Why a 1200GTO?
With the advent of the CCD camera, amateurs are exploring the skies to an ever increasing level of precision, easily exceeding the image quality of large observatories using film techniques decades ago. This new level puts a higher demand on the precision of the equatorial mounting. Many of the finest imagers today have been using our GTO mounts as a solid platform for a wide variety of instruments. Until the introduction of the 3600GTO at the Advanced Imaging Conferrence in 2007, the largest of these was our 1200GTO.
Since its introduction in 1998, the 1200GTO has gained a reputation for both tracking and pointing accuracy, essential to casual visual observation as well as advanced imaging. Quite a few 1200GTO and 900GTO (smaller cousin) mounts can be found at Mount Pinos in California, favorite observing site of many advanced photographers and imagers. You will find them at star parties and in observatories throughout the world.
These mounts are truly a marvel of engineering - maximum strength and rigidity with minimum weight. Our CNC lathes and mills carve out the excess material in both axes of the 1200 and 900 German Equatorials 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.
Over the years, a number of improvements have been incorporated into the design of the 1200GTO, among these are smoother azimuth adjusters; increased height of the polar forks to allow more room for your hand when making altitude adjustments; rounded profile of the base to prevent cords from catching; improved gear profiles in the motor gearbox for quieter operation and reduced backlash; motor bracket with built-in spring-action to keep the worms loaded at the proper setting; verifiable worm gear accuracy of 5 arc seconds or less; internal changes to improve overall accuracy; several pier adapter options; updated GTOCP3 control box with additional capability; updated keypad with larger memory capacity and LED fiber optic backlit panel; included PulseGuide and PEMPro software as described below. Each time we begin a production run, we ask ourselves what improvements we can make to improve the accuracy and functionality of the 1200GTO. As a result, the 1200GTO has evolved over the years to meet the needs of the advanced imager or visual observer.
The 1200 equatorial 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. You CAN have it all. This is the perfect mount for a large refractor, Newtonian, Cassegrain or astrograph. Telescopes commonly used include Astro-Physics 155-206mm refractors, 12-14" Schmidt-Cassegrains and 10-16" Ritchey-Chretiens and other instruments of similar size.
Our customers have been our greatest promoters through the years. Look for them at your next star party, read a few comments we have gathered and check out photos of various scopes on the 1200GTO. You are also welcome to ask any questions or check the archives of the ap-gto users group.
The 1200GTO mount is built from the ground up to be a precision imaging platform while still remaining totally user friendly. Consider these advantages and features:
Extremely solid, rugged, high payload mount, yet the equatorial head comes apart in two reasonably light-weight components for hassle-free field setup. No tools needed to assemble the mount in the field.
Operate with 12V battery.
You can take it to the darkest skies and power it with a commonly available 12V battery. In the observatory, we suggest a minimum 5 amp filtered, regulated power supply like our 13.8V, 5 amp Power Supply (PS13V5A). For a heavy payload in cold conditions, we offer a 15V, 10 amp power supply (PS15V10AC).
Clutches and setting circles.
Allow manual operation if power is not available.
|The 1200GTO’s ability to continue tracking when past the meridian is an absolute winner for me. It avoids meridian flips (=imaging time) and reduces the need for expensive rotators. Jan Rek. More…|
|. . . I love the ability to place the OTA on the "wrong side" of the mount when starting an imaging session ("premature meridian flip") and which I have used extensively. This feature is pure INGENUITY! Anthony Ayiomamitis., More…|
If your computer does not have serial port inputs, there are many USB to serial port adapters available on the market. Serial to USB connectivity has been simplified by the addition of Keyspan Serial-to-USB devices to our product line. Please review the products on this page to determine which one will work best for your set-up.
|I love my mount! And, it works just great in an automated setup! In fact, it's just waiting for ACP to start imaging once it gets a bit darker! James McMillan. More…|
Precise Mechanical Fabrication.Highly accurate mechanics.
|… did some autoguide testing and the results were very good – what strikes me was now smooth the PE was. James Providakes. More…|
|R.A. worm wheel||10.3" (26.2cm), 225 tooth aluminum|
|Declination worm wheel||7.2" (18.3cm), 225 tooth aluminum|
|R.A. shaft||3.35" (8.5cm) diameter|
|R.A. thrust bearings||9.5" (24.1cm) diameter|
|Dec. shaft||2.36" (6.0cm) diameter|
|Dec. thrust bearings||6.5" (16.5cm) diameter|
|Latitude range||22 to 69 degrees|
|Azimuth adjustment||Approximately 14 degrees|
|Setting circles||Porter Slip Ring design, engraved, pointer|
|Right ascension||4-minute increments, pointer, engraved both Northern/Southern|
|Declination||1 degree increments, engraved, pointer|
|Instrument Mounting||Click here for a PDF drawing of the declination hub hole-pattern.|
Approximately 140 lb. (63.6kg) scope and accessories, depending on length. Will accommodate Astro-Physics and similar refractors up to 206mm f8, 16" Cassegrains and Ritchey-Chretiens, 17" CDK
|Weight|| Equatorial head: 81
lbs. (36.7 kg), Dec axis is 31 lbs. (14.1kg), RA
axis is 50 lbs. (22.7kg)
Counterweight shaft: 14 lbs. (6.4kg)
Servo Motor Drive
The drive system uses a high-quality Swiss DC servo motor controlled by a microprocessor to an accuracy of 0.05 arc seconds per step. Tracking is very smooth, noticeably smoother than any stepper motor drive or inexpensive servo drive. The system can be accurately controlled over a speed range of 4800:1 which allows 0.25x sidereal for guiding to 1200x sidereal for 5 degrees per second. The circuit draws only 0.4 amps when tracking the stars, 2 amps with both motors slewing and requires only 12 volts to operate. This servo drive will satisfy the requirements of the sophisticated, advanced astrophotographer, yet is easy for the casual, visual observer to use. Please refer to GTOCP3 Control Box and Keypad for Servo Drive for additional information.
