Socket Mobile Telescope GTOCP2 User Manual

ASTRO-PHYSICS

1200 GERMAN EQUATORIAL WITH

GTO SERVO MOTOR DRIVE

Model GTOCP2

February 26, 2002

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ASTRO-PHYSICS

1200 GERMAN EQUATORIAL WITH

GTO SERVO MOTOR DRIVE

MODEL 1200GTO PARTS LIST – MODEL GTOCP2

FEATURES AND SPECIFICATIONS

INTRODUCTION

Why Polar Alignment is Important

Compensation for the Earth’s rotation

ASSEMBLY INSTRUCTIONS

Before You Leave Home

Gross Latitude Adjustment

Attach Pier Adapter to Pier Post

Assemble Pier (purchased separately)

Assemble Polar Axis Assembly to Pier or Tripod

Altitude and Azimuth Adjustments - Rough polar alignment

Assemble Declination Axis

Removing Declination Axis at the End of your Observing Session

Attach Mounting Plate (purchased separately)

Attach Mounting Rings (purchased separately)

Fine Polar Alignment

Methods for fine polar alignment

Altitude and Azimuth Adjustments

OPERATION OF THE MOUNTING

R.A. and Dec. Damper Knobs

R.A. and Dec. Clutch Knobs

Balancing Your Telescope

SERVO MOTOR DRIVE

GTO Control Box – Model GTOCP2

R.A. and Dec. Cable Connections

12V Connector

POWER Indicator Light

KEYPAD Connector

RS-232 Connectors

FOCUS Connector

RETICLE Connector

AUTOGUIDER Connector

+6V Connector

N and S Switch

Prevent the Cables from Tangling

1200 Motor Cables

Accessory Cables

Removing the GTO Control Box From 1200 Mount

GTO Keypad Controller Operation

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MOUNT MAINTENANCE AND ALIGNMENT

TROUBLESHOOTING

INSTALLATION OF ENCODERS AND ENCODER HOUSINGS -1200 MOUNT

Fitting Declination Encoder Housing

Fitting Right Ascension Encoder Housing

Periodic Maintenance

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ASTRO-PHYSICS

1200 GERMAN EQUATORIAL WITH

GTO SERVO MOTOR DRIVE

MODEL 1200GTO PARTS LIST – MODEL GTOCP2

Polar axis assembly (right ascension-R.A.) with Servo Box GTOCP2

Declination (Dec.) axis assembly

Pier top adapter with six (6) 5/16-18 x 5/8" button head screws with washers

(these may be attached to your pier post if you ordered one)

Stainless counterweight shaft with washer stop and black plastic knob (knob has 5/16 thread)

Y cable – R.A. portion is 12.5” long and Dec portion is 37.5” long

D.C. power cord (cigarette lighter adapter on one end) - 8’ long

GTO Keypad controller with 15’ coiled cable

Keypad Protector (KEYPRO)

DigitalSky Voice Software (CD-ROM)

Hex key set

8-32 thumbscrews (substitute these for 8-32 set screws that hold GTO Servo Control Box in place, if you wish)

In order to fully assemble your mount, you will need the following items sold separately: mounting plate, 10” O.D. pier,

counterweights, and portable rechargeable battery pack (or 110 to 12V DC converter). Several sizes and types are

available for your selection. Many of these items will be discussed throughout these instructions.

Several additional options are available:

Longer counterweight shaft – 27” useable length, part # M12661

Santa Barbara Instrument Group CCD Imaging cameras and ST-4 Autoguider or STV - if you plan to pursue CCD

imaging or astrophotography

Pier accessory trays for 10” pier and support bars - handy to keep your eyepieces close at hand

Polar axis telescope - threads into the base of the polar axis assembly. Many users find a polar axis telescope useful for

zeroing in on the pole quickly, particularly with telescopes that are not orthogonal to the mount.

Mounted encoders – Although you can use these with your mount, they are not necessary since the go-to functions of

the mount are more accurate. The 4000 steps of the encoders, which read the position of the shaft are very

coarse (324 arc seconds) while the encoder that is built into the servo motor itself is 0.05 arc seconds.

FEATURES AND SPECIFICATIONS

R.A. worm wheel:

Dec worm wheel:

Worm gear:

10.3”, 225-tooth aluminum

7.2”, 225-tooth aluminum

Brass

Azimuth adjustment: Approximately 14 degrees

Setting circles:

Porter Slip Ring design,

engraved

R.A. shaft:

R.A. thrust bearings: 9.5” diameter

Dec shaft: 2.36” diameter

3.35” diameter

Right ascension:

Declination:

Motors:

4-minute increments, pointer

1-degree increments, pointer

Zero-cogging servo motors

Dec thrust bearings: 6.5” diameter

Counterweight shaft: 18” useable length,

1.875” diameter,

Power Consumption: 0.4 amps at the sidereal rate

3 amps both motors slewing

Power requirements: 12 VDC, range 11.5 to 15

stainless steel,

Weight of mount:

total -91 lbs.

removable

20 to 68 degrees with or

without polar scope or

Dec axis - 30 lbs.

R.A axis - 47 lbs.

counterweight shaft -14 lbs.

