dates and times for Sunrises, Sunsets, Moonrises,  
Moonsets, Moonphases, Solar and Lunar Eclipses (for the next 100 years),  
meteor showers, equinoxes and solstices, and the minimums of Algol.  
One very practical use of the Date and Time menus is to use the Sunset option  
to determine when you can begin your astronomical observing on any given  
evening.  
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Select Item:  
Object  
Select Item:  
Event  
Select Item:  
Guided Tour  
Select Item:  
Glossary  
Select Item:  
Utilities  
Select Item:  
Setup  
Sunrise  
Sunset  
Moonrise  
Moonset  
Moon Phases  
Align  
Easy  
One Star  
Two Star  
Date  
Solar System  
Mercury  
Etc.  
Tour Objects  
A...  
Timer  
Set  
Start & Stop  
Alarm  
Set  
Accretion Disk  
Etc.  
Tonight's Best  
Star Groups  
Stars of the Night  
Moon  
B...  
C...  
D...  
E...  
F...  
G...  
H...  
I...  
Asteroids  
Comets  
Constellations  
Andromeda  
Etc.  
Deep Sky  
Named Object  
Galaxies  
Nebulae  
Planetary Neb.  
Etc.  
Next Full Moon  
Time  
On & Off  
Eyepiece Calc.  
Field of View  
Magnification  
Suggest  
Display Options  
Sun Warning  
Getting Started  
Brightness Adj.  
Contrast Adj.  
Battery Alarm  
Landmark Survey  
Sleep Scope  
Park Scope  
Next New Moon  
Next 1st Qtr  
Next 3rd Qtr  
Meteor Showers  
Quadrantids  
Lyrids  
Daylight Saving  
Telescope  
Model  
Focal Length  
Az/RA Ratio  
Alt/Dec Ratio  
Az/RA Percent  
Alt/Dec Percent  
Train Drive  
Tracking Rate  
Reverse L/R  
Reverse Up/Dn  
Calibrate Motor  
High Precision  
Targets  
J...  
Eta Aquarids  
Delta Aquarids  
Perseids  
Orionids  
Taurids  
Leonids  
Geminids  
Ursids  
K...  
L...  
M...  
N...  
O...  
P...  
Q...  
R...  
S...  
T...  
U...  
V...  
W...  
X...  
Y...  
Z...  
Star  
Named  
SAO Catalog  
Double  
Variable  
Etc.  
Cord Wrap  
Solar Eclipses  
Lunar Eclipses  
Min. of Algol  
Autumn Equinox  
Vernal Equinox  
Winter Solstice  
Summer Solstice  
Astronomical  
Terrestrial  
Site  
Satellite  
Select  
Add  
Delete  
Edit  
Select  
Add  
Delete  
Edit  
User Objects  
Select  
Owner Info  
Clone  
Add  
Delete  
Download  
Statistics  
Reset  
Edit  
Landmarks  
Select  
Add  
Delete  
Identify  
Browse  
Start Search  
Edit Parameters  
Fig. 2  
1 The  
Com  
plete  
Auto  
star M  
enu S  
tructu  
re.  
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M E N U S  
Object Menu  
Almost all observing with Autostar is performed using the Object menu category.  
(Note: Exceptions include Guided Tour and Landmark Survey. See GO TO SATURN,  
)
page 21, for an example of observing using the Object menu. Also see USING THE  
GUIDED TOUR, page 22.  
Autostar contains many libraries of viewable objects, such as stars, planets, comets,  
nebulae and so forth. When one of these objects is selected from a library, Autostar  
moves your telescope (if properly aligned) and points it at the selected object.  
The Object Menu options include:  
Solar System is a library of the eight planets (Earth is not included) in order out from  
the Sun, followed by the Moon, asteroids, and comets.  
Constellation is a library of all 88 Northern and Southern Hemisphere constellations.  
When this menu option is chosen and a constellation name appears on the first line  
of the screen, press GO TO once to change the second line to the name of the bright-  
est star in the constellation. Press GO TO a second time to slew the telescope to that  
star. Use the Scroll keys to cycle through the list of stars in the constellation, from  
brightest to dimmest.  
Deep Sky is a library of objects outside our Solar System such as nebulae, star clus-  
ters, galaxies, and quasars.  
Star is a library of stars listed in different categories such as named, double, variable,  
or nearby.  
Satellite is a library of Earth-orbiting objects such as the International Space Station,  
the Hubble Space Telescope, Global Positioning System (GPS) satellites, and geo-  
synchronous orbit satellites.  
Want to learn more about  
observing satellites?  
See page 34.  
User Objects allows the user to define and store in memory deep-sky objects of spe-  
cific interest that are not currently in the Autostar libraries. See Using Autostar to  
Find Objects Not in the Libraries, page 33 for more information.  
Landmarks stores the location of terrestrial points of interest in the permanent  
Autostar database.  
Want to learn more about  
Landmarks?  
Important Note: To use the Landmark function, the telescope must be  
located and aligned exactly as when the landmark was added to the data-  
base.  
See page 34.  
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Select: To select a Landmark already in the database (see ADD below), choose  
the "Select" option and scroll through the list. Press ENTER to select a  
Landmark, then press GO TO and the telescope slews to the object.  
Add: To add a Landmark, choose the "Add" option. Enter a name for the  
Landmark. Locate and center the Landmark in the eyepiece, then press ENTER.  
Identify is an exciting feature for an observer who wants to scan the night sky and  
start exploring. After the telescope has been properly aligned, use the Autostar Arrow  
keys to move about in the sky. Then follow this procedure:  
Important Note: Only use the Arrow keys to move the telescope during  
the Identify procedure. Do not loosen the telescope locks or move the  
base or alignment is lost.  
1. When a desired object is visible in the eyepiece, keep pressing MODE until the  
Select Item: Objectmenu is displayed. Press ENTER to select this menu.  
2. Scroll through the Object menu options until the Object: Identifyscreen  
appears.  
3. Press ENTER. Autostar searches the libraries for the identity of the object being  
observed.  
4. If the telescope is not directly on an Autostar library object, the nearest library  
object is located and displayed on the screen. Press GO TO and the telescope  
slews to that object.  
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Browse allows you to search the library for objects with certain parameters, much like  
a search engine. "Edit Parameters" lets you set various parameters for the search,  
such as: Object Type, Minimum Elevation, Largest, etc. Once you have set the param-  
eters of the search, select "Start Search" and press ENTER. Autostar will display the  
results of the search.  
Event Menu  
The Event menu provides access to dates and times of astronomical events. The  
Event database includes:  
Sunrise and Sunset calculates the time that the Sun rises or sets on the current date.  
Find rise and set times for other dates by entering a new date into the Setup: Date”  
menu.  
Want to learn more about  
using the Date menu?  
See the LXD55 TIPS box,  
page 24.  
Moonrise and Moonset calculates the time that the Moon rises or sets on the current  
date. Find rise and set times for other dates by entering a new date into the Setup:  
Datemenu.  
Moon Phases displays the date and time of the next Full, New, 1st Quarter, and 3rd  
Quarter Moon.  
Meteor Showers provides information on upcoming meteor showers, such as the  
Perseids, the Leonids, etc. Also lists the dates of the showers and when they reach  
maximum.  
Note: Meteors are fast moving objects that cover large areas of the sky and  
are usually best observed with the naked eye.  
WARNING!  
Never use  
a Meade  
Solar Eclipse lists upcoming Solar Eclipses, including the date and type (total, annu-  
lar, or partial) of eclipse, and the location and time of the first and last contacts of the  
Moon's shadow. Use the Scroll Up and Down keys to display the available data.  
Remember, never use a telescope to look at the Sun! See WARNING! to the left.  
®
LXD55-Series  
Telescope to look at  
the Sun! Looking at  
or near the Sun will  
cause instant and  
irreversible damage  
to your eye. Eye  
Lunar Eclipse lists upcoming Lunar Eclipses, including the date and type (total, par-  
tial, penumbral) of eclipse. Use the Scroll Up and Down keys to display the available  
data.  
Min. (Minimum) of Algol is the minimum brightness of the dramatic eclipsing binary  
star system, Algol. It is relatively close at a distance of 100 light years. Every 2.8 days  
during a 10-hour period, Algol undergoes a major change in apparent magnitude as  
one of the two stars passes behind the other. The combined magnitude of the two  
stars thus dips from +2.1 to a minimum of +3.4 halfway through the eclipse as the sec-  
ond star is hidden. Autostar calculates minimum magnitude time at mid-eclipse.  
damage is often  
painless, so there is  
no warning to the  
observer that dam-  
age has occurred  
until it is too late. Do  
not point the tele-  
scope or its viewfind-  
er at or near the Sun.  
Do not look through  
the telescope or its  
viewfinder as it is  
moving. Children  
should always have  
adult supervision  
while observing.  
Autumn and Vernal Equinox calculates the time and date of the fall or spring equi-  
nox of the current year.  
Winter and Summer Solstice calculates the time and date of the winter or summer  
solstice of the current year.  
Glossary Menu  
The Glossary menu provides an alphabetical listing of definitions and descriptions for  
common astronomical terms and Autostar functions. Access directly through the  
Glossary menu or through hypertext words embedded in Autostar. A hypertext word  
is any word in [brackets], usually found when using the Autostar Help function or  
when reading a scrolling message such as a description of a planet or star. Press  
ENTER whenever a hypertext word is on screen and Autostar goes to the glossary  
entry for that word.  
To access directly from the Glossary menu, use the Scroll keys to scroll through the  
alphabet. Press ENTER on the desired letter. Scroll to the desired entry and then  
press ENTER to read the description.  
Utilities Menu  
The Utilities menu provides access to several extra features within Autostar, including  
a countdown timer and an alarm. The Utilities functions include:  
Timer selects a countdown timer. This feature is useful for functions such as  
astrophotography and tracking satellites. To use the Timer, press ENTER, then  
choose Setor Start/Stop."  
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Set: Enter the time to be counted down, in hours, minutes, and seconds, then press  
ENTER.  
Start/Stop: Activates the timer set previously. Use the Scroll keys to toggle  
between ON and OFF. When ON is displayed, press ENTER to activate the timer.  
When the timer runs out, four beeps sound and the timer is deactivated.  
Alarm selects a time for an alarm signal as a reminder. To use the Alarm, press  
ENTER, then choose "Set" or "Start/Stop."  
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Set: Enter the time of day for the alarm to sound, in hours, minutes, and seconds,  
then press ENTER.  
Start/Stop: Activates the alarm set previously. Use the Scroll keys to toggle  
between on and off. When ON is displayed, press ENTER to activate the alarm.  
When the alarm time arrives, Autostar beeps. Press ENTER to deactivate the  
alarm.  
Eyepiece Calc calculates information about an eyepiece for the specific telescope to  
which Autostar is connected.  
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Field of View: Scroll through a list of available eyepieces. When an eyepiece is  
selected, the field of view is calculated.  
Magnification: Scroll through a list of available eyepieces. When an eyepiece is  
selected, the magnification is calculated.  
Suggest: Autostar calculates and suggests the best eyepiece for viewing, based  
on the telescope and the object being viewed.  
Display Options enables or disables Autostars two initial displays. If both displays  
are disabled, Autostar begins with the Date display.  
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Sun Warning: Turns the Sun Warningmessage on or off.  
Getting Started: Turns the Getting Startedmessage on or off.  
Tip:  
Brightness Adj: Adjusts the brightness of the display using the Scroll keys. When com-  
plete, press ENTER.  
If you notice that the text is  
"smearing" on the Autostar  
display, use the contrast  
adjustment menu.  
Contrast Adj: Adjusts the contrast of the display using the Scroll keys. When complete, press  
ENTER. The Contrast Adjustment feature is usually only required in very cold weather.  
Landmark Survey automatically slews the telescope to all user-defined landmarks  
with a short pause at each location. Press ENTER to start the survey. While a slew is  
in progress, press any key to skip that object and go to the next landmark on the list.  
To observe a landmark for a longer period, press MODE when paused on the object  
to stop the survey. Press ENTER to restart the survey at the first object on the list.  
Want to learn more about  
Landmarks?  
See page 34.  
Sleep Scope is a power saving option that shuts down Autostar and the telescope  
without forgetting its alignment. With "Sleep Scope" selected, press ENTER to acti-  
vate the Sleep function. Autostar goes dark, but the internal clock keeps running.  
Press any key, except ENTER, to re-activate Autostar and the telescope.  
Park Scope is designed for a telescope that is not moved between observing ses-  
sions. Align the telescope one time, then use this function to park the telescope. Next  
time it is powered up, enter the correct date and time no alignment is required.  
Pressing ENTER causes the telescope to move to its pre-determined Park position.  
Once parked, the screen prompts to turn off power.  
Important Note: When the "Park Scope" option is chosen and the display  
prompts you to turn off the telescope's power, Autostar is unable to be  
returned to operation without turning the power off and then back on.  
Cord Wrap moves the telescope in such a way as to prevent the cords and cables  
attached to your telescope assembly from getting wound around the assembly and tan-  
gled as the telescope slews to objects. This menu is set to "On" and cannot be  
changed by the user.  
Setup Menu  
Want to learn more about  
using the Date menu?  
See the LXD55 TIPS box,  
page 24.  
The Setup menus primary functions are for setting up telescope alignment. However,  
there are numerous other features available within the Setup menu, including:  
Date changes the date used by Autostar. This function is useful to check events in the  
past or future. For example, set the Date menu for a day three months in the future.  
Then check the "Select Item: Event" menu for the Sunset time on that date. See  
EVENT MENU, page 27.  
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Time changes the time entered into Autostar. Setting the correct time is critical for  
Autostar to properly calculate locations and events. Time may be set to 24-hour mode  
(military time) by selecting the "blank" option (i.e., no option is displayed) which fol-  
lows the "AM" and "PM" options.  
Daylight Saving is used to enable or disable Daylight Savings time.  
Note: Daylight Savings Time may be referred to by different names in vari-  
ous areas of the world. Check local time to verify.  
Telescope accesses several options, including:  
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Model: Allows you to select the telescope model connected to Autostar.  
Focal Length: Displays the focal length of the selected telescope.  
Az/R.A. Ratio and Alt/Dec. Ratio: The Az (Azimuth) or the R.A. (Right  
Ascension) ratio and Alt (Altitude) or Dec. (Declination) ratio refers to the gears of  
the telescope's motors. Do not alter these numbers.  
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Az/R.A. Percent: This option allows you to change the AZ (azimuth) or R.A. (right  
ascension) backlash, i.e., the way the Arrow keys move the telescope along the  
azimuth or R.A. axes. If you enter a value near 100, the telescope tube responds  
more quickly (it responds immediately at 100%) as you hold down an Arrow key  
and also slews (moves) the tube more quickly. If you enter a value near 0, it takes  
longer for the tube to respond as you hold down an Arrow key and also slews the  
tube more slowly. Experiment with this option. Try changing the percent value  
until you get a "feel" for the Arrow keys that is comfortable for you.  
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Alt/Dec. Percent: The option operates identical to the Az/R.A. Percent option  
(see above), but allows you to change the altitude or declination backlash, i.e.,  
the way the telescope responds to the Arrow keys when moving along the altitude  
or declination axes.  
Train Drive: Trains the Altitude/Declination and Azimuth/R.A. motors to locate  
objects with more precision.  
If you are experiencing any problems with pointing accuracy, follow the procedure  
described in TRAININGTHE DRIVE, page 20, to insure accurate pointing and track-  
ing.  
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Tracking Rate: Changes the speed at which the telescope tracks targets in the  
sky.  
a. Sidereal: The default tracking setting for Autostar; sidereal rate is the stan-  
dard rate at which stars move from East to West across the sky due to the  
rotation of the Earth.  
