1600GTO German Equatorial Mount with Standard Temperature Absolute Encoders – Includes APCC-PRO and PEMPro Supply
- Estimated Delivery : Up to 4 business days
- Free Shipping & Returns : On all orders over $200
Why a 1600GTO?
Thirty plus years of mount design and building expertise has been employed to engineer and manufacture our new 1600GTO mount into the most robust, high-precision mount in its class. We have enhanced its design and utility by incorporating additional optional features like absolute encoders and a precision polar scope to meet the needs of even the most demanding astro-imager or visual enthusiast.
We offer three versions: 1600GTO, 1600GTO-AE and 1600GTO-AEL. The latter two versions include the Standard Temperature Absolute Encoders or the Extended Temperature Absolute Encoders, respectively. If you order the 1G00GTO without the absolute encoders, you will be able to purchase them at a later date to install yourself.
This 1600GTO-AE version includes Standard Temperature absolute encoders installed at Astro-Physics prior to shipment.
The 1600GTO mount is built from the ground up to be a precision imaging platform while still remaining totally user-friendly. Consider these advantages and features:
Features to Enhance your Observing or Imaging Sessions
Semi-Portable
Semi-Portable
Extremely solid, rugged, high payload mount, yet the equatorial head comes apart into two components – a true advantage for a mount of this class.
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 15 amp filtered, regulated power supply like our 13.8-volt, 15-amp Power Supply (PS138V15A). For a heavy payload in cold conditions, we offer a 25 Amp Variable Volt Power Supply (PSVPW25A)
Azimuth and Altitude Adjustment is convenient and quick
- Major altitude adjustments are extremely easy to make. Simply shift the position of the bar into a new slot without having to line up obscure holes referenced in the manual. The large captain s wheel knob is also very easy to grasp and turn. If you travel to a star party at a different latitude, you can make changes to your setup very quickly. This also allows you to transport the RA assembly in a more compact, zero degree latitude configuration.
-
- Azimuth adjusters are positioned to the rear of mount which allows you to make minor corrections quite easily without reaching or moving around the mount. Since the knobs are in front of you as you look through the polar scope, the graduations can be more easily seen as you dial in your position.
-
- Built-in precision-rotating pier adapter for smooth azimuth adjustments.
-
- Altitude range now extends from 0-78 degrees, which makes it suitable for most anyone except the extreme polar locations.
-
Through-the-mount cabling
- Motor cables are built into the mount and routed internally to remove the possibility of snagging.
-
- Easily route additional cables through the large openings in the R.A. and Dec. axes. The top of the Dec. axis separates so that you can add cables with large connectors.
-
Clutches
Use the clutches to easily balance your setup, then lock the R.A. and Dec. axes so that they cannot move when the motors are engaged. Manual operation is possible if power is not available.
Image past the meridian
The mount will track and guide well past the meridian in either direction if the object is located so that the telescope will clear the pier. This allows the user to set up the mount for a long series of exposures without stopping in the middle to flip sides. One can start the telescope under the mount while pointing at an object in the eastern part of the sky and track it all the way deep into the western sky. This is very useful for long exposure H-alpha or in cases where a large number of individual exposures are needed for stacking. This feature of our GTO mounts has been a real customer favorite for many years.
Easy polar alignment for critical viewing
Our optional Right-Angle Polar Alignment Scope will allow you to quickly zero in on the pole or the polar alignment routine in PEMPro (included) will guide you through the process. You can even align the mount during the day with our clever Daytime Polar Alignment Routine (outlined in the Keypad Manual) for solar observing, viewing the planets at twilight, or just getting a jump start on a long night.
Multiple Options for Controlling your Mount in the Field or in Your Observatory
You have your choice of the GTO Keypad (KEYVFK2, optional), which is a full-featured handheld computer, PC computers using a wide variety of software with or without our ASCOM driver, Mac computers or even your mobile smart device (like your iPhone or iPad).
Auto-Adjusting Motor Gearboxes
Our motor gearboxes were designed to be responsive for precision astro-photography, while at the same time making it super easy to use and adjust.
- Spring-loaded worms maintain full contact under all guiding and slewing conditions
-
- Automatic setting for worm mesh requires no adjustments over long time periods
-
- Precision balance mechanism allows full backing off the worm from the worm wheel
-
- Inherent very low backlash gear train eliminates Dec reversal delays and provides high position accuracy during guiding. The Absolute Encoders remove any residual backlash for effortless guiding.
-
Absolute Encoders
Absolute Encoders on both axes provide error-free tracking, software readable absolute position, and customizable home and limit functions for robotic imaging.
Mechanical Features
Precise Mechanical Fabrication
Using modern CNC machining techniques, we make all components to a high-precision level, which results in a final package that is solid and accurate in all respects. The critical angles are accurately machined so that the mount is orthogonal to a very high degree. This results in pointing accuracies well below 1 arc minute for a properly aligned mount. Massive thrust bearings and preloaded shaft bearings provide excellent stability under all imaging situations.
Easy to Adjust and Maintain
The design of the 1600GTO is straightforward and easy to maintain. We provide information in the Support section of our website pertaining to typical adjustment issues.