Latitude range:

encoders attached (if you are

above 65° you will have to

remove one pier top knob)

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INTRODUCTION

The 1200 German equatorial was designed to meet the needs of the advanced observer who requires a mount with

maximum strength and rigidity and minimum weight. The excess material in both axes has been carved out while retaining a

heavily ribbed structure for internal strength and rigidity. A unique dovetail was machined into the mating surfaces of the

R.A. and Dec axes. This feature allows quick and easy assembly in the field without any tools.

The DC servo motor drive with GTO computer system, including the keypad controller with its digital display screen and

DigitalSky Voice software offer extraordinary sophistication for today’s observer. Whether you enjoy visual astronomy

exclusively or plan an aggressive astrophotography or CCD imaging program, this mount will allow you to maximize your

night out under the stars.

The advanced keypad features allow you to slew automatically to objects in a wide range of databases as well as any

RA/Dec coordinate. A large selection of common names for stars and other objects makes your selection a snap. The rapid

slew rate of 5 degrees per second (1200x) allows you to locate objects very quickly and accurately. You will be very pleased

with the intuitive operation of this controller. There are no complicated sequences of keystrokes to remember. It is so easy

to use that even it you don’t use it for a few months, you will feel at home with the keypad very quickly.

DigitalSky Voice software provides additional capabilities to control the movement of your telescope by using two-way

verbal communication with a microphone or by a few clicks of your computer mouse (or touchpad). You can remain at the

eyepiece while you direct your telescope with verbal commands. There is no need to put a flashlight in your mouth to see

the keyboard. You have total control with your voice and/or mouse. Voice control also allows you to retain your dark

adaptation.

The 1200 is equally at home in a permanent observatory or as a portable mounting for remote star parties thanks to the

ease with which the two axes come apart. This is the perfect mount for a large refractor, Newtonian, Cassegrain or

astrograph.

In order to maximize your pleasure on your first night out, we recommend that you familiarize yourself with the assembly

and basic operation of the mount indoors. The temperature will be comfortable, the mosquitoes at bay, and you'll have

enough light to see the illustrations and read the manual. Please take particular note of counterbalancing, use of the

clutches and operation of the keypad controller.

Why Polar Alignment is Important

Compensation for the Earth’s rotation

If you were to take a long exposure photograph with

Polaris (often called the north star) in the center of the

field, you would discover that all stars seem to revolve

around Polaris. This effect is due to the rotation of the

earth on its axis. Motor driven equatorial mounts were

designed to compensate for the earth's rotation by

moving the telescope at the same rate and opposite to

the earth's rotation. When the polar axis of the telescope

is pointed at the celestial pole (polar aligned) as shown

in Diagram 1, the mount will follow (track) the motions of

the sun, moon, planets and stars. As a result, the object

that you are observing will appear motionless as you

observe through the eyepiece or take astrophotos.

Diagram 1

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ASSEMBLY INSTRUCTIONS

Please read all instructions before attempting to set up your 1200 mount. The Model 1200 is very rugged, however like any

precision instrument, it can be damaged by improper use and handling. Please refer to Diagram 2 for an illustration of the

mount. The parts are labeled so that we can establish common terminology.

The following terms and abbreviations are used interchangeably in these instructions:

polar axis = right ascension axis = R.A. axis = R.A. housing

declination axis = dec. axis = dec. housing

Diagram 2

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Before You Leave Home

Since most of us must set up our instruments in the dark, in the cold or while battling mosquitoes, a bit of preplanning and

organization is important. There are few simple things that can be accomplished in the comfort of your home before heading

outside.

Gross Latitude Adjustment

The total latitude range of the 1200 mount is approximately 20-68 degrees with 4 adjustment positions. Since most

astronomers typically observe within one latitude range, this adjustment is made just once, if at all. Prior to shipment, we

preset the mount to your latitude range for your convenience. If you travel to another observing location, determine the

latitude of your observing site and make the appropriate adjustment.

The four positions for the altitude adjustments have the following approximate ranges:

55 degrees to 68 degrees latitude - top position

37 degrees to 59 degrees latitude - third position

28 degrees to 50 degrees latitude - second position

20 degrees to 37 degrees latitude - bottom position

How to change the position of the altitude adjuster bar

1. Use only the R.A. axis. DO NOT

attempt the make these adjustments

with the declination axis in place and

certainly not with an instrument fully

mounted.

2. Loosen both altitude-locking knobs

about 1 turn.

3. Locate the side of the polar axis that

does not have the motor/gear

housing box. Loosen (about 1 turn)

the polar axis pivot screw and altitude

adjuster bar fixing screws on this side

only. With your hand, push the polar

axis upwards so that the altitude

locking knobs are positioned at the

top of the altitude slot (this is the

maximum altitude position). Some

resistance will be felt with this

operation as you are pushing against

the weight of the polar housing and

the resistance of the remaining polar

axis pivot screw (which has not been

loosened).

Diagram 3

4. Before attempting to move the

altitude adjuster bar, you must tighten

the altitude-locking knob on the motor/gear

housing side. This will prevent any downward

movement of the polar axis during

positioning of the altitude adjuster bar.

