Meade Telescope ETX 90PE User Manual

Instruction Manual  
®
ETX Premier Edition Telescope Series  
AutoStar® — LNT— SmartFinder™  
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CONTENTS  
Quick-Start Guide .......................................................... 4  
Telescope Features ...................................................... 6  
AutoStar Features .......................................................... 9  
Getting Started ..............................................................12  
Parts Listing ..............................................................12  
How to Assemble Your Telescope & Tripod ..............12  
Using SmartFinder, Aligning SmartFinder ................13  
Choosing an Eyepiece..............................................14  
Observing ......................................................................15  
Observing by Moving the Telescope Manually..........15  
Terrestrial Observing ................................................15  
Observing Using AutoStar's Arrow Keys ..................15  
Slew Speeds ............................................................16  
Astronomical Observing, Observe the Moon............16  
To Track an Object Automatically ..............................16  
Moving Through AutoStar’s Menus......................16  
Initializing AutoStar for the First Time..................17  
Automatic Alignment............................................17  
Observe a Star Using Automatic Tracking ..........18  
Go To Saturn, Using the Guided Tour ................19  
Basic AutoStar Operation ..............................................20  
AutoStar Navigation Exercise ..................................20  
Entering Data, Moving Through AutoStar’s Menus ..21  
AutoStar Menus ............................................................22  
Menu Tree ................................................................22  
Objects Menu............................................................23  
Event Menu, Glossary Menu ....................................24  
Utilities Menu ............................................................25  
Setup Menu ..............................................................26  
Advanced AutoStar Operation........................................29  
Adding Observing Sites ............................................29  
Finding Objects Not in the Database........................30  
Observing Satellites..................................................30  
Create Your Own Guided Tour ..................................31  
Landmarks ................................................................34  
Identify ......................................................................35  
Advanced Alt/Az Alignment Methods........................36  
Smart Drive Training (PEC) ......................................37  
Browse ......................................................................38  
Photography ..................................................................39  
Photography with AutoStar Suite ..............................41  
Optional Accessories......................................................42  
Maintenance ..................................................................44  
Troubleshooting ........................................................45  
Specifications ................................................................47  
Appendix A: Equatorial (Polar) Alignment ......................50  
Equatorial Alignment, Celestial Coordinates ............50  
Polar Mounting with #884 Deluxe Field Tripod..........50  
Equatorial Mounting Procedure ................................51  
To Track a Star When Polar Mounted........................51  
Polar Alignment Modes, Locating Celestial Pole ......52  
Setting Circles ..........................................................53  
Appendix B: Latitude Chart ............................................54  
Appendix C: Training the Drive ......................................55  
Appendix D: Changing the LNT Module Battery ............56  
Appendix E: Basic Astronomy ........................................57  
WARNING!  
®
®
Never use a Meade ETX PE Telescope to  
look at the Sun! Looking at or near the Sun  
will cause instant and irreversible  
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 at or near  
the Sun. Do not look through the telescope  
as it is moving. Children should always have  
adult supervision while observing.  
Caution: Use care to install batteries in the  
orientation indicated by illustration in the  
battery slots of the battery compartment.  
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.  
If you are anxious to use your telescope  
for the first time, read the QUICK-START  
GUIDE on pages 4 and 5.  
® The name "Meade," “ETX,AutoStar” and the Meade logo  
are trademarks registered with the U.S. Patent Office and in  
principal countries throughout the world.  
“LNT [Level North Technology],SmartFinder,Deep Sky  
Imager,LPI,and “Tonight’s Best” are trademarks of Meade  
Instruments Corporation.  
Patents:  
US 6,304,376  
US 6,392,799  
US 6,563,636  
D 422,610  
Patent Pending  
© 2004 Meade Instruments Corporation.  
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QUICK-START GUIDE  
This Quick Start Guide demonstrates how to install the batteries and eyepiece, and how to observe using the AutoStar Arrow  
keys. If you wish to try out AutoStar’s “Go To” capabilities, check out the list of page references at the bottom of the following page.  
®
Remove the ETX telescope from its packaging and place  
it on a sturdy surface. Place the ETX on its side and  
remove the battery compartment cover (A) from the under-  
side of the drive base. Insert eight (user-supplied) AA-size  
batteries into the battery compartment (B) oriented as  
shown in the battery compartment. Replace the cover and  
return the telescope to an upright position (if you wish to  
attach the telescope to the deluxe field tripod, see page  
12).  
...and the other end of the coiled cord into the coiled cord  
port at the bottom of AutoStar handbox (H), as shown above.  
Tighten (to a "firm feel" only, do not overtighten) the vertical lock  
(I) and the horizontal lock (J). See page 7 and 8 for more infor-  
mation.  
Place the 26mm eyepiece (C) into the eyepiece holder on  
the telescope and tighten the attachment thumbscrew (D) to  
a "firm feel" only. See page 7, for more information. Remove  
the dust cover (E) from the end of the telescope tube.  
Flip the Power Switch (F) on the computer control panel to  
the ON position. A copyright message lights on AutoStar’s  
LCD display, followed by a warning not to look at the Sun.  
Press the AutoStar key prompted by the message when you  
are done reading.  
A “Getting Started” message displays. Press ENTER to skip  
this message.  
Make sure that the computer control panel power switch  
(F) is in the OFF position. Remove the Autostar handbox  
and the coiled cord from the packing materials. Plug one  
®
See pages 9 to 11 for more information about AutoStar’s  
keys.  
4end of the cord into the HBX port (G).  
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To change the speed at which the telescope moves (known as  
the “slew” speed) press a NUMBER KEY from 1 through 9. 1  
is the slowest speed and 9 is the fastest.  
Enter  
Key  
Scroll  
Down  
Key  
Scroll Up  
Key  
Make sure that the flip mirror control (K) is in the “Up” position,  
as shown the diagram above.  
AutoStar then displays: “Location Option: 1-Zipcode 2-City”.  
This option allows you to choose how you wish to enter the  
location of your observing site: you can enter your zip code  
or choose the site from a list of countries, states and cities.  
Press the number key “1” if you wish to enter by zip code.  
Then enter the five digits of the zip code of your observing  
site and press ENTER.  
Press the number key “2” if you wish to select your  
observing site from a list of country, states and cities. First,  
use a Scroll key to cycle through the list of countries and  
states (listed alphabetically). Press ENTER when the  
correct location displays. Next, use a Scroll key to cycle  
through the list of cities (also listed alphabetically). Press  
ENTER when the closest city displays.  
Finally “Telescope Models” displays. Using the SCROLL KEYS,  
cycle through the list of telescope models and press ENTER  
when your model displays.  
The display now displays "Setup: Align." See page 17 for more  
information.  
If AutoStar does not requests the Country/State, City and  
Telescope Model information, use the "Telescope Model"  
and "Site" options in the Setup menu to change this  
information. See pages 27 and 29 for more information.  
Sight along the side of the telescope’s main tube to locate an  
object. If you wish to learn how to align the telescope’s  
SmartFinder, see page 13.  
Use the telescope’s focus knob (L) to bring the object into  
focus.  
Arrow  
Keys  
Arrow  
Keys  
If you wish to learn more about observing with  
AutoStar and other features of your telescope, see:  
Number  
Keys  
Page 13 to learn how to use SmartFinder  
Page 17 to learn how to perform an Automatic Alignment  
Page 19 to learn how to “Go To” Saturn”  
Page 19 to learn about Guided Tours  
Page 22 for a Menu tree of AutoStar’s menus  
Pages 23 to 38 to learn more about AutoStar’s menus  
You can now use the Arrow keys to slew (move) the  
telescope up, down, right or left. Practice using the ARROW  
KEYS to center objects in the eyepiece.  
5
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TELESCOPE FEATURES  
2
17  
1
19  
E
5
9
16  
13  
B
C
D
A
B
10  
11  
10  
12  
Fig. 2 (Inset): Computer Control Panel. (A) On/Off switch;  
(B) Auxiliary ports; (C) Handbox port; (D) 12v connector; (E)  
Power indicator light.  
Fig. 1a: Side View  
Features of the ETX-90PE, ETX-  
105PE and ETX-125PE are identical,  
with the exception of the size of  
optical tube.  
18  
1
2
3
4
Fig. 1a, b and Fig. 2:  
The ETX Premier Telescope  
1
2
3
4
5
6
7
8
9
Eyepiece  
SmartFinder  
6
Holder Thumbscrew  
90° Eyepiece Holder  
Optical Tube  
16  
Vertical (Dec.) Lock  
Fork Arms  
Focus Knob  
Horizontal (R.A.) Lock  
10 Computer Control Panel  
A. ON/OFF Switch  
B. Auxiliary Ports (2)  
C. Handbox Port  
D. 12v  
15  
8
E. LED  
11 Base Housing  
12 Battery Compartment  
(bottom of base)  
14  
13 Right Ascension (R.A.)/  
Horizontal Setting Circle  
14 Flip-Mirror Control Knobs  
15 Photo Port  
7
16 Declination (Dec.)/Vertical  
Setting Circle  
17 SmartFinder Alignment Screws  
18 LNT Module  
13  
19 Dust Cap (not visible)  
Fig. 1b: Rear View  
6
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MEADE ETX: YOUR PERSONAL  
WINDOW TO THE UNIVERSE  
Caution:  
The Meade Premier Edition ETX-90PE, ETX-105PE and the ETX-125PE are  
extremely versatile, high-resolution telescopes. With pushbutton controls, automatic  
tracking of celestial objects and diffraction-limited imaging, an ETX Premier telescope  
may be all the telescope ever required by many terrestrial and astronomical  
observers.  
Using products other than  
standard Meade accessories  
may cause damage to the  
telescope’s internal  
electronics and may void the  
Meade warranty.  
Your ETX telescope reveals nature in an ever-expanding level of detail. Observe the  
feather structure of an eagle from 50 yards or study the rings of the planet Saturn from  
a distance of 800 million miles. Focus beyond the Solar System and observe  
majestic nebulae, ancient star clusters, remote galaxies and even stars recently  
discovered to have planets orbiting about them. Meade ETX Premier telescopes are  
instruments fully capable of growing with your interest and are ideal for both the  
casual observer and serious astronomer alike.  
B
Want to learn more  
about the eyepieces  
available for your ETX  
telescope?  
Telescope Controls  
Become acquainted with all of these controls before attempting observations through  
the telescope.  
See OPTIONAL  
ACCESSORIES, pages  
42 and 43.  
B Eyepiece: Place the supplied 26mm eyepiece into the 90° Eyepiece Holder (4,  
Fig. 1b) and tighten in place with thumbscrew (3, Fig.1b).  
C
Smartfinder™  
Provides an easier way to sight on objects than the main telescope’s eyepiece  
which has a narrow field of view. Comes pre-assembled on the telescope.  
c
G
Want to learn more  
about the  
D Eyepiece Holder Thumbscrew: Tightens the eyepiece in place. Tighten to a firm  
SmartFinder?  
feel only.  
See Aligning  
SmartFinder, page 13.  
e 90° Eyepiece Holder: Holds the eyepiece upright for easy viewing.  
F Optical Tube: The main optical component that gathers the light from distant  
objects and brings this light to a focus for examination with the eyepiece.  
G Vertical (Dec.) Lock: Controls the manual vertical movement of the telescope.  
Turning the vertical lock counterclockwise unlocks the telescope enabling it to be  
freely rotated by hand about the vertical axis. Turning the vertical lock clockwise  
(to a firm feel only) prevents the telescope from being moved manually, but  
engages the vertical motor drive clutch for AutoStar operation. When polar  
aligned, the vertical lock serves as the Declination or Dec. lock.  
Want to learn more  
about the Right  
Ascension and  
Declination setting  
circles? See page 54.  
Note: The vertical lock knob is a knurled knob located on the fork arm to  
the right of the focus knob (8, Fig. 1b). Mounted beneath the knob is a cir-  
cular scale without numbers. Do not confuse this scale with the Dec.  
setting circle (16, Fig. 1a) on the opposite fork arm which has a numbered  
scale used to locate astronomical objects.  
H Fork Arms: Hold the optical tube in place.  
Note: The telescope base and fork mount are designed with internal  
“rotational limit stops.The horizontal limit stop prevents the telescope  
from rotating more than 630° to avoid damage to the internal wiring. The  
vertical limit stop prevents the smartfinder from striking the fork mount  
when the telescope is pointed upward just past 90° and prevents the  
optical tube from striking the base if pointed downward more than 30°. Do  
not force the telescope to move beyond these stops or damage to the  
telescope will result.  
Caution:  
When loosening the Dec.  
lock, be sure to support  
the optical tube (5 Fig.  
1a). The weight of the  
tube could cause the tube  
to swing through the fork  
arms suddenly.  
i Focus Knob: Moves the telescope’s primary mirror in a finely-controlled motion  
to achieve precise image focus. The ETX telescopes can be focused on objects  
from a distance of about 11.5 ft (ETX-90PE) or 15 ft (ETX-105PE or  
ETX-125PE) to infinity. Rotate the focus knob clockwise to focus on distant  
objects and counterclockwise to focus on nearby objects.  
7
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j Horizontal (R.A.) Lock: Controls the manual horizontal rotation of the telescope.  
Loosen the horizontal lock counterclockwise to unlock the telescope, enabling it to  
be freely rotated by hand about the horizontal axis. Tightening the horizontal lock  
clockwise prevents the telescope from being rotated manually, but engages the hor-  
izontal motor drive clutch for AutoStar operation. When polar aligned, the horizon-  
Definitions  
Throughout this manual,  
you will notice the terms  
"Alt/Az," "Right  
Ascension," and  
"Declination." Alt/Az or  
more properly, altazimuth,  
is frequently used to refer to  
altitude or Declination (the  
up-and-down vertical  
movement of the telescope)  
and azimuth or Right  
Ascension (the side-to-side  
horizontal movement of the  
telescope). Right Ascension  
is abbreviated as "R.A."  
and Declination as "Dec."  
tal lock serves as the Right Ascension or R.A. lock.  
1) Computer Control Panel (see Fig. 2)  
A. ON/OFF Switch: Turns the Computer Control Panel and AutoStar  
handbox ON or OFF.  
Note: Always remove the batteries if they are not to be used for a long  
period of time.  
B. Auxiliary (AUX) Ports (2): Provide connection for current and future  
Meade accessories. See OPTIONAL ACCESSORIES, page 42.  
C. Handbox (HBX) Port: Plug the AutoStar handbox into this port.  
D. 12v: The 12v connector is designed to accept an external power  
supply such as the optional #541 AC Adapter or the #607 Power Cord  
(see OPTIONAL ACCESSORIES, page 42). When one of the external  
power supply options is used, the internal batteries are disconnected  
from the power circuit.  
E. LED: The red power indicator light illuminates when power is supplied  
to the connected handbox and to the telescope’s motor drive.  
1! Base Housing: Supports the telescope for placement on a flat, level surface,  
such as a tabletop or tripod.  
1@ Battery Compartment (not shown, underneath base): Install eight  
user-supplied AA batteries in this compartment. See page 12 for more  
information.  
Fig. 3a: Flip mirror control in  
the “up” position.  
1# Right Ascension (R.A.) Setting Circle: See page 53 for detailed information.  
1$ Flip-Mirror and Flip-Mirror Control Knobs: ETX telescopes include an internal  
mirror. With the flip-mirror control in the “up” position, as shown in Fig. 3a, light is  
diverted to the eyepiece. With the flip-mirror control in the “down” position, as  
shown in Fig. 3b, light proceeds straight out the photo port for photography. See  
PHOTOGRAPHY, page 39.  
Note: The flip-mirror control is in the “up” position when the control is  
vertical (perpendicular to the telescope tube).To place the flip-mirror in the  
“down” position, turn the control until it is horizontal.  
Fig. 3b: Flip mirror control in  
the “down” position.  
1% Photo Port: Attach any 35mm camera with a removable lens to this port using an  
optional #64ST T-Adapter or attach the #932 Erecting Prism for correctly  
oriented images through the eyepiece. See OPTIONAL ACCESSORIES, page 42.  
1*  
1(  
Want to learn more about  
aligning the  
SmartFinder?  
1^ Declination (Dec.) Setting Circle (on left fork arm): See page 53 for detailed  
See pages 13.  
information.  
1& SmartFinder Alignment Screws: Adjust these screws to align the SmartFinder.  
Note: The dust cap  
should be replaced  
after each observing  
session and the  
power turned off to  
the telescope. Verify  
that any dew that  
might have collected  
during the observing  
session has  
See pages 13 and 14 for more information.  
1* LNT (Level NorthTechnology) Module: This assembly has sensors which auto-  
matically points the telescope North, and detects the level and tilt of the telescope  
during automatic alignment. See page 17 for more information about Automatic  
Alignment. The LNT bracket also contains a LNT Module which supplies the time  
and date to AutoStar. The time is set at the factory. See ATOMIC TIME UPDATE  
MODULE PORT below.  
1( ATOMIC TIME UPDATE MODULE Port: Attach Meade’s ATOMIC TIME UPDATE  
MODULE optional accessory into this port. Your telescope’s time is set at the fac-  
tory before it is shipped, but the ATOMIC TIME UPDATE MODULE allows your tele-  
scope to update the time module from the NIST atomic clock in Fort Collins,  
Colorado.  
evaporated prior to  
replacing the dust  
cap. Do not  
overtighten.  
2) Dust Cap: Unthread the dust cap counterclockwise from the front lens of the  
telescope.  
8
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AUTOSTAR FEATURES  
¹
1 LCD Display  
2 ENTER Key  
3 MODE Key  
4 GO TO Key  
5 Arrow Keys  
6 Number Keys  
7 Scroll Keys  
8 Speed/? Key  
9 Coil Cord  
¸
µ
10 RS232 Port  
11 Light key  
12 Utility Light  
Fig. 4: The AutoStar Handbox.  
Tour the Cosmos with Just the Push of a Button  
Control of ETX Telescopes is through the operation of the standard-equipment #497  
AutoStar. Nearly all functions of the telescope are accomplished with just a few  
pushes of AutoStar’s buttons. Some of the major features of AutoStar are:  
Automatically move the telescope to any of the 30,000 objects stored in the  
database or manually enter the astronomical coordinates of any celestial object.  
Take a guided tour of the best celestial objects to view on any given night of the  
year.  
Want to learn more about  
downloading the latest  
updates of AutoStar  
software from the  
Meade website? See  
pages 28 and 42.  
Download the latest satellite data, guided tours and software revisions directly  
from the Meade website (www.meade.com) and share software with other  
AutoStar enthusiasts. (Requires optional #505 AstroFinder™ Cable Connector  
Kit. See OPTIONAL ACCESSORIES, page 42.)  
Access a glossary of astronomical terms.  
Calculate which eyepiece to use for optimum viewing of a celestial object.  
AutoStar provides control of virtually every telescope function. The AutoStar handbox  
has soft-touch keys designed to have a positive feel. The LCD (Liquid Crystal Display)  
is backlit with red LEDs (Light Emitting Diodes) for easy viewing in the dark.The back-  
lit display, key arrangement and sequential menu structure make AutoStar extremely  
user friendly.  
9
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B
2-Line LCD Display: This screen displays AutoStar's menus and information  
about the telescope.  
Top line: Lists the primary menu.  