Components are modular.
All electronics including the GTOCP4 control box, motors, gearbox or cables can be removed for servicing. The RA and Dec axes can be shipped separately, if needed.
GTO Servo Drive System
Gear Accuracy and PE Performance
The GTOCP4 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 and repeatable from one worm cycle to the next, which enables PE correction to be very accurate. The system can be precisely controlled over a speed range of 4800:1, which allows 0.25x sidereal for manual guiding to 1200x sidereal for 5 degree per second slewing. The circuit draws approximately 0.5 amps when tracking the stars, 2.5 amps with both motors slewing and requires only 12 volts to operate. The servo drive will satisfy the requirements of the sophisticated, advanced astro-imager, yet is easy for the casual, visual observer to use.
The heart of this mount is a precision gearbox using custom high-quality fine-pitch gears, coupled to a highly accurate worm and worm wheel. These parts are manufactured and assembled at our facility and individually tested to meet or exceed our periodic error specification of 5 arc seconds (+ – 2.5 arc sec.) before introducing any periodic error correction. The PE is smoothly variant with extremely low ripple or moment to moment error. In contrast, mounts that use commercial gearboxes have very small spur gears with tiny teeth and too few of them. This generally causes ripples in the tracking rate which are difficult to guide out.
Each mount is rigorously tested on our specialized periodic error tester. Only mounts that provide an accuracy of 5 arc seconds or better will pass this inspection. If the mount exhibits greater error, the substandard part is identified, replaced and the mount is retested.
Continual PEM Correction with the Absolute Encoders
As mentioned above, the spec of 5 arc seconds (+ – 2.5 arc sec.) is the maximum native mechanical error inherent in the mount s RA axis WITHOUT any software correction. The Absolute Encoders eliminate any remaining periodic error to continually optimize your mount s performance. You will not have to do periodic PEMPro runs like you would with non-encoder mounts. However, we include PEMPro so that you can utilize the polar alignment feature.
GTOCP4 Control Box
The GTOCP4 Control Box offers multiple connection options to suit your requirements including Wi-Fi, ethernet, USB and serial ports. In addition to all the features carried forward from previous control boxes, the GTOCP4 applies safety slew logic to all slew commands. Future software updates will be available via downloads from the Software Updates tab of our website.
The GTOCP4 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 1600GTO uses the same GTOCP4 Control Box as 1100GTO and Mach1GTO. In fact, the control boxes for all three mounts are interchangeable with one another in an emergency. However, the absolute encoder function is only available in the control boxes sold with those mounts.
Be sure to review extensive information regarding the GTOCP4.
GTO Keypad (optional purchase)
The Keypad (KEYVFK2) is a self-contained computer that allows you to control all essential telescope functions and includes an extensive database of objects. Many people do not want to bother with a computer in the field and like the handiness of the Keypad and its ability to operate in very cold temperatures. The Keypad is an ideal choice for these users.
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.
Optimized for Astronomy
Astro-Physics mounts and the Astro-Physics GTO Servo Control System are designed from the outset as tools for celestial observing and imaging. These mounts do not have any military or defense applications. Applications like missile, airplane, or very low earth orbit satellite tracking require faster tracking rates and more rapid changes to those tracking rates than our mounts allow. Note that the ISS is generally within the mount’s tracking rate capabilities.
Specifications
Dimension Calculator
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.
Mechanical Specifications
- Major altitude adjustments are extremely easy to make. Simply shift the position of the bar into a new slot without having to line up obscure holes referenced in the manual. The large captain s wheel knob is also very easy to grasp and turn. If you travel to a star party at a different latitude, you can make changes to your setup very quickly. This also allows you to transport the RA assembly in a more compact, zero degree latitude configuration.
- Azimuth adjusters are positioned to the rear of mount which allows you to make minor corrections quite easily without reaching or moving around the mount. Since the knobs are in front of you as you look through the polar scope, the graduations can be more easily seen as you dial in your position.
- Built-in precision-rotating pier adapter for smooth azimuth adjustments.
- Altitude range now extends from 0-78 degrees, which makes it suitable for most anyone except the extreme polar locations.
-
- Motor cables are built into the mount and routed internally to remove the possibility of snagging.
- Easily route additional cables through the large openings in the R.A. and Dec. axes. The top of the Dec. axis separates so that you can add cables with large connectors.
-
- Spring-loaded worms maintain full contact under all guiding and slewing conditions
- Automatic setting for worm mesh requires no adjustments over long time periods
- Precision balance mechanism allows full backing off the worm from the worm wheel
- Inherent very low backlash gear train eliminates Dec reversal delays and provides high position accuracy during guiding. The Absolute Encoders remove any residual backlash for effortless guiding.
-
Absolute Encoders
Absolute Encoders on both axes provide error-free tracking, software readable absolute position, and customizable home and limit functions for robotic imaging.