5. While supporting the altitude adjuster bar,

remove the two screws that support it on

each side (4 screws in all), but keep the two

ends of the bar in contact with the side of the

mount, don't remove it completely (this tip is

for your convenience).

Diagram 4

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6. Determine the latitude range that you need (refer to Diagram 3)

and position the hole that is marked “A” in Diagram 5 at that

location. Note that this hole is located at the rounded part of the

altitude bar.

7. Attach two of the screws (one on either side of the adjuster bar),

but do not tighten. Rotate the altitude adjuster bar around this pivot

point until one of the other holes lines up. Insert the remaining two

screws. Lightly tighten so that you still have some ability to move

the bar.

8. Note that the altitude adjustment knob is attached to a threaded

rod that travels through the altitude adjuster bar. Turn the knob so

that the altitude adjuster bar is positioned approximately in the

middle of the threaded rod. You should see about half of the

threaded rod protruding from both sides of the altitude adjuster

bar. This will allow you to move the mount fully within the altitude

range.

9. At the end of the threaded rod mentioned in the last step, you will

see a small brass altitude adjuster thrust pad. This is the part that

will come in contact with the polar axis as you ease it back into

position. Loosen the altitude locking knob (motor/gear side) and

lower the polar axis so that it rests comfortably on this pad. The

threaded rod should be positioned at a right angle to the polar axis

housing. Firmly tighten the altitude adjustment screws.

Diagram 5

10. Turn the altitude adjustment knob to raise or lower the polar axis to your approximate observing latitude. Tighten

the altitude locking knobs with finger pressure only. You do not need to tighten with the hex key.

11. Firmly tighten both polar axis pivot screws with the hex key.

Attach Pier Adapter to Pier Post

If you purchased the pier from Astro-Physics, the pier top adapter of the 1200 may be already attached to the top of the

pier. If you are constructing your own pier or tripod, you will need to incorporate this part. The pier adapter was designed to

fit into a 10" x 0.094" wall tube. Use six (6) screws to attach this part. Note that with the Astro-Physics pier, you can orient

the pier adapter so that one of the pier legs faces "north" or "south" as you prefer.

Assemble Pier (purchased separately)

Begin by assembling the portable pier at the

desired observing location. Note which

direction is north.

1. Slide the three legs onto the nubs of

the base and rotate the assembly so

that one of the legs points toward

north (or south, if that is your

preference).

2. Place the pier post on the base

orienting the center azimuth block

directly north. If you choose to have

one leg north, then the pier adapter

plate will have to be installed with the

azimuth block directly over a

turnbuckle. If you have one leg south,

the pier adapter plate will have to be

installed with the azimuth block over

and between two of the pier post

turnbuckles.

Diagram 6

3. Attach the tension rods. The

turnbuckles should be drawn tight

until the whole assembly is stiff enough to support your weight without movement.

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Assemble Polar Axis Assembly to Pier or Tripod

In order to track the motion of astronomical objects, the polar axis must be positioned so that an imaginary line drawn

through the center of the axis points toward the celestial pole. At this stage of the assembly process, you want to position

the mount so that it points roughly north.

1. Remove the four (4) hand knobs on the pier top adapter and keep them close at hand.

2. Prior to lifting the polar axis assembly into place, turn the fine azimuth adjustment knobs so that the space

between them is wide enough to allow the center azimuth block to fit easily between them. Ensure both pier top

and polar axis assembly mating surfaces are clean and free of dirt.

3. Place the polar axis assembly onto the pier top adapter so that the center azimuth block fits between the fine

azimuth adjustment knobs.

4. Move the base of the polar axis assembly so that the threaded holes of the pier top can be seen through each of

the four slots.

5. Thread the four hand knobs loosely in place (you will tighten these later after polar alignment).

Altitude and Azimuth Adjustments - Rough polar alignment

For rough polar alignment, your goal is to sight the celestial pole when looking through the polar alignment sight hole in the

center of the polar axis. You will need to make altitude (up/down) and azimuth (side-to-side) adjustments to the position of

the mount.

We recommend that you do your rough polar alignment with the R.A. axis only since you will be making major adjustments

to the position of the mount at this time. The remainder of the mount, telescope and counterweights would add considerable

weight and require more hand effort. Later, you will do your final polar alignment with the telescope and counterweights

attached, but the adjustments will be small.

1. If the R.A. encoder housing and encoder adapter are installed (part # ENC1200 - Mounted Encoders to use with

Digital Setting Circles - are available as an optional purchase), you may remove them to complete these steps.

Please refer to the section entitled “ Installation of Encoders and Encoder Housings – 1200 Mount“. Alternatively,

you can simply sight up the side of the polar axis to see Polaris.

2. If you examine the polar axis assembly, you will see that the center of the R.A. shaft is hollow. If you have not

done so already, loosen (1/2 turn) the four pier knobs.

NOTE: If you have already attached the Dec. axis, remove the sight hole cover and rotate the internal Dec. shaft

by moving the top of the Dec. axis (or the cradle plate if it is attached) to reveal the sight hole that has been drilled

into it. Now, you can look through the shaft to the other side.