LXD55 TIPS  
O b s e r v in g C o n s id e r a t io n s  
Try to pick an observing site away from street and house lights and car head-  
lights. While this is not always possible, the darker the site, the better.  
Give your eyes about ten minutes to adjust to the darkness before observing.  
Give your eyes a rest from observing every ten or fifteen minutes to relieve  
eyestrain.  
Try not to use a standard flashlight. Experienced observers use red LED flash-  
lights, the red utility light on the Autostar handbox, or tape red cellophane over  
their flashlights to use for setup and map reading so they dont have to con-  
tinually readjust their eyes to the darkness. Be careful not to shine bright lights  
if there are other observers in the area. Do not shine a flashlight into the tele-  
scope while someone is observing!  
Dress warmly. It gets chilly when youre sitting for prolonged periods.  
Practice setting up your equipment during the day or in a lighted area to  
become familiar with it before going to a dark site.  
Use your 26mm eyepiece to view terrestrial objects and wider areas of space,  
such as open star clusters. Use an optional 9mm eyepiece when you wish to  
view something up close, such as craters on the Moon or the rings of Saturn.  
Know your observing site. If youre going to try out an unfamiliar site, check it  
out in the daylight for possible obstructions and pitfalls.  
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b. Lunar: Choose this option to properly track the Moon over long observing  
sessions.  
c. Custom: Allows entry of user-defined tracking rates.  
Tip:  
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Reverse L/R: Reverses the functions of the Left and Right Arrow keys (i.e., the  
Right key moves the telescope to the left).  
The Reverse L/R and U/D  
functions are useful if you  
are observing in the  
Southern hemisphere.  
Reverse U/D: Reverses the functions of the Up and Down Arrow keys (i.e., the  
Up key moves the telescope down).  
Calibrate Motor: If the telescope motors appear to have a problem, use this  
option to retest the motors before performing a Reset. This option is also used if  
an Autostar unit is moved between telescopes, to match Autostar to the new tel-  
escope. To calibrate the motors, select this option and press ENTER.  
Tip:  
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High Precision: If High Precision is turned on, when looking for a faint celestial  
object (i.e., a nebula or galaxy), Autostar first slews to a nearby bright star and  
displays "ENTER to Sync." Center the star in the eyepiece, then press ENTER.  
At that point the telescope has a high precision alignment to that part of the sky  
and it then slews to the object that was originally requested.  
If the "ENTER to Sync"  
feature is accessed by  
mistake (holding the  
ENTER key for more than  
2 seconds), press MODE  
to return to the previous  
screen.  
Targets switches between Astronomical targets and Terrestrial targets. If  
"Astronomical" is selected, the telescope tracking motor is activated and any object  
you observe will remain centered in the eyepiece. If "Terrestrial" is selected, the track-  
ing motor is turned off. To learn how to track an object automatically, see page 18.  
Site provides access to several options including:  
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Select: Displays the currently selected observing site. Use the Scroll keys to  
cycle through all available sites (see ADD below). Press ENTER when the site  
you wish to select displays. Use this option when you move to a different geo-  
graphic location.  
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Add: Allows you to add new observing sites to the database (up to six sites may  
be stored). Scroll through the list of Countries/States. Press ENTER when the site  
you wish to add displays. Then choose the desired city in the same manner.  
Want to learn more about  
adding and editing  
sites? See page 32.  
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Delete: Deletes a stored site from the database.  
Time Zone  
Atlantic  
Eastern  
Central  
Mountain  
Pacific  
Shift  
Edit: Edits a selected site, including: the name, latitude, longitude, and time  
zone. Time Zone refers to the Greenwich Mean Time (GMT) time zone shift.  
Users West of Greenwich, England use -hours, East of Greenwich use +”  
hours. For the United States, look up the time zone shift in Table 1.  
-4 Hours  
-5 Hours  
-6 Hours  
-7 Hours  
-8 Hours  
-9 Hours  
-10 Hours  
Note: Autostar compensates for daylight savings time, if selected. See  
SETUP MENU: DAYLIGHT SAVING, page 29.  
Alaska  
Hawaii  
Owner Info accesses the owner information menu, including:  
Table 1: Time Zone Shift.  
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Name: Users may enter both their first and last names using the Up and Down  
Arrow keys to cycle through the alphabet. Use the Right and Left Arrow keys to  
move through the text. Press ENTER when the entry is complete.  
Note: The Download and  
Clone functions require  
the optional #505  
Astrofinder Software and  
Cable Connector Kit. See  
the instruction sheet  
included with the kit for  
more information on how  
to download.  
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Address: Use the Up and Down Arrow keys to enter your street address, city,  
state, and zip code. Press ENTER when the entry is complete.  
Download transfers information from a personal computer or another Autostar.  
During the operation, the warning Downloading Do Not Turn Offappears.  
Clone uploads information from one Autostar handbox to another. Three options are  
available:  
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Catalogs: Sends only user-defined object information, such as new satellite  
orbits or comet data to another Autostar handbox.  
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Software: Sends only the basic Autostar software. This is useful if one user has  
downloaded a new version of Autostar software from the Meade website  
(www.meade.com) and wants to pass this software along to friends.  
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All: Everythinguser-defined information and Autostar softwareis sent to anoth-  
er Autostar.  
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Statistics provides basic statistical data about Autostar, including:  
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Characters Free: Shows how much room is available in user-defined object  
memory.  
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Version: Shows the current version of the Autostar software.  
Reset completely resets Autostar. Most values entered into the menus revert to fac-  
tory defaults. Autostar requires initialization after a Reset before proceeding with  
observations. See INITIALIZING AUTOSTAR, page 19.  
LXD55 TIPS  
Surf the Web  
One of the most exciting resources for astronomy is the internet. The internet is full  
of websites with new images, discoveries, and the latest astronomical information.  
For example, when comet Hale-Bopp made its approach to our Sun in 1998,  
astronomers around the world posted new photos daily.  
You can find websites for almost any topic relating to astronomy on the internet. Try  
the following key word searches: NASA, Hubble, HST, astronomy, Messier, satellite,  
nebula, black hole, variable stars, etc.  
Check out Meades website for the latest product and technical information. You can  
download the latest software revisions, links to other astronomical sites, coordinates  
of celestial objects and the latest satellite tracking information for your Autostar  
handset. See page 34 for more information. Youll find our website at:  
Here are some other sites you might find interesting:  
Sky & Telescope:  
http://www.Skyand Telescope.com  
Astronomy:  
The Starfield:  
Astronomy Picture of the Day:  
Heavens Above (satellite observing information):  
Photographic Atlas of the Moon:  
Hubble Space Telescope Public Pictures  
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U S E F U L A U T O S T A R P R O C E D U R E S  
Before trying out the examples in this section, familiarize yourself with the basic oper-  
ations of Autostar described earlier in this manual. The following examples assume  
that you have a basic knowledge of Autostar and understand how to scroll to a desired  
menu or menu option, and how to enter numbers and text. It also assumes that you  
have initialized and aligned your telescope.  
Adding Observing Sites  
If you plan to observe using Autostar at different geographic locations, you can store  
up to six observation sites in Autostar's memory to help simplify your telescope setup.  
Perform these procedures using the Site options (Add, Select, Delete, Edit) of the  
Setup menu.  
To Add a Site to the user-defined site list:  
In this example, you will choose a city and add it to the database list. You will then  
select the site to enable it.  
1. Navigate to the "Setup: Site" menu. Press ENTER,  
2. Scroll through the options until "Site: Add" displays. Press ENTER.  
3. Scroll through the list of countries/states. Press ENTER when the country/state  
you wish to add displays.  
4. Scroll through the list of cities. Press ENTER when the city you wish to add dis-  
plays. The Site is now added to the database. You may add 5 sites using this  
method (the sixth site is the site you added during the manual initialization  
process).  
5. To choose a site, navigate to "Setup: Select." Press ENTER. Scroll through the  
list of sites. When the desired site displays, press ENTER.  
To Edit a Site  
In this procedure, you will enter a location that is not available in the Autostar data-  
base by editing data of a nearby site. You will edit the location's name, latitude. lon-  
gitude and the time zone shift. You will then select the site to enable it.  
You will need to know the latitude and longitude of your location to perform this pro-  
cedure.  
1. Using the Add option, choose a site on the list that is closest to your observing  
site and press ENTER so that the site is added to your observing sites list.  
Choosing a site already on the list (as opposed to using the "Custom" feature)  
makes it easier to edit, as the "Time Zone" value may not need to be changed.  
2. Scroll to "Site: Edit" and press ENTER. "Edit: Name" displays. Press ENTER.  
3. The name of the site you have just entered to your list displays; if it does not,  
scroll to the site.  
4. Using the Arrow keys, change the name of the site so that it now reads the name  
of your observing location. Press ENTER. "Edit: Name" displays again.  
5. Press the Scroll Down key and "Edit: Latitude" displays. Press ENTER.  
6. Using the Number Keys, enter the latitude of your observing site and then press  
ENTER. "Edit: Latitude" displays again.  
7. Press the Scroll Down key and "Edit: Longitude" displays. Press ENTER.  
8. Using the Number Keys, enter the longitude of your observing site and then press  
ENTER. "Edit: Longitude" displays again.  
Time Zone  
Atlantic  
Eastern  
Central  
Mountain  
Pacific  
Shift  
-4 Hours  
-5 Hours  
-6 Hours  
-7 Hours  
-8 Hours  
-9 Hours  
-10 Hours  
9. Press the Scroll Down key and "Edit: Time Zone" displays. Press ENTER. (If the  
site you chose from the list in step 1 has the same Time Zone as the site you are  
editing, just press ENTER again to go on to the next step.) "Time Zone" refers to  
the Greenwich Time Zone shift. Users West of Greenwich, use "-" hours (one  
hour per time zone) and users East of Greenwich use "+" hours. For the United  
States, look up the shift in TABLE 1, at the left.  
Alaska  
Hawaii  
Table 1: Time Zone Shift.  
10. After entering the shift, press ENTER. "Edit Time Zone" displays.  
32  
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11. Press MODE. "Site: Edit" displays.  
12. Using the Arrow keys, scroll to "Site: Select." The site you have just edited dis-  
plays. Press ENTER to select the site or press MODE to exit.  
Using Autostar to Find Objects Not in the Libraries  
In this procedure, you will enter coordinates of celestial objects that do not appear in  
any of the Autostar libraries. You will enter the object's name and R.A. and Dec. coor-  
dinates (required information). You may also enter the object's magnitude and size  
(optional information).  
Although Autostar contains an extensive database of celestial objects (stars, nebulae,  
planets, etc.) that you can observe, you may eventually want to view objects that are  
not part of a library. Autostar provides a feature that allows you to enter an object's  
R.A and Dec. coordinates in the "User: Objects" option of the Object menu and allows  
automatic slewing of the telescope to the user-entered coordinates.  
In order to use this menu option, you first need to look up the R.A. and Dec. coordi-  
nates of the object or objects you wish to observe. Check out your local library, com-  
puter store, or bookstore for astronomy books, CD Roms, or magazines (such as Sky  
& Telescope or Astronomy), to find coordinates of celestial objects. The objects/coor-  
dinates you enter become part of your own permanent database, called "User  
Objects."  
To enter coordinates of an object into the "User: Objects" option of the Object  
menu:  
1. Make sure Autostar has been initialized and the telescope has been aligned.  
Tip:  
2. After the telescope is aligned, "Select Item: Object" displays. (If necessary, use  
the Scroll keys to scroll through the menus, as previously described, to find this  
option.) Press ENTER.  
Entering R.A. and Dec.  
Coordinates of an object  
without using the menus:  
If you do not wish to navigate  
through the menus, a more  
direct way to enter coordi-  
nates is to press and hold  
MODE for two seconds or  
more. R.A. and Dec. coordi-  
nates display. Press GO TO.  
"Object Position" and a set of  
coordinates displays. Enter  
the R.A. and Dec. coordinates  
of any celestial object using  
Number keys, overwriting the  
coordinates currently dis-  
played. As soon as the coor-  
dinates are entered, Autostar  
slews the telescope to the  
coordinates. Note that the tel-  
escope must be initialized  
(see page 19), placed in the  
Home position (see page 17),  
and aligned (see page 21) for  
this procedure to operate  
properly.  
3. "Object: Solar System" displays. Keep pressing the Scroll Up key until "Object:  
User Object" displays and press ENTER.  
4. "User Object: Select" displays. Press the Scroll Down key once. "User Object:  
Add" displays. Press ENTER.  
5. "Name" displays on the top line and a blinking cursor on the second line. Use the  
Arrow keys, as previously described, to enter the name of the object you wish to  
add to the database. When you are finished, press ENTER.  
6. "Right Asc.: 00.00.0" displays. Use the Number keys to enter the digits for the  
Right Ascension coordinate of your object. When you are finished, press ENTER.  
7. "Declination: +00°.00' " displays. Use the Number keys to enter the digits for the  
Declination coordinate of your object. If necessary, use the Scroll Keys to change  
"+" to "-." When you are finished, press ENTER.  
8. Autostar then prompts you to enter the size of the object. This step is optional.  
Use the Number keys to enter the size (in arc-minutes), if so desired, and press  
ENTER to go to the next display. If you do not wish to enter this information, sim-  
ply press ENTER.  
9. Autostar then prompts you to enter the magnitude of the object. This step is also  
optional. Use the Number keys to enter this information, if so desired, and press  
ENTER to go to the next display. "User Object: Add" displays again.  
However, if you wish to store  
the coordinates of an object  
in memory, use the method  
described at the right.  
To GO TO a user-entered object  
In this procedure, you will choose an object from the User Object list and GO TO the  
object.  
1. With "User Object: Add" displayed, press the Scroll Up key once. "User Object:  
Select" displays. Press ENTER.  
2. Use the Scroll keys (if necessary) to scroll to the desired object. Press ENTER.  
3. The name of the object and the Right Ascension and Declination coordinates dis-  
play.  
4. Press GO TO and the telescope slews to the object.  
33  
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Observing Satellites  
In this procedure, you will prepare your telescope to observe a satellite pass.  
1. Navigate to the "Object: Satellite" menu option and press ENTER.  
2. Use the Scroll keys to scroll through the list of satellites.  
3. Select a satellite from the list and press ENTER.  
4. "Calculating...." and then "Tracking..." displays. If the satellite is going to make a  
pass, "Located" displays.  
5. Use the Scroll keys to display data about the pass: aos acquisition of signal and  
los loss of signal. If you subtract the aos from the los, you can calculate how  
long the satellite will be visible. Location information also displays.  
6. "Alarm" displays after the location information. Press ENTER and Autostar auto-  
matically sets the alarm to sound a minute before the satellite's scheduled  
appearance. You may return to regular observations until the alarm goes off.  
7. When the alarm goes off, return to the Satellite menu and press a Scroll key until  
the desired satellite is on the top line of the display.  
8. Press GO TO. Autostar slews the telescope to where the satellite should appear.  
The motor drive stops and a countdown is displayed.  
Note: If the scheduled appearance position of the satellite is obstructed  
(i.e., by a building, tree, or hill), press ENTER and Autostar starts to move  
the telescope along the expected satellite track. When the track clears the  
obstruction, press ENTER again to pause the telescope, then continue  
with this procedure.  
9. With about 20 seconds left on the countdown timer, start watching through the tel-  
escope viewfinder for the satellite to enter the field of view.  
10. When the satellite enters the viewfinder field of view, press ENTER. The tele-  
scope starts to track with the satellite.  