Bottom line: Displays other menus that may be chosen, menu options,  
telescope status or information about a function that is being per-  
formed.  
c
d
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 MOV-  
ING THROUGH AUTOSTAR’S MENUS, page 21 and AUTOSTAR MENUS, page 22.  
MODE Key: Press to return to the previous menu or data 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.”  
If MODE is pressed and held for two seconds or more, information about the  
telescope's status displays. When the status displays, press one of the Scroll  
keys (7, Fig. 2) to display the following information:  
• Right Ascension and Declination (astronomical) coordinates  
• Altitude (vertical) and Azimuth (horizontal) coordinates  
• Local Time and Local Sidereal Time (LST)  
• Timer and Alarm Status  
• Date  
• Site coordinates  
• Battery status  
• SmartFinder Finder Set menu (see below)  
Press MODE again to return to the previous menu.  
Finder Set menu: Select the Finder Set menu to access options that will allow you to  
set the intensity and blink rate of the SmartFinder red dot.  
To set the blink rate of SmartFinder’s red dot (circled numbers refer to Fig. 4):  
1. Press and hold MODE c for two seconds. R.A and Dec. coordinates display.  
2. Keep pressing the Scroll Down key h until “Finder Set: Set” displays.  
3. Press ENTER b. “Finder Set: Intensity” displays.  
4. Press the Scroll Down key h. “Finder: Blink On” displays.  
5. Press ENTER b. A time value, in seconds, displays. For example, “00.5” may  
display. 00.5” (one-half second) is the amount of time, in seconds, that the red  
dot will blink “on.”  
6. Use the Number keys g and the Arrow keys f to change the time value. For  
example, you may wish to change the amount of time the red dot stays on to 10.2  
seconds: Press “1,press the Right Arrow key f, press “0,press the Right Arrow  
key f, press “2. An alternate method is to use the Scroll keys h to scroll  
through the time values. Once the time value is entered, press ENTER b.  
7. Press the Scroll Down key h. “Finder: Blink Off” displays. Press ENTER b. A  
time value, “00.1” (one-tenth second), may display. For example, you may wish to  
change the amount of time the red dot stays off to 00.7 seconds: Press the Right  
Arrow key f twice (as the first two values are already zero), then press “7. Or  
you may use the Scroll keys h to scroll through the time values.  
8. The SmartFinder’s red dot will now blink on for 10.2 seconds and turn off for 0.7  
seconds, and then repeat the cycle until you change the values again. Press and  
hold MODE c to exit this function.  
Similarly, you can set the Intensity value by scrolling through the intensity values with  
then Scroll keys h. The option lets you select a value of intensity for the red dot from  
0 (Off) to 14 (Full Intensity).  
e
Want to learn more  
about using the GO TO  
function? See page 19.  
e
GO TO Key: After the telescope is aligned, press to slew (move) the telescope to  
the coordinates of the currently 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  
during the alignment or GO TO procedures to activate a "spiral search."  
Want to learn how to  
perform a spiral  
search? See page 19.  
10  
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Also, 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."  
Additionally, use the Arrow keys to to move the cursor across the display: Use the  
Right or Left Arrow key to move the cursor from one number to the next in the dis-  
play.  
f
Arrow Keys: The Arrow keys have several functions. Press an Arrow key 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. Use the Arrow keys to move the  
telescope vertically up and down. The Left Arrow key rotates the telescope  
horizontally counterclockwise, while the Right Arrow key rotates it clockwise.  
g
Want to learn more  
about changing slew  
speeds? See page 16.  
g
h
Number Keys: Press to input digits 0 to 9. To change the speed at which the  
telescope moves (known as the “slew” speed) press a NUMBER KEY from 1  
through 9. 1 is the slowest speed and 9 is the fastest.  
Scroll Keys: Press to access options within a selected menu. The menu is  
displayed on the first line of the screen. Options in the 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.  
The Scroll keys also control the speed of text scrolling on the AutoStar display.  
When text is scrolling, press and hold the Up Scroll key for a faster display speed  
and the Down Scroll key for a slower display speed.  
i
? Key: Press to access the "Help" file. "Help" provides on-screen information on  
how to accomplish whatever task is currently active.  
Press 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, ALIGN-  
MENT, etc., press 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
1)  
RS232 Port: Plug in optional cable to download the latest satellite data and  
software revisions directly from the Meade website (www.meade.com). You can  
also share software with other AutoStar enthusiasts or control your telescope  
remotely from your PC. (Requires optional #505 AstroFinder™ Software and  
Cable Connector Kit. See OPTIONAL ACCESSORIES, page 42.)  
Coil Cord Port/Coil Cord: Plug one end of the supplied AutoStar coil cord into  
this port located at the bottom of the handbox and the other end into the HBX port  
of the Computer Control Panel.  
1!  
1@  
Light/0 Key: Press to turn on Utility light (12, Fig. 4).  
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.  
ETX TIPS  
Star Charts  
Even with the AutoStar's large 30,000 object library, star charts and  
planispheres are still useful for a variety of reasons. In particular, they are a  
great aid in planning 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 AutoStar Suiteand other star locator  
software. 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.  
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GETTING STARTED  
Parts Listing  
Getting the telescope ready for first observations requires only a few minutes. When  
first opening the packing box, note carefully the following parts:  
ETX Premier Telescope with fork mount system and SmartFinder  
#497 AutoStar handbox with coil cord.  
One or more eyepieces, packed in plastic storage containers.  
Hex-wrench, packed with the instruction manual. See MAINTENANCE,  
page 44.  
Cover  
#884 Deluxe Field Tripod; two attachment knobs; spreader tray with sepa-  
rate spring, washers (2) and tension knob; leg extension lock knobs.  
Batteries  
Fig. 5: Battery installation.  
How to Assemble Your Telescope and Tripod  
Assembly of the ETX telescope requires eight AA-size (user-supplied) batteries.  
1. Remove the ETX telescope from its packaging and place it on a sturdy surface.  
Place the ETX on its side and remove the battery compartment cover from the  
underside of the drive base. Insert eight (user-supplied) AA-size batteries into the  
battery compartment oriented as shown in the battery compartment. Replace the  
cover and return the telescope to an upright position.  
Caution: Use care to install batteries as indicated by the diagrams in the  
battery compartment. 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. Always remove the batteries if they are not to be used for a long  
period of time.  
Fig. 6: Spread tripod legs.  
Note: AutoStar does not require batteries; the telescope’s batteries  
supply power to AutoStar.  
2. Assemble the #884 Deluxe Field Tripod:  
Step a: Spread the tripod (1, Fig. 6) legs apart to a fully open position.  
Step b: Slide the spreader tray (2, Fig. 7) onto the central threaded rod.  
Step c: Slide a washer, followed by the spring, another washer and the  
tension knob (3, Fig. 8) onto the threaded rod. Tighten the tension knob  
Fig. 7: Slide spreader on rod.  
to a firm feel.  
Step d: Adjust the height of the tripod by loosening the leg lock knobs (4, Fig. 9)  
and adjusting the height of the inner leg extensions.Then retighten the lock  
knobs.  
3. Mount your telescope in the altazimuth (alt/az) mode. If you wish to mount your  
telescope in the equatorial mode, see EQUATORIAL ALIGNMENT, page 50.  
Note: Throughout this manual, you will notice the term "Alt/Az," or more  
properly, altazimuth.This term is frequently used to refer to altitude or the  
up-and-down vertical movement of the telescope). Azimuth refers to the  
side-to-side horizontal movement of the telescope.  
Fig. 8: Tension knob  
assembly.  
Step e: Loosen the latitude control latch (6, Fig. 10) and lift up the tilt-plate (5, Fig.  
10) so that you can easily access the underside of the plate. Relock the  
latitude control latch, so the assembly doesn't slip while you are attaching  
the telescope.  
Step f: Line up the mounting hole (7, Fig. 11) on the base of the telescope  
marked "High Latitude Leg" with the attachment knob (8, Fig. 11) that is  
closest to the latitude control bar (9, Fig. 11). Line up the other  
mounting hole with the attachment knob at the bottom of the tilt-plate.  
Thread both attachment knobs into the base of the telescope.Tighten to  
a firm feel only. (See Fig. 12.)  
Fig. 9: Adjust tripod height.  
Step g: Unlock the latitude control latch (10, Fig. 13) and lower the tilt-plate until  
it is level (push the tilt-plate down until it stops; this is the level  
position). Lock the latitude control latch.  
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¹
Ƹ
ƹ
ƺ
Fig. 15: Insert eyepiece.  
Fig. 16: Tighten vertical  
lock.  
Fig. 17: Tighten horizontal  
lock.  
Fig. 10: Loosen control latch .  
4. Place the 26mm eyepiece (12, Fig. 15) into the eyepiece holder on the  
telescope and tighten the attachment thumbscrew (13, Fig. 15) to a "firm feel" only.  
Make sure that the flip-mirror control (14, Fig. 15) is in the “up” position, as shown  
in the above photo. See page 14, for more information. Remove the dust cover (15,  
Fig. 15) from the end of the telescope tube.  
5. Make sure that the computer control panel power switch (A, Fig. 2) is in the OFF  
position. Remove the AutoStar handbox and the coiled cord from the packing  
materials. Plug one end of the cord into the HBX port (C, Fig. 2)and the other end  
of the coiled cord into the coiled cord port at the bottom of AutoStar handbox, as  
shown above.  
Fig. 11: High latitude leg  
mounting hole and  
corresponding attachment  
knob.  
6. Tighten (to a "firm feel" only, do not overtighten) the vertical lock (Fig. 6) and the hor-  
izontal lock (Fig. 9)  
.
Using SmartFinder  
As with most astronomical telescopes, an eyepieces presents a narrow field of view  
to the observer. As a result it is sometimes difficult to locate objects just using your  
eyepiece. The SmartFinder has a projected red dot that helps you to locate objects  
as you move your telescope.  
To turn on SmartFinder’s red dot (continuous, without blinking):  
1. Press and hold MODE for two seconds. R.A and Dec. coordinates display.  
2. Keep pressing the Scroll Down key until “Finder Set: Set” displays.  
3. Press ENTER. “Finder Set: Intensity” displays.  
4. Press the Scroll Down key. Finder: Blink On” displays.  
5. Press ENTER. A time value, in seconds, displays. For example, “00.5” may  
display. 00.5” is the amount of time, in seconds, that the red dot will blink “on.”  
(For this example, you may select or enter any value except “00.0.) Press  
ENTER.  
Fig. 12: Attach telescope to  
tripod.  
6. Press the Scroll Down key. Finder: Blink Off” displays.  
7. Press ENTER. Use the Number keys to enter “00.0” or press the Scroll Down  
key until “00.0” displays. “00.0” is the amount of time in seconds that the  
red dot will remain “off.This value, along with the value you chose in the  
“Finder: Blink On” menu, allows the red dot to remain on without blinking.  
“00.0” means there is no “off” time, so the dot will remain on continuously,  
without blinking.  
µ
Fig. 13: Level tilt-plate.  
8. Use these menus to set other blink rates. For example, If you select “00.1” in  
the Blink Off menu, and “00.2” in the Blink On menu, the red dot will blink on  
for .2 seconds and then blink off for .1 second, and then repeat the cycle until  
you change the values again.  
9. Press and hold MODE to exit this function.  
Aligning SmartFinder  
In order for the SmartFinder to be useful, it must first be aligned with the main tele-  
scope, so that both the SmartFinder and the main telescope are pointing at  
precisely the same location. To align the SmartFinder:  
¹
Fig. 14: Handbox HBX port.  
1. Point the main telescope at some well-defined distant (perhaps a mile away) land  
object, such as a telephone pole or sign. Center the object, as precisely as  
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possible, in the SP 26mm eyepiece's field of view. Tighten the vertical and  
horizontal locks (6 and 9, Fig. 1) so that the tube cannot move and the object  
remains centered.  
ƹ
2. While looking through the SmartFinder, turn the top or side alignment screws (13  
and 14, Fig. 18), until the red dot of the SmartFinder points at precisely the same  
position as the view through the eyepiece of the main telescope.  
Ƹ
The SmartFinder is now aligned to the main telescope. Unless the alignment screws  
are disturbed or the LNT Module is moved out of place, the SmartFinder should  
remain aligned indefinitely.  
Choosing an Eyepiece  
The magnification or power, at which a telescope is operating is determined by two  
factors: the focal length of the telescope and the focal length of the eyepiece.  
Fig. 18: Turn the top (13) or  
side (14) Smartfinder  
adjustment screws.  
Telescope Focal Length is the distance that light travels inside the telescope before  
reaching a focus. In the mirror-lens design of the ETX models, the focal length is  
compressed by the telescope’s secondary mirror, so that a long focal length is housed  
in the short ETX optical tube. For example, the ETX-90PE’s focal length is 1250mm  
or about 49”. This means that if the ETX–90PE were a classical refracting-type of  
telescope, the optical tube would be more than four feet long instead of the  
ETX–90PE's compact 11” tube length.  
Eyepiece Focal Length is the distance light travels inside the eyepiece before  
reaching focus. Focal length is usually printed on the side of the eyepiece, for example,  
26mm. Low-power eyepieces are typically available in 26mm, 32mm and 40mm sizes  
(see OPTIONAL ACCESSORIES, page 42). The low-power eyepiece provided with your  
ETX is designed to provide a wide, comfortable field of view with high image resolution.  
Fig. 19: Meade Super  
Plössl eyepieces.  
Calculating Magnification: On a telescope, such as the ETX, different eyepiece focal  
lengths are used to achieve different magnifications, from low to high. A 26mm eye-  
piece yields 48X (“48-power”) on the ETX-90PE, 57X on the ETX-105PE and 73X on  
the ETX-125PE. A variety of powers may be obtained with the addition of optional eye-  
pieces as well as the #126 2X Barlow Lens which doubles the power of an eyepiece  
(see OPTIONAL ACCESSORIES, page 42). To calculate magnification, divide the focal  
length of the telescope’s optical tube by the focal length of the eyepiece. For example:  
Tip: If you plan on  
viewing using higher  
magnification eyepieces,  
first locate, center and  
focus the object using a  
low-power eyepiece  
(e.g., 26mm eyepiece).  
Then remove the low-  
power eyepiece and  
replace it with a higher-  
power eyepiece; the  
object should still be  
centered in the field of  
view. Objects are much  
easier to locate and  
center at lower powers;  
higher powers are  
Telescope Focal Length divided by Eyepiece Focal Length  
1250mm divided by 26mm  
= Power  
= 73X  
With Barlow: 73 x 2  
= 146X  
The eyepiece power or magnification is therefore 73X and 146X with the Barlow.  
Most observers should have 3 or 4 eyepieces plus the #126 2X Barlow to achieve the  
full range of reasonable magnifications possible with ETX models.  
ETX TIPS  
employed simply by  
changing eyepieces.  
Too Much Power?  
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  
beginning observer is to “overpower” a telescope by using high magnifications  
which the telescope 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. 20a and 20b). Powers  
above 300X should be employed only under the steadiest atmospheric  
conditions.  
AutoStar can calculate the best eyepiece for you to use. Try out the “Eyepiece  
Calc” feature in the Utilities menu.  
Fig. 20a & 20b: Jupiter: Examples  
of the right amount of  
Most observers should have three or four additional eyepieces to achieve the full  
range of reasonable magnifications possible with the ETX telescopes. See  
OPTIONAL ACCESSORIES, page 42.  
magnification and too much  
magnification.  
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OBSERVING  
Observing by Moving the Telescope Manually  
If you wish to observe a distant land object, such as a mountain top or a bird, you can  
observe by merely pointing the telescope and looking through the eyepiece.  
1. Loosen the telescope’s horizontal lock (9, Fig. 1a) and vertical lock (6, Fig. 1b).  
2. Move your telescope to observe distant street signs, mountains, trees and other struc-  
tures. Use the SmartFinder to help sight-in on an object.  
3. Center the object with SmartFinder’s red dot and then in the telescope  
eyepiece. When the object is centered in your eyepiece, remember to re-tighten the  
horizontal and vertical locks.  
4. Practice focusing objects using the focus knob (8, Fig. 1b).  
5. Once you get a feel for how your telescope moves and focuses, try to view  
something more challenging, like a bird or a distant moving train.  
Note:  
Viewing conditions vary  
widely from night-to-night  
and site-to-site. Turbulence  
in the air, even on an  
apparently clear night, can  
distort images. Low-power  
eyepieces, such as the  
26mm supplied with your  
telescope, are better suited  
to resolving images in poor  
viewing conditions.  
You can also observe stars and objects in the night sky using this method, but note that  
objects begin to slowly drift across the eyepiece field. This motion is caused by the rotation  
of the Earth. As you become familiar with the AutoStar handbox operation, you can coun-  
teract the drift using the automatic tracking feature (see TO TRACK AN OBJECT AUTO-  
MATICALLY, page 16) or by using AutoStar's GO TO capabilities (see GO TO SATURN,  
page 19).  
Terrestrial Observing  
ETX telescopes are excellent high-resolution terrestrial (land) telescopes. Viewing terres-  
trial objects requires looking along the Earth's surface through heat waves. These heat  
waves often cause degradation of image quality. Lower power eyepieces, like the 26mm,  
magnify these heat waves less than higher power eyepieces (such as a 9mm eyepiece).  
Therefore, lower power eyepieces provide a steadier, higher quality image. If the image is  
fuzzy or ill-defined, reduce to a lower power eyepiece, where the heat waves do not have  
such an effect on image quality. Observing in early morning hours, before the ground has  
built up internal heat, produces better viewing conditions than during late afternoon hours.  
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.  
Observing Using AutoStar Arrow Keys  
You may observe land and astronomical objects using AutoStar's Arrow keys to move the  
telescope.  
1. Tighten the horizontal (9, Fig. 1a) and vertical locks (6, Fig. 1b).  
2. Make sure that AutoStar’s coiled cord is connected to the computer control panel’s  
HBX port (C, Fig. 2).  
Do not look through the  
telescope's eyepiece  
while it is rapidly moving.  
Children should always  
have adult supervision  
while observing.  
3. Flip the Power Switch (A, Fig. 2) on the computer control panel to the ON  
position. A copyright message lights on AutoStar’s LCD display, followed by a warning  
not to look at the Sun. Press the AutoStar key prompted by the message when you are  
done reading. See page 9 to 11 for more information about AutoStar’s keys.  
4. A “Getting Started” message displays. Press ENTER to skip this message.  
5. AutoStar then displays: “Location Option: 1-Zipcode 2-City”. This option allows you to  
choose how you wish to enter the location of your observing site: you can enter your  
zip code or choose the site from a list of countries, states and cities.  
Important Note:  
AutoStar requests the  
Country/State, City and  
Telescope Model  
Press the number key “1” if you wish to enter by zip code. Then enter the five  
digits of the zip code of your observing site and press ENTER.  
information only the first  
time AutoStar is activated.  
Subsequently, AutoStar  
uses the location and  
model number you have  
chosen.  
Press the number key “2” if you wish to select your observing site from a list of coun-  
try, states and cities. First, use a Scroll key to cycle through the list of countries and  
states (listed alphabetically). Press ENTER when the correct location displays. Next,  
use a Scroll key to cycle through the list of cities (also listed alphabetically). Press  
ENTER when the closest city displays.  