3. Azimuth adjustments: Move the entire pier or tripod east or west until the mount is oriented approximately

towards the pole (an imaginary line drawn through the hollow shaft). Use the two fine azimuth adjustment knobs,

one on each side of the mount, to make adjustments. You must back off the opposing azimuth knob in order to

move the other knob in that direction. Please refer to Diagram 4.

One turn of the azimuth knob is approximately 0.53 degrees (32 arc minutes).

4. Altitude (latitude) adjustments: Loosen the altitude locking knobs. Move the polar axis up or down with the large

altitude adjustment knob located in the front of the polar axis assembly. The tommy bar can be positioned in any

of the threaded holes located in the altitude adjustment knob. Use this bar to help you turn the knob. Please refer

to Diagrams 3 and 4. We have found that fine altitude adjustments also can be made by using the turnbuckle on

the north leg of our pier, if used.

One turn of the altitude knob is approximately 0.5 degrees (30 arc minutes).

5. Continue your azimuth and altitude adjustments until you can sight Polaris in the polar alignment sight hole. At

this point, you have achieved rough polar alignment, which may be sufficient for casual visual observations if you

are not planning to slew to target objects with the keypad. When the R.A. motor is engaged, it will compensate for

the rotation of the earth and keep the target object within the eyepiece field of view. Your target object will slowly

drift since polar alignment at this stage is only approximate. However, you can make corrections with your hand

controller as we will discuss later.

6. Tighten the altitude locking knobs by hand.

7. Tighten the pier knobs firmly by hand.

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Assemble Declination Axis

1. Do not have your telescope or counterweights

connected to the Dec. axis assembly for either

assembly or disassembly of the Dec. and RA axes.

2. Position the R.A. axis as shown in Diagram 7 with the

pocket "A" at the top, opposite the altitude adjuster

knob. Firmly tighten R.A. clutch knobs.

3. During shipment, the Dec. axis assembly lock knobs

will be fully screwed into the Dec. axis. For correct

assembly, these lock knobs should be unscrewed at

least 7 full turns and no more then 8.5 full turns. This

is between 5/16" and 3/8" out from the "shipped"

tightened position.

Note: These lock knobs can be completely removed

from the Dec. axis assembly with about 9.5 full turns

out.

4. Position the Dec. axis above the R.A. axis as shown

in Diagram 8, a light movement (wiggle) in the

downward direction (arrow "A") will help to correctly

seat the principle dovetail(s) and parallel guides.

Diagram 7

5. When both Dec. and R.A. assemblies are fully seated,

hand tighten both Dec. lock knobs.

6. Thread the counterweight shaft into the

Dec. axis.

7. Remove the hand knob and safety

washer from the base of the

counterweight shaft. Add sufficient

counterweights (10 or 18 lb.

counterweights are purchased

separately) to the declination shaft to

balance the telescope you intend to

use. Always use two hands to attach or

move them on the shaft.

8. Reattach the hand knob and safety

washer to the end of the declination

shaft. This will help to prevent injury if

someone accidentally loosens the

counterweight knob.

NOTE: Firm tightening of the

counterweight knob will not damage

the surface of the counterweight shaft.

The pin that tightens against the

stainless counterweight shaft is

constructed of brass. Likewise the

bronze sleeve that has been press fit

into the center of the counterweight will

prevent marring of the shaft as you

move the counterweight up and down.

Removing Declination Axis at the End of

your Observing Session

Diagram 8

1. Unscrew the lock knobs 5.5 to 7 full turns (this is still 5/16" to 3/8" out from the fully tightened position) and

slide/tilt the Dec. axis assembly in an upwards direction (arrow "B").

2. For transport/storage we recommend fully tightening the lock knobs.

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Attach Mounting Plate (purchased separately)

Several mounting plates are available for the 1200 mount. If you own more than one instrument, you may need more than

one plate. Follow the appropriate directions for the plate(s) that you have.

18" FLAT MOUNTING PLATE (FP1800)

This plate is 18" long and 7.5" at its widest point

in the center. The width of the plate tapers to 5.5"

at each end. Four pairs of keyhole slots that

measure 3.2" between centers are provided. The

two inner pairs are 13.75" apart and the outer two

pairs are 17" apart. You can drill additional holes

to suit your needs. This plate also fits the 900

German Equatorial.

Attach this plate with six 1/4-20 x 1" flat head

socket cap screws at the locations indicated by

the filled holes on the diagram.

Diagram 9

15” RIBBED MOUNTING PLATE (1200RP15)

This plate is 14.75” long, 7.75” at its widest point

5” at each end and 1” thick. The underside of the

plate is carved into a ribbed pattern to maximize

the strength and minimize the weight - 3 lbs. A

pair of keyhole slots that measure 3.2” between

centers are provided at each end. The distance

between the pairs is 13.75”.

Attach this plate with six 1/4-20 x 3/4“ socket

head cap screws at the locations indicated by the

filled holes on the diagram. Note that the plate is

asymmetrical. Attach the plate so that the long

end points toward the sky.

Diagram 10

24" RIBBED MOUNTING PLATE (1200RP)

For larger instruments, the ribbed structure

of this plate provides the maximum support.