11. Use the Autostar Arrow keys to center the object in the viewfinder, then look  
through the eyepiece to view the object.  
Satellite orbits change and new satellites (including the Space Shuttle) are launched.  
Visit the Meade website (www.meade.com) approximately once a month to get  
updated information and instructions on how to download this data to Autostar. If  
orbital parameters are more than one month old, the satellite pass may not happen at  
the time predicted by Autostar. Downloading requires the optional #505 AstroFinder™  
Software and Cable Connector Kit. See OPTIONAL ACCESSORIES, page 38.  
Note: Satellite observing is an exciting challenge. Most satellites are in  
low orbit, travelling at approximately 17,500 mph. When visible, they move  
quickly across the sky and are only in the field of view for a few minutes,  
requiring Autostar to slew the telescope rapidly. Best viewing is near  
Sunrise or Sunset when the sky is still dark. Viewing in the middle of the  
night can be problematic because the satellite may pass overhead, but not  
be visible as it is in the Earth's shadow.  
Landmarks  
Tip:  
To use the Landmark func-  
tion, the telescope must be  
located and aligned exactly  
as when the landmark(s)  
was added to the database.  
This menu option allows you to define and store terrestrial objects in the Landmark  
database. First, a landmark needs to be stored in memory using the "Landmark: Add"  
option. To view a landmark, use the "Landmark: Select" option. Landmarks may also  
be viewed using the "Landmark Survey" option in the Utilities menu.  
To Add a landmark to the database:  
In this procedure, you will store the location of terrestrial landmarks in Autostar's  
memory.  
1. Note for future reference where the telescope is located. Select an easily recog-  
nizable reference object and center the object in the telescope eyepiece. Each time  
you wish to view landmarks you have added to the database, setup the telescope  
in this location and center the reference object in the eyepiece. If you do not use a  
consistent point of reference, the telescope will not be able to locate the objects you  
have added to the database.  
34  
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Another setup method is to select an object from the Landmark database. See TO  
SELECT A LANDMARK FROMTHE DATABASE below. Then manually move the tele-  
scope's optical tube and center this object in the telescope eyepiece.  
2. Display the "Setup: Targets" menu option. Choose "Terrestrial" and press  
ENTER. "Setup: Targets" displays again. Choosing this option turns off tracking  
for astronomical objects which is not useful for the viewing of terrestrial objects  
such as those in the Landmark database. Be sure to change this option back to  
"Astronomical" when you wish to view celestial objects again.  
3. Press MODE once. "Select Item: Setup" displays.  
4. Press the Scroll Down key once and "Select Item: Object" displays. Press  
ENTER. "Object: Solar System" displays.  
5. Press the Scroll Up key twice and "Object: Landmarks" displays. Press ENTER.  
"Landmark: Select" displays.  
6. Press the Scroll Down key once. "Landmark: Add" displays. Press ENTER.  
7. "Landmark Name" displays. Using Arrow keys, enter a name for the landmark  
you wish to add to the database. When finished, press ENTER.  
8. "Center Landmark. Press Enter" displays. Using only the Arrow keys (do not  
manually move the telescope), move the telescope to the desired landmark and  
center the object in the eyepiece. Press ENTER. The object is now stored in  
memory.  
9. "Landmark: Add" displays. If you wish to add more landmarks, repeat steps 5  
through 7.  
To Select a landmark from the database  
1. Make sure the telescope is located and aligned exactly as when the desired land-  
mark was entered into memory.  
2. Display the "Landmark: Select" menu option. Press ENTER.  
3. Use the Scroll keys to scroll through the list of objects you have previously  
entered. When the desired object displays, press ENTER to select the object.  
Use the Scroll keys to scroll through location information about the object, if  
desired. Press GO TO to slew the telescope to the landmark.  
4. Press MODE to exit.  
To perform a Landmark Survey  
This procedure allows you to perform a tour of the objects entered in the "Object:  
Landmark" menu optionnote that the Landmark Survey will function only if you have  
previously entered objects in the Landmark menu.  
1. Navigate to the "Utilities: Landmark Survey" menu and press ENTER.  
2. "Landmark Survey: Slewing..." displays. The telescope moves to the first object  
on the Survey list and displays the name of the object.  
3. Press MODE to pause the Survey. Press ENTER to restart the survey at the first  
object of the survey.  
To Check on the Available Memory  
Autostar has a limited amount of memory. Once you begin to store Landmarks, user  
objects and other bits of information in Autostar, you will begin to use up memory. This  
procedure allows you to check on how much memory is still available.  
1. Navigate to the "Setup: Statistics" menu option and press ENTER.  
2. "Statistics: 37.2K Char. Free" displays. This is the amount of memory that is still  
available to the user.  
35  
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P H O T O G R A P H Y  
Photography through an LXD55 Schmidt-Newtonian telescope requires an LXD55-Series T  
-
Adapter supplied) attached to the telescope (Fig. 22). Through-the-telescope photog-  
(
raphy is possible with any 35mm camera body with a removable lens. In this way, the tel-  
escope effectively becomes the lens of the camera.  
Unthread the focuser extension tube (Fig. 23) from the focuser drawtube to remove  
from the focuser assembly. The T-Adapter (2, Fig. 22) threads onto the focuser, fol-  
lowed by the camera body (1, Fig. 22).  
To orient an object in the viewfinder of the 35mm camera body, use a small jewelers  
screwdriver to slightly loosen three adjustment screws around the outer knurled ring  
of the T-Adapter. Rotate the camera body to achieve proper orientation of the object;  
then re-tighten the adjustment screws.  
d
C
B
Photography through a long lens such as the LXD55-Series requires special technique  
for good results, and the photographer should probably expect to waste a roll or two  
of film in acquiring this technique. Long-lens photography has its own rewards, how-  
ever, rewards that short-focus lenses cannot duplicate.  
Fig. 22: LXD55-Series T-Adapter  
attached to focuser assembly and  
camera.  
(1) Camera Body, (2) T-Adapter,  
(3) Focus Knob.  
A few tips on photography with the LXD55-Series telescopes:  
1. Use a cable-operated shutter release. Touching the camera body to initiate shut-  
ter operation almost certainly introduces undesirable vibrations.  
Focuser  
Extension  
Tube  
2. Focus the image with extreme care. While observing the subject through the cam-  
eras reflex viewfinder, turn the telescopes focus knob (3, Fig. 22) to achieve the  
sharpest possible focus. Note that some 35mm cameras may have an optional  
focusing screen (available from the manufacturer) for use with a long telephoto  
lens. This screen provides a brighter and clearer image to focus, and is highly rec-  
ommended.  
3. Correct shutter speeds vary widely, depending on lighting conditions and film  
used. Trial-and-error is the best way to determine proper shutter speed in any  
given application.  
Note: The camera used with your telescope may have an exposure meter  
that is still active when the standard lens is removed and the body is con-  
nected to the telescope with the T–Adapter. If used for terrestrial photog-  
raphy, the camera meter should be acceptable. If used for astrophotogra-  
phy, the meter probably will not provide good results since camera meters  
are not made to compensate for a dark sky.  
Fig. 23: Focuser Extension Drawtube  
with eyepiece holder and eyepiece  
attached.  
4. Terrestrial photography through the LXD55-Series is sensitive to heat waves rising  
from the Earths surface. Long distance photography is best accomplished in the  
early morning hours before the earth has had time to build up heat.  
5. Photography of the Moon and planets through the LXD55-Series can be especial-  
ly gratifying, but points 1 through 4 should be particularly noted in this case.  
36  
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O P T IO N A L A C C E S S O R IE S  
A wide assortment of professional Meade accessories is available for the LXD55-Series  
telescope models. The premium quality of these accessories is well-suited to the qual-  
ity of the instrument itself. Consult the Meade General Catalog for complete details  
on these and other accessories.  
6f/5  
8f/4  
10f/4  
Eyepiece/Apparent Field  
Power/Actual Field  
Power/Actual Field  
Power/Actual Field  
Super Plössl Eyepieces (4-elements; 1.25” O.D.)  
6.4mm/52°  
9.7mm/52°  
12.4mm/52°  
15mm/52°  
20mm/52°  
26mm/52°  
32mm/52°  
40mm/44°  
119/0.44°  
79/0.66°  
61/0.85°  
51/1.02°  
38/1.36°  
29/1.77°  
24/2.18°  
19/2.31°  
127/0.41°  
84/0.62°  
65/0.79°  
54/1.96°  
41/1.28°  
31/1.67°  
25/2.05°  
20/2.17°  
159/0.33°  
105/0.50°  
82/0.63°  
68/0.77°  
51/1.02°  
39/1.33°  
32/1.64°  
25/1.73°  
Super Wide Angle Eyepieces (6-elements; 1.25” O.D., except as noted)  
Fig. 24: Series 4000 Eyepieces.  
13.8mm/67°  
55/1.21°  
42/1.58°  
31/2.15°  
24/2.81°  
19/3.52°  
59/1.14°  
45/1.49°  
33/2.02°  
25/2.64°  
20/3.30°  
74/0.91°  
56/1.19°  
41/1.62°  
32/2.11°  
25/2.64°  
18mm/67°  
24.5mm/67°  
32mm/67° (2" O.D.)  
40mm/67° (2" O.D.)  
Ultra Wide Angle Eyepieces (8-elements; 1.25” O.D., except as noted)  
4.7mm/84°  
6.7mm/84°  
8.8mm/84° (1.25  
162/0.52°  
114/0.74°  
87/0.97°  
54/1.54°  
173/0.49°  
121/0.69°  
92/0.91°  
58/1.45°  
216/0.39°  
152/0.55°  
115/0.73°  
73/1.16°  
"
- 2  
"
O.D.)  
O.D.)  
14mm/84° (1.25  
"
- 2  
"
Fig. 25: #140 2x Barlow Lens.  
5f/9.3  
6f/8  
8f/10  
Eyepiece/Apparent Field  
Power/Actual Field  
Power/Actual Field  
Power/Actual Field  
Super Plössl Eyepieces (4-elements; 1.25” O.D.)  
6.4mm/52°  
9.7mm/52°  
12.4mm/52°  
15mm/52°  
20mm/52°  
26mm/52°  
32mm/52°  
40mm/44°  
184/0.28°  
122/0.43°  
95/0.55°  
79/0.66°  
59/0.88°  
45/1.15°  
37/1.41°  
30/1.49°  
188/0.28°  
124/0.42°  
97/0.54°  
80/0.65°  
60/0.87°  
46/1.13°  
38/1.39°  
30/1.47°  
313/0.17°  
206/0.25°  
161/0.32°  
133/0.39°  
100/0.52°  
77/0.68°  
63/0.83°  
50/0.88°  
Fig. 26: #905 Variable Polarizer.  
Super Wide Angle Eyepieces (6-elements; 1.25” O.D., except as noted)  
13.8mm/67°  
18mm/67°  
24.5mm/67°  
86/0.78°  
66/1.02°  
48/1.39°  
37/1.82°  
30/2.27°  
87/0.77°  
67/1.01°  
49/1.37°  
38/1.79°  
30/2.23°  
145/0.46°  
111/0.60°  
82/0.82°  
63/1.07°  
50/1.34°  
32mm/67° (2" O.D.)  
40mm/67° (2" O.D.)  
Ultra Wide Angle Eyepieces (8-elements; 1.25” O.D., except as noted)  
4.7mm/84°  
6.7mm/84°  
8.8mm/84° (1.25  
251/0.33°  
176/0.48°  
O.D.) 134/0.63°  
255/0.33°  
179/0.47°  
136/0.62°  
86/0.98°  
426/0.20°  
299/0.28°  
227/0.37°  
143/0.59°  
Fig. 27: Series 4000 8 - 24mm Zoom  
Eyepiece.  
"
- 2  
"
14mm/84° (1.25  
"
- 2  
"
O.D.)  
84/1.00°  
37  
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Series 4000 8 - 24mm Zoom Eyepiece: The internal zoom optics of this eyepiece  
move on smooth, precisely machined surfaces which maintain optical collimation at  
all zoom settings. A scale graduated in 1mm units indicates the zoom focal length in  
operation. An excellent addition to any eyepiece set.  
#140 2x Barlow Lens: A 3-element design, doubles each eyepiece power while  
maintaining uncompromised image resolution, color correction, and contrast. Insert  
the #140 into the telescopes eyepiece holder first, followed by the diagonal (as appli-  
cable) and eyepiece. The #126 2x Barlow Lens, a compact 2-element alternative to  
the #140, may also be employed with any LXD55-Series telescope.  
#905 Variable Polarizer (1.25"): The #905 system includes 2 Polarizer filters mount-  
ed in a specially-machined cell, for glare-reduction in observing the Moon. Rotate the  
thumbscrew at the side of the unit to achieve light transmission between 5% and  
25% of its original value. The #905 inserts into the diagonal of the telescope, followed  
by an eyepiece.  
Fig. 28: Series 4000 Photo-Visual  
Series 4000 Photo-Visual Color Filters: Color filters significantly enhance visual  
and photographic image contrast of the Moon and planets. Each filter threads into  
the barrel of any Meade 1.25" eyepiece, and into the barrels of virtually all other eye-  
piece brands as well. Meade filters are available in 12 colors for lunar and planetary  
applications, and in Neutral Density as a lunar glare-reduction filter.  
Series 4000 Nebular Filters: A modern boon to the city-dwelling deep-space  
observer, the interference nebular filter effectively cancels out the effects of most  
urban light pollution, while leaving the light of deep-space nebular emissions virtual-  
ly unattenuated. Meade Series 4000 Nebular Filters utilize the very latest in coating  
technology, and are available with threaded cells for eyepieces or for attachment to  
the rear cells of Meade Schmidt-Cassegrain models.  
#928 45° Erect-Image Diagonal Prism: Primarily used for terrestrial viewing, this  
prism presents a correctly-oriented image at a comfortable 45° viewing angle.  
Fig. 29: Series 4000 Nebular Filters.  
#505 AstroFinderSoftware and Cable Connector Kit: With Meade AstroFinder  
loaded into your PC, Autostar-equipped telescopes, such as the LXD55-Series, may be  
remotely controlled from the PC display. The #505 Connector Cable Set, permitting  
connection of the LXD55-Series, Autostar, and PC, is included with each AstroFinder  
package. A Cable Connector Kit is also available without the software.  
#547 Power Adapter with Cable: Includes a 25 ft. cord and permits powering from a  
standard home (115v AC) outlet. The #547F Power Adapter is available for 220v AC  
outlets.  
#607 Cigarette Lighter Adapter: Power a LXD55-Series telescope by means of an  
automobile cigarette lighter plug. The LXD55 telescope may be powered for a full  
nights observing without risk of car-battery drain.  
#62T-Adapter: The T-Adapter is the basic means of prime-focus photography through  
all Meade Schmidt-Cassegrain models. Thread the T-Adapter on to the rear cell of  
your telescope, followed by a T-Mount for your 35mm camera, and the camera body  
is rigidly coupled to the telescope.  
Fig. 30: #505 Cable Connector Kit.  
#777 Off-Axis Guider: The Off-Axis Guider provides a means during long-exposure  
astrophotography for the photographer to monitor the tracking of the telescope to  
assure that the telescope remains precisely positioned on the object being pho-  
tographed. Like the T-Adapter, the Off-Axis Guider couples the camera body to the tel-  
escope but it also causes a small amount of the guidestars incoming light to be divert-  
ed at a right angle, where the stars position can be examined for tracking errors with  
an illuminated reticle eyepiece; position corrections can then be effected using  
Autostar.  