6. Finally Telescope Models” displays. Using the SCROLL KEYS, cycle through the list of  
telescope models and press ENTER when your model displays.  
If you wish to change this  
information, use the  
"Telescope Model" and  
"Site" options in the Setup  
menu. See pages 27 and  
29 for more  
7. The display now displays "Align: Automatic."  
You can now use the ARROW KEYS to slew (move) the telescope up, down, right or left.  
Practice using the ARROW KEYS to center objects in the eyepiece.To change the speed  
at which the telescope moves (known as the “slew” speed), press a NUMBER KEY from 1  
through 9. 1 is the slowest speed and 9 is the fastest.  
information.  
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Slew Speeds  
AutoStar has nine slew speeds that move the optical tube at rates that are directly  
proportional to the sidereal rate and have been calculated to accomplish specific  
functions. Press the Number key to change the slew speed.  
The nine available speeds are:  
Number Key 1 =  
Number Key 2 =  
Number Key 3 =  
Number Key 4 =  
Number Key 5 =  
Number Key 6 = 128x =  
Number Key 7 = 1.0° =  
Number Key 8 = 1.5° =  
Number Key 9 = Max =  
1x =  
2x =  
8x =  
16x =  
64x =  
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  
60 arc-min/sec or 1.0°/sec  
90 arc-min/sec or 1.5°/sec  
approx. 4.5°/sec  
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 9mm eyepiece.  
Speeds 4, 5 or 6: Enable centering of an object in the field of a low-to-moderate  
power eyepiece, such as a 26mm.  
Speeds 7 or 8: Best used for rough centering of an object in the SmartFinder.  
Speed 9: Moves the telescope quickly from one point in the sky to another.  
Astronomical Observing  
Used as an astronomical instrument, your telescope has many optical and electro-  
mechanical capabilities. It is in astronomical applications where the high level of  
optical performance is readily visible.The range of observable astronomical objects is  
limited only by the observer’s motivation.  
Observe the Moon  
Point your telescope at the Moon (note that the Moon is not visible every night) and  
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 overly bright surface appear flat and  
rather uninteresting. Try using a neutral density Moon filter when observing the Moon  
(see OPTIONAL ACCESSORIES, page 42). Not only does it cut down the Moon's bright  
glare, but it also enhances contrast, providing a more dramatic image.  
Go To  
Mode  
Enter  
Arrow  
keys  
Number  
keys  
Help  
To Track an Object Automatically  
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 (follows) the  
stars and other objects in the night sky. If the telescope is not tracking an  
astronomical object, the object will drift out of the eyepiece field of view. The tracking  
function automatically keeps an object centered in the telescope’s eyepiece.  
Scroll  
keys  
Fig. 21: AutoStar keys.  
To automatically track objects, you need to learn how the AutoStar keypad operates  
in order to move through its menus. You'll also need to initialize and align your  
telescope.  
Moving Through AutoStar’s Menus  
Tip:  
The AutoStar database is organized in levels for quick and easy navigation.  
When multiple choices are  
available within an  
AutoStar Menu option, the  
current option is usually  
displayed first and high-  
lighted by a right pointing  
Press ENTER to go deeper into AutoStar's menu levels.  
Press MODE to move back toward the top menu level.  
Press the Scroll keys to move up and down through the options  
available for each level.  
Press the Arrow keys to enter characters and digits. The Arrow keys  
are also used to move the telescope.  
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Initializing AutoStar for the First Time  
Definition:  
Initialization is a  
This section describes how to initialize AutoStar. Perform this procedure the first time  
you use AutoStar or after performing a Reset (see RESET, page 28).  
procedure that makes sure  
that AutoStar operates  
correctly. When you first  
use AutoStar, it doesn't yet  
know where the  
observation location site is.  
AutoStar also needs to  
know the time and date,  
which is set at the factory  
and may also be reset  
using Meade’s optional  
Atomic Clock Update  
Module accessory.  
AutoStar will ask you to choose your observing location and your telescope’s model  
number from the list it displays.You will be prompted to enter this information only the  
first time you use AutoStar. If you wish to change your location information (or if  
AutoStar does not ask you for this information information the first time that you use  
it), go to the Site option of the Setup Menu to select your location. See pages 27 and  
29 for more information.  
1. Tighten the vertical and horizontal locks (6, Fig. 1b and 9, Fig. 1a) if necessary.  
2. Make sure that AutoStar is connected to the HBX port (C, Fig. 2) of the  
telescope’s computer control panel.  
3. Flip the telescope power switch (A, Fig. 2) to the ON position.  
AutoStar uses this  
The AutoStar screen displays a copyright message, followed by a short beep.  
Then AutoStar takes a few moments to start up the system.  
information (along with  
detecting tilt, level and  
North) to precisely  
calculate the location of  
celestial objects (such as  
stars and planets) and to  
move your telescope  
correctly for various  
operations.  
4. A message displays that warns not to look at the Sun. At the end of this message,  
press the key prompted by AutoStar to signify that the message has been read  
and understood.  
5. The Getting Started menu displays a scrolling message. Press ENTER (2, Fig.  
4) to bypass the Help tutorial and continue with initialization.  
6. AutoStar then displays: “Location Option: 1-Zipcode 2-City”. This option allows  
you to choose how you wish to enter the location of your observing site: you can  
enter your zip code or choose the site from a list of countries, states and cities.  
Note:  
Press the number key “1” if you wish to enter by zip code. Then enter the five  
digits of the zip code of your observing site and press ENTER.  
Throughout this manual,  
you will notice the term  
"alt/az." Alt/az is frequently  
used to refer to altitude  
(vertical) and azimuth  
(horizontal). Alt/az is just  
one of many methods used  
by amateur astronomers to  
help locate stars in the  
night sky.  
Press the number key “2” if you wish to select your observing site from a list of  
country, states and cities. First, use a Scroll key to cycle through the list of coun-  
tries and states (listed alphabetically). Press ENTER when the correct location  
displays. Next, use a Scroll key to cycle through the list of cities (also listed alpha-  
betically). Press ENTER when the closest city displays.  
7. AutoStar then requests the telescope model number. Use the Scroll keys to cycle  
through the database of models. Press ENTER when your model number dis-  
plays.  
Another method of  
alignment is called  
8. System initialization is complete and the screen reads "Align: Automatic."  
“Equatorial ” (also known  
as “Polar”). To learn more  
about equatorial alignment,  
see page 50.  
Automatic Alignment  
After initializing, AutoStar will automatically align your telescope for you. AutoStar is  
in the alt/az mode (see the margin Note to the left) by default the first time you  
power it on, so you do not need to select this mode. If you wish to align your telescope  
in the equatorial (polar) mode, see EQUATORIAL ALIGNMENT, page 50.  
During automatic alignment, you will be asked to set the telescope in the home  
position. Then AutoStar will automatically detect the level position and the tilt of your  
telescope, and also detects North (note that the telescope may not be pointing North  
after it does so).  
After finding North, AutoStar picks two stars from its database. AutoStar moves the  
telescope to the first alignment star and the user is asked to center the star in the  
eyepiece. The process is then repeated with a second star to complete the alignment.  
The following explains in detail how to perform the alt/az automatic alignment procedure.  
Fig. 22: The vertical lock.  
How to perform the Automatic Alignment procedure  
1. Set Home Position: AutoStar then prompts you to set the telescope in the Alt/Az  
Alignment home position. To set your telescope in the Alt/Az home position when  
using the Automatic Alignment menu:  
If necessary, tighten the telescope’s vertical lock (6, Fig. 1b).  
Unlock the horizontal lock (9, Fig. 1a). This will allow you to rotate the  
telescope tube and fork arm assembly.  
Fig. 23: The horizontal  
lock.  
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Grasp the telescope by  
counterclockwise until it stops (Fig. 24).  
a
fork arm and rotate the telescope  
Re-lock the horizontal (9, Fig. 1a) and vertical locks (6, Fig. 1b).  
2. Level, Tilt and Find North: Next your telescope begins to move. AutoStar  
moves your telescope so that it can calculate the level position and tilt of your tel-  
escope, and also calculate the location of True North. While it is performing these  
functions, the following messages will appear on AutoStar’s display: “Calc Level,”  
“Calc North” and “Calc Tilt.”  
Note: During this step in the procedure, the telescope may not become  
level or actually point to North. AutoStar is merely moving the  
telescope about so that it can calculate these positions.  
Fig. 24 [top view]: Rotate the  
telescope tube counterclock-  
wise until it stops.  
3 . Star Alignment: Next, AutoStar continues to move the telescope (you don’t need  
to press any buttons) in order to choose two stars for alignment. AutoStar will  
display a name of a star and the word “Slewing” as it moves to the first star. It will  
then prompt you to center the star.  
Important Note: The  
home position for  
Automatic Alignment is  
different than the home  
position used with One  
Star and Two Star Alt/az  
alignments. See page 36  
for setting the Home  
Position during One Star  
and Two Star Altaz  
However, when the telescope slews to the first star, it may not appear in the field  
of view in the eyepiece. Use the SmartFinder (2, Fig. 1a) to locate the star. The  
alignment star will be easy to recognize—it will be the brightest star in the area  
of the sky where the telescope is pointing. Look through the SmartFinder and use  
the Arrow keys to move the telescope until the star is visible. Then look through  
the eyepiece and center the star using the Arrow keys. Press ENTER. Repeat the  
procedure for the second alignment star.  
When the procedure is performed correctly, "Alignment Successful" displays. If  
AutoStar does not display this message, perform this procedure again.  
NOTE: The alignment stars may change from night to night. All that is  
required is for the observer to center the selected stars in the eyepiece  
when prompted.  
Alignment  
Star  
Observe a Star using the Automatic Tracking Feature  
In this example, the AutoStar Arrow keys are used to find a star and then AutoStar's  
tracking feature automatically keeps the star centered in your  
telescope's eyepiece. Make sure you have initialized and aligned your telescope  
before you try out this feature (see page 17).  
Fig. 25: During alignment, the  
alignment star is always the  
brightest star in the area of  
the sky at which the  
1. Once your telescope has been aligned, “Align Successful” and then “Select Item:  
Object” display. Push the Scroll Up key once and “Select Item: Setup” displays  
telescope is pointing.  
2. Press ENTER. “Setup: Align” displays.  
3. Press the Scroll Down key repeatedly until "Setup: Targets" displays. Press  
ENTER.  
Important Note:  
While performing the  
automatic tracking  
4. "Targets: Terrestrial" displays. Press one of the Scroll keys once. "Targets:  
Astronomical" now displays.  
procedure, only use the  
Arrow keys to move the  
telescope. Once the  
telescope has been  
aligned, do not loosen the  
telescope’s vertical or  
horizontal locks (6 and 9,  
Fig. 1a and 1b) or move  
the base manually or  
alignment will be lost.  
ETX TIPS  
Which One’s the Alignment Star?  
If you’re not familiar with objects in the night sky, 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  
smartfinder. When you view an alignment star in the SmartFinder, it stands out  
dramatically from the rest of the stars in that portion of the sky. The SmartFinder  
will help you locate a star more quickly than the eyepiece. Using AutoStar, set the  
slew speed to 6 (press Number key 6) or higher and use the Arrow keys to  
center the alignment star in the SmartFinder. If your SmartFinder 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, page 19.  
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5. Use the Arrow keys (5, Fig. 2) to locate a bright star in the night sky. Use the  
smartfinder (2, Fig. 1a) to help line up on the star. You may choose any unob-  
structed, 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  
necessary to once again center the star in the eyepiece. The tracking motors will  
then keep the star you have chosen in the center of the eyepiece.  
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 sometimes  
occurs during an alignment  
procedure.)  
6. Press and hold the ENTER key for a few seconds and then release to stop track-  
ing.You may repeat the procedure to locate another star or object using the Arrow  
keys. Then press ENTER to re-engage the tracking motors.  
Go To Saturn  
Press GO TO when the  
telescope stops slewing.  
The telescope begins to  
move in a spiral pattern at  
a very slow speed around  
the search area.When the  
object does become visi-  
ble, press MODE to stop  
the spiral search. Then use  
the Arrow keys to center  
After performing the Automatic Alignment procedure, the motor drive begins  
operating and the telescope is aligned for a night of viewing. Objects in the eyepiece  
will maintain their position even though the Earth is rotating beneath the stars.  
This exercise demonstrates how to select a celestial object, the planet Saturn, for  
viewing from AutoStar’s database.  
NOTE: Saturn is not visible the entire year and you may need to choose  
another object from AutoStar's database; however, the procedure, as  
described below, remains the same. If Saturn (or any other object) is not  
currently visible in the sky, AutoStar displays “Below Horizon.”  
1. After the telescope is aligned, “Select Item: Object” displays. If “Select Item:  
Object” is not displayed on your handbox, keep pressing MODE until it does  
display. Press ENTER.  
Important Note:  
2. “Object: Solar System” displays. Press ENTER.  
The first time you use your  
telescope or if you are  
experiencing any problems  
with pointing accuracy,  
follow the procedure  
described in APPENDIX  
C:TRAINING THE DRIVE,  
page 55, to insure accu-  
rate pointing and tracking.  
3. “Solar System: Mercury” displays. Keep pressing the Scroll Down key until “Solar  
System: Saturn” displays (or you may choose another object from the Solar  
System list if Saturn is not visible).  
4. Press ENTER. “Calculating” displays. Then “Saturn” and a set of coordinates  
displays. Note that Saturn’s (and other planets’) coordinates change throughout  
the year.  
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 moves the telescope so that it "tracks"  
Saturn (or whatever other object you may have chosen); i.e., Saturn remains  
centered in the eyepiece.  
Using the Guided Tour  
This example demonstrates using “Tonight’s Best” Guided Tour.  
1. After observing Saturn, press MODE twice so that “Select Item: Object” displays  
again.  
Tip: Try out the Guided  
Tour feature; the “Tonight’s  
Best” Guided Tour will  
point your telescope at the  
best objects visible in the  
sky for every given night of  
the year. The objects in this  
tour may change from  
night to night.  
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  
displays, 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.  
Tour objects are selected based on location’s time and date.  
You can easily create your  
own Guided Tour using the  
optional Meade’s AutoStar  
Suite software. See  
Press ENTER to display information about the object. Press GO TO to move the  
telescope to the object.  
PHOTOGRAPHY WITH  
MEADE’S AUTOSTAR  
SUITE, page 41 for more  
information.  
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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AUTOSTAR OPERATION  
OBJECT MENU  
SETUP MENU  
Automatic alignment  
permits all telescope  
operations with only  
minimal setup.  
Select Item:  
Object  
Want to see Mars? The Orion nebula?  
The Andromeda galaxy? Select from  
over 30,000 objects and press  
GO TO to move the telescope  
automatically to an object.  
Select Item:  
Setup  
Select Item:  
Event  
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.  
The Universe of  
Autostar  
Select Item:  
Utilities  
Select Item:  
Guided Tour  
GUIDED TOUR  
Autostar escorts you  
GLOSSARY  
What is an elliptical galaxy?  
on a tour of tonight's  
How far away is the Sun?  
best celestial objects  
at your viewing location.  
Expand your knowledge of  
astronomy by displaying terms  
and definitions, and other information.  
Select Item:  
Glossary  
Fig. 26: The AutoStar Universe: The six primary categories listed in the Select menu.  
It is important to understand that menu selections are set in a loop (Fig. 27a). This  
means that pressing the Scroll Down key cycles down through all the available options  
within a given category, then returns to the first option. The Scroll Up key 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:  
Fig. 27a: Menus set in a loop.  
1. Press the Scroll Down key four times or the Scroll Up key once.  
The screen in Fig. 27b shows two lines of information in the AutoStar display. The top  
line shows the current menu level. The second line displays an option which may be  
selected. Some options are submenus that offer more choices. The Scroll keys move  
up and down within the list of available options, showing one option at a time.  
Setup  
Align  
When an option is displayed on the second line, press the ENTER key to choose that  
option.  
Date  
Time  
Daylight Saving  
Telescope  
Targets  
etc.  
Press the MODE key to return back to the last menu.This can be useful to exit a menu  
or if the wrong menu option is chosen.  
IMPORTANT NOTE: No matter how many levels into AutoStar are trav-  
eled, each press of the MODE key moves up a level, until the top level,  
"Select Item," is reached. Once Select Item displays, press MODE to  
return to the topmost level, "Select Item: Object."  
Fig. 27b: Menu options display 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  
calculates Sunset time so an evening observing session can be planned.  
NOTE: To perform an accurate calculation, AutoStar MUST be properly  
initialized with the location of the observing site. See INITIALIZING  
AUTOSTAR, page 17, before proceeding with this exercise.  
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  
Tip:  
When multiple choices  
are available within a  
menu option, the current  
option is usually  
displayed first and  
highlighted by a right  
pointing arrow (>).  
ܖ
To enter numbers and text:  
a) Use the Number keys, or  
b) Use the Arrow keys to scroll through numbers 0 - 9 and the alphabet. The  
Down Arrow key begins with the letter "A;" the Up Arrow key begins with digit  
"9."  
ܖ
ܖ
To move the cursor across the display:  
Use the Right or Left Arrow key to move the cursor from one number to the next  
in the display.  
Press ENTER when the desired information has been entered.  
Moving Through AutoStar’s Menus  
AutoStar's menus are organized for quick and easy navigation:  
ܖ
ܖ
ܖ
ܖ
Press ENTER to go deeper into AutoStar's menu levels.  
Press MODE to move back toward the top menu level.  
Press the Scroll keys to move up and down through the options or lists.  
Press the Arrow keys to move the cursor across the display.  
ܖ
Press the Help (?) key to access on-line help.  
ETX TIPS  
Look into the Future  
The 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 menu or select an option in the Event menu.  
AutoStar, using the Event menu, 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 mini-  
mums of Algol.  
One very practical use of the Event menu is to check the Sunset option to  
determine when you can begin your astronomical observing session.  
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AUTOSTAR'S MENUS  
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Object Menu  
Use the OBJECT menu  
to select an object from the  
database.  
Almost all observing with AutoStar is performed using the Object menu category. (The  
two exceptions are the Guided Tours and Landmark Survey. See GOTO SATURN, page  
19, for an example of observing using the Object menu. Also see USING THE GUIDED  
)
When your telescope is  
aligned and you select an  
object from any of these  
lists, you just need to press  
the GO TO key to move the  
telescope so that it is  
pointed at the selected  
object.  
TOUR, page 19.  
Many AutoStar menu categories contain lists or databases. The AutoStar object data-  
base is a list of viewable objects, such as stars, planets, comets, nebulae and so forth.  
When one of these objects is selected from the object database and is above the hori-  
zon, AutoStar moves your telescope (if properly aligned) and points it at the selected  
object.  
Note: Most celestial objects are visible in the sky for only part of the night  
and also only visible part of the year. If an object is not visible on the night  
you are observing, AutoStar displays a message that the object is below  
the horizon.  
Over 30,000 objects are  
available for ETX-90PE,  
ETX-105PE and ETX-  
125PE models.  
The Object Menu options include:  
The available objects  
include planets,  
Solar System is a database of the eight planets (Earth is not included) in order out  
from the Sun, followed by the Moon, asteroids and comets.  
constellations, individual  
stars, double stars, star  
clusters, galaxies, quasars,  
satellites, asteroids and  
comets.  