Our machinist begins with thick aluminum

plate and carves a strong rib structure. The

final result is 1.5" thick, 24" long and 7.6" at

its widest point. The width of the plate

tapers to 5.5" at each end. A pair of keyhole

slots that measure 3.2" between centers are

provided at each end. The distance between

these pairs of holes is 23". Due to the ribbed

structure, you may not be able to drill

Diagram 11

additional holes for non-Astro-Physics

mounting rings. The plate weighs an

amazing 9.5 lbs. for its size. This is a view of the rib structure on the underside of the 24" plate.

Attach this plate with six 1/4-20 x1" socket head cap screws at

the location indicated by the filled holes on the diagram.

DOVETAIL FOR LOSMANDY D SERIES PLATE (DOVELM)

This Astro-Physics plate attaches to the 400, 600E, 900 and

1200 mounts. If you already own one of the Losmandy DAP

series (fits Astro-Physics refractors), DC series (for Celestron

8", 11" or 14" SCTs) or DM series (for Meade 8", 10" and 12"

SCTs) plates, this is the mounting plate for you.

Attach this plate with four 1/4-20 x 3/4" socket head cap screws

and two 1/4-20x5/8" flat head socket cap screws at the

locations indicated by the filled holes on the diagram.

Diagram 12

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Attach Mounting Rings (purchased separately)

Our flat and ribbed plates are constructed with keyhole slots at the location where your mounting rings attach. This feature

enables you to partially loosen the screws on your rings just enough to insert them into the larger part of the keyhole, then

slide the rings to the narrow part and tighten them with a hex key. You can even accomplish this with the rings on the scope,

although this maneuver may be difficult to accomplish with a large, heavy instrument.

We prefer this keyhole method to the standard way of completely removing the screws and dropping them in the grass.

Fine Polar Alignment

For casual observation, you may skip this section and move to “Operation of the Mounting” (tighten your altitude locking

knobs (2) and pier knobs first). If you plan to use any of the go-to functions of the 1200GTO or do astrophotography, you

must polar align.

Methods for fine polar alignment

•

Polar Alignment Scope – Our optional polar scope (PASILL2) will allow you to quickly align your mount on the pole

stars. The reticle was designed for use in both the Northern and Southern hemispheres. Even users of the GTO

computerized mounts will find these polar scopes useful, particularly if your telescope is not orthogonal to the

mount (please refer to the keypad manual for a discussion of orthogonality). If you have a polar alignment scope,

please read the instructions sheets that come with it.

•

GTO Keypad – Please refer to the instruction manual for the GTO Servo Drive and read the section describing the

startup sequence.

•

DigitalSky Voice computer program – Please read the corresponding manual.

JMI Digital Setting Circles – Please read the instructions included with your JMI unit. You must have the encoders

installed on your 1200 mount (part #1200ENC). Refer to the section of this manual entitled “Installation of

Encoders and Encoder Housings –1200 Mount.

•

Star Drift method – Traditionally, this has been regarded as the most accurate method of polar alignment, however

it is also the most time consuming. If you are planning long exposure astrophotos, we suggest that you use the

polar axis telescope, then tweak the final polar alignment by star drifting. Please refer to the “GTO Quick Star Drift

Method of Polar Alignment” procedure in the GTO Keypad Controller Manual. By using these instructions, you can

use modern methods to star drift more rapidly.

Altitude and Azimuth Adjustments

1. Loosen the altitude locking knobs (2) and pier knobs (4) and refer back to the section on “Altitude and Azimuth

Adjustments - Rough polar alignment”.

2. Follow one of the methods of polar alignment mentioned above.

3. When polar alignment has been achieved, tighten at these locations (note that the polar axis pivot screws should

have been tight throughout the fine polar alignment process):

Altitude locking knob (2) - hand tighten

Pier knobs (4) -hand tighten

4. For a permanent installation, all knobs in step 3 above may be firmly tightened with the assistance of a hex

wrench.

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OPERATION OF THE MOUNTING

R.A. and Dec. Damper Knobs

The R.A. and Dec. damper knobs are not intended as axis locks. They should be tightened with light finger pressure so that

a slight resistance can be felt when pushing an unclutched axis by hand. This really adds to the "feel" at the end of the

scope with the drives adjusted correctly.

The purpose of the damper knob is to add a bit of friction to the shaft so that gusty winds do not move the axes in their

bearings. If there is the slightest amount of backlash between worm and worm wheel, a wind load could theoretically move

the axis back and forth by that backlash amount. Also, in the absence of backlash, there is always a very tiny clearance

(.0002") between the shafts and the mating parts. The damper knobs force the shaft to make full contact in 3 places to

eliminate the associated play.

R.A. and Dec. Clutch Knobs

1. What do they do?

The four R.A. and four Dec. clutch knobs depicted in Diagram 2 have the function of connecting the R.A. and Dec.

axes to their respective drive worm wheel gears. Their function is progressive, from no tension (axes free to move

- as required during correct balancing of the telescope) to a completely "locked up" state.

2. How can you find out what they really do?

As shipped, all 1200 mounts have all four R.A. and Dec. clutch knobs firmly hand tightened. This will give you a

good idea of the maximum tightness (clutch action) that can be achieved by hand effort alone. At this point, you

must bear in mind that for optimum performance all four clutch knobs on each axis (R.A. or Dec.) should be

tightened evenly with the same tension i.e. all four half tight, all four fully tight, etc.