Piggyback Brackets: Piggyback photography is one of the most popular and easiest  
ways to get started in astrophotography. Attach your 35mm camera, with its own  
35mm-to-250mm lens, atop your LX200GPS in equatorial mode, and guiding the cam-  
era through the main telescope, wide-field photos of the Milky Way of remarkable  
detail and clarity can be taken.  
38  
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Dew Shield: In moist climates, water particles suspended in the atmosphere may  
condense on the front surface of the telescope's correcting plate. This dew formation  
may be inhibited to a significant extent by the addition of a dew shield, essentially an  
extension tube attaching to the front-cell of the telescope. #608 for Meade Schmidt-  
Cassegrain SC-8 model.  
#905 Variable Polarizer (1.25"): #1A Skylight Filter: The #905 system includes 2  
Polarizer filters mounted in a specially-machined cell, for glare-reduction in observ-  
ing the Moon. Rotate the thumbscrew at the side of the unit to achieve light trans-  
mission between 5% and 25% of its original value. The #905 inserts into the diago-  
nal of the telescope, followed by an eyepiece. The #1A Skylight Filter threads onto  
the rear cell of the Meade Schmidt-Cassegrains SC-8 model and effectively seals the  
interior of the telescope from dust. All other rear cell accessories may then be thread-  
ed to the #1A filter. The filter increases visual and photographic contrast, decreases  
glare, and helps to penetrate haze.  
#1205 Electric focuser: For use with LXD55 Schmidt-Cassegrain SC-8 model.  
Meade electric focusers are uniquely designed to yield smooth, precise microfocus-  
ing of the image, without disabling the manual focus knob, which may be used for  
rapid coarse focusing. Includes push-button hand controller with self-contained (user  
provided) battery.  
#1209 Microfocuser: For use with LXD55 Schmidt-Cassegrain SC-8 model.  
Supplied with a handbox, the microfocuser threads directly to the rear cell of model  
SC-8. Permits precise focusing of the image during visual or photographic applica-  
tion, during CCD applications maintains precise image centration on even the small-  
est CCD chips. Operates at four speeds, from extremely slow to fast; accepts both  
2" and 1.25" eyepiece barrels. Requires 8 x AAA (user-supplied batteries).  
Optional #497 Autostar Computer Controller for LXD55 EC Users: One of the  
most important advances in telescope control in the past 25 years, the Meade  
Autostar Computer Controller turns your LXD55 EC model into an automatic celestial  
object locating system. Just plug Autostar into the telescopes HBX port in place of the  
standard-equipment Electronic Controller, do a quick telescope alignment, and you  
are ready to observe any object in the Autostars 30,000-object database.  
Any of Autostars database objects can be called up and entered on the hand con-  
troller display in seconds. The observer then simply presses the GO TO pushbutton  
and watches as the telescope automatically slews to the object and places it in the  
field of view. Autostar moves the telescope to automatically track (follow) the object  
across the sky. Autostar brings into easy access objects that were previously unreach-  
able for all but the most dedicated of amateur astronomers.  
To find out more about these and other accessories available for your telescope,  
check out the Meade General Catalog or contact your local Meade dealer.  
39  
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M A IN T E N A N C E  
General Maintenance  
LXD55-Series telescopes are precision optical instruments designed to yield a lifetime  
of rewarding applications. Given the care and respect due any precision instrument,  
your LXD55 will rarely, if ever, require factory servicing. Maintenance guidelines  
include:  
a. Avoid cleaning the telescopes optics: A little dust on the front surface of the tele-  
scopes correcting lens causes virtually no degradation of image quality and  
should not be considered reason to clean the lens.  
b. When absolutely necessary, dust on the front lens should be removed with gen-  
tle strokes of a camel hair brush or blown off with an ear syringe (available at any  
pharmacy). DO NOT use a commercial photographic lens cleaner.  
c. Organic materials (e.g., fingerprints) on the front lens may be removed with a  
solution of 3 parts distilled water to 1 part isopropyl alcohol. You may also add 1  
drop of biodegradable dishwashing soap per pint of solution. Use soft, white  
facial tissues and make short, gentle strokes. Change tissues often.  
Caution: Do not use scented or lotioned tissues or damage could result  
to the optics.  
d. Do not, for any reason, remove the correcting plate from its machined hous-  
ing for cleaning or other purposes. You will almost certainly not be able to  
replace the corrector in its proper rotational orientation and serious degra-  
dation of optical performance will result. Meade Instruments assumes no  
liability for damage incurred to the telescope in this way.  
e. If the LXD55 is used outdoors on a humid night, water condensation on the tele-  
scope surfaces will probably result. While such condensation does not normally  
cause any damage to the telescope, it is recommended that the entire telescope  
be wiped down with a dry cloth before the telescope is packed away. Do not,  
however, wipe any of the optical surfaces. Rather, simply allow the telescope to  
sit for some time in the warm indoor air, so that the wet optical surfaces can dry  
unattended.  
f. If your LXD55 is not to be used for an extended period, perhaps for one month or  
more, it is advisable to remove the batteries from the telescope. Batteries left in  
the telescope for prolonged periods may leak, causing damage to the telescopes  
electronic circuitry.  
g. Do not leave your LXD55 inside a sealed car on a warm summer day; excessive  
ambient temperatures can damage the telescopes internal lubrication and elec-  
tronic circuitry.  
Alignment (Collimation) of the Schmidt-Newtonian Optical  
System  
All Meade Schmidt-Newtonian telescopes are precisely collimated at the factory  
before packing and shipment, and it is probable that you will not need to make any  
optical adjustments before making observations. However, if the telescope sustained  
rough handling in shipment, you may need to re-collimate the optical system. Such  
re-collimation is not a difficult procedure in any case.  
Note: It is not necessary  
for the user to collimate the  
refractor models.  
SC-8 Schmidt-Cassegrain  
users see the following  
section, ALIGNMENT OF  
THE SCHMIDT-CASSEGRAIN  
OPTICAL SYSTEM, page 42.  
The collimation procedure for the Meade Schmidt-Newtonians is slightly different from  
that of other Newtonian reflecting telescopes, because of the "fast" f/4 to f/5 focal ratio  
of the primary mirror. In typical Newtonian reflectors with more conventional focal  
ratios (i.e. longer focal ratios), when the observer looks down the focuser tube (with-  
out an eyepiece in the focuser), the images of the diagonal mirror, primary mirror,  
focuser tube, and the observer's eye appear centered relative to each other. However,  
with the short focal ratio primary mirror of the Schmidt-Newtonian, correct collimation  
requires that the diagonal mirror be offset in 2 directions: (1) away from the focuser  
and (2) towards the primary mirror, in equal amounts. This offset is approximately 1/8"  
in each direction. Note that these offsets have been performed at the factory prior to  
40  
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b
c
d
Focuser drawtube  
Diagonal mirror  
Reflection of primary  
mirror  
Tip:  
A useful tool for making  
collimation easier is to make  
a hole in the plastic cap that  
comes with the eyepiece to  
protect it during shipping.  
Use a drill to make a 1/8"  
hole in the center of the cap  
and place it over the eye-  
piece holder for use during  
the collimation procedure.  
e
Reflection of secondary  
mirror (darkened due to  
back lighting)  
f
g
Primary mirror clips  
Reflection of observer's eye  
b c d e  
f g  
Fig. 31a: The view you will see while collimating a Schmidt-Newtonian telescope.  
shipment of your telescope. It is only necessary for you to confirm that the telescope  
has not been badly jarred out of collimation, and to perform the final fine-tuning of Step  
4, below.  
Fig. 31a shows a correctly collimated Schmidt-Newtonian telescope, as it appears  
when viewed through the focuser with the eyepiece removed.  
To check and, if necessary, set the optical collimation, follow these steps.  
1. Observe through the focuser and orient your body so that the telescope's primary  
mirror is to your right, and the correcting plate end of the telescope tube is to your left.  
The diagonal mirror will appear centered as shown (2, Fig. 31a). If the diagonal  
appears off center, then adjust the 4 collimation screws on the plastic diagonal mirror  
housing.  
Fig. 31b: The four collimation screws  
on the diagonal mirror housing.  
2. If the reflection of the primary mirror (3, Fig. 31a) is not centered on the surface of  
the diagonal mirror, adjust the 4 collimation screws on the plastic diagonal mirror  
housing to center the reflection.  
As described above, the 4 collimation screws (Fig. 31b) on the plastic diagonal mirror  
housing are used for two different adjustments during the collimation procedure.  
knurled knob  
thumb screw  
Important Note: Do not force the 4 screws past their normal travel, and  
do not rotate any screw or screws more than 2 full turns in a counter-  
clockwise direction (i.e., not more than 2 full turns in their "loosening"  
direction), or else the diagonal mirror may become loosened from its  
support. Note that the diagonal mirror collimation adjustments are very  
sensitive: generally turning a collimation screw 1/2-turn will have a dra-  
matic effect on collimation.  
3. If the reflection of the diagonal mirror is not centered within the reflection of the pri-  
mary mirror, adjust the 3 collimation screws located on the rear of the primary mirror  
cell.  
Fig. 31c: The six collimation screws  
on the rear of the primary mirror cell.  
Note: There are 6 screws (Fig. 31c) on the primary mirror cell. The 3  
knurled knobs are the collimation screws, and the 3 smaller thumb screws  
are locking screws. The locking screws must be loosened slightly in order  
to adjust the collimation screws.  
Proceed by "trial and error" until you develop a feel for which collimation screw to turn  
in order to change the image in any given way.  
41  
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b
c
Fig. 32: Correct (1) and incorrect (2) collimation as viewed during a star test.  
4. Perform an actual star test to confirm the accuracy of steps 1 through 3. Using the  
SP 26mm eyepiece, point the telescope at a moderately bright (second or third mag-  
nitude) star, and center the image in the main telescope's field of view.  
Note: A small paper ring is  
attached to the primary mir-  
ror. This ring was attached  
at the factory for purposes  
of laser collimation. The ring  
will not diminish your tele-  
scope's imaging capabilities  
and does not need to be  
removed.  
5. Bring the star's image slowly in and out of focus until you see several disks sur-  
rounding the star's center. If steps 1 through 3 were done correctly, you will see con-  
centric (centered with respect to each other) circles (1, Fig. 32).  
An improperly collimated instrument will reveal oblong or elongated circles (2, Fig.  
32). Adjust the 3 collimating screws on the primary mirror housing until the circles  
are concentric on either side of the focus.  
In summary, the 4 adjustment screws on the plastic diagonal mirror housing change  
the tilt of the secondary mirror so that it is correctly centered in the focuser draw-  
tube, and so that the primary mirror appears centered when looking into the focuser.  
The 3 collimating knobs on the primary mirror change the tilt of the primary mirror  
so that it reflects the light directly up the center of the drawtube.  
Alignment (Collimation) of the Schmidt-Cassegrain Optical  
System  
The optical collimation (alignment) of any astronomical telescope used for serious  
purposes is important, but in the case of the Schmidt-Cassegrain design of the model  
SC-8, such collimation is absolutely essential for good performance. Take special care  
to read and understand this section well so that your model SC-8 will give you the best  
optical performance.  
As part of final optical testing, every Meade Schmidt-Cassegrain is precisely colli-  
mated at the Meade factory before shipment. However, vibrations in shipping can  
cause the optical system to become misaligned. Re-aligning the optics is, however, a  
straightforward process.  
To check the collimation of your SC-8, center a bright star that is overhead, or use a  
hot spotof reflected Sunlight from a chrome car bumper, with the supplied 26mm  
eyepiece. Allow the telescope to adjust to the temperature of your observation site  
before proceeding; temperature differences between the optics and the outside air  
can cause distortion in the images.  
With the star or hot spot centered, de-focus the image. You will notice that the out of  
focus star image looks like a ring of light surrounding a dark central spot; the dark cen-  
tral spot is in fact the shadow of the secondary mirror. Turn the focus knob until the  
ring of light fills about 10% of the eyepiece field-diameter. If the dark central spot is  
offset in (i.e., not concentric with) the ring of light, your telescopes optical system is  
misaligned and requires collimation.  
Follow these steps for collimation of the optical system:  
a. The only adjustments possible, or necessary, on the SC-8 models are from the  
three screws (Fig. 33b) located at the edge of the outer surface of the secondary  
mirror housing.  
42  
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1
2
3
Fig. 33a: Defocused star images. Misaligned (1, 2), Aligned  
Fig. 33b: Collimation screws.  
Caution: Do not force the three collimation  
screws past their normal travel and do not loosen them more than two full  
turns in a counterclockwise direction or the secondary mirror may come  
loose from its support.You will find that the adjustments are very sensitive,  
usually requiring only one-half turn or less to produce the desired result.  
b. While looking at the defocused star image, notice which direction the darker shad-  
ow is offset in the ring of light or notice which part of the ring is the thinnest (1,  
Fig. 33a). Place your index finger in front of the telescope so that it touches one  
of the collimation set screws. You will see the shadow of your finger in the ring of  
light. Move your finger around the edge of the black plastic secondary mirror sup-  
port until you see the shadow of the finger crossing the thinnest part of the ring of  
light. At this point, look at the front of the telescope where your finger is aiming. It  
will either be pointing directly at a set screw, or it will be between two set screws  
aiming at the set screw on the far side of the black plastic secondary mirror sup-  
port. This is the set screw that you will adjust.  
c. Using the Autostar's Arrow keys at the slowest slew speed, move the defocused  
image to the edge of the eyepiece field of view (2, Fig. 33a), in the same direc-  
tion as the darker shadow is offset in the ring of light.  
d. Turn the set screw that you found with the pointing exercise while looking in the  
eyepiece. You will notice that the star image will move across the field. If while  
turning the defocused star image flies out of the eyepiece field, then you are turn-  
ing the screw the wrong way. Turn the opposite direction and bring the image  
back to the center of the field.  
e. If the screw you are turning becomes very loose, tighten the other two screws by  
even amounts. If the screw you are turning gets too tight, unthread the other two  
by even amounts.  
f. When you bring the image to center (3, Fig. 33a), carefully examine the evenness  
of the ring of light (concentricity). If you find that the dark center is still off in the  
same direction, continue to make the adjustment in the original turning direction.  
If it is now off in the opposite direction, you have turned too far and you need to  
turn in the opposite direction. Always double check the image in the center of the  
field of the eyepiece.  
g. You may find after your initial adjustment that the dark center is off in a new direc-  
tion (e.g., instead of being off side-to-side it is now off in an up-and-down direc-  
tion). In this case repeat steps b through f to find the new adjustment screw.  
h. Now try a higher power eyepiece (e.g., 9mm or less) and repeat the above tests.  
Any lack of collimation at this point will require only very slight adjustments of the  
three set screws. You now have good collimation of the optics.  
i.  
As a final check of alignment, examine the star image in focus with the higher  
power eyepiece as suggested (j), under good viewing conditions. The star point  
should appear as a small central dot (commonly referred to as an Airy disc) with  
a diffraction ring surrounding it. To give a final precision collimation, make  
extremely slight adjustments of the three set screws, if necessary, to center the  
Airy disc in the diffraction ring. You now have the best alignment of the optics pos-  
sible with this telescope.  
43  
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Inspecting the Optics  
A Note About the Flashlight Test: If a flashlight or other high-intensity light source  
is pointed down the main telescope tube, the view (depending upon the observers  
line of sight and the angle of the light) may reveal what appears to be scratches, dark  
or bright spots, or just generally uneven coatings, giving the appearance of poor qual-  
ity optics. These items are only seen when a high intensity light is transmitted through  
lenses or reflected off the mirrors, and can be seen on any high quality optical sys-  
tem, including giant research telescopes.  
The optical quality of a telescope cannot be judged by the flashlight test;" the true  
test of optical quality can only be conducted through careful star testing.  