Constellation is a database of all 88 Northern and Southern Hemisphere  
constellations. To use this menu:  
1. When this menu option is chosen and “Andromeda” displays, use the Scroll keys  
to scroll through the constellation list.  
2. Press ENTER to select a constellation and to display the coordinates of the con-  
stellation. Press one of the Scroll keys and information about the constellation will  
scroll across the display screen.  
3. Press GO TO to display the list of stars in the constellation. Use the Scroll keys  
to scroll through the list of stars in the constellation, from the brightest to  
dimmest.  
Also, try out the Guided  
Tour feature; the “Tonight’s  
Best” Guided Tour will point  
your telescope at the best  
objects visible in the sky for  
every given night of the  
year.  
4. Press ENTER to select a star and use the Scroll keys to display information about  
the star. Press GO TO again to slew the telescope to that star.  
Note: Use MODE to abort any of these operations.  
Deep Sky is a database of objects outside our Solar System such as nebulas, star  
clusters, galaxies and quasars.  
Star is a database of stars listed in different categories such as named, double,  
variable or nearby.  
Want to learn more about  
Observing Satellites? See  
page 32.  
Satellite is a database of Earth-orbiting objects such as the International Space  
Station, the Hubble Space Telescope, Global Positioning System (GPS) satellites and  
geosynchronous orbit satellites.  
User Objects allows the user to define and store in memory deep-sky objects of  
specific interest that are not currently in the AutoStar database. See page 30 for more  
information.  
Want to learn more about  
Landmarks? See page 34.  
Landmarks stores the location of terrestrial points of interest in the permanent  
AutoStar database.  
IMPORTANT NOTE: To use the Landmark function, the telescope must be  
located and aligned exactly as when the landmark was added to the  
database.  
ܖ
ܖ
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:  
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IMPORTANT NOTE FOR ALL ALIGNMENT-BASED OPERATIONS:  
Only use the Arrow keys to move the telescope during the Identify  
procedure. Do not loosen the telescope locks or move the base or the  
alignment will be lost.  
1. When a desired object is visible in the eyepiece, keep pressing MODE until the  
“Select Item: Object” menu is displayed. Press ENTER to select this menu.  
2. Scroll through the Object menu options until the “Object: Identify” screen appears.  
3. Press ENTER. AutoStar searches the database for the identity of the object being  
observed.  
4. If the telescope is not directly on an AutoStar database object, the nearest  
database object is located and displayed on the screen. Press GO TO and the  
telescope slews to that object.  
Browse allows you to search the database 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  
parameters of the search, select "Start Search" and press ENTER. AutoStar will  
display the results of the search.  
Want to learn more about  
using the Browse menu?  
See page 38.  
Use the Event menu  
Event Menu  
to look up dates of various  
astronomical events, such  
as sunrises and sunsets,  
eclipses, moon phases,  
meteor showers, equinoxes  
and solstices...  
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. See DATE, page 26 and also see ETX TIPS, page 21.  
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:  
Date” menu. See DATE, page 26 and also see ETX TIPS, page 21.  
...and not just for the  
current date. Set any date,  
past or future, when  
initializing AutoStar and  
you can check the time for  
other events.  
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.  
WARNING!  
Never use  
your ETX  
NOTE: Meteors are fast moving objects that cover large areas of the sky  
Telescope to  
and are usually best observed with the naked eye.  
look at the Sun! Looking  
at or near the Sun will  
cause instant and  
irreversible 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 at or near the  
Sun. Do not look through  
the telescope as it is  
moving. Children should  
always have adult  
Solar Eclipse lists upcoming Solar Eclipses, including the date and type (total,  
annular 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.  
Lunar Eclipse lists upcoming Lunar Eclipses, including the date and type (total,  
partial, 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  
second star is hidden. AutoStar calculates minimum magnitude time at mid-eclipse.  
supervision while  
observing.  
Autumn and Vernal Equinox calculates the time and date of the fall or spring  
equinox of the current year.  
Winter and Summer Solstice calculates the time and date of the winter or summer  
solstice of the current year.  
Use the Glossary menu  
to look up definitions of  
astronomical terms and get  
a description of AutoStar  
features.  
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  
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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:  
Use the Utilities menu  
to perform many of  
Timer selects a countdown timer.This feature is useful for functions such as astropho-  
tography and tracking satellites. See OBSERVING SATELLITES, page 30. To use the  
Timer, press ENTER, then choose “Set” or “Start/Stop."  
AutoStar’s useful features,  
such as setting an alarm,  
adjust the display contrast,  
calculate the best eyepiece  
for viewing an object, set  
up your own landmark  
survey, and so forth.  
ܖ
Set: Enter the time to be counted down, in hours, minutes and seconds, then press  
ENTER.  
ܖ
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."  
ܖ
ܖ
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.  
Tip:  
The Contrast Adjustment  
feature is usually only  
required in very cold  
weather.  
Eyepiece Calc calculates information about an eyepiece for the specific telescope to  
which AutoStar is connected.  
If you adjust the contrast  
so that you can no longer  
read the display, turn off  
the power and turn it on  
again. When Version  
appears on the display (the  
initial display screens are  
not affected by the  
ܖ
ܖ
ܖ
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.  
Contrast control), press  
MODE.  
Display Options enables or disables AutoStar’s two initial displays. If both displays  
are disabled, AutoStar begins with the Date display.  
ܖ
ܖ
Sun Warning: Turns the SUN WARNING message on or off.  
Getting Started: Turns the GETTING STARTED message on or off.  
Tips:  
To use the Landmark  
function, the telescope  
must be located and  
aligned exactly as when  
the landmark(s) was added  
to the database.  
Brightness Adj: Adjusts the brightness of the display using the Scroll keys. When  
complete, press ENTER.  
Contrast Adj: Adjusts the contrast of the display using the Scroll keys. When complete,  
press ENTER.  
NOTE: This feature is usually only required in very cold weather.  
To add objects to the  
Landmark database, the  
telescope must be located  
and aligned exactly as  
when the original objects  
were added to the  
Beep: Turns the beep on or off.  
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. See  
LANDMARKS, page 34, for information about creating a Landmark survey.  
database.  
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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  
activate 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, pressing ENTER and the telescope moves 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, when set to "On," 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 tangled as the telescope slews to objects. "Off" is the default setting.  
Setup Menu  
The Setup menu’s primary function is to align the telescope (see AUTOMATIC ALIGN-  
MENT, page 17). However, there are numerous other features available within the  
Setup menu, including:  
Use the Setup menu  
to perform many of the  
features that apply to the  
set up of your telescope,  
such as training the drive,  
selecting terrestrial or  
astronomical modes,  
changing observing site  
information.  
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 24.  
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 which follows 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  
various areas of the world. Check local time to verify.  
Telescope accesses the several options, including:  
ܖ
ܖ
ܖ
Model: Allows you to select the telescope model connected to AutoStar.  
Focal Length: Displays the focal length of the selected telescope.  
Az/RA Ratio and Alt/Dec Ratio: The ratios refers to the gears of the telescope's  
motors. Do not alter these numbers.  
ܖ
Az/RA Percent: The Az (Azimuth)/RA (Right Ascension) Percent allows you to  
adjust the amount of azimuth backlash taken out by AutoStar. Azimuth backlash  
is the way the Arrow keys move the telescope along the azimuth (horizontal) axis.  
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.  
ܖ
ܖ
Alt/Dec Percent: The Alt (Altitude)/Dec (Declination) Percent operates identical  
to the Az/RA Percent option (see above), but allows you to adjust the altitude  
backlash, i.e., the way the Arrow keys move the telescope when moving along the  
altitude (vertical) axis.  
Train Drive: Trains the Altitude and Azimuth motors to locate objects with more  
precision.  
The first time you use your telescope or if you are experiencing any problems with  
pointing accuracy, follow the procedure described in APPENDIX C: TRAINING THE  
DRIVE, page 55, to insure accurate pointing and tracking.  
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ܖ
Tracking Rate: Changes the speed at which the telescope tracks targets in the  
sky.  
a. Sidereal: The default setting for AutoStar; sidereal rate is the standard rate  
at which stars move from East to West across the sky due to the rotation of  
the Earth.  
b. Lunar: Choose this option to properly track the Moon over long observing  
sessions.  
c. Custom: Allows entry of user-defined tracking rates.  
ܖ
ܖ
ܖ
Reverse L/R: Reverses the functions of the Left and Right Arrow keys (i.e., the  
Right key moves the telescope to the left).  
Reverse UP/DOWN: Reverses the functions of the Up and Down Arrow keys  
(i.e., the Up key moves the telescope down).  
Calibrate Sensors: This menu allows you to improve your telescope's pointing  
accuracy to alignment stars. It calibrates to correct slight mechanical misalign-  
ment due to transport, vibration, or aging. It is recommended that calibration be  
performed after the LNT Module batteries are changed (see page 56 for more  
information).  
When this menu is selected, the telescope slews to Polaris. AutoStar then  
prompts you to center Polaris and to press ENTER. AutoStar uses the position of  
Polaris to fine tune the position of North and also for detecting level.  
ܖ
ܖ
Quiet Slew: Sets the maximum slew rate to 1.5° for quieter operation.  
Max Elevation: Allows you to enter a value in degrees that sets a limit as to how  
far the optical tube can swing upward during a programmed slew. (Note that it  
does not prevent you from performing a manual slew past this limit.) This is  
useful when you have a camera or other peripheral attached to the telescope—  
you can prevent it from striking the telescope base.  
ܖ
Min AOS (Acquisition of Signal): Allows you enter a value in degrees. This  
value represents the altitude at which your telescope begins to slew when  
acquiring a satellite track. This is useful when you are observing satellites, but a  
tall tree or building is obstructing the telescope. For example, you might begin to  
track the satellite at 15° altitude, instead of 5°. See OBSERVING SATELLITES,  
page 30, for more information about satellites.  
ܖ
ܖ
ܖ
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.  
Want to learn more about  
Periodic Error  
Correction? See page 37.  
Smart Drive: Allows you to perform periodic error correction (PEC) on the R.A.  
worm gear and can only be used with polar mounted telescopes. Must be  
performed with a high powered reticle (eg. 9mm). PEC Training for the the ETX  
telescopes will take about 24 minutes.  
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.  
Tip:  
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 and the  
telescope is aligned, the tracking motor is turned off. To learn how to track an object  
automatically, see page 16.  
Site provides access to several options including:  
ܖ
Select: Displays the currently selected observing site or zip code. Use the Scroll  
keys to cycle through all the sites. Press ENTER when the site you wish to select  
displays. Use  
this  
option  
when  
you  
move  
to  
a
different  
geographic location. The cities you have chosen or zip codes you have “added”  
will appear at the top of this list (see ADD below).  
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ܖ
Add: 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. Choose Zip  
Code to enter your zip code, if you wish. Choose “Custom” if you wish enter the  
name of an observing site. In this method, you will enter its name, plus its longi-  
tude and latitude. See the margin note on page 29 for more information.  
Want to learn more about  
adding and editing sites?  
See page 29.  
Time Zone  
Atlantic  
Eastern  
Central  
Mountain  
Pacific  
Shift  
Delete: Deletes a stored site from the database.  
-4 Hours  
-5 Hours  
-6 Hours  
-7 Hours  
ܖ
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 above.  
-8 Hours  
Alaska  
-9 Hours  
NOTE: AutoStar compensates for daylight savings time, if selected. See  
Hawaii  
-10 Hours  
“Setup Menu: Daylight Saving,page 26.  
Table 1: Time Zone Shift.  
Calculations are for standard  
time.  
Owner Info accesses the owner information menu, including:  
ܖ
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:  
ܖ
Address: Use the Up and Down Arrow keys to enter your street address, city,  
The Download function  
requires the optional #505  
Astrofinder Software and  
Cable Connector Kit. See  
the instruction sheet  
included with the kit for  
more information on how to  
download. Also see  
OPTIONAL ACCESSORIES,  
page 42.  
state and zip code. Press ENTER when the entry is complete.  
Download transfers information from another AutoStar. During the operation, the  
warning “Downloading Do Not Turn Off” appears.  
Clone uploads information from one AutoStar handbox to another. Three options are  
available:  
ܖ
ܖ
Catalogs: Sends only user-defined object information, such as new satellite  
orbits or comet data to another AutoStar handbox.  
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.  
ܖ
All: Everything – user-defined information and AutoStar software – is sent to  
another AutoStar.  
Statistics provides basic statistical data about AutoStar, including:  
ܖ
Characters Free: Shows how much room is available in user-defined object  
memory.  
ܖ
Version: Shows the current version of the AutoStar software.  
Reset completely resets AutoStar. Most values entered into the menus revert to  
factory defaults. AutoStar requires initialization again after a Reset before proceeding  
with observations. See INITIALIZING AUTOSTAR, page 17.  
ETX TIPS  
Join an Astronomy Club, Attend a Star Party  
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 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 with your ETX telescope. See page 40 for more information about photography  
with the ETX.  
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.  
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ADVANCED AUTOSTAR  
OPERATION  
Before trying out the examples in this section, familiarize yourself with the basic  
operations 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 AutoStar and have placed the telescope in the "Home"  
position (when appropriate).  
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. You are given a choice to enter a zip code (press “1”) or select a city from the list  
(press “2”). If you choose “Zip,enter the digits of your zip code and press ENTER.  
4. If you choose “City,” scroll through the list of countries/states. Press ENTER when the  
country/state you wish to add displays.  
5. Scroll through the list of cities. Press ENTER when the city you wish to select displays.  
The sites you choose will appear at the top of the Select list (all other available sites  
will be listed after the sites you have chosen).  
6. To choose a site, navigate to "Site: Select." Press ENTER. Scroll through the list of  
sites. Both Zip Codes and Cities are displayed. When the desired zip code or site  
displays, press ENTER.  
Note: You may also add a  
custom site to the list by  
choosing “Site: Select” and  
pressing Enter. Scroll down  
the list until “Custom”  
displays. Then add the  
name of your site and press  
ENTER. Enter the  
latitude of the site and  
press ENTER. Enter the  
longitude of the site. Press  
ENTER and you have  
created a custom site entry  
which you may select at  
any time from the “Site:  
Select” list.  
To Edit a Site:  
In this procedure, you will enter a location that is not available in the AutoStar database by  
editing data of  
a
nearby site. You will edit the location's name, latitude,  
longitude 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  
procedure. This information is available on most maps.  
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.  
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.  
Time Zone  
Atlantic  
Eastern  
Central  
Mountain  
Pacific  
Shift  
-4 Hours  
-5 Hours  
-6 Hours  
-7 Hours  
-8 Hours  
Alaska  
Hawaii  
-9 Hours  
-10 Hours  
Table 1: Time Zone Shift.  
Calculations are for standard  
time.  
10. After entering the shift, press ENTER. "Edit Time Zone" displays.  
11. Press MODE. "Site: Edit" displays.  
12. Using the Arrow keys, scroll to "Site: Select." The site you have just edited  
displays. Press ENTER to select the site or press MODE to exit.  
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Using AutoStar to Find Objects Not in the Database  
In this procedure, you will enter coordinates of celestial objects that do not appear in  
any of the AutoStar database lists.You will enter the object's name and R.A. and Dec.  
coordinates (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 the database. 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.  
coordinates of the object or objects you wish to observe. Check out your local library,  
computer store or bookstore for astronomy books, CD Roms or magazines (such as  
Sky & Telescope or Astronomy), to find coordinates of celestial objects. The  
objects/coordinates 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.  
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.  
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,  
simply 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.  
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  
display.  
4. Press GO TO and the telescope slews to the object.  
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.  
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3. Select a satellite from 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  
automatically 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  
telescope SmartFinder for the satellite to enter the field of view.  
10. When the satellite enters the SmartFinder field of view, press ENTER. The  
telescope starts to track with the satellite.  
11. Use the AutoStar Arrow keys to center the object in the SmartFinder, then look  
through the eyepiece to view the object.  
Satellite orbits change and new satellites (including the Space Shuttle) are launched.  
Visit the Meade web site (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 42.  
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.  
How to Create Your Own Guided Tour  
When a Guided Tour is selected, AutoStar slews your telescope to a predetermined list  
of objects and displays information about each object, such as type of object,  
constellation location, R.A. and Dec coordinates and so forth. AutoStar contains a few  
Guided Tours which are programmed at the factory. But it is also possible for an  
observer to create a custom Guided Tour.  
Note:  
Meade’s AutoStar Suite  
provides an easy way for  
an observer to create their  
own Guided Tour. See  
PHOTOGRAPHY WITH  
MEADE’S AUTOSTAR SUITE,  
page 41, and also  
OPTIONAL ACCESSORIES,  
page 42, for more  
A tour is basically an ASCII text file that contains a list of directions and descriptions.  
Each line of a tour is either a comment line, a command line or a description.  
What you will need:  
A PC with text editor or word processing software installed (the tour must be  
saved as a "text only" or as a "MS-DOS text" file).  
information.  
The Meade #505 Cable Connector Kit to download tour information to the AutoStar  
handbox.  
Tour Modes  
The objects chosen for a tour list are selected from AutoStar's database or by  
entering the object's RA and Dec coordinates. The tour is presented in one of two  
modes:  
Automatic Mode: The title of an object appears on the first line and descriptive text  
scrolls on line 2.  
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Interactive Mode: Tour name appears on the first line of the AutoStar display and the  
name of the object displays on line 2. To display descriptive text in this mode, the user  
must press ENTER.  
Comment Line  
Information in the Tour program that is not displayed, such as authorship, revision  
history, copyrights, etc. All comments begin with a "/" character in column 1 of the line.  
For example:  
/ Extreme Objects  
/ (c) 2000 Meade Instruments Corporation  
Command Line  
This line contains programming commands, including: R.A. and DEC. coordinates, a  
title string, a description string and a keyword.  
RA: Enter the Right Ascension of an object in the following format: HH:MM:SS.  
Eg., 18:51:05  
Dec: Enter the Declination of an object in the following format: DDdMMmSSs.  
Eg., – 06d16m00s  
Title String: Text within a title string is displayed as the title of the object. A title string  
can contain up to 16 characters and must be surrounded by quotation marks. For  
example. "M64" or "My Favorite Star."  
In Interactive Mode, the title string appears on line 2 until it is selected with the  
ENTER key.  
In Automatic Mode or after Interactive Mode selection, the title string appears on line  
1 while the description scrolls across line 2.  
Keywords: Action to be performed during a tour. AutoStar recognizes the following  
keywords:  
TITLE  
TEXT  
USER  
NGC  
IC  
SAO  
MOON  
LUNAR ECLIPSE  
STAR  
MESSIER  
SATELLITE  
METEOR SHOWER DEEP SKY  
LANDMARK DEFINE  
CALDWELL  
ASTEROID  
PLANET  
COMET  
CONSTELLATION  
PICK ONE/PICK END AUTO SLEW ON/OFF #END  
Description String: Description of an object. Must be surrounded by quotation  
marks. If the description is longer than one line, each line must end with a quotation  
mark and a hard return. Begin the next description line with a quotation mark.  
If quotation marks are to be displayed in the on-screen description, use two quote  
marks at the beginning and end of the desired phrase. For example: "The Orion  
Nebula is considered ""awesome"" by many who view it."  