In order to feel the effect of the clutch knobs, you may wish to partially assemble your mount. Fit together the R.A.

and Dec. assemblies plus mounting plate and counterweight shaft. Do not put scope and counterweights on at

this stage. With the above assembly (with the clutch knobs firmly hand tightened - "as shipped"), you can feel the

amount of force needed to move each axis by hand. Grab each end of the telescope mounting plate and move it

with a backward and forward movement of the Dec. axis. You will feel considerable resistance to this motion.

Perform the same operation on the R.A. axis by moving the counterweight shaft backward and forward. With a

well balanced telescope, the above tightness of the clutch knobs will be sufficient for all normal conditions of use.

Now if you proceed to mount up and balance your telescope you can "feel" what this resistance in R.A. and Dec.

(movement backwards and forwards) is like when you make these motions from the eyepiece end of your

telescope as you would during normal use when slewing (pushing) by hand to acquire an astronomical object

within the field of view of your finder or scope.

3. How tight can the clutch be and can you do any damage by pushing against them?

The maximum tightness of this clutch system is 1/3 turn (with a 5/32 allen key) further in than the tension you can

achieve with the knobs by hand. You will see that each clutch knob has a 5/32 hex socket for tightening with an

allen key. With this extra 1/3 turn on each clutch knob, the axis (axes) will be considered completely "locked up"

and you should not attempt to push your scope by hand against this "locked up" resistance, or undue stress will

be placed on the worm wheel/worm and bearings.

However, if you are undertaking a very long astrophoto exposure, it is advisable to increase the pressure on each

clutch knob (with the 5/32 key) by about 1/8 turn on Dec. and 1/8th turn on R.A. You may safely slew the scope by

hand with this tension, however you will notice considerably more effort is required to achieve movement. This is

the absolute maximum tension that can be used for hand slewing. As a general rule, if you have a big scope (7" or

8" refractor) with all the accessories, you will need more clutch tension than a 5" or 6" scope.

Balancing Your Telescope

For proper operation, the telescope must be adequately counterbalanced. Start by balancing the tube assembly.

1. Tighten the 4 R.A. axis clutch knobs.

2. Loosen the 4 Dec. axis clutch knobs (about 3/4 to 1 turn) so that the telescope moves freely about the declination

axis (be careful because if your telescope is significantly out of balance, it may swing rapidly in the out-of-balance

direction!)

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3. Position the R.A. axis so that the counterweights are in their "lowest" position i.e. the declination axis assembly is

in the meridian (this is the usual way that German equatorials are depicted, as shown in diagram 2.)

4. Loosen the tube mounting rings and slide the tube up and down for balancing. This is best done with the tube in

the horizontal position.

5. The scope is balanced when it stays put (does not move) with the clutches loose and movement back and forth

about the declination axis has the same feel in both directions.

6. Now, tighten the declination axis clutch knobs and position the telescope horizontal and the declination axis

horizontal. The center of the counterweights is now the same height as the middle of the tube.

7. Loosen the R.A. clutch knobs (again be careful, because if your scope is significantly out of balance, it may swing

rapidly in the out of balance direction).

8. Move the counterweight(s) up or down to achieve the correct balance in R.A. Again, movement back and forth

about the R.A. axis should have the same feel in both directions.

9. Try to anticipate any balance problems due to the extra weight of diagonals, heavy eyepieces, finders, solar filters,

etc. If the scope moves by itself, when the clutches are loose, then the scope is not counterbalanced adequately.

If you are doing astrophotography or imaging, a small amount of imbalance (more weight on the east side of the

mount) is permissible and indeed desirable.

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SERVO MOTOR DRIVE

GTO Control Box – Model GTOCP2

The GTO control box contains all of the circuitry to drive the two servo motors and the logic required to navigate the sky. It

will be operational and track at the sidereal rate when connected to both motors of the mount and a power source. In order

to control the movement of the mount, you will need to connect at least one of these:

•

GTO Keypad controller

Computer with astronomical software such as DigitalSky Voice (included) or Software Bisque’sTheSky™ (purchased

separately).

The GTO Servo Control Box is mounted directly onto the polar axes of the 1200 mount. Please remember that this box

contains advanced electronics and must be treated with the same care given to other fine equipment. You can see that the

unit is built to be rugged, however it is not indestructible.

R.A. and Dec. Cable Connections

A “Y” cable with 10-pin connectors is included with your mount. Attach the connector from which the two cables emerge to

the GTO Control Panel. Attach the short part of the “Y” cable to the R.A. motor housing and the long part of the cable to the

Dec motor housing. Lock all connectors. Refer to the section below for further information about positioning the cables.

12V Connector

Place the DC power cord (included with your mount) into the phono plug outlet marked 12V on the GTO Control Panel and

lock in place. Plug the cigarette lighter plug end of the cord into your power source. The acceptable voltage range is 11.5 to

16. Suggested power sources include: portable rechargeable battery pack, auto or marine battery, or power supply (filtered

and regulated) for 110 volts with a minimum output of 5 amps at 12V DC.