Meade Customer Service  
If you have a question concerning your LXD55-Series telescope, contact the Meade  
Instruments Customer Service Department at:  
Telephone: (949) 451-1450  
Fax: (949) 451-1460  
Customer Service hours are 8:30 AM to 4:30 PM, Pacific Time, Monday through  
Friday. In the unlikely event that your LXD55-Series telescope requires factory servic-  
ing or repairs, write or call the Meade Customer Service Department first, before  
returning the telescope to the factory, giving full particulars as to the nature of the  
problem, as well as your name, address, and daytime telephone number. The great  
majority of servicing issues can be resolved by telephone, avoiding return of the tele-  
scope to the factory. If factory service is required, you will be assigned a Return  
Goods Authorization (RGA) number prior to return.  
44  
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S P E C IF IC A T IO N S  
6" f/5 Model SN-6, SN-6EC Specifications  
Optical design..............................................Schmidt-Newtonian  
Clear aperture..............................................6" (152mm)  
Focal length ................................................762mm  
Focal ratio (photographic speed) ................f/5  
Resolving power ..........................................0.74 arc secs  
Coatings ......................................................Meade EMC Super Multi-Coatings  
Ultra-High Transmission Coating optional  
Mounting......................................................Die-cast aluminum  
Input Voltage ..............................................12v DC  
Alignment ....................................................German-type equatorial mount  
Slew Speeds................................................SN-8: 1x sidereal to 4.5°/sec  
in 9 increments  
SN-8EC: 2x sidereal to 4.5°/sec  
in 4 increments  
Tripod ..........................................................Variable-height field tripod  
Accessories ................................................6 x 30mm finder  
T-Adapter  
Super Plössl 26mm eyepiece  
1.25" and 2" eyepiece holders  
Battery pack for 8 D-cell batteries  
(user-supplied)  
SN-6: Autostar Controller  
SN-6EC: Electronic Controller  
Polar Finder Reticle Batteries......................Maxell LR41 or equivalent  
Net telescope weight ..................................13 lbs.  
Net tripod weight..........................................35 lbs.  
8" f/4 Model SN-8, SN-8EC Specifications  
Optical design..............................................Schmidt-Newtonian  
Clear aperture..............................................8" (203mm)  
Focal length ................................................812mm  
Focal ratio (photographic speed) ................f/4  
Resolving power ..........................................0.56 arc secs  
Coatings ......................................................Meade EMC Super Multi-Coatings  
Ultra-High Transmission Coating optional  
Mounting......................................................Die-cast aluminum  
Input Voltage ..............................................12v DC  
Alignment ....................................................German-type equatorial mount  
Slew Speeds................................................SN-8: 1x sidereal to 4.5°/sec  
in 9 increments  
SN-8EC: 2x sidereal to 4.5°/sec  
in 4 increments  
Tripod ..........................................................Variable-height field tripod  
Accessories ................................................6 x 30mm finder  
T-Adapter  
Super Plössl 26mm eyepiece  
1.25" and 2" eyepiece holders  
Battery pack for 8 D-cell batteries  
(user-supplied)  
SN-8: Autostar Controller  
SN-8EC: Electronic Controller  
Polar Finder Reticle Batteries......................Maxell LR41 or equivalent  
Net telescope weight ..................................24 lbs.  
Net tripod weight..........................................45 lbs.  
45  
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10" f/4 Model SN-10 Specifications  
Optical design..............................................Schmidt-Newtonian  
Clear aperture..............................................10" (254mm)  
Focal length ................................................1016mm  
Focal ratio (photographic speed) ................f/4  
Resolving power ..........................................0.45 arc secs  
Coatings ......................................................Meade EMC Super Multi-Coatings  
Ultra-High Transmission Coating optional  
Mounting......................................................Die-cast aluminum  
Input Voltage ..............................................12v DC  
Alignment ....................................................German-type equatorial mount  
Slew Speeds................................................1x sidereal to 4.5°/sec in 9 increments  
Tripod ..........................................................Variable-height field tripod  
Accessories ................................................6 x 30mm finder  
T-Adapter  
Super Plössl 26mm eyepiece  
1.25" and 2" eyepiece holders  
Battery pack for 8 D-cell batteries  
(user-supplied)  
Autostar Controller  
Polar Finder Reticle Batteries......................Maxell LR41 or equivalent  
Net telescope weight ..................................30 lbs.  
Net tripod weight..........................................55 lbs.  
5" f/9.3 Model AR-5, AR-5EC Specifications  
Optical design..............................................Achromatic Refractor  
Clear aperture..............................................5" (127mm)  
Focal length ................................................1180mm  
Focal ratio (photographic speed) ................f/9.3  
Resolving power ..........................................0.90 arc secs  
Coatings ......................................................Meade EMC Super Multi-Coatings  
Mounting......................................................Die-cast aluminum  
Input Voltage ..............................................12v DC  
Alignment ....................................................German-type equatorial mount  
Slew Speeds................................................SN-8: 1x sidereal to 4.5°/sec  
in 9 increments  
SN-8EC: 2x sidereal to 4.5°/sec  
in 4 increments  
Tripod ..........................................................Variable-height field tripod  
Accessories ................................................8 x 50mm finder  
1.25" diagonal  
Super Plössl 26mm eyepiece  
1.25" and 2" eyepiece holders  
Battery pack for 8 D-cell batteries  
(user-supplied)  
AR-5: Autostar Controller  
AR-5EC: Electronic Controller  
Polar Finder Reticle Batteries......................Maxell LR41 or equivalent  
Net telescope weight ..................................15 lbs.  
Net tripod weight..........................................35 lbs.  
6" f/8 Model AR-6 Specifications  
Optical design..............................................Achromatic Refractor  
Clear aperture..............................................6" (152mm)  
Focal length ................................................1200mm  
Focal ratio (photographic speed) ................f/8  
Resolving power ..........................................0.74 arc secs  
Coatings ......................................................Meade EMC Super Multi-Coatings  
Mounting......................................................Die-cast aluminum  
Input Voltage ..............................................12v DC  
46  
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Alignment ....................................................German-type equatorial mount  
Slew Speeds................................................1x sidereal to 4.5°/sec in 9 increments  
Tripod ..........................................................Variable-height field tripod  
Accessories ................................................8 x 50mm finder  
1.25" diagonal  
Super Plössl 26mm eyepiece  
1.25" and 2" eyepiece holders  
Battery pack for 8 D-cell batteries  
(user-supplied)  
Autostar Controller  
Polar Finder Reticle Batteries......................Maxell LR41 or equivalent  
Net telescope weight ..................................27 lbs.  
Net tripod weight..........................................45 lbs.  
8" f/10 Model SC-8 Specifications  
Optical design..............................................Achromatic Refractor  
Clear aperture..............................................8" (203mm)  
Focal length ................................................2000mm  
Focal ratio (photographic speed) ................f/10  
Resolving power ..........................................0.56 arc secs  
Coatings ......................................................Meade EMC Super Multi-Coatings  
Ultra-High Transmission Coating optional  
Mounting......................................................Die-cast aluminum  
Input Voltage ..............................................12v DC  
Alignment ....................................................German-type equatorial mount  
Slew Speeds................................................1x sidereal to 4.5°/sec in 9 increments  
Tripod ..........................................................Variable-height field tripod  
Accessories ................................................8 x 50mm finder  
1.25" diagonal  
Super Plössl 26mm eyepiece  
1.25" and 2" eyepiece holders  
Battery pack for 8 D-cell batteries  
(user-supplied)  
Autostar Controller  
Polar Finder Reticle Batteries......................Maxell LR41 or equivalent  
Net telescope weight ..................................24 lbs.  
Net tripod weight..........................................45 lbs.  
Autostar Specifications  
Processor ............................................................................68HC11, 8MHz  
Flash Memory ............................................................1.0MB, reloadable  
Keypad........................................................................20 key alphanumeric  
Display ........................................................................2 line, 16 character LCD  
Backlight......................................................................Red LED  
Utility Light ..................................................................Yes  
Coil Cord ....................................................................24"  
Database ....................................................................30,223 objects  
Autostar Dimensions  
Length ........................................................................6.56" (16.6cm)  
Width (LCD end) ........................................................3.19" (80cm)  
Width (Connector end)................................................2.25" (57cm)  
Depth ..........................................................................0.81" (21cm)  
Autostar net weight ....................................................1.12 lbs (0.51kg)  
Maxell is a trademark of Hitachi Maxell, Ltd.  
47  
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A P P E N D IX A : C E L E S T IA L  
C O O R D IN A T E S  
A celestial coordinate system was created that maps an imaginary sphere surround-  
ing the Earth upon which all stars appear to be placed. This mapping system is simi-  
lar to the system of latitude and longitude on Earth surface maps.  
In mapping the surface of the Earth, lines of longitude are drawn between the North  
and South Poles and lines of latitude are drawn in an East-West direction, parallel to  
the Earths equator. Similarly, imaginary lines have been drawn to form a latitude and  
longitude grid for the celestial sphere. These lines are known as Right Ascension  
and Declination.  
The celestial map also contains two poles and an equator just like a map of the Earth.  
The poles of this coordinate system are defined as those two points where the Earths  
north and south poles (i.e., the Earth's axis), if extended to infinity, would cross the  
celestial sphere. Thus, the North Celestial Pole (1, Fig. 34) is that point in the sky  
where an extension of the North Pole intersects the celestial sphere. The North Star,  
Polaris is located very near the North Celestial Pole. The celestial equator (2, Fig. 34)  
is a projection of the Earths equator onto the celestial sphere.  
Just as an object's position on the Earths surface can be located by its latitude and  
longitude, celestial objects may also be located using Right Ascension and  
Declination. For example, you could locate Los Angeles, California, by its latitude  
(+34°) and longitude (118°). Similarly, you could locate the Ring Nebula (M57) by its  
Right Ascension (18hr) and its Declination (+33°).  
I
Right Ascension (R.A.): This celestial version of longitude is measured in units  
of hours (hr), minutes (min), and seconds (sec) on a 24-hour "clock" (similar to  
how Earth's time zones are determined by longitude lines). The "zero" line was  
arbitrarily chosen to pass through the constellation Pegasus a sort of cosmic  
Greenwich meridian. R.A. coordinates range from 0hr 0min 0sec to 23hr 59min  
59sec. There are 24 primary lines of R.A., located at 15-degree intervals along  
the celestial equator. Objects located further and further East of the zero R.A. grid  
line (0hr 0min 0sec) carry higher R.A. coordinates.  
North  
Celestial  
Pole  
(Vicinity  
of Polaris)  
+90 Dec.  
Star  
I
Declination (Dec.): This celestial version of latitude is measured in degrees, arc-  
minutes, and arc-seconds (e.g., 15° 27' 33"). Dec. locations north of the celestial  
equator are indicated with a plus (+) sign (e.g., the Dec. of the North celestial pole  
is +90°). Dec. locations south of the celestial equator are indicated with a minus  
() sign (e.g., the Dec. of the South celestial pole is 90°). Any point on the celes-  
tial equator (such as the the constellations of Orion, Virgo, and Aquarius) is said  
to have a Declination of zero, shown as 0° 0' 0."  
1
12  
11  
1
13  
10  
2
14  
15  
9
8
16  
17  
18  
7
Earths  
Rotation  
6
5
19  
4
3
20  
Celestial  
Equator  
21  
22  
23  
0
Right Ascension  
0 Dec.  
2
South  
Celestial  
Pole  
-90 Dec.  
Setting Circles  
Setting circles included with the LXD55-Series models permit the location of faint celes-  
tial objects not easily found by direct visual observation. With the telescope pointed at  
the North Celestial Pole, the Dec. circle (19, Fig. 1d) should read 90° (understood to  
mean +90°). Each division of the Dec. circle represents a 1° increment. The R.A. cir-  
cle (31, Fig. 1d) runs from 0hr to (but not including) 24hr, and reads in increments of  
5min.  
Fig. 34: Celestial Sphere.  
Using setting circles requires a developed technique. When using the circles for the  
first time, try hopping from one bright star (the calibration star) to another bright star  
of known coordinates. Practice moving the telescope from one easy-to-find object to  
another. In this way, the precision required for accurate object location becomes evi-  
dent.  
Note You may also enter an object's R.A. and Dec. coordinates using the  
"User: Objects" option of Autostar's Object menu. Autostar then automat-  
ically slews the telescope to the entered coordinates.  
To use the setting circles to locate an object not easily found by direct visual  
observation:  
Insert a low-power eyepiece, such as a 26mm, into the focuser assembly. Pick out a  
bright star with which you are familiar (or is easily located) that is in the area of the  
sky in which your target object is located. Look up the R.A. coordinate of the bright  
48  
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star, and also of the object you wish to locate, in a star atlas. Point the object at the  
bright star. Then loosen the R.A. setting circle lock knob (32, Fig. 1d) and turn the  
R.A. setting circle to read the correct R.A. coordinate of the bright star; lock the R.A.  
setting circle lock knob onto the object. Next, loosen the R.A. lock (33, Fig. 1d) and  
turn the telescope in R.A. to read the correct R.A. coordinate of the object. Tighten the  
R.A. lock (33, Fig. 1d). If the procedure has been followed carefully, the desired object  
should now be in the telescopic field of a low-power eyepiece.  
If you do not immediately see the object you are seeking, try searching the adjacent  
sky area. Keep in mind that, with the 26mm eyepiece, the field of view of the LXD55-  
Series is about 0.5°. Because of its much wider field, the viewfinder may be of signif-  
icant assistance in locating and centering objects, after the setting circles have been  
used to locate the approximate position of the object.  
See USING AUTOSTAR TO FIND OBJECTS NOT IN THE LIBRARIES, page 33, for infor-  
mation on how to manually enter coordinates into Autostar.  
Locating the Celestial Pole  
To get basic bearings at an observing location, take note of where the Sun rises (East)  
and sets (West) each day. After the site is dark, face North by pointing your left shoul-  
der toward where the Sun set. To precisely point at the pole, find the North Star  
(Polaris) by using the Big Dipper as a guide (Fig. 35).  
Little Dipper  
Polaris  
Big Dipper  
Cassiopeia  
One- and Two-Star Polar Alignment  
Autostar provides three different methods for Polar Alignment: Easy, One-Star and  
Fig. 35: Locating Polaris.  
Two-Star. See EASY ALIGNMENT, page 21, for that procedure.  
One-Star Polar Alignment  
Polar One-Star Alignment requires some knowledge of the night sky. Autostar pro-  
vides a library of bright stars and one star from this library is chosen by the observer  
for alignment. Polaris is chosen by Autostar. The rest of the procedure is almost iden-  
tical to the EASY ALIGNMENT, page 21, except that Autostar prompts you to point the  
telescope at Polaris and center it in the telescope's eyepiece.  
Two-Star Polar Alignment  
Polar Two-Star Alignment requires some knowledge of the night sky. Autostar pro-  
vides a library of bright stars and two stars from this library are chosen by the observ-  
er for alignment. Polaris is chosen by Autostar. The rest of the procedure is almost  
identical to the EASY ALIGNMENT, page 21, except that Autostar prompts you to point  
the telescope at Polaris and center it in the telescope's eyepiece.  
49  
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A P P E N D IX B : E N H A N C IN G  
Reticle LED Knob  
P O IN T IN G P R E C IS IO N  
The Polar Alignment Viewfinder  
Eyepiece  
Typically Autostar's pointing capabilities are sufficient for most telescope observers,  
and the use of the polar alignment viewfinder is unnecessary for them. However, for  
those observers who need to meet the more demanding requirements of astropho-  
tography, the polar alignment viewfinder allows the telescope mount to be more pre-  
cisely aligned with true North. The polar alignment viewfinder contains a reticle, lit by  
an LED (Figs. 36 and 37).  