Writing a Tour  
Using the list of commands listed above, a custom tour can be created. Placing the  
word AUTO SELECT before any of the command lines activates Automatic Mode and,  
when selected, AutoStar automatically searches and finds the designated object.  
The following is a list of command lines, complete with keywords and necessary  
strings:  
TITLE  
Title must be the first keyword in your tour after any comment lines and must be 15  
characters or less. AutoStar displays this title when "Guided Tour" is selected from the  
menus.  
For example: TITLE "A Star's Life"  
TEXT "title string" "description string"  
This command allows you to display a text title and description.  
USER ra dec "title string" "description string"  
This command line allows you to access a specific object with your own description.  
Enter USER, then the RA and DEC of a desired object and its title and description.  
Use the format described in the Command Line section.  
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The following commands specify objects that are already in the AutoStar database. If  
these commands follow the command AUTO SELECT, the object's title displays on  
line 1 and its description scrolls across line 2.  
Do not add a description string after the following command lines; these commands  
access objects with existing description in the AutoStar database.  
NGC xxxx  
Enter NGC followed by the desired New General Catalog number and AutoStar  
provides the user with a description of the object from its database. For example: NGC  
4256  
IC xxxx  
Enter IC followed by the desired Index Catalog number and AutoStar provides the  
user with a description of the object from its database. For example: IC 1217  
SAO xxxxxx  
Enter SAO followed by the desired SAO number and AutoStar provides the user with  
a description of the object from its database. For example: SAO 30200  
Messier xxx  
Enter MESSIER followed by the desired Messier number and AutoStar provides the  
user with a description of the object from its database. For example: M 101  
CALDWELL xxx  
Enter CALDWELL followed by the Caldwell number and AutoStar provides the user  
with a description of the object from its database. For example: CALDWELL 17  
PLANET "name"  
Enter PLANET and then the name of the desired planet in quotes. AutoStar provides  
the user with a description of the selected planet from its database. For example:  
PLANET "Pluto"  
MOON  
This command accesses information about the Moon from the AutoStar database.  
SATELLITE "name"  
Enter SATELLITE and then the name of the desired satellite in quotes. AutoStar  
displays information about the satellite from its database. For example: SATELLITE:  
"Intl Space Stn"  
ASTEROID "name"  
Enter ASTEROID and then the name of the desired asteroid in quotes. AutoStar  
displays information about the asteroid from its database. For example: ASTEROID:  
"Ceres"  
COMET "name"  
Enter COMET and then the name of the desired comet in quotes. AutoStar displays  
information about the comet from its database. For example: COMET: "Halley"  
LUNAR ECLIPSE  
If LUNAR ECLIPSE is part of the tour, AutoStar checks its database every time the  
tour is activated to see if a lunar eclipse is visible that evening. If no eclipse is visible,  
this option is skipped and the tour proceeds on to the next object.  
METEOR SHOWER  
If METEOR SHOWER is part of the tour, AutoStar checks its database every time the  
tour is activated to see if a meteor shower is visible that evening. If no meteor  
shower is visible, this option is skipped and the tour proceeds on to the the next  
object.  
DEEP SKY "name"  
Enter DEEP SKY followed by the name of the desired object in quotes. For example:  
DEEP SKY "Small Magellanic Cloud"  
CONSTELLATION "name"  
Enter CONSTELLATION followed by the name of the desired constellation in quotes.  
For example: CONSTELLATION "Leo Major"  
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STAR "name"  
Enter STAR followed by the name of the desired star in quotes. For example: STAR  
"Vega"  
LANDMARK az alt "title" "description"  
Enter the azimuth (az) for the desired object in the following format: xxxdxxmxxs. For  
example: 123d27m00s. Then enter the altitude of the desired object in the following  
format: xxdxxmxxs. Then enter the title string and description string in quotes. For  
example:  
LANDMARK 123d27m00s 57d20m20s "Landmark 1" "North corner of apartment  
building"  
PICK ONE / PICK END  
These two statements are used to surround a list of items that AutoStar can choose  
from during a tour. AutoStar begins at the top of the PICK ONE list and displays the  
first object from the list that is above the horizon and ignores the rest.  
This statement is useful for developing tours that can be presented year round. For  
each object type you wish to use to illustrate in your tour, pick 10 to 12 examples  
spaced across the range of right ascension. Bracket them by the PICK ONE / PICK  
END statements. One current example displays for the user. For example:  
AUTO SELECT TEXT "Globular Cluster" "Globular clusters are huge balls of stars."  
"They contain 50,000 to 100,000 stars and are located on the fringes of our""galaxy."  
PICK ONE  
AUTO SELECT MESSIER 13  
AUTO SELECT MESSIER 15  
AUTO SELECT MESSIER 92  
AUTO SELECT MESSIER 4  
AUTO SELECT MESSIER 68  
AUTO SELECT NGC 1234  
AUTO SELECT TEXT "None Available" "I'm sorry. There are no bright globular"  
"clusters visible at this time."  
PICK END  
AUTO SLEW ON / AUTO SLEW OFF  
With AUTO SLEW ON enabled in the tour, AutoStar automatically slews the telescope  
to objects first before displaying the text description. This feature is useful when  
designing tours in which observing certain objects is required. For example, an astron-  
omy professor may require his students to observe six objects, four of which AutoStar  
automatically slews to in a tour. The students would have to manually slew to the last  
two objects. He would then place AUTO SLEW ON before his first required object and  
AUTO SLEW OFF after the fourth object.  
#END  
To end a tour, type the command #END on a separate line at the very end of the tour.  
Downloading Tours  
Once a tour is written and stored as an ASCII file (saved either as a "text only" or "MS  
DOS text" file), load it into AutoStar using the AutoStar Update Utility on your PC. As  
tours are downloaded into the handbox, AutoStar examines the programming. If it  
doesn't understand the terminology used within a tour, it flags questionable areas and  
displays them in a pop-up window on your computer screen. Make the necessary  
corrections and try to download again. See the instruction sheet with your #505 Cable  
Connector Kit for more information about downloading data to and interfacing with  
AutoStar.  
Landmarks  
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.  
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To Add a landmark to the database:  
In this procedure, you will store the location of terrestrial landmarks in AutoStar's  
memory.  
1. Set the telescope in the home position, if necessary. Note for future reference  
where the telescope is located and if you have aligned the telescope, which  
alignment method is used.  
Important Note: To use the Landmark function, the telescope must be  
located and aligned exactly as when the landmark(s) was added to the  
database.  
2. Display the "Setup: Targets" menu option. Choose "Terrestrial" and press ENTER  
– "Setup:Targets" displays again. Choosing this option turns off tracking for astro-  
nomical objects and 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 man-  
ually move the telescope), move the telescope to the desired landmark and cen-  
ter the object in the eyepiece. Press ENTER. The object is now stored in memo-  
ry.  
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  
landmark 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 option—note that the Landmark Survey will function only if you have  
previously entered objects in the Landmark menu.  
1. Navigate to "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 amount of memory in AutoStar.  
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.  
Identify  
This procedure allows you to use AutoStar to identify objects you have found in the  
night sky using the Arrow keys. If the object is not in AutoStar's database, AutoStar  
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displays information about an object in its database that is closest to the one you  
queried about.  
IMPORTANT NOTE: For this function to operate properly, you must first  
set the telescope in the home position and initialize AutoStar. If you  
physically move the telescope after initialization, this function will fail to  
operate properly.  
In this procedure, you will center an object you wish to have identified by AutoStar in  
the telescope eyepiece and use the "Identify" menu to find out information about the  
object or the nearest object to it in the AutoStar database.  
1. Center the object you wish to have identified in the telescope's eyepiece.  
2. Navigate to the "Object: Identify" option and press ENTER.  
3. "Searching..." displays. When AutoStar finishes calculating, the name of the  
closest object displays.  
4. Press a Scroll key to display information about this object. AutoStar displays  
some or all the following information about the object with each press of a Scroll  
key:  
Displayed information:  
Catalog or common name of object  
Type of object  
Right Ascension  
Declination  
Example:  
Messier 107, NGC6171 orion Nebula, etc  
Globular Cluster, Nebula, Black Hole, etc.  
16:32:4  
13°03'  
Constellation  
Magnitude  
Virgo orion, etc.  
3
Size  
2'  
Scrolling message  
"This Globular Cluster is 10,000 light  
years away...."  
Advanced Alt/Az Alignment  
If you would rather choose your own alignment stars from the AutoStar database  
during the Alt/Az alignment procedure, AutoStar offers additional alignment methods.  
Information for Equatorial (Polar) alignment is discussed in APPENDIX A, page 50.  
In order to perform either Two-Star, Easy Align or One-Star Alt/az alignment, you will  
first need to put the telescope in the home position:  
If necessary, tighten the telescope’s vertical lock (6, Fig. 1b).  
Unlock the horizontal lock (9, Fig. 1a). This will allow you to rotate the  
telescope tube and fork arm assembly.  
Fig. 29a [top view]: Rotate the  
telescope tube counterclock-  
wise until it stops.....  
Grasp the telescope by  
a
fork arm and rotate the telescope  
counterclockwise until it stops (Fig. 29a).  
Turn the telescope clockwise about a quarter of a turn (Fig. 29b). until a fork  
arm is directly over the computer control panel (Fig. 29c).  
Re-lock the horizontal (9, Fig. 1a) and vertical locks (6, Fig. 1b).  
Two-Star Alt/Az Alignment and Easy Align  
Two-Star Alignment requires some knowledge of the night sky. AutoStar provides a  
database of bright stars and two stars from this database are chosen by the  
observer for alignment (Easy Align operates the same as Two-Star Alignment, except  
that AutoStar picks the two alignment stars from its database).  
Fig. 29b [top view]: ....then  
rotate it clockwise a quarter  
turn.....  
1. Perform steps 1 and 2 as described in AUTOMATIC ALIGNMENT, page 17.  
2. With "Align: Easy" displayed, use the Scroll keys to display "Align: Two Star."  
Press ENTER. (If you wish to use Easy Align, press ENTER when “Align: Easy”  
displays.)  
3. Place the telescope in the home position as described in the AUTOMATIC  
ALIGNMENT procedure. When you have finished, press ENTER.  
4. "Select Star" displays. AutoStar then displays a database of stars for the  
observer to choose from. Use the Scroll keys to scroll to a star on the list that you  
wish to align upon. Select a star that you can easily locate in the night sky. Press  
ENTER.  
5. The telescope slews to the star. Use the Arrow keys to move the telescope until  
the star is centered in the eyepiece. Press ENTER.  
6. Repeat procedure for the second alignment star. The telescope is aligned and  
you are now ready to use AutoStar's GO TO capabilities for a night of observing.  
Fig. 29c [side view]: ....until a  
fork arm is over the computer  
control panel.  
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One-Star Alt/Az Alignment  
One-Star Alignment requires some knowledge of the night sky. AutoStar provides a  
database of bright stars. One-Star Alignment is identical to Two-Star Alt/Az: Alignment  
(see TWO-STAR ALT/AZ ALIGNMENT, above), except only one star from this database  
is chosen by the observer for alignment.  
IMPORTANT NOTE: The accuracy of One-Star Alt/Az Alignment, unlike  
the Two-Star and Easy (Alt/Az) Alignment procedures, depends on how  
well the observer levels the telescope and how close to North the tele-  
scope is pointed when setting the Home Position. Because the other  
methods use two stars to align upon, they are more precise than One-  
Star Alignment.  
Want to learn more  
about Parking your  
telescope? See page  
26.  
Smart Drive Training (Periodic Error Correction)  
If you wish to improve the gear performance on your telescope, first, perform the train  
the drive procedure (see page 55).Then use the Periodic Error Correction (PEC) Train  
menu option to remove the slight perturbations from center that occur due to the  
mechanical nature of a telescope. To perform this procedure, you need to use a high-  
power reticle eyepiece, such as the 9mm reticle (see OPTIONAL ACCESSORIES, page  
42).  
Important Note: In order for the PEC training to operate and be updated  
properly, you must “park” the telescope to maintain PEC (see PARK  
SCOPE, page 26, for more information).  
PEC Train Menu Option  
To perform the procedure on the R.A. axis, pick a bright star in the South that has  
minimal movement and is about 30° above the horizon (Note: If in the Southern  
hemisphere, pick a star in the North that is about 30° above the horizon). This  
procedure takes about 24 minutes for the ETX Premier telescopes.  
Important Note: The Train option overwrites any previous PEC data.  
1. Select "PEC Train" from the Smart Drive menu (in the "Setup: Telescope" menu)  
and press ENTER.  
ETX TIPS  
Observing Considerations  
Try to pick an observing site away from street and house lights and car  
headlights. 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  
flashlights, the red utility light on the AutoStar handbox or tape red cellophane  
over their flashlights to use for setup and map reading so they don’t have to  
continually 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  
telescope while someone is observing!  
Dress warmly. It gets chilly when you’re 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 optional higher power eyepieces, such as a  
9mm eyepiece (see OPTIONAL ACCESSORIES, page 42 for more details), when  
you wish to view something up close, such as craters on the Moon or the rings  
of Saturn.  
Bring your instructions manual along with you when you observe. Become  
familiar with its layout, so it will be easier for you to look up information with just  
a (red) flashlight.  
Invite your friends and family to come and observe with you. But practice  
locating 3 or 4 objects to show them beforehand; if you have long delays, they  
will become bored and lose interest. Also, demonstrate how to focus the  
telescope in a well-lit area before you go to to the observing site.  
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2. Look through the reticle. Use the Arrow keys to keep the star centered in the reticle  
cross-hairs. AutoStar displays a count of the 150 positions of the worm gear. When  
the count reaches 150, one cycle is complete. A full cycle takes about 24 minutes.  
3. Press MODE to exit.  
PEC Update Menu Option  
PEC Update does not overwrite the data, but updates the training using information  
gathered from both the last and the current training sessions. Press the MODE key to  
exit from this option. If you wish to further refine your training, select this menu again  
and repeat the procedure.  
PEC Erase Menu Option  
Select this option to erase all PEC training data.  
Browse  
This menu allows you to search the database for objects with certain parameters,  
much like a search engine. The "Edit Parameters" option lets you set various  
parameters for the search and "Start Search" activates the search. A typical search  
might be performed as follows:  
1. Select "Browse" from the Object menu. Press ENTER. "Browse: Start Search"  
displays.  
2. Press one of the Scroll Keys and "Browse: Edit Parameters" displays. Press  
ENTER.  
3. "Edit Parameters: Largest (mins)" displays. "Mins" stands for arc-minutes. Press  
ENTER.  
4. "Largest (mins)" and a value displays. Using the Number keys, enter a size in  
arc-minutes. AutoStar will search for objects up to this size and no larger. Press  
ENTER.  
5. "Edit Parameters: Largest (mins)" displays again. Press the Scroll Down key. "Edit  
Parameters: Smallest (mins)" displays. Enter the value for the smallest size of an  
object that AutoStar will search for in the database. Continue with "Brightest,"  
Faintest," and "Minimum Elevation," using the procedure described in steps 3 and  
4.  
6. After "Minimum Elevation," "Object Type" displays. Press ENTER." "+Black Hole"  
displays.If you do not wish to have "Black Holes" in your search, press ENTER  
and the "+" changes to a "–." Press the Scroll Down to scroll to the next item.  
"+Diffuse Nebula" displays. Continue to scroll through the list and press ENTER  
if you wish to change the "+" to a "–" or vice-versa.  
7. After you have scrolled to the last item on the "Object Type" list, press MODE  
twice and the Scroll Down key once. "Browse: Start Search" displays. Press  
ENTER. "Start Search: Next" displays. Press ENTER. AutoStar searches the  
database and displays the first object that matches the search parameters you  
have entered. Use the scroll keys to display information about the object. Press  
MODE and "Start Search: Next" displays again. Press ENTER and the next item  
matching the parameters displays. Repeat this procedure to display all the  
objects.  
8. Press MODE repeatedly to leave this menu.  
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PHOTOGRAPHY  
7
2
1
3
5
4
6
Fig. 30: Example of photography through the ETX using the #64 T-Adapter: (1) Short  
section of #64 T-Adapter; (2) Extension section of #64 T-Adapter; (3) Knurled attachment ring;  
(4) T-mount; (5) Flip-mirror control in “up” position; (6) 35mm camera body; (7) Format 1.  
Photography with a 35mm Camera  
Photography through your ETX model requires the addition of the optional #64  
T-Adapter (see OPTIONAL ACCESSORIES, page 42). With the #64 T-Adapter attached  
to the telescope (Fig. 30), through-the-telescope photography is possible with any  
35mm camera body with a removable lens. In this way the telescope effectively  
becomes the lens of the camera.  
Fig. 31a: Flip mirror control in  
the “up” position.  
For through-the-telescope photography, turn the flip-mirror control (5, Fig. 30) to the  
“down” position, allowing light to pass straight through the telescope and out the photo  
port (Figs. 31a and 31b). With the flip-mirror control in the “down” position and the  
photo port’s dust cover removed, you can see the front lens of the telescope when you  
look through the photo port. The #64 T-Adapter threads onto the photo port, followed  
by a T-mount for the particular brand of 35mm camera being used, followed by the  
camera body (with the camera lens removed).  
The #64 T-Adapter consists of two sections (1 and 2, Fig. 30), which are threaded  
together in shipment. You may use either of the following photographic mounting  
formats to couple the camera body to the telescope’s photo port thread.  
Fig. 31b: Flip mirror control in  
the “down” position.  
• Format 1: Camera Body + T-Mount + Section (1) of the #64 T-Adapter (7, Fig. 30).  
ETX-90PE  
ETX-105PE  
ETX-125PE  
1250mm at f/13.8  
1640mm at f/15.6  
1900mm at f/15  
Format 1 utilizes only the short section of the #64 T-Adapter to permit close-coupling  
of a camera body to the telescope. In this format vignetting will occur; the  
photographic image will appear on film with a slight darkening at the corners of the  
35mm frame (see Fig. 32a).  
Fig. 32a: Example of a format  
1 photo.  
• Format 2: Camera Body + T-Mount + Sections (1) and (2) of the #64 T-Adapter (see  
Fig. 30).  
ETX-90PE  
ETX-105PE  
ETX-125PE  
1450mm at f/16  
1830mm at f/17.4  
2310mm at f/18  
Format 2 utilizes both sections of the #64 T-Adapter threaded together to form a rigid  
unit. In this configuration there is no field vignetting; images are illuminated to the  
edges of a standard 35mm frame (see Fig. 32b).  
Fig. 32b: Example of a format  
2 photo.  
To frame an object in the viewfinder of the 35mm camera body, slightly loosen the  
knurled attachment ring (3, Fig. 30), which threads the #64 T-Adapter to the  
telescope’s photo port; rotate the camera body to achieve proper framing of the  
object; then re-tighten the knurled ring.  
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Photography through a long lens, such as the ETX, requires special technique for  
good results.The photographer should expect to use several rolls film in acquiring this  
technique. Long-lens photography has its own rewards, however, which short-focus  
lenses cannot duplicate.  
A Few Tips on Photography  
1.Use the standard tripod or the optional table tripod ( see OPTIONAL ACCESSORIES,  
page 42) as a platform for the telescope. At effective focal lengths of 1250mm to  
1450mm (ETX-90PE), 1640mm to 1830mm (ETX-105PE) or 1900mm to 2310mm  
(ETX–125PE), even small external vibrations can easily ruin an otherwise good  
photo.  