There is no on-off switch. We recommend that you plug the power cable into the servo box after the keypad controller. To

turn the unit off, simply disconnect the power cable.

Considerations for observatory installations: We suggest that you disconnect your GTO Control Box from 110V when

you are not using your mount so that if your observatory experiences a power surge or lightening strike, your mount

electronics will not be damaged. If you operate your mount remotely, you will have to leave your power cable connected

just as you do for the rest of your electronic equipment. You may want to consider surge protectors or other protective

measures to protect from voltage spikes.

POWER Indicator Light

This LED will remain illuminated when your power source has sufficient output to drive the motors. If the voltage falls below

11 volts, the power light will go out and the motors will stop. The keypad controller will not function properly.

For mounts shipped after 02-25-00: If the LED turns yellow, this means that your motors are overloaded, probably due to an

unbalanced load on your mount. Refer to the troubleshooting section of the manual for the solution.

KEYPAD Connector

Attach the 5-pin male connector of the keypad controller and lock in place (push in the knurled ring then turn).

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RS-232 Connectors

These serial port connections are used to connect your mount to your PC computer. You must provide your own straight-

through (non-crossing) cables with a 9-pin (DB9) male connector to interface with the GTO panel. We have provided the

locking posts to secure the cable firmly. If your serial cable does not have a 9-pin connector, you can use a gender changer

or adapter to convert it.

When you are controlling the position of the mount with a computer program such as DigitalSky Voice™ or TheSky™, the

microprocessor chip located in the servo drive box will send continual RA and Dec coordinate data via the cable

connections to your computer. When you use the software to give instructions to slew to a new object, the commands (RA

and Dec coordinates) are sent to the mount.

We provide two serial port connections on the mount so that you can use two software programs simultaneously. For

instance, you can give verbal commands in DigitalSky Voice while using TheSky as a planetarium program. Since the

mount will update the RA and Dec coordinates simultaneously, both programs are continually updated with the data from

the mount. You can watch the screen display of TheSky to see where your telescope is pointing as it slews. This is most

effective if you have a reasonably fast computer with plenty of RAM. If you try this with a 100MHz processor and only 32 MB

of RAM, the response time will be slow since both programs must be continuously updated with position data.

You must have two serial ports available on your computer to take use both serial ports simultaneously. If you use a laptop,

you may need to purchase a PCMCIA adapter to gain an additional serial port. Socket Communications offers adapters for

many computers. Check out their web site at www.socketcom.com.

If you have only one serial port available on your PC and wish to operate DigitalSky Voice and TheSky simultaneously, you

can use the Link Bridge feature of DigitalSky Voice. Please refer to the documentation provided with DigitalSky Voice and

our website for further information.

FOCUS Connector

Attach the 3.5mm phono plug connector of your JMI Motofocus or Meade electric focuser (optional accessories) here. Refer

to the section regarding focus adjustment in the GTO Keypad Manual for instructions on using the keypad controller to

adjust focus. Alternatively, you can verbally control the focus using the Focus Mode of DigitalSky Voice software.

RETICLE Connector

If you wish to use a plug-in type guiding eyepiece with an illuminated reticle (available from several manufacturers), insert

the 3.5mm phono plug into this connector for power. Reticle brightness can be adjusted with the hand control. Refer to the

section pertaining to reticle illuminator adjustment in the GTO Keypad Manual for further information.

AUTOGUIDER Connector

This connector interfaces with the RJ-11-4 modular jack of an autoguider cable, purchased separately or as part of a CCD

Imaging Camera or Autoguider. The autoguider will be functional and ready to go as soon as you plug it in. Please refer to

the appropriate manual from the manufacturer for operation of the autoguider.

We offer cables for all SBIG cameras. Please refer to our price list or call for further information.

+6V Connector

This 6-volt output accepts 3.5mm phono plugs. It is used primarily to power the Pentax 6x7 camera directly from the mount

with a cord sold for that purpose (our part # CORD01).

N and S Switch

Select northern (N) or southern (S) hemisphere as needed. When you slide the switch to the opposite position, the tracking

direction of the drive will reverse. The power cord must be removed and re-attached to make this work.

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Prevent the Cables from Tangling

The movement of the mount across the meridian during slewing functions is calculated so that the cables will not tangle if

they are set up properly. In addition to the motor and power cables that are provided with the mount, you may have

additional cables for other accessories. These may be powered from the GTO Control Panel or from another power source.

We suggest that you position your cabling carefully to avoid a tangled mess. When your cables are set up, move the

telescope manually throughout the normal range of movement to be sure that the cables do not catch on anything and that

you have enough length. Here are a few pointers:

1200 Motor Cables

Note that the “Y” cable for the 1200 mount originates at the GTO Control Panel connector, then splits into two. The short

portion connects to the RA motor box and is not likely to be in the way because this axis remains in the same position. The

longer Dec portion of the cable must be set up properly to ensure that as the Dec axis moves, the cable follows smoothly.

Please insert this cable into the cable mount in the upper left corner of the GTO Servo Control Box as shown above. When

the connector is attached to the Dec motor box, the cable should be positioned as shown in the photograph.