To align your telescope to North using the polar alignment viewfinder:  
Fig. 36: The polar alignment  
viewfinder.  
1. Set your telescope in the home position (see page 17). Then loosen the Dec.  
lock (17, Fig. 1d) and rotate the optical tube 90°. Re-tighten the Dec. Lock.  
2. Loosen the R.A. Lock (33, Fig. 1d).  
3. Remove the polar viewfinder cap (18, Fig. 1d).  
4. If you have not already done so, remove the plastic separating the watch batter-  
ies inside the polar alignment reticle. See step 12, page 13.  
5. Turn the polar alignment reticle LED knob to turn on the LED and look through  
the reticle.  
6. Northern Hemisphere: Move the telescope mount until Polaris is superimposed  
on the graduated area of the reticle (between 40' and 60'). The center crosshair  
denotes the North celestial pole. Southern Hemisphere: The four-sided figure in  
the reticle represents a grouping of four stars in Octantis (Sigma, Tau, Chi, and  
Upsilon) for use in the Southern Hemisphere. Move the telescope mount on its  
R.A. axis until the four stars depicted in the reticle are superimposed on the four  
star group that matches the reticle pattern.  
7. Use the latitude T-handle screws (26, Fig. 1d) and the fine azimuth control knobs  
(27, Fig. 1d) to fine tune the mount adjustment until the reticle pattern is more  
precisely superimposed over the appropriate position as described in step 6.  
Fig. 37: The view inside the polar  
alignment viewfinder reticle.  
Note: Not all pointing positions are possible with the polar alignment reticle,  
as the tripod is a limiting factor as to how far the optical tube and mount can  
be moved.  
8. Tighten the R.A. Lock (33, Fig. 1d). Return the optical tube to the home position.  
Note: Remember to turn off the polar alignment reticle LED.  
Axis Alignment Procedure  
In order for the equatorial mount to accurately point to astronomical objects using the  
GO TO feature of the Autostar handbox, the optical axis of the optical tube must be  
aligned with the R.A. axis of the mount. In most cases, the telescope will perform  
adequately without making any adjustments, but performing one of the following  
alignment methods before the initial use of the telescope, and periodically thereafter,  
will increase the mounts pointing accuracy.  
When the optical axis is perfectly aligned to the R.A. axis and the declination set to 90°,  
all objects will rotate about a point in the center of the eyepiece, as the mount is rotated  
about the R.A. axis. A misalignment in elevation results in the center of rotation shifting  
up or down. A misalignment in attitude results in the center shifting left or right.  
The telescope is moved manually in Method #1 to correct for attitude misalignment  
and then for elevation misalignment. Autostar moves the telescope in Method #2; this  
method is recommended for beginners.  
Method 1: Manual Alignment  
Procedure #1:To correct for attitude misalignment  
Important Note: Throughout the following procedures, the directional refer-  
ences up/down/left/right are used. No matter which type of telescope model  
you are using, these directions are to be interpreted relative to real-world  
targets. For example, left/right moves the image along the horizon, and  
up/down moves the image vertically.  
Fig. 38: A. Elevation Alignment;  
B. Attitude Alignment.  
Perform this procedure during the daytime. You will need to have a clear line of  
sight to a wide, distinct landmark with a clear, horizontal feature.  
1. Plug in Autostar and turn on the power as described previously in this manual.  
You will use Autostar's Arrow keys in the course of this procedure.  
50  
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2. Loosen the R.A. Lock (33, Fig. 1d) and the Dec. Lock (17, Fig. 1d). Point the tube  
so that it is above the tripod leg marked with a star. Retighten the Dec. Lock.  
Move the counterweight shaft and mount so that it is parallel to the horizon. This  
is position A. See Fig. 39. Retighten the R.A. Lock.  
3. If using a Schmidt Newtonian model, rotate the optical tube (you will need to  
loosen the cradle ring lock knobs (13, Fig. 1a) to do so) to make sure the focuser  
extends horizontally from the optical tube while in position A and do not rotate the  
tube for the remainder of the alignment procedure.  
If using a refractor model, use the diagonal assembly to rotate the eyepiece  
during testing. However, be careful that the diagonal is placed flush against the  
focuser and tightened in place using the thumbscrews. It is important that the  
diagonal does not slip during the procedure.  
4. Adjust the tripod legs, polar axis altitude and/or polar axis azimuth so that the  
wide, horizontal object you have chosen as a target is positioned across the mid-  
dle of the eyepiece.  
Procedure #1: Step 4  
Step 5  
Step 6  
Step 7  
Fig. 39: Position A.  
Important Note: The image will appear right-side-up, but reversed left-for-  
right, in the eyepiece of a refractor telescope. The image will appear  
upside-down, but correct left-for-right, in the eyepiece of a Scmidt-  
Newtonian telescope, if the eyepiece extends horizontally from the tube, as  
described in Step #3.  
5. Loosen the R.A. Lock (Tip: Make sure you do not accidentally loosen the Dec.  
Lock. If you do, restart the procedure beginning at Step #2). Rotate the telescope  
180° in the R.A. axis ONLY, until the optical tube is in position B. See Fig. 40.  
Note the position of your target in the eyepiece.  
6. Using the Autostar Up and Down Arrow keys ONLY, move the optical tube in Dec.  
axis until your target is HALFWAY back to the center of the eyepiece.  
7. Rotate the telescope 180° in the R.A. axis ONLY, to return the optical tube to posi-  
tion A. Verify that your target is in the same location in the eyepiece vertically as  
in the previous step (that is, it is not higher or lower or absent from the eyepiece).  
Ignore side-to-side misalignment (that is, if it has moved to the right or left).  
Fig. 40: Position B.  
8. Repeat steps 6 and 7, if necessary, alternating positions A and B, until the hori-  
zontal object is in the same vertical location in the eyepiece in both positions.  
9. The Dec. optical axis is now calibrated to be at 90 degrees. For Procedure #2,  
DO NOT adjust the declination of the optical tube, either manually or with the  
handbox.  
Procedure #2:To correct for elevation misalignment  
After performing the attitude correction, select an object that is at a very great distance  
(at least a mile away) to approximate infinity. Ideally, the object should be unique, with  
several identifiable objects to the left and right of it.  
Procedure #2: Step 2  
Step 4  
Step 5  
Step 6  
1. Rotate the mount about the R.A. axis only and move the optical tube to position A.  
2. WITHOUT moving the declination axis from its position determined in the previ-  
ous alignment, adjust the legs, latitude, and azimuth of the tripod to center the  
object in the eyepiece.  
3. Rotate the telescope 180° in the R.A. axis ONLY, until optical tube is in position B.  
51  
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4. Observe the position of the object in the eyepiece. Assuming that the declination  
was properly set in the previous procedure, the object should have moved only  
horizontally (that is, side-to-side) from its original position. It may be out of the  
eyepiece altogether.  
5. Using the adjustment mechanism on the bottom of the cradle (Fig. 41), move the  
reference object approximately half the distance towards the center of the eye-  
piece.  
To adjust the cradle screws, use the supplied hex key to loosen the two outside  
screws. Then adjust the position of the object by tightening or loosening the cen-  
ter screw. Perform this adjustment on both sets of screws. When finished, retight-  
en the outer screws.  
Before moving the optical tube, note the location that the telescope is centered  
on relative to the reference object. Depending on the telescope type and acces-  
sories in use, you may need to move the optical tube opposite to the direction that  
appears in the eyepiece. The best way to be sure is to move the optical tube  
(using the cradle screws) a little, and verify that the correct direction was moved  
through the eyepiece.  
Fig. 41: Cradle adjustment screws.  
6. WITHOUT moving the declination axis from its position determined in the previ-  
ous alignment, and WITHOUT adjusting the cradle position further, adjust the  
legs, latitude, and azimuth of the tripod to center the object in the eyepiece again.  
7. Rotate the telescope 180° in the R.A. axis ONLY, to return the optical tube to posi-  
tion A.  
8. Repeat steps 5 through 8, if necessary, alternating between position A and posi-  
tion B, and bringing the reference object halfway of the remaining distance to cen-  
ter. Stop the procedure once the distance between the object in position A and  
position B is less than one third the width of the eyepiece.  
9. As a final check, select another object and place it into the center of the eyepiece.  
Rotate the mount about the R.A. axis. Watch the motion of that object. It is  
acceptable if it moves slightly, but should remain in the eyepiece the entire time.  
Tips  
I
When moving to position A or B, it is usually sufficient to merely level the Dec.  
axis by eye. Whether in position A or B, the counterweight shaft should appear to  
be horizontal when looked at from several feet away.  
I
If you are finding it difficult to lower the altitude of the tripod head without the  
counterweight banging into the forward tripod leg, increase the length of the two  
rear tripod legs to introduce a tilt into the whole mount.  
I
I
Before starting the alignment procedure, it is helpful to have the tripod azimuth  
adjustment knobs even, to allow an equal range of travel in either direction.  
Make sure the focuser lock is tightened once focus is achieved. Otherwise, grav-  
ity may cause the focuser to move during rotation of the telescope and introduce  
error into the procedure.  
LXD55 TIPS  
Star Charts  
Star charts and planisphere are very useful tools and are great aids in plan-  
ning a night of celestial viewing.  
A wide variety of star charts are available in books, in magazines, on the inter-  
net and on CD Roms. Meade offers AstroFinderand other star locator soft-  
ware. Contact your Meade dealer or Meade's Customer Service department  
for more information.  
Astronomy and Sky and Telescope magazines print star charts each month  
for up-to-the-minute maps of the heavens.  
The Norton Star Atlas and Reference Handbook by A. Norton and Sky Atlas  
2000 by W. Tirion and R. Sinnot are two of the most popular star charts on the  
market.  
52  
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Method 2: Axis Alignment Using Autostar  
Perform this procedure during the daytime. You will need to have an unobstructed  
view of an easily sighted landmark, such as a light post. Use a low-power eyepiece,  
such as the supplied 26mm. This procedure assumes that you have some familiarity  
with Autostar's menu structure (you will need to locate the "Setup: Telescope"  
menu). If necessary, refer to AUTOSTAR'S MENUS, page 25.  
Note: For best result, perform this procedure after you have trained the  
drive. See page 20.  
1. Adjust the latitude T-handle screws (26, Fig. 1d) so that the latitude is set to  
45° or higher. See Step #6, page 12, for information about setting the latitude  
controls.  
Motor at  
back of  
mount  
2. Refer to Fig. 42 while performing this step. The Dec. motor (B) must be posi-  
tioned so that it is at the back of the mount. The optical tube (A) must be  
approximately horizontal (i.e., parallel with the horizon) and the counterweight  
shaft must be pointing straight down..  
If using a Schmidt-Newtonian model, loosen the cradle ring locks knobs (C)  
and move the optical tube until the eyepiece (D) points downward as shown in  
the Fig. 42. Re-tighten the cradle ring locks.  
Fig. 42: Method #2 Setup. (A) Optical  
Tube; (B) Dec. Motor; (C) Cradle  
Ring Lock Knobs; (D) Eyepiece.  
If using a refractor model, use the diagonal assembly to rotate the eyepiece  
to a convenient viewing angle during testing. However, be careful that the diag-  
onal is placed flush against the focuser and tightened in place using the thumb-  
screws. It is important that the diagonal does not slip during the procedure.  
3. Make sure that both the R.A. and Dec. locks (17 and 33, Fig. 1d) are tightened  
to a firm feel.  
4. Turn on Autostar and go to "Setup: Telescope." Press ENTER.  
5. Press one of the Scroll keys until "LXD 55 Adjust" displays and then press  
ENTER. A message displays that tells you to center a landmark. If the landmark  
is not visible in your eyepiece, lift and move the entire telescope and tripod  
assemblytry not to move the tube too far from the horizontal position (no  
more than 5° up or down), as described in Step #2. You may also use the fine  
azimuth controls (27, Fig. 1d) for side to side movement and the Autostar  
Up/Down Arrows for small adjustments to the declination axis.  
6. Caution: Before pressing ENTER, step back from the telescope assembly,  
as the telescope will begin to rotate about two axes. When the landmark is  
centered (Step #5), press ENTER.  
The telescope first moves 180° on the Dec. axis and then rotates 180° on the  
R.A. axis. Autostar displays "Slewing....".  
When the telescope has completed the 180° slew, the telescope will be under  
the mount instead of over it. The counterweight shaft is now pointed upwards  
and the cradle adjustment screws (Fig. 40) are easily accessible.  
7. Autostar again prompts you to center the landmark you have chosen in the  
eyepiece. Use the Arrow keys to center the object and then press ENTER.  
8. The telescope moves again on the R.A. axis. Use the cradle screw adjustment  
mechanism on the bottom of the cradle to center the landmark in the eyepiece.  
To adjust the cradle screws, use the supplied hex key to loosen the two outside  
screws. Then adjust the position of the landmark by tightening or loosening the  
center screw. Perform this adjustment on both sets of screws. When finished,  
retighten the outer screws. The axis is now aligned.  
Note: This procedure maximizes the pointing accuracy of the telescope provid-  
ed the telescope is always placed on the mount in the same fashion. A mark  
made on the mount under the saddle will ensure this alignment is maintained.  
53  
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A P P E N D IX C : L A T IT U D E C H A R T  
Latitude Chart for Major Cities of the World  
To aid in the polar alignment procedure (see pages 17-21), latitudes of major cities around the world are listed below. To determine the lati-  
tude of an observing site not listed on the chart, locate the city closest to your site. Then follow the procedure below:  
Northern hemisphere observers (N): If the site is over 70 miles (110 km) north of the listed city, add one degree for every 70 miles. If the  
site is over 70 miles South of the listed city, subtract one degree per 70 miles.  
Southern Hemisphere observers (S): If the site is over 70 miles (110 km) north of the listed city, subtract one degree for every 70 miles. If  
the site is over 70 miles South of the listed city, add one degree per 70 miles.  