Caution: With the #64 T-Adapter and a camera body mounted to the ETX  
photo port, the telescope can be rotated vertically only 45°. Moving past  
this point may damage the telescope and camera.  
2. Use a cable-operated shutter release with your camera. Touching the camera body  
to operate the shutter will almost certainly introduce undesirable vibrations.  
3. Focus the image with extreme care. While observing the subject through the  
camera’s reflex viewfinder, turn the ETX's focus knob (8, Fig. 1b) 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  
recommended.  
4. 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 an ETX model may have an exposure meter  
that is still active when the standard lens is removed and the body is  
connected to the telescope with the T-mount. If used for terrestrial  
photography, the camera meter should be acceptable. If used for  
astrophotography, the meter probably will not provide good results since  
camera meters are not made to compensate for a dark sky.  
5. Terrestrial photography through an ETX model is sensitive to heat waves rising  
from the Earth’s surface. Long distance photography is best accomplished in the  
early morning hours before the earth has had time to build up heat.  
6. Photography of the Moon and planets through an ETX model can be especially  
gratifying, but points 1 through 4 should be particularly noted in this case. Lunar or  
planetary photography requires that the telescope be polar aligned (see  
EQUATORIAL (POLAR) ALIGNMENT, page 50).  
Note: Long-exposure photography of deep-sky objects is not practical with  
an ETX model, since this type of photography requires special electronic  
and optical guiding devices not available for this telescope.  
Photography with a Digital Camera  
Although digital cameras still cannot match the quality of images provided by  
traditional 35mm cameras, they provide some significant advantages to the casual  
astrophotographer: You do not have to develop the images (instant images), lower  
costs, computer and internet readiness. And because unwanted photos are easily  
discarded, they provide the freedom to experiment.  
Digital cameras present some problems for the astrophotographer: Many models  
have lenses that cannot be removed, difficulties in attaching to a telescope, possible  
vignetting, lack manual focusing and shorter exposure times.  
Shorter exposure times is one of the biggest drawback. Long exposures with digital  
cameras introduce undesirable noise and artifacts into a digital image. This limits the  
range of astro images to the Moon, planets and bright stars.  
Some tips for better photos:  
If you cannot remove the lens to your camera, look for a commercially available  
digital t-adapter. New solutions for attaching a digital camera to a telescope are  
becoming available as time goes by.  
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If the camera is not directly coupled to the eyepiece, keep it as close to the  
eyepiece as possible and center the image to be photographed to minimize  
vignetting (darkening of the edges of the photo).  
Try to block ambient light (from street lights, house, etc.) from the eyepiece and  
the camera with a piece of cardboard, a screen, etc.  
Keep extra (charged) batteries on hand for your camera as digital cameras often  
drain batteries in a short period of time. Rechargeable Lithium batteries provide  
power for a longer period than non-rechargeable batteries. If practical, use an AC  
adapter.  
Avoid short-focus eyepieces. They present many difficulties for digital cameras.  
If using manual focus, set to infinity. Otherwise, using the camera's autofocus is  
OK.  
Experiment with your camera's exposure, brightness and /or contrast settings.  
Keep notes for future reference.  
Clean eyepieces and camera lens as needed.  
Many digital cameras have a manual ISO setting. Short exposures times work the  
best.  
Use your camera's highest image quality and lowest compression settings.  
Although this fills up your camera's memory more quickly, it produces the best  
quality photos.  
Use the camera's timer or remote shutter release (if available for your camera) to  
minimize vibration. Wireless shutter releases may be available for some model  
digital cameras. If you do not have  
a
shutter release, use the  
camera’s timer (sometimes called “self-timer”), which is available with most  
digital cameras. The timer may also minimize vibration.  
Photography with Meade’s AutoStar Suite™  
The AutoStar Suite with Meade LPI™ (Lunar Planetary Imager) or Meade Deep Sky  
Imager™ turns your Meade ETX telescope, AutoStar and PC into even more powerful  
and easy-to-use astronomical instrument.  
LPI (Fig. 34) and Deep Sky Imager (Fig. 33) combine the power of an electronic  
astronomical imager with the simplicity of a web cam. Check out the following imager  
features:  
• Achieve great results the first time out on the Moon, planets, brighter deep-sky  
objects and terrestrial targets.  
• Easy to use with real-time display of object on your PC screen. Just center, focus  
and shoot.  
Fig. 33: The Deep Sky Imager.  
• Magic Eye software-assisted focusing.  
• Automatic and manual exposure control from .001 to 15 seconds (up to 450x longer  
than web cams).  
• Automatically takes multiple exposures.  
The AutoStar Suite Software includes powerful tools to help you get the most from  
your Meade ETX telescope:  
• Sophisticated planetarium program with over 19 million objects.  
• Select objects from the planetarium display and the telescope slews to those  
objects.  
• Create time-lapse movies of objects, such as Jupiter  
• Create your own Guided Tours.  
Fig. 34: The Lunar Planetary Imager.  
• Advanced Image Processing Software including Unsharp Masking, Convolution  
Filtering and many other features.  
• Control all AutoStar functions from your PC.  
Talking Telescope software translates AutoStar text to synthesized speech through  
PC speaker.  
• Includes a cable to connect your ETX model to your PC.  
See the CD Rom that is included with AutoStar Suite for more information and instruc-  
tion manual.  
41  
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OPTIONAL ACCESSORIES  
A wide assortment of professional Meade accessories are available for the for ETX  
telescopes. Meade accessories greatly extend many important applications to the  
telescope, from low-power, wide-field terrestrial viewing to high-power lunar and  
planetary observing. The premium quality of these accessories is well-suited to the  
quality of the instrument itself.  
Meade telescopes and accessories, including optional accessories for ETX  
telescopes, are available at more than 3,000 dealer locations in the U.S. and Canada  
and through Meade international distributors worldwide. Once you have identified the  
accessories you wish to order, contact your local Meade authorized dealer. To find a  
dealer near you call (949) 451-1450 or visit the Meade website at www.meade.com.  
#505  
Cable  
Connector  
Kit:  
With  
Meade  
AstroFinder  
software loaded into your PC, AutoStar-equipped ETX–90PE, ETX-105PE, and ETX-  
125PE telescopes may be remotely controlled from the PC display. The #505 Cable  
Connector Set, permitting connection of ETX, AutoStar and PC, is included with each  
AstroFinder package.  
Eyepieces: For higher and lower magnifications, Meade Super Plössl (SP) and  
Super Wide Angle (SWA) eyepieces (Fig. 35), as well as the Series 4000 8mm to  
24mm Zoom eyepiece, yield high-resolution imaging with all ETX telescope models.  
A useful selection includes the SP 9.7mm, SP 12.4mm and SWA 16mm. Under good  
seeing conditions, Meade Series 5000 Ultra Wide Angle 4.7mm and 6.7mm eyepieces  
present the widest obtainable fields of view at high powers and are well suited for  
observing the Moon and planets (other eyepieces are available in this series). Powers  
obtained with each eyepiece are shown in the following table.  
ETX-90PE  
ETX-105PE  
ETX-125PE  
Eyepiece  
Power 2x Barlow  
Power 2x Barlow Power 2x Barlow  
SP 6.4mm  
SP 9.7mm  
SP 12.4mm  
SP 15mm  
SP 20mm  
SP 26mm *  
SP 32mm  
SP 40mm  
195X  
129X  
101X  
83X  
63X  
48X  
390X  
258X  
202X  
166X  
126X  
96X  
230  
152  
119  
98  
74  
57  
459  
303  
237  
196  
147  
113  
92  
297X  
196X  
153X  
127X  
95X  
73X  
59X  
48X  
594X**  
392X  
306X  
253X  
190X  
146X  
119X  
96X  
Fig. 35: Optional  
Eyepieces yield higher and  
lower magnifying powers.  
39X  
31X  
78X  
62X  
46  
37  
74  
Barlow  
SWA 16mm  
SWA 20mm  
SWA 24mm  
78X  
63X  
52X  
156X  
126X  
104X  
92  
74  
61  
184  
148  
122  
119X  
106X  
79X  
238X  
211X  
158X  
UWA 4.7mm  
UWA 6.7mm  
266X  
187X  
N/A  
374X **  
313  
219  
N/A  
439**  
404X  
284X  
N/A  
567X**  
*
Included as standard-equipment with the ETX models.  
** Use these eyepieces only under extremely steady atmospheric conditions.  
Fig. 36: Use the #126 2x  
Barlow Lens to double the  
magnification of the  
#126 2x Barlow Lens: An amplifying lens, the multi-coated #126 2x Barlow (Fig. 36)  
doubles the power of all eyepieces with which it is used. Insert the #126 into the  
telescope’s eyepiece holder first, followed by an eyepiece. Example: By itself, the  
26mm eyepiece yields a power of 73X with the ETX-125PE; when used with the #126  
2x Barlow Lens, this eyepiece yields 146X.  
eyepiece employed.  
#64 T-Adapter: The basic means of photography through any ETX Astro telescope,  
the #64 T-Adapter threads to the rear cell of the telescope, followed by a T-Mount  
appropriate to the user’s brand of 35mm camera. In this way, the camera body is  
rigidly coupled to the telescope's optical system, which in effect becomes the cam-  
era's lens (see PHOTOGRAPHY, page 38).  
Fig. 37: #825 Right-Angle  
Viewfinder.  
42  
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#932 45° Erecting Prism: All ETX models include an internal optically-flat mirror to  
reflect light to the telescope’s 90° astronomical observing position. In this position the  
telescope’s image is upright, but reversed. For terrestrial observing with an ETX  
model, the #932 Erecting Prism (Fig. 38) correctly orients the eyepiece image and  
provides a convenient 45° observing angle.  
#774 Hard Carrying Case (for the ETX-90PE), #776 Hard Carrying Case (for the  
ETX-105PE) and #775 Hard Carrying Case (for the ETX-125PE): For secure  
portability of ETX Astro Telescope models in the field, Meade hard carrying cases (Fig.  
39) are fully lined with fitted foam inserts. They accept the complete ETX Astro  
Telescope plus optional accessories.  
Fig. 38: The #932 45°  
Erecting Prism.  
#765 Soft Carry Bag:The Meade soft-padded carry bag (Fig. 40) is well suited to trav-  
el with the ETX-90PE Astro Telescope. Each carry bag includes a shoulder strap and  
permits ready transport of the complete telescope, including accessories.  
Power Adapters and Cords: In addition to their internal battery packs, ETX-90PE,  
ETX-105PE, and ETX-125PE telescopes may be powered from standard 115vAC  
home electricity with the #541 AC Adapter. The #541 plugs into any standard home  
outlet and includes a 25 ft. cord connecting to the telescope’s control panel. Input  
voltage to the telescope is 12vDC. Alternately, an ETX telescope may be powered in  
the field from an automobile cigarette lighter plug by using the #607 Power Cord, a  
25-ft. cord that plugs into the telescope’s control panel and supplies 12vDC directly  
from the car battery.  
Fig. 39: #774 Hard  
Carrying Case shown with  
an ETX-90PE.  
#1244 Electric Focuser (for the ETX-90PE and ETX-105PE) and #1247 Electric  
Focuser (ETX-125PE): Meade-engineered for smooth, rapid focusing with any  
ETX model, each electric focuser (Fig. 41) includes coarse and micro-fine speeds.The  
standard-equipment hand controller accepts one (user-supplied) 9-volt battery and  
focuses the ETX telescope. On the ETX models, the focuser plugs into and is  
powered by, the telescope’s control panel, with operation effected through either the  
AutoStar or the optional #497 AutoStar Computer Controller.  
Fig. 40: The #765 Soft  
Carry Bag for the  
ETX-90PE.  
#887 Advanced Field Tripod for the ETX-105PE or ETX-125PE: For extra stability in  
sensitive applications of the ETX-105PE or the ETX-125PE even at the highest mag-  
nifications, the fixed height #887 Tripod permits either altazimuth or  
equatorial orientation of the telescope for astronomical or terrestrial observing. The  
#887 includes an equatorial wedge for polar alignment. The tripod's 2"-diameter steel  
legs collapse for easy transport in the field.  
Series 4000 Plössl 9mm Illuminated Reticle Eyepiece: The most advanced com-  
mercially-available illuminated reticle eyepiece, this Series 4000 Plössl 9mm model,  
powered by an internal battery, includes micrometric x-y positioning controls which  
greatly facilitate locking onto the guide star:Turn the finely-threaded controls and place  
the reticle’s crossline pattern precisely at the desired position in the field. The sharp,  
high-power imaging of the 4-element, multi-coated Plössl optical system is comple-  
mented by a rubber eyecup (foldable for eyeglass wearers) that shuts out distracting  
stray light from the observer’s eye. The upper (lens) section of the eyepiece rotates on  
a fine thread for precise diopter adjustment to the user’s eye. Reticle pattern is a dou-  
ble crossline with two concentric circles.  
Fig. 41: #1244 Electric  
Focuser.  
Deep Sky Imager: This high-performance, easy-to-use and affordable color CCD  
camera (Fig. 42) suppresses electronic noise and does not compress data from the  
sensor to increase picture quality. The Deep Sky Imager uses a full 16-bit analog-to-  
digital converter to enhance picture depth, contrast and dynamic range. It is USB com-  
patible for easy interface with most Windows-based laptop computers. Includes  
AutoStar Suite which automatically sorts, aligns and combines the best images, result-  
ing in a highly detailed color image.  
Fig. 42: Meade Deep Sky  
Imager  
Atomic Time Update Module: For use with all Meade ETX Premier Edition  
telescopes, this optional accessory allows you update the LNT Module with the time  
signal from the NIST atomic clock in Fort Collins, Colorado.  
43  
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MAINTENANCE  
Your ETX model telescope is a precision optical instrument designed to yield a  
lifetime of rewarding observations. Given the care and respect due any precision  
instrument, the telescope will rarely require factory servicing or maintenance. Use the  
following guidelines:  
1. Avoid cleaning the telescope’s optics: a little dust on the front surface of the  
telescope’s correcting lens causes virtually no degradation of image quality and  
should not be considered reason to clean the lens.  
2. When absolutely necessary, remove dust from the front lens with gentle strokes of  
a camel-hair brush or blow it off with an ear syringe (available at any pharmacy).  
Do not use a commercial photographic lens cleaner.  
3. You may remove organic materials (e.g., fingerprints) from the front lens with a  
solution of 3 parts distilled water to 1 part isopropyl alcohol. A single drop of  
biodegradable dishwashing soap may be added per pint of solution. Use soft, white  
facial tissues and make short, gentle strokes. Change tissues often.  
Caution: Do not use scented, colored or lotioned tissues or damage could  
result to the optics.  
4. In the very rare situation where cleaning the inside surface of the corrector lens  
becomes necessary, unthread the lens cell located at the front of the main tube.  
The entire correcting lens and secondary mirror system are mounted in this cell.  
You may use the lens-cleaner solution described in step 3 to clean the inside  
surface of the lens.  
Caution: Do not touch the aluminized circular surface of the secondary  
mirror with a finger, a tissue or any other object. This will almost certainly  
scratch the mirror surface.  
Note: When cleaning the inside surface of the correcting lens, leave the lens  
mounted in its metal cell throughout the process. Do not remove the lens  
from its metal housing or optical alignment of the lens will be lost,  
necessitating a return of the telescope to the Meade factory.  
5. If your ETX model is used outdoors on a humid night, telescope surfaces may accu-  
mulate water condensation. 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 being packed away. Do not, however, wipe any of the  
optical surfaces. Rather, simply allow the telescope to sit for some time in warm  
indoor air, so that the wet optical surfaces can dry unattended. In addition, the dust  
cap should not be placed back on to the optical tube until the telescope is thor-  
oughly dry.  
6. If your ETX model is not to be used for an extended period, perhaps for one month  
or more, it is advisable to remove the eight AA-size batteries from inside the drive  
base. Batteries left installed for prolonged periods may leak, causing damage to the  
telescope’s electronic circuitry (see HOWTO ASSEMBLEYOURTELESCOPE ANDTRI-  
POD, page 12).  
7. The super-gloss anodized finish of any ETX model’s deep-violet optical tube fades  
if left in direct sunlight for prolonged periods.  
8. Do not leave your ETX model outdoors on a warm day or inside a sealed car for an  
extended period of time; excessive ambient temperatures can damage the  
telescope’s internal lubrication and electronic circuitry.  
9. A (English-format) hex wrench is provided with ETX models. This wrench is used  
as follows:  
Small wrench (.05”): Use the small wrench to tighten the set-screws of  
any knobs that may loosen (e.g., the focus knob or flip-mirror control  
knob).  
44  
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Storage and Transport  
When the telescope is not in use, store it in a cool, dry place. Do not expose the instru-  
ment to excessive heat or moisture. It is best to store the telescope in its  
original box with the vertical and horizontal locks (6 and 9, Fig. 1a and 1b) in the  
unlocked positions. If shipping the telescope, use the original box and packing  
material to protect the telescope during shipment.  
When transporting the telescope, take care not to bump or drop the instrument; this  
type of abuse can damage the optical tube and/or the objective lens and knock the  
optics out of alignment. It is highly recommended to use an optional carry case to  
transport the telescope (see OPTIONAL ACCESSORIES, page 42).  
Inspecting the Optics  
A few words about the so-called “Flashlight Test:" If a flashlight or other  
high-intensity light source is pointed down the main telescope tube, the view  
(depending upon the observer’s line of sight and the angle of the light) may reveal  
what appear to be scratches, dark or bright spots or uneven coatings, giving the  
appearance of poor quality optics. These effects 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 system, 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.  
Troubleshooting  
The following suggestions may be helpful with operation of the ETX-90PE,  
ETX-105PE and ETX-125PE.  
The power indicator light on the telescope does not come on or there is no  
response when pressing the AutoStar Arrow keys:  
• Verify that the Computer Control panel power switch (A, Fig. 2) is in the ON  
position.  
• Verify that the AutoStar coil cord is firmly connected to the HBX port (C, Fig. 2).  
• If using internal power (batteries), verify that the batteries are installed correctly and  
that they have sufficient charge (see HOW TO ASSEMBLE YOUR TELESCOPE AND  
TRIPOD, page 12).  
Note: If the batteries are getting low on charge, there will be a marked  
difference in the slew speed. The speed indicator lights may also flash and  
the speed may change. If any of these symptoms occurs, turn the power off  
and replace the batteries.  
• If using an external power source, verify that it is properly connected between the  
12-volt connector (D, Fig. 3) and either a wall plug (AC source) or a car cigarette  
lighter (DC source).  
• If AutoStar does not respond to commands, move the power switch to OFF and  
then back to ON.  
• If the telescope does not slew after power is applied or if the motor quits or stalls,  
verify that there are no physical obstructions that would impede telescope  
movement.  
• If all physical obstacles are removed and the telescope still does not move  
properly, turn off the power and unplug AutoStar. Plug AutoStar back in and turn the  
power back on.  
Unable to see an image through the eyepiece:  
• Confirm that the lens cover has been removed from the telescope.  
• Confirm that the flip-mirror control (14, Fig. 1b) is in the “up” position if using the  
eyepiece holder (4, Fig. 1b) so that light is directed to the eyepiece (1, Fig. 1a).  