Mechanical Features
Precise Mechanical Fabrication
Using modern CNC machining techniques, we make all components to a high-precision level, which results in a final package that is solid and accurate in all respects. The critical angles are accurately machined so that the mount is orthogonal to a very high degree. This results in pointing accuracies well below 1 arc minute for a properly aligned mount. Massive thrust bearings and preloaded shaft bearings provide excellent stability under all imaging situations.Easy to Adjust and Maintain
The design of the 1600GTO is straightforward and easy to maintain. We provide information in the Support section of our website pertaining to typical adjustment issues.Components are modular.
All electronics including the GTOCP4 control box, motors, gearbox or cables can be removed for servicing. The RA and Dec axes can be shipped separately, if needed.GTO Servo Drive System
Gear Accuracy and PE Performance
The GTOCP4 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 and repeatable from one worm cycle to the next, which enables PE correction to be very accurate. The system can be precisely controlled over a speed range of 4800:1, which allows 0.25x sidereal for manual guiding to 1200x sidereal for 5 degree per second slewing. The circuit draws approximately 0.5 amps when tracking the stars, 2.5 amps with both motors slewing and requires only 12 volts to operate. The servo drive will satisfy the requirements of the sophisticated, advanced astro-imager, yet is easy for the casual, visual observer to use.
The heart of this mount is a precision gearbox using custom high-quality fine-pitch gears, coupled to a highly accurate worm and worm wheel. These parts are manufactured and assembled at our facility and individually tested to meet or exceed our periodic error specification of 5 arc seconds (+ – 2.5 arc sec.) before introducing any periodic error correction. The PE is smoothly variant with extremely low ripple or moment to moment error. In contrast, mounts that use commercial gearboxes have very small spur gears with tiny teeth and too few of them. This generally causes ripples in the tracking rate which are difficult to guide out.
Each mount is rigorously tested on our specialized periodic error tester. Only mounts that provide an accuracy of 5 arc seconds or better will pass this inspection. If the mount exhibits greater error, the substandard part is identified, replaced and the mount is retested.
Continual PEM Correction with the Absolute Encoders
As mentioned above, the spec of 5 arc seconds (+ – 2.5 arc sec.) is the maximum native mechanical error inherent in the mount s RA axis WITHOUT any software correction. The Absolute Encoders eliminate any remaining periodic error to continually optimize your mount s performance. You will not have to do periodic PEMPro runs like you would with non-encoder mounts. However, we include PEMPro so that you can utilize the polar alignment feature.
GTOCP4 Control Box
The GTOCP4 Control Box offers multiple connection options to suit your requirements including Wi-Fi, ethernet, USB and serial ports. In addition to all the features carried forward from previous control boxes, the GTOCP4 applies safety slew logic to all slew commands. Future software updates will be available via downloads from the Software Updates tab of our website.
The GTOCP4 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 1600GTO uses the same GTOCP4 Control Box as 1100GTO and Mach1GTO. In fact, the control boxes for all three mounts are interchangeable with one another in an emergency. However, the absolute encoder function is only available in the control boxes sold with those mounts.
Be sure to review extensive information regarding the GTOCP4.
GTO Keypad (optional purchase)
The Keypad (KEYVFK2) is a self-contained computer that allows you to control all essential telescope functions and includes an extensive database of objects. Many people do not want to bother with a computer in the field and like the handiness of the Keypad and its ability to operate in very cold temperatures. The Keypad is an ideal choice for these users.
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.
Optimized for Astronomy
Astro-Physics mounts and the Astro-Physics GTO Servo Control System are designed from the outset as tools for celestial observing and imaging. These mounts do not have any military or defense applications. Applications like missile, airplane, or very low earth orbit satellite tracking require faster tracking rates and more rapid changes to those tracking rates than our mounts allow. Note that the ISS is generally within the mount’s tracking rate capabilities.
Specifications
Dimension Calculator
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.
Mechanical Specifications
Clutches
Use the clutches to easily balance your setup, then lock the R.A. and Dec. axes so that they cannot move when the motors are engaged. Manual operation is possible if power is not available.
Image past the meridian
The mount will track and guide well past the meridian in either direction if the object is located so that the telescope will clear the pier. This allows the user to set up the mount for a long series of exposures without stopping in the middle to flip sides. One can start the telescope under the mount while pointing at an object in the eastern part of the sky and track it all the way deep into the western sky. This is very useful for long exposure H-alpha or in cases where a large number of individual exposures are needed for stacking. This feature of our GTO mounts has been a real customer favorite for many years.
Easy polar alignment for critical viewing
Our optional Right-Angle Polar Alignment Scope will allow you to quickly zero in on the pole or the polar alignment routine in PEMPro (included) will guide you through the process. You can even align the mount during the day with our clever Daytime Polar Alignment Routine (outlined in the Keypad Manual) for solar observing, viewing the planets at twilight, or just getting a jump start on a long night.
Multiple Options for Controlling your Mount in the Field or in Your Observatory
You have your choice of the GTO Keypad (KEYVFK2, optional), which is a full-featured handheld computer, PC computers using a wide variety of software with or without our ASCOM driver, Mac computers or even your mobile smart device (like your iPhone or iPad).
Auto-Adjusting Motor Gearboxes
Our motor gearboxes were designed to be responsive for precision astro-photography, while at the same time making it super easy to use and adjust.
Through-the-mount cabling
