Astro-Physics – High-end German Equatorial Mounts

HIGH-QUALITY PROFESSIONAL ASTRONOMICAL MOUNTS

Astro-Physics 130mm/ f/6.3 StarFire GTX Refractor "Gran Turismo"

Astro-Physics 130mm/ f/6.3 StarFire GTX Refractor "Gran Turismo"

Keeping to the same quality standards that have made the fully-apochromatic refractors legendary, Roland Christen's company has been building German Equatorial GoTo mounts for more than three decades. Their proven stability, accuracy and durability is the reward for anyone who can endure the traditionally long delivery times.

"El Capitano" at Dome C of the Concordia Station in Antarctica"

"El Capitano" at Dome C of the Concordia Station in Antarctica"

Two "el Capitan" mounts are working in the Antarctic for several years now, even at temperatures of -75°C. They are perhaps the most spectacular example of the durability of the sturdy Astro-Physics mounts and are representative for many more exemplars that often run for decades at our customers without failures.

Astro-Physics GTO 1600

Astro-Physics GTO 1600

With a very accurate manufactured worm gear the Astro-Physics mounts are equally well-suited for smooth, effortless tracking of celestial objects as well as for all visual and photographic purposes.

Astro-Physics supplies 4 mounts with 30kg to 135kg instrument load. The GTO 1100 and GTO 1600 series are especially remarkable, because they are fully transportable - despite their high instrument load. This is possible because the declination axis can be separated from the rest of the mount. Even the GTO 1600, with 90 kg instrument load, can be transported and set up by one person!

Astro-Physics GTO-1100

The separation of RA and DE axis and on the right: The CNC machined dovetail of the RA axis to accommodate the DE axis

The connection of the two components is achieved by a CNC-machined dovetail receptor clamp which has the same uncompromising stability. This is also used by "normal" dovetails.

In the case of the GTO3600, the declination axis can also be separated, but this mount is transportable only to a limited extent and better used as a stationary mount.

At the moment, the GTOMACH1 is the only mount of German design in its weight class, in which ALL cable connections to the telescope (CCD camera, electric focusing, etc.) are passed through the polar axis.


State-of-the-art CNC machine technology and hydraulic circular grinding machines

All parts of Astro-Physics mounts have been CNC-machined and milled out of solid aluminum. In this way, it is possible to circumvent the expensive, labor-intensive production of blanks made of aluminum sand casting.

By using state-of-the-art CNC machining techniques, where surface and angular(!) accuracies of 1 micron allow highly accurate fits, all "blind" volumes of axis and housing parts that do not contribute to the rigidity of the design are erased from the solid aluminum.

Due to the ingenious combination of two tapered roller bearings and three thrust bearings in each of the two housing parts, the axles themselves are even more relieved and stabilized by the shape of the axle housing. This results in a mount of high rigidity and freedom from vibration with a surprisingly low weight.

Features of GTO Servo Drive (applies to all 4 models)Astro-Physics GTOCP4

Why does Astro-Physics choose servomotors instead of stepper motors to drive their mounts?

The torque and thus the acceleration of stepper motors reaches their maximum value at low frequencies and drops sharply at high frequencies. Therefore, relatively large motors are necessary to develop enough torque for positioning at the required speeds. At low speeds, so like during normal tracking, such engines have far too much force and then often run uneasily, which can easily lead to vibrations of the telescope.

In addition, stepper motors have natural resonances. In these frequency ranges, the smoothness deteriorates again rapidly. Servo motors, on the other hand, are characterized by high torque even at high speeds, very good running smoothness over the whole speed range and higher efficiency. In order to obtain the same positioning accuracy as with stepper motors, however, a higher electronic effort must be driven.

All functions of the servo drive can be controlled from a laptop or PC. Astro-Physics has a fully supported, working ASCOM V2 driver for all Astro-Physics GTO mounts. This is the recommended method for controlling the mount with a personal computer under the Windows operating system. Please refer to this link http://www.astro-physics.com/index.htm?products/accessories/software/ascom/ascom für weitere Informationen und Links zu der ASCOM-Plattform und dem Astro-Physics V2 ASCOM-Treiber.

 

GTOCP4 Controll Box for Servo Drive

For the first time in a couple of years Astro-Physics introduces a new control electronic, the GTOCP4 for all Astro-Physics mounts. All GTO mounts produced since 1998 can easily be upgraded.

Some Features of the GTOCP4:

  • completely redesigned with modern chip technology, resulting in faster processing speed and increased memory capacity for future feature additions
  • GTOCP4 supports floating point operands to improve calculation accuracy and coordinate conversions
  • includes features from the latest version of the GTOCP3
  • Backward Compatibility: All of this is in a compact size that fits all previous GTO mounts (400 GTO, 600 E, Mach 1, 900/1100/1200/1600 and und 3600 GTO)

Further information and technical details about the GTO Control Box are available here.

 

Astro-Physics Keypad

GTo in Perfection via Handcontroller (optional)

ALL Astro-Physics mounts with servo motors are controlled via the GTO control system and can be operated completely via the keypad. The interface between the hand control and the mount is the GTO control box. It is mounted directly on the pole block, except at the MACH1. There, the GTO control box is attached at the tripod.

The Keypad can be used with all versions of the Astro-Physics GTO Control Boxes: GTOCP1, GTOCP2, GTOCP3 and GTOCP4.

The Keypad is intuitive and easy to use and is equipped with great features to make the observing session productive and pleasurable. Entering long, hard-to-remember keyboard sequences has been deliberately avoided.

This "handheld computer", which even cold winter nights can not harm, is the usual hand control box for controlling the mount equipped with a variety of options:

  • programming of the periodic worm error and the gear play in right ascension and declination are possible, of course
  • fully automatic positioning of the mount on the object you have entered
  • a choice of different correction and pointing speeds are available
  • contains more than 17,000 objects in extensive databases
  • mehrere eingebaute Software Routinen erlauben eine schnelle und einfache Justierung der Polachse
  • several built-in software routines allow quick and easy polar alignment

The control software can be updated via internet. A PC or laptop is not needed. If required, all mounts can also be controlled via the following external software packages:

  • PulseGuide
  • TheSky
  • GUIDE
  • Desktop Universe Earth Centered Universe (ECU)
  • SkyMap Pro
  • Starry Night Pro
  • any software that is ASCOM compliant. .

Further information and technical details about the GTO Keypad is available here.

 

Further information and technical details about the Astro-Physics German Equatorial Mounts is available here:

Astro-Physics 1100 GTO

Astro-Physics GTO-1100

Astro-Physics 1600 GTO

Astro-Physics GTO-1600

Astro-Physics GTO-MACH 1

Astro-Physics 3600 GTO

Astro-Physics GTO-3600


Delivered over a period of almost 15 years, the GTO 1200 is no longer available and will be replaced by the GTO 1600 (LINK TO THE PRODUCT). More information about the GTO 1200 and other older mounts can be found on the Astro-Physics product history page.


Accessories for the GTO mounts from Astro-Physics

Of course, there are many mechanical accessories for the mounts - from the instrument mounting plate to dovetail clamps to the transportable pier. - For details, see our Astro-Physics price list or visit the Astro Physics website (www.astro-physics.com).

 

 

Leave a Reply