Confirm that the flip-mirror control is in the “down” position if using the #932  
Erecting Prism or doing photography with an ETX model (see TELESCOPE  
FEATURES, page 6 and PHOTOGRAPHY, page 38).  
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Object appears in the SmartFinder but not in the eyepiece:  
• The SmartFinder is not properly aligned with the telescope (see ALIGNING  
SMARTFINDER page 13).  
,
Slew speed does not change when you press the SPEED key or the telescope  
moves slowly even though the fast slew speed is chosen:  
• The battery power may be low (see HOW TO ASSEMBLE, page 12).  
Telescope does not track a celestial object:  
• Make sure that the telescope is correctly aligned. See AUTOMATIC ALIGNMENT, page  
17, for more information.  
Images through the eyepiece appear unfocused or distorted:  
• The magnification may be too high for the viewing conditions. Back off to a lower  
power eyepiece (see CHOOSING AN EYEPIECE, page 14).  
• If inside a warm house or building, move outside. Interior air conditions may distort  
terrestrial or celestial images, making it difficult, if not impossible, to obtain a sharp  
focus. For optimal viewing, use the telescope outside in the open air instead of  
observing through an open or closed window or screen.  
• If viewing a land object on a warm day, heat waves will distort the image (see  
TERRESTRIAL OBSERVING, page 15).  
• For clear viewing of objects, turn the focus knob (8, Fig. 1b) slowly since the “in-  
focus” point of a telescope is precise. Turning the focus knob too quickly may cause  
the focus point to pass without notice.  
• The optics within the telescope need time to adjust to the outside ambient  
temperature to provide the sharpest image. To cool down the optics, set the  
telescope outside for 10 to 15 minutes before observing begins.  
Telescope moves off a terrestrial object while observing:  
• Verify that the vertical and horizontal locks are tight (see TELESCOPE FEATURES,  
page 6).  
Telescope does not move past a certain point:  
• The built-in vertical or horizontal rotational “stops” may have been reached. See #6,  
page 7.  
Telescope pauses when changing slew direction:  
• This pause is normal.  
A terrestrial object appears reversed left-for-right:  
• An eyepiece in the standard 90° observing position (4, Fig. 1b) reverses an object  
left-for-right: To view a correctly oriented image requires the optional #932 Erecting  
Prism (see OPTIONAL ACCESSORIES, page 42).  
Meade Customer Service  
If you have a question concerning your ETX model, call the Meade Instruments  
Customer Service Department at (949) 451-1450. Customer Service hours are 7:00  
AM to 6:00 PM, Pacific Time, Monday through Friday. In the unlikely event that the ETX  
requires factory servicing 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 telescope to the factory.  
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SPECIFICATIONS  
Specifications: ETX-90PE Astro Telescope  
Optical design . . . . . . . . . . . . . . . . . . . . Maksutov-Cassegrain  
Primary mirror diameter . . . . . . . . . . . . . . . . . . . 96mm (3.78”)  
Clear aperture. . . . . . . . . . . . . . . . . . . . . . . . . . . . 90mm (3.5”)  
Focal length . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1250mm  
Focal ratio (photographic speed). . . . . . . . . . . . . . . . . . . f/13.8  
Near focus (approx) . . . . . . . . . . . . . . . . . . . . . . 11.5 ft (3.5m)  
Resolving power . . . . . . . . . . . . . . . . . . . . . . . . . . 1.3 arc secs  
Super multi-coatings (EMC) . . . . . . . . . . . . . . . . . . . . standard  
Limiting visual stellar magnitude (approx.) . . . . . . . . . . . . 11.7  
Image scale . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.16°/inch  
Maximum practical visual power . . . . . . . . . . . . . . . . . . . 325X  
Optical tube dimensions  
(dia. x length) . . . . . . . . . . . 10.4cm x 27.9cm (4.1” x 11”)  
Secondary mirror obstruction (dia.; %) . . 27.9mm (1.1”); 9.6%  
Telescope mounting . . . . . . . . . . . . . . . . fork type; double tine  
Setting circle diameters. . . . . . . . . . . . . . . . Dec.: 3.5”; R.A.: 7”  
SmartFinder. . . . . . . . . . . Red dot projected onto finder’s lens  
LNT Module . . . . . . High accuracy, temperature-compensated  
. . . . . . . . . . . . . . . . . oscillator, updatable using Meade’s  
. . . . . . . . . . . . . . . . . . . . . . . . optional ATUM accessory  
Input voltage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 volts DC  
Motor Drive System DC servo motors with encoders, both axes  
Bearings:  
Altitude. . . . . . . . . . . . . . . . . . . . . . . UHMW polyethylene  
Azimuth . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . PTFE  
Materials:  
Tube body . . . . . . . . . . . . . . . . . . . . . . . . . . . . . aluminum  
Mounting . . . . . . high-impact ABS, aluminum-reinforced  
Primary mirror. . . . . . . . . . . . . . . . . . . . . . . . Pyrex® glass  
Correcting lens . . . . . . . . . . . BK7 optical glass, Grade-A  
Telescope dimensions:  
. . . . . . . . . . . . . . . . 38cm x 18cm x 22cm (15” x 7” x 9”)  
Telescope net weight:  
(incl. AutoStar & batteries) . . . . . . . . . . . . 3.5kg (7.8 lbs)  
Telescope shipping weight. . . . . . . . . . . . . . . . 5.8kg (12.8 lbs)  
Battery Life (approx.):  
with AutoStar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 hrs  
Specifications: ETX-105PE Astro Telescope  
Optical design . . . . . . . . . . . . . . . . . . . . Maksutov-Cassegrain  
Primary mirror diameter . . . . . . . . . . . . . . . . . . 116mm (4.56”)  
Clear aperture. . . . . . . . . . . . . . . . . . . . . . . . . . 105mm (4.13”)  
Focal length . . . . . . . . . . . . . . . . . . . . . . . . . . 1470mm (57.8”)  
Focal ratio (photographic speed) . . . . . . . . . . . . . . . . . . . . f/14  
Near focus (approx) . . . . . . . . . . . . . . . . . . . . . . . . 4.6m (15 ft)  
Resolving power . . . . . . . . . . . . . . . . . . . . . . . . . . 1.1 arc secs  
Super multi-coatings (EMC) . . . . . . . . . . . . . . . . . . . . standard  
Limiting visual stellar magnitude (approx.) . . . . . . . . . . . . 12.1  
Image scale . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 0.99°/inch  
Maximum practical visual power. . . . . . . . . . . . . . . . . . . . 420x  
Optical tube dimensions  
(dia. x length) . . . . . . . . 12.4cm x 32.8cm (4.88” x 12.9”)  
Secondary mirror obstruction (dia.; %) . . . 3.3cm (1.32”); 9.4%  
Telescope mounting . . . . . . . . . . . . . . . . fork type; double tine  
Setting circle diameters . . . . . . . . . . . . . Dec.: 3.81”; R.A.: 7.8”  
47  
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SmartFinder. . . . . . . . . . . Red dot projected onto finder’s lens  
LNT Module . . . . . . High accuracy, temperature-compensated  
. . . . . . . . . . . . . . . . . oscillator, updatable using Meade’s  
. . . . . . . . . . . . . . . . . . . . . . . . optional ATUM accessory  
Input voltage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 volts DC  
Motor Drive System . . . DC servo motors with encoders, both axes  
Bearings:  
Altitude. . . . . . . . . . . . . . . . . . . . . . . . . . . . . ball bearings  
Azimuth . . . . PTFE thrust bearing and radial ball bearing  
Materials:  
Tube body . . . . . . . . . . . . . . . . . . . . . . . . . . . . . aluminum  
Mounting . . . . . . ABS, with internal aluminum structure  
Primary mirror. . . . . . . . . . . . . . . . . . . . . . . . Pyrex® glass  
Correcting lens . . . . . . . . . . . BK7 optical glass, Grade-A  
Telescope dimensions:  
. . . . . . . . . . . . . 43cm x 25cm x 20cm (17” x 10” x 8”)  
Telescope net weight:  
(incl. AutoStar & batteries) . . . . . . . . . . . 6.1kg (13.5 lbs)  
Telescope shipping weight. . . . . . . . . . . . . . . . 8.3kg (18.4 lbs)  
Battery Life (approx.):  
with AutoStar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 hrs  
Specifications: ETX-125PE Astro Telescope  
Optical design . . . . . . . . . . . . . . . . . . . . Maksutov-Cassegrain  
Primary mirror diameter . . . . . . . . . . . . . . . . . . 138mm (5.43”)  
Clear aperture. . . . . . . . . . . . . . . . . . . . . . . . . . . 127mm (5.0”)  
Focal length . . . . . . . . . . . . . . . . . . . . . . . . . . 1900mm (74.8”)  
Focal ratio (photographic speed) . . . . . . . . . . . . . . . . . . . . f/15  
Near focus (approx) . . . . . . . . . . . . . . . . . . . . . . . . 4.6m (15 ft)  
Resolving power . . . . . . . . . . . . . . . . . . . . . . . . . . 0.9 arc secs  
Super multi-coatings (EMC) . . . . . . . . . . . . . . . . . . . . standard  
Limiting visual stellar magnitude (approx.) . . . . . . . . . . . . 12.5  
Image scale . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 0.76°/inch  
Maximum practical visual power . . . . . . . . . . . . . . . . . . . 500X  
Optical tube dimensions  
(dia. x length) . . . . . . . . . . 14.6cm x 36cm (5.75” x 14.2”)  
SmartFinder . . . . . . . . . . . . . . . . . . . . . . 8 x 25mm right-angle  
Secondary mirror obstruction (dia.; %) . . 39.4mm (1.6”); 9.6%  
Telescope mounting . . . . . . . . . . . . . . . . fork type; double tine  
Setting circle diameters. . . . . . . . . . . . . . . . Dec.: 4.3”; R.A.: 9”  
SmartFinder. . . . . . . . . . . Red dot projected onto finder’s lens  
LNT Module . . . . . . High accuracy, temperature-compensated  
. . . . . . . . . . . . . . . . . oscillator, updatable using Meade’s  
. . . . . . . . . . . . . . . . . . . . . . . . optional ATUM accessory  
Input voltage . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 volts DC  
Motor Drive System . . . DC servo motors with encoders, both axes  
Bearings:  
Altitude. . . . . . . . . . . . . . . . . . . . . . . . . . . . . ball bearings  
Azimuth . . . . . . . . . . . . . . . . . . . . . . . . . . . . ball bearings  
Materials:  
Tube body . . . . . . . . . . . . . . . . . . . . . . . . . . . . . aluminum  
Mounting . . . . . . . ABS, with internal aluminum structure  
Primary mirror. . . . . . . . . . . . . . . . . . . . . . . . Pyrex® glass  
Correcting lens . . . . . . . . . . . BK7 optical glass, Grade-A  
Telescope dimensions:  
. . . . . . . . . . 48cm x 23cm x 27cm (19” x 8.9” x 10.8”)  
Telescope net weight:  
(incl. AutoStar & batteries) . . . . . . . . . . . 6.9kg (15.2 lbs)  
Telescope shipping weight. . . . . . . . . . . . . . . 11.4kg (25.2 lbs)  
Battery Life (approx.):  
with AutoStar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20 hrs  
48  
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AutoStar Specifications  
Processor ............................................................................68HC11, 8MHz  
Flash Memory ............................................................1MB, reloadable  
Keypad ........................................................................20 key alphanumeric  
Display ........................................................................2 line, 16 character LCD  
Backlight......................................................................Red LED  
Utility Light ..................................................................Yes  
RS-232........................................................................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)  
ETX 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 Mars made its closest approach in 60,000 years to our Sun in  
2003, astronomers around the world posted new photos daily.  
On the internet, you can find websites for almost any topic relating to astronomy. Try  
the following key word searches: NASA, Hubble, HST, astronomy, Messier, satellite,  
nebula, black hole, variable stars, etc.  
Check Meade’s 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  
handbox. See page 30 for more information. You’ll find our website at:  
Here are some other sites you might find interesting:  
Sky & Telescope:  
http://www.SkyandTelescope.com  
Astronomy:  
• The Starfield:  
• Astronomy Picture of the Day:  
• Heavens Above (satellite observing information):  
• Photographic Atlas of the Moon:  
• Hubble Space Telescope Public Pictures  
49  
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APPENDIX A: EQUATORIAL  
(POLAR) ALIGNMENT  
Equatorial Alignment  
In equatorial (or "polar") Alignment, the telescope is oriented so that the horizontal and  
vertical axes of the telescope are lined up with the celestial coordinate system.  
Important Note:  
The "Telescope: Mount"  
option of the Setup menu is  
set to "Alt/Az" as the default  
mount by the factory. If the  
telescope is equatorially  
mounted, you must choose  
the "Polar" option from the  
AutoStar "Telescope: Mount"  
menu.  
In order to equatorial align your telescope, it is essential to have an understanding of how  
and where to locate celestial objects as they move across the sky. This section provides a  
basic introduction to the terminology of equatorial-aligned astronomy and includes  
instructions for finding the celestial pole and for finding objects in the night sky using  
Declination and Right Ascension.  
Celestial Coordinates  
A
celestial coordinate system was created that maps an imaginary sphere  
surrounding the Earth upon which all stars appear to be placed. This mapping system is  
similar 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 Earth’s  
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 Earth’s 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. 43) is that point in the sky where an exten-  
sion of the North Pole intersects the celestial sphere. The North Star, Polaris, is located  
very near the North Celestial Pole (1, Fig. 43). The celestial equator (2, Fig. 43) is a pro-  
jection of the Earth’s equator onto the celestial sphere.  
So just as an object's position on the Earth’s 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°).  
North  
Celestial  
Pole  
(Vicinity  
of Polaris)  
+90 Dec.  
Star  
1
12  
11  
1
13  
10  
2
14  
15  
9
8
16  
17  
18  
19  
ܖ
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 merid-  
ian. 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.  
7
Earth’s  
Rotation  
6
5
4
3
20  
Celestial  
Equator  
21  
22  
23  
0
Right Ascension  
0 Dec.  
2
South  
Celestial  
Pole  
-90 Dec.  
ܖ
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 celestial equator  
(such as the the constellations of Orion, Virgo and Aquarius) is said to have a  
Declination of zero, shown as 0° 0' 0."  
Fig. 43: Celestial Sphere.  
Polar Mounting your Telescope with the #884 Deluxe Field Tripod  
As the Earth rotates on its axis, astronomical objects appear to move across the sky in an  
arc. This apparent motion is not obvious to the unaided eye, but when viewed through a  
telescope such as an ETX, this motion is rapid indeed. If the motor drive has not been  
engaged,  
celestial  
objects  
viewed  
in  
the  
telescope  
eyepiece  
drift  
entirely out of the field of view in 15 to 60 seconds, depending on the magnification  
employed.  
However, by mounting your telescope and turning on the motor drive, you can  
counteract the drift of objects in the eyepiece. The two basic types of mounting are:  
altazimuth (alt/az) and equatorial. For many ETX owners, it will not be necessary to  
equatorially mount the telescope; alt/az mounting will suffice. The AutoStar Controller  
allows the telescope to be mounted in the altazimuth (alt/az) mode for most  
observing purposes. See AUTOMATIC ALIGNMENT, page 17, for more information.  
50  
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However, owners who wish to perform astrophotography or use the Meade LPI or Deep  
Sky Imager (see PHOTOGRAPHY WITH MEADE’S AUTOSTAR SUITE, page 41, for more  
information) will find equatorial mounting indispensible to their needs.  
Equatorial Mount  
Equatorial mounting lines up the telescope’s polar axis with the North Celestial Pole (or the  
South Celestial Pole if observing in the southern hemisphere).  
When using an equatorially mounted telescope, tracking (following) celestial objects is  
possible by turning on your ETX telescope's motor drive.The motor counteracts the Earth's  
rotation and keeps objects in the field of view of the eyepiece for hands-off tracking.  
³
Equatorial Mounting Procedure  
1. Assemble the tripod as described in Step #2 of How to Assemble Your Telescope and  
Fig. 44: Loosen control latch.  
Tripod, page 12.  
2. Loosen the latitude control latch (1, Fig. 44) and lift up the tilt-plate (2, Fig. 44) so that  
you can easily access the underside of the plate. Relock the latitude  
control latch, so the assembly doesn't slip while you are attaching the telescope.  
High latitude  
leg mounting  
hole.  
Attachment  
knob.  
3. Turn the tripod, so that the face of the tilt-plate points North (Figs. 48 and 49, on next  
page). If you attach the telescope to the tripod indoors, be sure to orient the face of  
the tilt-plate to point North after moving the telescope outdoors. Equivalently, point the  
tripod leg (5, Fig. 48) North. This is the leg opposite from the latitude control bar (4,  
Fig. 48).  
4. Line up the mounting hole on the base of the telescope labeled "High Latitude Leg"  
with the attachment knob that is closest to the latitude control bar (see Fig. 45). Line  
up the other mounting hole with the remaining attachment knob. Thread both  
attachment knobs into the base of the telescope. Tighten to a firm-feel only.  
Latitude  
control  
bar.  
5. Determine the latitude of your observing location from a road map, atlas or the  
LATITUDE CHART FOR MAJOR CITIES OF THE WORLD, page 54. Loosen the  
latitude control latch (1, Fig. 47, on next page) and adjust the latitude control bar (4,  
Fig. 47) so that your observing site's latitude is just visible above the flat surface of the  
tripod head. Retighten the latch.  
Fig. 45: High latitude leg  
mounting hole and  
corresponding attachment  
knob.  
6. If you have not already done so orient the tripod leg (see Step #3 and 5, Fig. 48) so  
that it is pointing due North (if the location of Polaris, the North Star, is known, point  
the telescope directly at Polaris. Observers located in the Earth’s Southern  
Hemisphere must point the telescope due South).  
7. The telescope is now equatorially mounted; the tripod must not be moved or else the  
alignment will be lost. Instead, use one of the following methods to move the  
telescope's optical tube to a desired celestial object.  
(a) Loosen the vertical and/or horizontal locks (6 and 9, Fig. 1a and 1b) to permit  
the optical tube to be freely moved manually. Tighten the locks once you center  
on the object.  
»
(b) With the horizontal and vertical locks in their “locked” positions, use the Arrow  
keys to move the optical tube.  
Note: For most astronomical observing requirements, approximate  
settings of the telescope's latitude and North-pointing tripod leg (Steps #5  
and #6) are acceptable. Do not allow undue attention to precise equatorial  
mounting of the telescope to interfere with your enjoyment of the instrument.  
Using an Equatorially Mounted Telescope  
Fig. 46: Attach telescope to  
tripod.  
Once your telescope is equatorially mounted, the telescope motor drive will keep a  
celestial object in the telescope eyepiece's field of view.  
To Track a Star When Polar Mounted:  
Make sure you have initialized your telescope before you try out this feature (see  
INITIALIZING AUTOSTAR, page 17).  
1. Tighten the vertical and horizontal locks (6 and 9, Fig. 1a and 1b) if necessary.  
2. Make sure that AutoStar is connected to the HBX port (C, Fig. 2) of the  
telescope’s computer control panel.  