NORTH AMERICA  
City  
Albuquerque  
Anchorage  
Atlanta  
Boston  
Calgary  
Chicago  
Cleveland  
Dallas  
Denver  
Detroit  
Honolulu  
Jackson  
Kansas City  
Kenosha  
Las Vegas  
Little Rock  
Los Angeles  
Mexico City  
Miami  
Minneapolis  
Nashville  
New Orleans  
New York  
Oklahoma City  
Ottawa  
Philadelphia  
Phoenix  
Portland  
Salt Lake City  
San Antonio  
San Diego  
San Francisco  
Seattle  
SOUTH AMERICA  
City  
Bogotá  
São Paulo  
Buenos Aires  
Montevideo  
Santiago  
State/Prov./Country Latitude  
Country  
Colombia  
Brazil  
Argentina  
Uruguay  
Chile  
Latitude  
4° N  
New Mexico  
Alaska  
Georgia  
Massachusetts  
Alberta  
Illinois  
Ohio  
Texas  
Colorado  
Michigan  
Hawaii  
Mississippi  
Missouri  
Wisconsin  
Nevada  
Arkansas  
California  
Mexico  
35° N  
61° N  
34° N  
42° N  
51° N  
42° N  
41° N  
33° N  
40° N  
42° N  
21° N  
32° N  
39° N  
45° N  
36° N  
35° N  
34° N  
19° N  
26° N  
45° N  
36° N  
30° N  
41° N  
35° N  
45° N  
40° N  
33° N  
46° N  
41° N  
29° N  
33° N  
38° N  
47° N  
39° N  
23° S  
35° S  
35° S  
34° S  
10° N  
Caracas  
Venezuela  
ASIA  
City  
Beijing  
Hong Kong  
Seoul  
Taipei  
Tokyo  
Sapporo  
Bombay  
Calcutta  
Hanoi  
Country  
China  
China  
South Korea  
Taiwan  
Japan  
Japan  
India  
India  
Vietnam  
Saudi Arabia  
Latitude  
40° N  
23° N  
37° N  
25° N  
36° N  
43° N  
19° N  
22° N  
21° N  
21° N  
Jedda  
Florida  
AFRICA  
City  
Cairo  
Cape Town  
Rabat  
Tunis  
Minnesota  
Tennessee  
Louisiana  
New York  
Oklahoma  
Ontario  
Pennsylvania  
Arizona  
Oregon  
Utah  
Texas  
California  
California  
Washington  
District of Columbia  
Country  
Egypt  
South Africa  
Morocco  
Tunisia  
Latitude  
30° N  
34° S  
34° N  
37° N  
Windhoek  
Namibia  
23° S  
AUSTRALIA AND OCEANIA  
City  
Adelaide  
Brisbane  
Canberra  
Alice Springs  
Hobart  
Perth  
Sydney  
Melbourne  
Auckland  
State/Country  
South Australia  
Queensland  
New South Wales  
Northern Territory  
Tasmania  
Western Australia  
New South Wales  
Victoria  
Latitude  
35° S  
27° S  
35° S  
24° S  
43° S  
32° S  
34° S  
38° S  
37° S  
Washington  
EUROPE  
City  
Amsterdam  
Athens  
Bern  
Copenhagen  
Dublin  
Frankfurt  
Glasgow  
Helsinki  
Lisbon  
London  
Madrid  
Oslo  
Paris  
Rome  
Country  
Netherlands  
Greece  
Switzerland  
Denmark  
Ireland  
Germany  
Scotland  
Finland  
Portugal  
England  
Spain  
Norway  
France  
Italy  
Sweden  
Austria  
Poland  
Latitude  
52° N  
38° N  
47° N  
56° N  
53° N  
50° N  
56° N  
60° N  
39° N  
51° N  
40° N  
60° N  
49° N  
42° N  
59° N  
48° N  
52° N  
New Zealand  
Stockholm  
Vienna  
Warsaw  
54  
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A P P E N D IX D : E C H A N D B O X  
Important Note:  
The Electronic  
Fast  
Controllers available for  
Meade's ETX and DS  
telescope series are not  
compatible and will not  
operate with the LXD55  
EC series models. Do  
not plug in other tele-  
scope series' EC hand-  
boxes into the LXD55  
computer control panel,  
nor plug the LXD55 EC  
series handboxes into  
any other telescope  
series computer control  
panel.  
Medium  
Moderate  
Slow  
Fig. 43: Electronic Controller. (1) Arrow Keys; (2) Indicator  
Lights; (3) SPEED Key; (4) Coil Cord; (5) MODE Key; (6) OUT  
Key; (7) IN Key.  
The model SN-6EC, model SN-8EC, and model AR-5EC come equipped with an  
Electronic Controller (EC) handbox, rather than the Autostar Handbox. The Electronic  
Controller provides you with the means to control the telescope motors from a com-  
pact handbox. The Electronic Controller (Fig. 3) has soft-touch keys designed to have  
a positive feel, even through gloves.  
The primary functions of the Electronic Controller are to move (slew) the telescope to  
an object, to set operation for the Northern or Southern Hemispheres, and to indicate  
the slew speed.  
Users of the EC models should follow the procedures described in GETTING STARTED,  
BALANCING THE TELESCOPE, ALIGNING THE VIEWFINDER, CHOOSING AN EYEPIECE,  
and OBSERVING BY MOVING THE TELESCOPE MANUALLY, pages 11 - 16. Other sec-  
tions relevant to EC users include: OBSERVE THE MOON and SETTING POLAR HOME  
POSITION, page 17, and PHOTOGRAPHY, OPTIONAL ACCESSORIES, GENERAL  
MAINTENANCE, SPECIFICATIONS, and CELESTIAL COORDINATES, pages 36 - 40 and  
44 - 49. LATITUDE CHARTS, page 54, and BASIC ASTRONOMY, pages 61 - 62, may  
also be useful. Note that SLEW SPEEDS, page 16, refers to Autostar functions only.  
Slew speed functions of the Electronic Controller are covered in this appendix.  
The following numbers refer to Fig. 43 above.  
Arrow Keys: Press one of the four Arrow keys to slew the telescope (i.e., up,  
down, left, and right) at any one of four slew speeds (see SPEED KEY below).  
Light No.  
Light Status  
Light 1  
Important Note: If you reverse directions while using the Arrow keys to  
slew to objects, there may be a slight pause as the telescope motors com-  
pensate for the reversal of the internal gears.  
On  
Light 2  
Light 3  
Light 4  
Blinking  
Off  
Indicator Lights: The four red LED (Light Emitting Diode) lights indicate the cur-  
rent slew speed of the telescope.  
Note: For purposes of this manual, the lights are identified as 1 through 4, with  
1 being the top light and 4 being the bottom light.  
Fig 44: Indicator Light Key.  
The procedures in this manu-  
al identify the status of the  
four indicator lights as depict-  
ed above: on, blinking, or off.  
SPEED Key: Press SPEED to change the speed at which the telescope slews to  
an object. Each press of the SPEED key changes the slew speed to the next  
slower setting. If the controller is already on the slowest slew speed (light 4),  
pressing SPEED cycles back to the highest speed (light 1). Slew speeds are sig-  
nified by the indicator lights (2, Fig. 43).  
Coil Cord: Plug into the HBX connector of the Computer Control Panel.  
55  
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MODE Key: Press and hold MODE to place the Electronic Controller into the  
Mode function, i.e., to select operation for the Northern or Southern Hemisphere.  
See TRACKING RATES, page 57.  
OUT Key: Use this key to decrease the tracking rate. See TRACKING RATES,  
page 57.  
IN Key: Use this key to increase the tracking rate. See TRACKING RATES, page  
57.  
Modes of Operation  
When both the A and B screws are in place, the Northern hemisphere polar mode  
is selected when power is applied (i.e., the motor drive is activated for operation in  
the Earths Northern Hemisphere). This is the factory default mode.  
Remove mode screw B (2, Fig. 44) to make the Southern Hemisphere polar mode  
the automatic default of the Electronic Controller when power is applied (i.e., the  
motor drive is activated for operation in the Earths Southern Hemisphere ).  
Remove mode screw A to disable the tracking function. Select either the Northern  
hemisphere polar mode or the Southern Hemisphere polar mode, as described  
above, to make the tracking function available. See CHANGING THE POLAR MODE,  
page 58, for more information.  
Meade Instruments Corporation  
35-4702-00  
Tested to comply  
CC  
C
FC  
with FCC Standards  
FOR HOME OR OFFICE USE  
A
B
B
C
Note: Removing either A or B screw affects only the telescope’s default  
mode; you may still make mode changes when desired using the MODE key.  
Fig. 45: Mode screws on rear of  
Electronic Controller. (1) Mode Screw  
A; (2) Mode Screw B.  
Slew Speeds  
The Electronic Controller has four slew speeds that are directly proportional to the  
sidereal rate. Press SPEED to change the slew speed (use the Arrow keys to slew  
the telescope in the desired direction). Note each slew speed corresponds to one of  
the four LED's of the Electronic Controller.  
Definition: Sidereal.  
As the Earth rotates  
beneath the night sky,  
the stars appear to move  
from East to West. The  
speed at which the stars  
move is called the side-  
real rate. You can setup  
your telescope to move  
at the sidereal rate so  
that it automatically  
Light 1 (top LED): The fastest speed. Use to move the telescope quickly from one  
point in the sky to another.  
Light 2: Best for centering an object in the viewfinder.  
Light 3: Best for centering an object in the field of a low-to-moderate power eyepiece,  
such as the standard SP 26mm.  
Light 4: The slowest speed. Use to center an object in the field of view of high-power  
eyepieces, such as the optional 6.7mm or 12.4mm.  
The four available speeds are:  
tracks the stars and  
Light 1 =1200 x sidereal (300 arc-min/sec or 5°/sec)  
Light 2 = 32 x sidereal (8 arc-min/sec)  
other objects in the night  
sky. The tracking function  
automatically keeps an  
object more or less cen-  
tered in the telescope’s  
eyepiece.  
Light 3 =  
Light 4 =  
8 x sidereal (2 arc-min/sec)  
2 x sidereal (0.5 arc-min/sec )  
The two slowest speeds (2x and 8x sidereal) can be used for manual tracking of  
astronomical objects while observing through the eyepiece.  
See pages 17 and 18 for  
more information.  
To move the telescope using the Electronic Controller:  
1. Insert a low-power eyepiece (e.g., SP 26mm) into the eyepiece holder (2, Fig. 1)  
and tighten the eyepiece thumbscrew (1, Fig. 1).  
2. Tighten the R.A. and Dec. locks (17 and 33, Fig. 1), if necessary.  
3. Verify that the On/Off switch (24D, Fig. 1) on the telescopes Computer Control  
panel is off.  
4. Plug in the Electronic Controller coil cord (4, Fig. 42) to the HBX port (24A, Fig.  
1) on the Computer Control panel.  
5. Flip the power switch to ON. The LED (24C, Fig. 1) on the Computer Control  
panel lights.. The Speed indicators lights will cycle off and on in sequence.  
6. Press any key on the Electronic Controller and the telescope slews momentarily  
in the vertical and horizontal directions to test the motors.  
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7. When the test is complete, light 1 remains on; lights 2, 3, and 4 turn off.  
8. Use the four Arrow keys (1, Fig. 42) to slew the telescope to the desired object.  
To change the slew speed, press SPEED.  
9. Fine-adjust the position of the object with the Electronic Controller Arrow keys so  
that it is centered in the viewfinder. The object is now ready to be viewed through  
the telescopes eyepiece.  
Tracking Rates  
In polar mode the Electronic Controller normally tracks objects at the sidereal rate (see  
TRACKING OBJECTS, page 17). For most observing sessions (once the telescope has  
been polar aligned and the tracking motor activated), there is little need to change this  
speed.  
For objects, like the Moon or a comet, that move at slightly different rates, the Electronic  
Controller Arrow keys (1, Fig. 42) are sufficient to move the telescope slightly as the object  
very slowly moves off-center through the eyepiece field.  
To change the tracking rate, for extended observations of an object not moving at the  
sidereal rate, follow the procedure for the appropriate hemisphere:  
Use the following procedure to change tracking rates when using the Northern  
Hemisphere polar mode. Refer to Fig. 46a.  
1. Press and hold MODE (5, Fig. 42) until the Mode function is active (i.e., lights 1  
and 2 are on steady; lights 3 and 4 signify whatever tracking mode was last cho-  
sen).  
2. Press SPEED (3, Fig. 42) until lights 1, 2, and 3 are on steady with light 4 blink-  
ing. The telescope is now in the Northern Hemisphere polar mode.  
3. Press IN (7, Fig. 42) and light 4 comes on steady. The tracking rate is now 0.5%  
faster than sidereal. If the object you're tracking is moving faster than the sidere-  
al rate, look through the eyepiece and press IN. Each time you press IN, the track-  
ing rate increases by 0.5%. Note that when the Mode function is active, the  
tracking motor stops. To restart the tracking motor, press MODE again.  
Experiment with this function to get the right speed: Press IN to set the tracking  
rate. Then press MODE and look through the eyepiece. Continue pressing IN and  
MODE until the object remains centered with little or no drifting in the eyepiece.  
Step 2.  
Step 3.  
Note: The tracking rate can be increased by up to 65%.  
4. To use a rate slower than sidereal, press OUT (6, Fig. 42) until light 4 blinks again  
(sidereal rate). Press OUT again and light 4 goes out, signifying a tracking rate  
0.5% slower than sidereal. Note that when the Mode function is active, the  
tracking motor stops. To restart the tracking motor, press MODE again.  
Experiment with this function to get the right speed: Press OUT to set the track-  
ing rate. Then press MODE and look through the eyepiece. Continue pressing  
OUTand MODE until the object remains centered with little or no drifting in the  
eyepiece.  
Step 4.  
Step 5.  
Fig. 46a: Indicator Light Key  
for changing tracking rates in  
the Northern Hemisphere  
Polar mode.  
Note: The tracking rate can be decreased by up to 65%.  
5. Press and hold MODE until only a single light is on. This exits the Mode function.  
If Northern or Southern Hemisphere polar mode was chosen, the motor drive  
starts operating at the sidereal rate.  
6. Use the four Arrow keys (1, Fig. 42) to slew the telescope to the desired object.  
To change the slew speed, press SPEED.  
Step 2.  
Step 3.  
Use the following procedure to change tracking rates when using the Southern  
Hemisphere polar mode. Refer to Fig. 46b.  
1. Press and hold MODE (5, Fig. 3) until the Mode function is active (i.e., lights 1 and  
2 are on steady; lights 3 and 4 signify the tracking mode last chosen).  
2. Press SPEED (3, Fig. 3) until lights 1 and 2 are on steady, light 3 is off, and Light  
4 is blinking.  
Step 5.  
Step 4.  
3. Press IN (7, Fig. 3) and light 4 comes on steady. The tracking rate is now 0.5%  
faster than sidereal. Note that when the Mode function is active, the tracking  
motor stops. To restart the tracking motor, press MODE again. Experiment  
with this function to get the right speed: Press IN to set the tracking rate. Then  
press MODE and look through the eyepiece. Continue pressing IN and MODE  
until the object remains centered with little or no drifting in the eyepiece.  
Fig. 46b: Indicator Light Key  
for changing tracking rates in  
the Southern Hemisphere  
Polar mode.  
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Note: The tracking rate can be increased by up to 65%.  
4. To use a rate slower than sidereal, press OUT (6, Fig. 3) until light 4 blinks again  
(sidereal rate). Press OUT key and light 4 goes out, signifying a tracking rate  
0.5% slower than sidereal. Note that when the Mode function is active, the  
tracking motor stops. To restart the tracking motor, press MODE again.  
Experiment with this function to get the right speed: Press OUT to set the track-  
ing rate. Then press MODE and look through the eyepiece. Continue pressing  
OUT and MODE until the object remains centered with little or no drifting in the  
eyepiece.  
Note: The tracking rate can be decreased by up to 65%.  
5. Press and hold MODE until only a single light is on. This exits the Mode function.  
If Northern or Southern Hemisphere polar mode was chosen, the motor drive  
starts operating at the sidereal rate.  
6. Use the four Arrow keys (1, Fig. 3) to slew the telescope to the desired object. To  
change the slew speed, press SPEED.  
Changing the Polar Mode  
To use the Electronic Controller to change to Northern or Southern Hemisphere polar  
mode, use the following procedure. This procedure also allows you to select a  
"Tracking Disabled" setting. Refer to Fig. 47.  
Step 4.  
Step 3.  
1. Complete the SETTING THE POLAR HOME POSITION procedure, described on  
page 17.  
2. Complete steps 2 through 8 as described in TO MOVETHETELESCOPE USINGTHE  
ELECTRONIC CONTROLLER, page 56, to initialize the Electronic Controller.  
3. Press and hold MODE until lights 1 and 2 are on steady Ignore lights 3 and 4;  
they may or may nor appear as depicted in the figures to the left (how these lights  
appear depend upon what has previously has been set).  
Step 5.  
Step 6.  
4. Press SPEED once. This changes the system to polar mode for the Earths  
Southern Hemisphere, with the motor drive set to operate at the sidereal rate.  