The GTOCP3 Control Box contains all of the circuitry to drive the two servo motors and the logic required to navigate the sky. It can be easily removed from the mount, if required.
The GTO Keypad is a self-contained computer that serves as the communication center for the operation of your GTO mount. We have designed the interface and firmware to be as intuitive and easy to use as possible while filling it with terrific features to make your observing session productive and pleasurable.
All of the 1200GTO electronics are now lead-free. Astro-Physics believes that we who love the night sky should also love and protect our good earth. Please refer to GTOCP3 Control Box and Keypad for Servo Drive for more detailed information.
PulseGuide is a stand-alone Windows (98, ME, 2000, NT4, XP, Vista and Windows 7) utility that provides complete remote control of Astro-Physics Mach1GTO, 400GTO, 600EGTO, 900GTO, 1200GTO and 3600GTO mounts. It derives its name from its most distinctive feature, pulse guiding, which can improve unguided tracking. Specifically, it can help correct tracking errors caused by polar misalignment and atmospheric refraction. You can also train PulseGuide to track objects moving relative to the stars, such as asteroids, comets, and the moon. In addition to pulse guiding, PulseGuide also has many useful utility features. With just a few exceptions, it supports the entire serial Astro-Physics command protocol. More ....
PulseGuide was written by Ray Gralak of Sirius-Imaging. Please refer to his web site http://www.pulseguide.com for further developments and enhancements. The software will be provided on a CD-ROM with your 1200GTO mount. Previous owners of any Astro-Physics mounts can download the software free-of-charge, courtesy of Ray. Many, many thanks to Ray for this powerful program.PEMPro Software, Version 2
Pier Adapter Options
Prior to 2004, the Standard Pier Adapter was included with the mount, however there are now several options available for your consideration. If you plan to have multiple pier installations, perhaps one permanent and another portable, you may wish to purchase an extra adapter to install on the the second pier. This will make your setup and switchover much quicker. Many customers have found this to be advantageous.
If you do not purchase one of our pier adapters described below, for instance, if you purchase the Monolith Pier from Particle Wave Technologies, you will need to purchase the Pier Adapter Knob Kit (part# 12KBKIT) in order to attach your mount to the Monolith.Standard Pier Adapter (1200SPA)
The diagram shows several dimensions that are commonly requested. In addition, if the scope is horizontal and pointing north or south, the measurement from the top of the pier to the middle of the cradle plate is 11.25." Please note that these dimensions will vary somewhat depending on your latitude. We quote them for 42 degrees because that is the latitude of Astro-Physics and all of our equipment is set up that way. It is also a good average value.
To determine the appropriate pier height for your system and to calculate many of the dimensions that vary with your latitude setting, please try this Excel spreadsheet Latitude Dimension Calculator.
All Astro-Physics mounts are supported by a dedicated staff who will assist with any issues that may arise. You can talk to a real person in a timely manner. Astro-Physics staff also participate the ap-gto user groups in the Yahoogroups forum. The user group is comprised of GTO owners who are willing to share their wealth of experience using their mounts as well as imaging strategies and other concerns of advanced amateurs.
We have prepared some pertinent support documents relating to this mount and many of our other products on our Technical Support page. You may find the information that you need simply by clicking here.
Price and Delivery Information
With rare exception, the 1200GTO is
not available on the shelf for immediate purchase. We typically maintain notification
lists so that we can notify prospective customers when the mount is available
to order. Please refer to our availability page for more information
on our notification lists. If you are not already on the notification list for
the 1200GTO, you can sign up on our online
notification form. An automatic confirmation e-mail will be sent to you
for your records. Refer to Notification
Update periodically to find out the status our mount and telescope production
runs - what we are making throughout the year.
Price and availability
|1200GTO||$9,950.00||NO LONGER AVAILABLE|
1200GTO - What's Included?
Items that You will Need for Your Mount
Additional Accessories to Consider
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Inc. - All Rights Reserved
This page was last modified: September 20, 2013
11250 Forest Hills Road, Machesney Park, IL 61115, U.S.A.
Phone: 815-282-1513 Fax: 815-282-9847