3. Flip the telescope power switch (A, Fig. 2) to the ON position.  
The AutoStar screen displays a copyright message displays, followed by a short beep.  
Then AutoStar takes a few moments to start up the system.  
4. A message displays that warns not to look at the Sun. At the end of this message,  
press the key prompted by AutoStar to signify that the message has been read and  
understood.  
51  
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5. Press ENTER repeatedly until “Setup: Align” displays.  
6. Press the Scroll Down key repeatedly until "Setup:Telescope" displays. Press ENTER.  
Telescope: Telescope Model” displays.  
7. Press the Scroll Down key repeatedly until "Telescope: Mount" displays. Press  
ENTER. “Scope Mounting: Alt/az” displays.  
8. Press the Scroll Down key once. "Scope Mounting: Alt/az" displays. Press ENTER.  
"Telescope: Mount" displays again.  
9. Press Mode once. “Setup: Telescope” displays.  
¿
10. Press the Scroll Down key once. "Setup: Targets" displays.  
³
11. Press ENTER. "Targets: Terrestrial" displays. Press one of the Scroll keys once.  
"Targets: Astronomical" now displays.  
Fig. 47: Set latitude.  
12. Use the Arrow keys to locate a bright star in the night sky. Use the SmartFinder (2,  
Fig. 1) 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 necessary to once again center  
the star in the eyepiece. The tracking motors will then keep the star you have chosen  
in the center of the eyepiece.  
North  
Celestial  
Pole  
+
¿
13. Press and hold the ENTER key for a few seconds and then release to stop  
tracking. You may repeat the procedure to locate another star or object using the  
Arrow keys. Then press ENTER to re-engage the tracking motors.  
Caution: Do not move the tripod or adjust the latitude setting while  
observing or the mounting alignment will be lost.The telescope's motor drive dis-  
engages when the Horizontal and the Vertical lock levers are unlocked and  
re-engages when the levers are relocked.  
´
Fig. 48: Example of Polar  
Alignment. Note that the face  
of the tilt-plate points North.  
AutoStar Polar Alignment  
AutoStar provides three different (manual) methods for polar alignment: Easy,  
One-Star and Two-Star.  
North  
Celestial  
Pole  
Easy Polar Alignment  
Two alignment stars are chosen by AutoStar based on the date, time and location. First,  
choose "Polar" from the "Setup: Telescope: Mount" menu. The rest of the  
procedure is identical to the Alt/Az AUTOMATIC ALIGNMENT, page 17.  
+
One-Star Polar Alignment  
Polar One-Star Alignment requires some knowledge of the night sky. AutoStar  
provides a database of bright stars and one star from this database is chosen by the  
observer for alignment. Polaris is chosen by AutoStar. First, choose "Polar" from the  
"Setup: Telescope: Mount" menu. The rest of the procedure is almost identical to the Alt/Az  
ONE STAR ALT/AZ ALIGNMENT, page 36, except that AutoStar prompts you to point the  
telescope at Polaris and center it in the telescope eyepiece.  
Two-Star Polar Alignment  
Polar Two-Star Alignment requires some knowledge of the night sky. AutoStar provides a  
database of bright stars and two stars from this database are chosen by the observer for  
alignment. First, choose "Polar" from the "Setup: Telescope: Mount" menu. The rest of the  
procedure is almost identical to the Alt/Az TWO STAR ALT/AZ ALIGNMENT, page 36.  
Fig. 49: Example of Polar  
Alignment. Note that the face  
of the tilt-plate points North.  
This is the Polar home  
position.  
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 shoulder toward  
where the Sun sets. To precisely point at the pole, find the North Star (Polaris) by using the  
Big Dipper as a guide (Fig. 50, next page).  
Important Note:  
Important Note: For almost all astronomical observing requirements,  
approximate settings of the telescope’s latitude and Polar axis are  
acceptable. Do not allow undue attention to precise Polar Alignment of the  
telescope to interfere with your basic enjoyment of the instrument.  
In order to select any of  
three polar alignment  
options, you must first  
select "Polar" in the  
"Mount" option of the  
"Setup: Telescope" menu.  
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Setting Circles  
The ETX models are equipped with R.A. and Dec. setting circles (13 and 16, Fig. 1a) to  
aid in locating faint celestial objects when the telescope has been polar aligned. Setting cir-  
cles emulate the celestial coordinates found on star charts or in sky catalogs. Any charted  
object is easily located by coordinates in R.A. (in hours, minutes and seconds, from 0h 0m  
0s to 23h 59m 59s) and Dec. (in degrees from 0° to 90°).  
Little Dipper  
Polaris  
With an ETX model polar aligned, use the Arrow keys to move the telescope in R.A. (left  
and right keys) and Dec. (up and down keys).  
Big Dipper  
Cassiopeia  
Note: The Dec. setting circle is located on the left arm of the telescope fork  
mount. The right arm of the mount contains a graduated circle (mounted  
behind the knurled knob of the vertical lock), without Dec. numbers.  
Fig. 50: Locating Polaris  
Declination Setting Circle: The Dec. setting circle (Fig. 51) has been factory set to read  
the correct Declination of celestial objects.  
Because the smooth knob on this fork mount arm need never be loosened, the Dec.  
setting circle should always remain calibrated. If for some reason this knob becomes  
loose and the Dec. setting circle must be recalibrated, level the optical tube (5, Fig. 1a)  
so that it is parallel to the drive base. Loosen the smooth knob covering the Dec. setting  
circle until the setting circle moves freely. Reposition the setting circle so that the 0  
setting aligns with the Dec. pointer (the molded triangle beneath the setting circle).  
Retighten the Dec. knob.  
Right Ascension Setting Circle: Since celestial objects move in R.A., the R.A. setting  
circle (Fig. 52) must be reset as each object is located during an observing session. The  
R.A. pointer is located on the drive base 90° counterclockwise from the telescope’s  
Computer Control panel (10, Fig. 1a) immediately under the R.A. circle.  
20  
10  
0
To use the setting circles to find astronomical objects, the ETX must first be polar aligned.  
It is advisable that the motor drive be turned on and that a low-power eyepiece (e.g., a  
26mm eyepiece) be employed. Then use the following procedure:  
Fig. 51: Section of  
Declination setting circle.  
1. Identify the celestial coordinates (R.A. and Dec.) of a bright, easy-to-find object, such as  
a bright star. (Avoid using Polaris or any object near Polaris.) Coordinates of bright stars  
are listed in astronomy magazines, text books or star charts. Center this object in the  
telescope’s field of view.  
12  
12  
11  
13  
10  
14  
2. Manually turn the R.A. circle (13, Fig. 1a) to read the R.A. of the object at the R.A.  
pointer (the molded triangle beneath this setting circle).  
Fig. 52: Section of Right  
Ascension setting circle.  
3. The R.A. circle is now calibrated to read the correct R.A. of any object at which the  
telescope is pointed. The Dec. circle is already calibrated through polar alignment.  
4. To find another object, again identify the R.A. and Dec. coordinates.Then, without touch-  
ing the setting circles, move the telescope (manually, by unlocking the vertical and hor-  
izontal locks or by slewing the telescope using the Arrow keys) so that the R.A. and Dec.  
pointers read the coordinates of the second object.  
5. If the above procedure has been followed carefully, the second object will now be in the  
telescope’s field of view.  
Note: Since the second object (i.e., the object to be located) is in constant  
motion, once the R.A. circle is calibrated (step 2, above) the telescope should  
be moved rapidly to read the coordinates of the second object. Otherwise the  
second object will no longer be in the position indicated by the R.A. circle.  
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 familiar.  
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APPENDIX B: LATITUDE CHART  
Latitude Chart for Major Cities of the World  
To aid in the polar alignment procedure (see page 51), latitudes of major cities around the world are listed below. To determine the latitude 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  
State/Prov./Country Latitude  
Country  
Colombia  
Brazil  
Argentina  
Uruguay  
Chile  
Latitude  
4° N  
New Mexico  
Alaska  
Georgia  
Massachusetts  
Alberta  
Illinois  
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  
Bogotá  
São Paulo  
Buenos Aires  
Montevideo  
Santiago  
23° S  
35° S  
35° S  
34° S  
10° N  
Caracas  
Venezuela  
Ohio  
Texas  
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  
Colorado  
Michigan  
Hawaii  
Mississippi  
Missouri  
Wisconsin  
Nevada  
Arkansas  
California  
Mexico  
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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APPENDIX C: TRAINING THE DRIVE  
Train the telescope motors using AutoStar. Perform this procedure if you are experiencing any pointing accuracy problems. Fig.  
53 depicts the complete Drive Training procedure.  
Note: Use a terrestrial object, such as a telephone pole or lamp post, to train the drive. Complete this exercise once  
every 3 to 6 months to maintain the highest level of telescope pointing accuracy.  
ETX TIPS  
Verify that AUTOSTAR  
Press > until it  
1
2
Further Study....  
12  
INITIALIZATION is  
complete.  
is centered  
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 (some  
of the topics are easy and some are quite challenging). Try look-  
ing up some of these in the AutoStar glossary.  
Scope slews left.  
Bring target back  
to center using  
Press MODE until  
Select Item is displayed.  
the Right Arrow key.  
Select Item  
3
Object  
Press < until it  
is centered  
Also included below is a small sampling of books, magazines  
and organizations that you might find helpful.  
13  
Press the scroll  
up key once.  
Scope slews right.  
Bring target back  
to center using  
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 quark star? A  
gamma burster? An Einstein lens?  
Select Item  
Setup  
4
the Left Arrow key.  
Access the Setup  
menu.  
Train Drive  
Az. Train  
14  
Menu returns to  
Az. training.  
Setup  
5
Align  
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 supernova?  
Multiple presses.  
Train Drive  
Alt. Train  
Altitude  
15  
16  
Setup  
6
(vertical)  
training.  
Telescope  
Access the  
Telescope menu.  
Drive Setup  
For this op. . .  
Reminder to  
use terrestrial  
target.  
Telescope  
Telescope Model  
7
9. What is the Inflationary Big Bang? What is dark matter?  
What are MACHO's?  
Multiple presses.  
10. How are extrasolar planets discovered? What is an accre-  
tion (or protoplanetary) disk?  
Center reference  
object  
17  
11. What are the differences between elliptical, spiral and irreg-  
ular galaxies? Can globular clusters be older than the uni-  
verse itself?  
Center target  
using Arrow  
keys.  
Telescope  
Train Drive  
8
Choose the Train  
Drive option.  
Press until it  
is centered  
Books  
18  
1. The Guide to Amateur Astronomy by Jack Newton and  
Philip Teece  
Scope slews down.  
Bring target back  
to center using  
Train Drive  
Az. Train  
Azimuth  
9
2. The Sky: A User’s Guide by David Levy  
3. Turn Left at Orion by Guy Consolmagno & Dan Davis  
4. Astrophotography for the Amateur by Michael Covington  
Magazines  
the Up Arrow key.  
(horizontal)  
training.  
Press until it  
is centered  
19  
Drive Setup  
For this op. . .  
Reminder to  
10  
Scope slews up.  
Bring target back  
to center using  
1. Sky & Telescope  
Box 9111, Belmont, MA 02178  
2. Astronomy  
use terrestrial  
target.  
the Down Arrow key.  
Box 1612, Waukesha, WI 53187  
Center reference  
object.  
Organizations:  
Train Drive  
Az. Train  
Multiple presses.  
11  
20  
1. Astronomical League  
Center target  
using Arrow  
keys.  
Executive Secretary  
MODE  
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  
Select Item  
Object  
21  
65 North Catalina Ave, Pasadena, CA 91106  
Fig. 53: Training the Drive Procedure.  
And watch Jack Horkheimer, Star Gazer, on your local PBS  
55  
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APPENDIX D:CHANGING THE  
LNT MODULE BATTERY  
The LNT Module uses a lithium coin CR2023 battery that will last about 5 years and  
is installed with the original LNT Module assembly. After you replace the battery, you  
will need to recalibrate the telescope’s sensors and reset the time and date. You will  
need a new battery. Also, you may use Meade’s optional Atomic Time Update  
Module, although this is not necessary.  
Side  
Alignment  
screw  
Top Alignment  
screw  
To replace the battery:  
1. Remove the top alignment screw cap/long bolt from the LNT Module. See Fig.  
54.  
2. Remove the side alignment screw cap/long bolt from the LNT Module. Take note  
that there are two springs inside the LNT. One spring sits between the top and  
bottom of the unit. The second spring is on the side of the unit that rests  
between the bottom and the top sections. One long bolt passes through the top  
spring and the other long bolt passes through the side spring. Set the springs  
aside as you will need to replace it later in this assembly . See Fig. 55 and 56.  
Fig. 54: The LNT Module, with  
alignment screws and Atomic Time  
Update port visible.  
Important Note: Note there is some wiring inside the LNT Module. Be careful  
not to pull on the wiring. If it is necessary to move the wiring aside, do so  
carefully.  
Top Alignment  
screw  
Atomic Time  
Update Port  
3. Carefully lift the top section of the unit from the bottom section. Do not remove  
the bottom section or disassemble the rest of the unit.  
4. Remove the old battery. Note the spring.  
5. Insert the new (user-supplied) battery. Take care to orient the battery so that the  
side with the battery markings is facing the top.  
6. Replace the top spring in place and the LNT Module cover.  
7. Replace the top bolt and tighten the cap to a firm feel.  
Side  
Alignment  
screw hole  
8. Hold the side spring in place with your fingers and slide the spring between  
between the top and bottom sections. The spring should line up with the  
mounting holes for the side long bolt. Slide the long bolt through the side hole,  
then through the spring and finally through the bottom of the LNT Module and  
tighten to a firm feel.  
Spring  
Fig. 55: Interior side view of LNT  
Module.  
9. Next you will need to recalibrate the LNT Module sensors. Select Calibrate  
Sensors from the Setup: Telescope menu. A scrolling message displays.  
Top Alignment  
screw hole  
10. The message prompts you to place the telescope in the home position:  
Loosen the telescope’s vertical lock (6, Fig. 1B). This will allow you to move  
the telescope’s optical tube up and down.  
Level the tripod head. See Step #3g, page 12. Level the optical tube by  
lining up 0° on the Dec setting circle (16, Fig. 1a) with the Dec pointer  
(the small molded triangle under the setting circle).  
Cover  
Retighten the vertical lock (6, Fig. 1b) to a firm feel only.  
Unlock the horizontal lock (9, Fig. 1a). This will allow you to rotate the  
Battery  
telescope tube and fork arm assembly.  
Grasp the telescope by  
counterclockwise until it stops.  
a
fork arm and rotate the telescope  
Re-lock the Horizontal lock (9, Fig. 1).  
11. Press ENTER. The telescope will automatically find North, detect level and the tilt  
of you telescope, and calibrate the sensors.  
12. Next, follow the instructions included with the Atomic Time Update Module  
optional accessory to reset the clock.  
Side  
Alignment  
screw hole  
Spring  
OR  
Enter the date and time manually using the Date and Time options in the Setup  
menu.  
Fig. 56 Interior top view of  
SmartFinder unit.  
56  
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APPENDIX E:BASIC  
ASTRONOMY  
In the early 17th century Italian Scientist Galileo, using a telescope smaller than your  
ETX, 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 phases of  
Venus! Because of his observations, Galileo correctly realized Earth's movement 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  
determined 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 understood. 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  
variable stars, the Moon and our solar system comes from observations made by  
amateur astronomers. So as you look through your Meade ETX telescope, keep in  
mind Galileo.To him, a telescope was not merely a machine made of glass and metal,  
but something far more—a window of incredible discovery.  
AutoStar Glossary  
Be sure to make use of AutoStar’s 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 24, for more information.  
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 Moon’s  
surface at an angle. It casts shadows and adds a sense of depth to the view (Fig. 57).  
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  
filter 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. 57: The Moon. Note  
the deep shadows in the  
craters.  
Using your ETX model, brilliant detail can be observed on the Moon, including  
hundreds of lunar craters and maria, described below.  
Craters are round meteor impact sites covering most of the Moon’s 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, seas) are smooth, dark areas scattered across the lunar  
surface. These areas are ancient impact basins that were filled with lava from the  
interior of the Moon by the depth and force of the meteor or comet impact.  
12 Apollo astronauts left their bootprints on the Moon in the late 1960’s and early  
1970’s. However, no telescope on Earth can see these footprints or any other  
artifacts. In fact, the smallest lunar features that may be seen with the largest  
telescope on Earth are about one-half mile across.  
Note: Except during its early or late crescent phases, the Moon can be an  
exceptionally bright object to view through the telescope. To reduce the  
brightness and glare, use the #905 Variable Polarizing Filter (see the MEADE  
GENERAL CATALOG for more information).  
57  
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Planets  
Planets change positions in the sky as they orbit around the Sun. To locate the  
planets on a given day or month, consult a monthly astronomy magazine, such as Sky  
and Telescope or Astronomy. Listed below are the best planets for viewing through  
your ETX model telescope.  
Tip:  
Enter a date in the Date  
menu and you can  
determine if a planet(s)—  
or any other object in the  
database—will be visible  
during the night of the  
entered date.  
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 com-  
pletely obscures any surface detail.  
After entering a new date,  
go to the Object menu  
and select the desired  
planet from the menu.  
Then keep pressing one  
of the Scroll keys until the  
rise and set times display.  
Press MODE to exit.  
Mars is about half the diameter of Earth. Through the telescope it appears as a tiny  
reddish-orange disk.You may see a hint of white at one of the planet’s polar ice caps.  
Approximately every two years, when Mars is closest to Earth, additional detail and  
coloring on the planet's surface may be visible.  
Jupiter (Fig. 58) is the largest planet in our solar system, with a diameter 11 times  
that of Earth. Jupiter appears as a disk with dark lines stretching across the surface.  
These lines are cloud bands in the atmosphere. Four of Jupiter’s 29 (and still  
counting!) moons (Io, Europa, Ganymede and Callisto) can be seen as star-like points  
of light when you use even the lowest magnification. The number of moons  
visible on any given night changes as they circle around the giant planet.  
Saturn (Fig. 59) is nine times the diameter of Earth and appears as a small, round  
disk with rings extending out from either side. 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.Saturn’s rings are composed of  
billions of ice particles.The major division in Saturn's rings, called the Cassini Division,  
is generally visible through all three ETX models. Titan, the largest of Saturn’s moons,  
can also be seen as a bright, star-like object near the planet.  
Fig. 58: The planet Jupiter.  
Jupiter's four largest  
moons can be observed in  
a different position every  
night.  
Deep-Sky Objects  
You can use star charts 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 illuminated by nuclear fusion in their core.  
Because of their vast distances from our solar system, all stars appear as pinpoints of  
light, regardless 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.  
Open Clusters are loose groupings of young stars, all recently formed from the same  
diffuse nebula. The Pleiades (Fig. 60) is an open cluster 410 light years from Earth.  
Several hundred stars of the cluster are visible through your telescope.  
Fig. 59: Saturn has the  
most extensive ring struc-  
ture in our Solar System.  
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 clos-  
est 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.  
Fig. 60: The Pleiades is  
one of the most beautiful  
open clusters.  
58  
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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 owner’s 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.  
6001 Oak Canyon, Irvine, California 92618  
ܖ
 (949) 451-1450  
ܖ
© 2004  
14-1010-29 10/04  
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