5. Press SPEED a second time. This changes the system to polar mode for the  
Earths Northern hemisphere, with the motor drive set to operate at the sidereal  
rate.  
Step 8.  
Fig. 47: Indicator Light Key for  
Changing the Polar Mode.  
6. Press SPEED a third time to disable tracking.  
7. Use the SPEED key as described in the above steps to cycle among these three  
modes (Southern Hemisphere polar, Northern Hemisphere-polar, or Tracking  
Disabled) until the desired mode is shown by the appropriate light configuration.  
8. Press and hold MODE until just one light is on. This exits the Mode function. If  
you choose Northern or Southern Hemisphere polar mode, the motor drive starts  
operating at the sidereal rate.  
9. Use the four Arrow keys to slew the telescope to the desired object. To change  
the slew speed, press SPEED.  
Optional Autostar Computer Controller for LXD55 EC Users  
One of the most important advances in telescope control in the past 25 years, the  
Meade Autostar Computer Controller turns your LXD55 EC model into an automatic  
celestial object locating system. Just plug Autostar into the telescopes HBX port in  
place of the standard-equipment Electronic Controller, do a quick telescope align-  
ment, and you are ready to observe any object in the Autostars 30,000-object data-  
base.  
Best of all, the Meade Autostar is easy to use. Even the most novice observer will  
locate dozens of fascinating celestial objects the very first night out. Study Saturn and  
its ring system; the primary cloud belts of Jupiter as well as its four major satellites;  
the moon-like phases of Mercury and Venus; prominent features on Mars. The Moon  
stands out in stark, almost three-dimensional detailcraters, mountain ranges, and  
fault lines. In our galaxy, the telescope displays hundreds of nebulae, star clusters,  
double and multiple stars, and variable starsplus dozens of external galaxies in all  
their variation of form and structure.  
Any of Autostars database objects can be called up and entered on the hand con-  
troller display in seconds. The observer then simply presses the GO TO pushbutton  
and watches as the telescope automatically slews to the object and places it in the  
field of view. Autostar moves the telescope to automatically track (follow) the object  
across the sky. Autostar brings into easy access objects that were previously unreach-  
able for all but the most dedicated of amateur astronomers.  
58  
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A P P E N D IX E : M O U N T IN G  
T H E M O D E L S C -8 S C H M ID T -  
C A S S E G R A IN O P T IC A L  
T U B E  
Slot  
Groove  
How to Attach the Optical Tube to the Mount  
The LXD55 model SC-8 Schmidt-Cassegrain assembles and operates identically to  
all the other LXD55 models equipped with an Autostar handbox, with one exception:  
the optical tube is attached to the mount with a mounting bracket rather than the cra-  
dle ring assembly. The optical tube is shipped with the mounting bracket already  
attached. To attach the mounting bracket /optical tube assembly to the mount, perform  
the following steps.  
Screws at the  
back-end of  
the bracket  
Locking Knobs  
1. Perform steps 1 through 6 as described in HOWTO ASSEMBLEYOURTELESCOPE,  
pages 11 and 12.  
Fig. 48: Mounting the SC bracket and  
optical tube to the mount.  
2. Slide the mounting bracket into the cradle assembly mounting slot. For most  
applications, set the groove in the bracket next to the cradle locking knob, so that  
the bolt of the cradle locking knob will enter the groove when the knob is tight-  
ened. Tighten both the cradle locking knob and the secondary locking knob to a  
firm feel. See Fig. 48.  
If you are using heavy accessories (such as a camera, microfocuser, etc.) on the  
back end of the tube, you may need to balance the tube differently to keep the  
tube from drifting downward: Slide the mounting bracket and tube forward, until  
the screws at the back end of the tray touch the mount. See Figs. 48 and 49.  
Then tighten the cradle locking knob and the secondary locking knob to a firm  
feel.  
Screws at the  
back-end of  
the bracket  
3. Continue the assembly with step 9 as described in HOWTO ASSEMBLEYOURTEL-  
ESCOPE, page12, and complete all the subsequent steps. All other procedures  
are identical as described earlier in this manual.  
Fig. 49: Adjusting the balance of the  
optical tube when using heavy acces-  
sories.  
59  
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A P P E N D IX F :  
B A S IC A S T R O N O M Y  
In the early 17th century Italian Scientist Galileo, using a telescope smaller than your  
LXD55, turned it skyward instead of looking at the distant trees and mountains. What  
he saw, and what he realized about what he saw, has forever changed the way  
mankind thinks about the universe. Imagine what it must have been like being the first  
human to see moons revolve around the planet Jupiter or to see the changing phas-  
es of Venus! Because of his observations, Galileo correctly realized Earth's move-  
ment and position around the Sun, and in doing so, gave birth to modern astronomy.  
Yet Galileo's telescope was so crude, he could not clearly make out the rings of  
Saturn.  
Galileo's discoveries laid the foundation for understanding the motion and nature of  
the planets, stars, and galaxies. Building on his foundation, Henrietta Leavitt deter-  
mined how to measure the distance to stars, Edwin Hubble gave us a glimpse into the  
possible origin of the universe, Albert Einstein unraveled the crucial relationship of  
time and light, and 21st-century astronomers are currently discovering planets around  
stars outside our solar system. Almost daily, using sophisticated successors to  
Galileo's telescope, such as the Hubble Space Telescope and the Chandra X-Ray  
Telescope, more and more mysteries of the universe are being probed and under-  
stood. We are living in the golden age of astronomy.  
Unlike other sciences, astronomy welcomes contributions from amateurs. Much of the  
knowledge we have on subjects such as comets, meteor showers, double and vari-  
able stars, the Moon, and our solar system comes from observations made by ama-  
teur astronomers. So as you look through your Meade LXD55-Series telescope, keep  
in mind Galileo. To him, a telescope was not merely a machine made of glass and  
metal, but something far morea window of incredible discovery. Each glimpse offers  
a potential secret waiting to be revealed.  
Autostar Glossary  
Be sure to make use of Autostars Glossary feature. The Glossary menu provides an  
alphabetical listing of definitions and descriptions of common astronomical terms.  
Access directly through the Glossary menu or through hypertext words embedded in  
Autostar. See GLOSSARY MENU, page 27, for more information.  
Objects in Space  
Listed below are some of the many astronomical objects that can be seen with your  
LXD55-Series telescope:  
The Moon  
The Moon is, on average, a distance of 239,000 miles (380,000km) from Earth and is  
best observed during its crescent or half phase when Sunlight strikes the Moons sur-  
face at an angle. It casts shadows and adds a sense of depth to the view (Fig. 50).  
No shadows are seen during a full Moon, causing the overly bright Moon to appear  
flat and rather uninteresting through the telescope. Be sure to use a neutral Moon fil-  
ter when observing the Moon. Not only does it protect your eyes from the bright glare  
of the Moon, but it also helps enhance contrast, providing a more dramatic image.  
Fig. 50 The Moon. Note  
the deep shadows in the  
craters.  
Using your LXD55-Series telescope, brilliant detail can be observed on the Moon, includ-  
ing hundreds of lunar craters and maria, described below.  
Craters are round meteor impact sites covering most of the Moons surface. With no  
atmosphere on the Moon, no weather conditions exist, so the only erosive force is  
meteor strikes. Under these conditions, lunar craters can last for millions of years.  
Maria (plural for mare) are smooth, dark areas scattered across the lunar surface.  
These dark areas are large ancient impact basins that were filled with lava from the  
interior of the Moon by the depth and force of a meteor or comet impact.  
Twelve Apollo astronauts left their bootprints on the Moon in the late 1960's and early  
1970's. However, no telescope on Earth is able to see these footprints or any other  
artifacts. In fact, the smallest lunar features that may be seen with the largest tele-  
scope on Earth are about one-half mile across.  
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Planets  
Planets change positions in the sky as they orbit around the Sun. To locate the plan-  
ets on a given day or month, consult a monthly astronomy magazine, such as Sky  
and Telescope or Astronomy. You can also consult Autostar for information about  
planets. Scroll to the "Object: Solar System" menu and scroll through the lists of plan-  
ets. When a planet you are interested in displays, press ENTER. Use the Scroll keys  
to display information about the planet, such as the planet's coordinates, and the rise  
and set times (Tip: enter a date in the Date menu and you can determine if a plan-  
et(s) will be visible during the night of the entered date by checking its rise and set  
times). Listed below are the best planets for viewing through the LXD55-Series.  
Venus is about nine-tenths the diameter of Earth. As Venus orbits the Sun, observers  
can see it go through phases (crescent, half, and full) much like those of the Moon.  
The disk of Venus appears white as Sunlight is reflected off the thick cloud cover that  
completely obscures any surface detail.  
Fig. 51: The giant planet,  
Jupiter. The four largest  
moons can be observed  
in a different position  
every night.  
Mars is about half the diameter of Earth, and appears through the telescope as a tiny  
reddish-orange disk. It may be possible to see a hint of white at one of the planets  
Polar ice caps. Approximately every two years, when Mars is closest to Earth in its  
orbit, additional detail and coloring on the planet's surface may be visible.  
Jupiter is the largest planet in our solar system and is eleven times the diameter of  
Earth. The planet appears as a disk with dark lines stretching across the surface (Fig.  
51). These lines are cloud bands in the atmosphere. Four of Jupiters moons (Io,  
Europa, Ganymede, and Callisto) can be seen as star-likepoints of light when using  
even the lowest magnification. These moons orbit Jupiter so that the number of  
moons visible on any given night changes as they circle around the giant planet.  
Saturn is nine times the diameter of Earth and appears as a small, round disk with  
rings extending out from either side (Fig. 52). In 1610, Galileo, the first person to  
observe Saturn through a telescope, did not understand that what he was seeing  
were rings. Instead, he believed that Saturn had ears.Saturns rings are composed  
of billions of ice particles ranging in size from a speck of dust to the size of a house.  
The major division in Saturn's rings, called the Cassini Division, is occasionally visi-  
ble through the LXD55-Series. Titan, the largest of Saturns moons can also be seen  
as a bright, star-like object near the planet.  
Fig. 52: Saturn has the  
most extensive ring struc-  
ture in our Solar System.  
Deep-Sky Objects  
Star charts can be used to locate constellations, individual stars and deep-sky  
objects. Examples of various deep-sky objects are given below:  
Stars are large gaseous objects that are self-illuminated by nuclear fusion in their  
core. Because of their vast distances from our solar system, all stars appear as pin-  
points of light, irrespective of the size of the telescope used.  
Nebulae are vast interstellar clouds of gas and dust where stars are formed. Most  
impressive of these is the Great Nebula in Orion (M42), a diffuse nebula that appears  
as a faint wispy gray cloud. M42 is 1600 light years from Earth.  
Fig. 53: The Pleiades is  
one of the most beautiful  
open clusters.  
Open Clusters are loose groupings of young stars, all recently formed from the same  
diffuse nebula. The Pleiades is an open cluster 410 light years away (Fig. 53).  
Through the LXD55-Series, numerous stars are visible.  
Constellations are large, imaginary patterns of stars believed by ancient civilizations  
to be the celestial equivalent of objects, animals, people, or gods. These patterns are  
too large to be seen through a telescope. To learn the constellations, start with an  
easy grouping of stars, such as the Big Dipper in Ursa Major. Then, use a star chart  
to explore across the sky.  
Galaxies are large assemblies of stars, nebulae, and star clusters that are bound by  
gravity. The most common shape is spiral (such as our own Milky Way), but galaxies  
can also be elliptical, or even irregular blobs. The Andromeda Galaxy (M31) is the  
closest spiral-type galaxy to our own. This galaxy appears fuzzy and cigar-shaped. It  
is 2.2 million light years away in the constellation Andromeda, located between the  
large Wof Cassiopeia and the great square of Pegasus.  
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LXD55 TIPS  
Further Study....  
This manual gives only the briefest introduction to astronomy. If you are interested  
in pursuing further studies in astronomy, a few topics are suggested below that are  
worth reading up on. Try looking up some of these in the optional Autostar glossary.  
Also included below is a small sampling of books, magazines, and organizations  
that you might find helpful.  
Topics  
1. How is a star born? How does a solar system form?  
2. How is the distance to a star measured? What is a light year? What is red shift  
and blue shift?  
3. How are the craters on our Moon formed? Is there water under the surface of  
the Moon?  
4. What is a black hole? A neutron star? A gamma burster? An Einstein lens?  
5. What are stars made of? Why are stars different colors? How is the elemental  
composition of a star determined? What is an Lyman Alpha forest?  
6. What is the difference between a Type 1 and a Type II supernova?  
7. What is the importance of studying the composition of comets? Where do  
comets come from?  
8. How old is our Sun? Will our Sun evolve into a planetary nebula or go super-  
nova?  
9. What is the Inflationary Big Bang? What is dark matter? What are MACHO's?  
10. How are extrasolar planets discovered? What is an accretion (or protoplane-  
tary) disk?  
11. What are the differences between elliptical, spiral, and irregular galaxies? Can  
globular clusters be older than the universe itself?  
Books  
1. The Guide to Amateur Astronomy by Jack Newton and Philip Teece  
2. The Sky: A Users Guide by David Levy  
3. Turn Left at Orion by Guy Consolmagno & Dan Davis  
4. Astrophotography for the Amateur by Michael Covington  
5. Observing for the Fun of It by Melanie Melton  
6. Will Black Holes Devour the Universe? and 100 Other Questions about  
Astronomy by Melanie Melton  
Magazines  
1. Sky & Telescope  
Box 9111, Belmont, MA 02178  
2. Astronomy  
Box 1612, Waukesha, WI 53187  
Organizations:  
1. Astronomical League  
Executive Secretary  
5675 Real del Norte, Las Cruces, NM 88012  
2. The Astronomical Society of the Pacific  
390 Ashton Ave., San Francisco, CA 94112  
3. The Planetary Society  
65 North Catalina Ave., Pasadena, CA 91106  
And watch Jack Horkheimer, Star Gazer, on your local PBS station.  
62  
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MEADE LIMITED WARRANTY  
Every Meade telescope, spotting scope, and telescope accessory is warranted by Meade Instruments Corporation (Meade)  
to be free of defects in materials and workmanship for a period of ONE YEAR from the date of original purchase in the U.S.A.  
and Canada. Meade will repair or replace a product, or part thereof, found by Meade to be defective, provided the defective  
part is returned to Meade, freight-prepaid, with proof of purchase. This warranty applies to the original purchaser only and is  
non-transferable. Meade products purchased outside North America are not included in this warranty, but are covered under  
separate warranties issued by Meade international distributors.  
RGA Number Required: Prior to the return of any product or part, a Return Goods Authorization (RGA) number must be  
obtained from Meade by writing, or calling (949) 451-1450. Each returned part or product must include a written statement  
detailing the nature of the claimed defect, as well as the owners name, address, and phone number.  
This warranty is not valid in cases where the product has been abused or mishandled, where unauthorized repairs have been  
attempted or performed, or where depreciation of the product is due to normal wear-and-tear. Meade specifically disclaims  
special, indirect, or consequential damages or lost profit which may result from a breach of this warranty. Any implied warranties  
which cannot be disclaimed are hereby limited to a term of one year from the date of original retail purchase.  
This warranty gives you specific rights. You may have other rights which vary from state to state.  
Meade reserves the right to change product specifications or to discontinue products without notice.  
P R O D U C T S D I V I S I O N  
AMDeVaA dN CeE IDnstruments Corporation  
World’s Leading Manufacturer of Astronomical Telescopes for the Serious Amateur  
6001 Oak Canyon, Irvine, California 92618 I (949) 451-1450  
FAX: (949) 451-1460 I www.meade.com  
© 2003  
14-7300-01 10/03D  
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