Accessory Cables

Accessories may include Kendrick Dew Removers, CCD cameras and autoguiders, focus motors, illuminated guiding

eyepiece reticles, power cords for the Pentax 6x7 camera, etc. As you attach each accessory, carefully assess the best

position to assure complete movement as your telescope slews from one side of the mount to the other. If an external

power source is used, determine the optimum location for the battery. We prefer to use tie wraps (not glamorous, but

effective) or cable ties (from electronic supply store or catalog) to secure our cables to the mount, telescope, rings or bind

them together. Plastic adhesive cable mounts, available from electronic supply stores, are an alternative choice. We prefer

to use ties since we cannot bear to attach adhesive cable mounts to our telescopes or mounts.

If we use tie wraps to secure several cables together and plan to use that same setup in our next observing session, we

keep the ties in place when we disassemble our equipment. The setup for the next session is much quicker.

Removing the GTO Control Box From 1200 Mount

The GTO control box can be removed easily from the RA axis. It is secured by two 8-32 set

screws located at the base of the GTO Servo Control Box. Loosen the screws with one of the

hex keys from the set included with the mount. Lift the box up from the bottom and tilt so that it

frees from the dovetail connection.

Some people have a permanent observatory, yet prefer to store their electronics in their home

to keep them clean and free of cobwebs. If you do, you may wish to substitute the 8-32

thumbscrews (included with your mount) for the setscrews. This will allow you to remove and

install your GTO control box without tools.

GTO Keypad Controller Operation

Please refer to the manual for the GTO Keypad Controller for complete instructions.

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MOUNT MAINTENANCE AND ALIGNMENT

Under normal operating conditions, minimal maintenance is required. Every 12 months the clutch knobs (4 for Dec. and 4

for R.A.) should be removed and 1 or 2 drops of light oil (3 in 1 household oil) should be put in the exposed hole. If the R.A.

and Dec. axes are attached together for a long time in outside conditions (i.e. in a permanent observatory) then the mating

surfaces should be lightly oiled or greased - if you expect to get them apart again after 10 years.

Your 1200 is a precision instrument with very accurate worm and wheel adjustments. Please be careful if you place the

mount on a flat surface, i.e. the ground or trunk of your car. The gear alignment may be affected if the R.A. and Dec.

motor/gear box assemblies sustain undue lateral force. This is true of any fine instrument. We suggest that you transport

and store the mount in a case or in a well-padded box.

TROUBLESHOOTING

Additional troubleshooting questions are in the GTO Keypad Controller manual. Please refer to them.

The LED on the GTO Control Box changes from red to yellow and the motors stop or go out completely (for

mounts shipped after 02-25-00).

1. The motors are overloaded, probably due to an unbalanced load on your mount.

Rebalance your telescope, and then press one of the N-S-E-W buttons to reset the keypad. Re-enter the last

object on your keypad and the scope will slew to the correct position. Even though your motors had stopped, the

logic in the control box retained the scope position in memory. As long as you didn’t change the pointing position of

the scope, you are still calibrated.

If the scope was moved during re-balancing, simply enter a nearby bright star on the hand controller, press GOTO

and allow the mount to finish slewing. You can then move the scope manually or with the N-S-E-W buttons to

center the star in the eyepiece, and press the #9 RECAL button. This will recalibrate the mount.

Additional explanation: The GTO drive circuit includes logic for overload protection to prevent burning out the

expensive servomotors in case of severe overload on the two axes. The primary cause is an unbalanced load in

R.A. If the extra load opposes the motor rotation, the motor must work harder to track at the sidereal rate and the

current will rise to high levels. If the current exceeds the trip point for more than a minute, the logic will shut the

motor off and tracking stops. It typically takes about 4 lb. of unbalance to trip the overload, but a very heavy load of

scopes, accessories and counterweights on the mount can decrease this unbalance threshold.

2. The voltage of your battery has probably gone below 10.5 volts.

3. The current rating of your AC-DC power supply is too low.

Additional explanation: During slewing, the two motors draw up to 3 amps from a 12 volt source. This may increase

when the temperature approaches freezing or below. It is recommended that your supply be rated at 5 amps, 12

volts DC minimum (18 volts max.). If you also power other equipment (CCD cameras, dew heaters, etc.) from the

same source, you will need a supply capable of up to 10 amps. The more equipment you have, the more current

capability you will need. For portable applications, we recommend a heavy-duty marine battery designed for deep

discharge applications. The most common problems are due to inadequate power supply.

The keypad reset (or locked up) when I plugged my CCD camera, PC (or other equipment) into the same

battery as the GTO mount was using. The battery has a meter which shows 12V.

The meter is reading an average and will not show dips. Gel cells have internal resistance, which will cause voltage drop

when the load changes. When you connect an additional CCD camera and PC the load will drop below 9 volts and the

keypad will reset or it may affect the GTO circuit itself and cause the keypad to lock up.

We recommend that you use a large marine battery that is not a gel cell and hook everything up to it before calibrating the

GTO.

If any problems occur, please don't hesitate to contact Astro-Physics for assistance.

ASTRO-PHYSICS INC

11250 Forest Hills Road

Rockford, IL 61115

Telephone: (815)-282-1513

Fax: (815)-282-9847

[email protected]

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