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Astro-Physics Mach1GTO CP4 German Equatorial Mount with Keypad

Astro-Physics Mach1GTO CP4 German Equatorial Mount with Auto-Adjusting Motor/Gearboxes and Astro-Physics GTO Keypad controller.

8 999,00 €

-322,00 €

9 321,00 €

Pack description

Astro-Physics Mach1GTO CP4 German Equatorial Mount with Auto-Adjusting Motor/Gearboxes and Astro-Physics GTO Keypad controller.

Pack content

Astro-Physics Mach1GTO CP4 German Equatorial Mount with Auto-Adjusting Motor/Gearboxes: observatory performance in a lighweight and transportable size!

The Mach1GTO will be the first Astro-Physics mount to ship with the long-awaited GTOCP4 Control Box and feature a completely new Auto-Adjusting Motor/Gearboxes.

The new Astro-Physics GTO CP4 control panel

GTOCP4 Control Box

The GTOCP4 Control Box offers multiple connection options to suit your requirements including wifi, 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 firmware updates will available via direct downloads.

See dedicated page for further details.

Auto-Adjusting Motor/Gearboxes

The all new motor/gearboxes were designed to be more responsive for precision astro-photography, while at the same time making it super easy to use and adjust. Here are some key features:

  • Spring-loaded worms maintain full contact under all guiding and slewing conditions
  • Automatic setting for worm mesh requires no adjustments over long time periods
  • Very easy to do precision balance by new mechanism which allows full backing off the worm from the worm wheel
  • Very low backlash geartrain eliminates Dec reversal delays and provides high position accuracy during guiding
  • Geartrain components are made with high-strength stainless alloy for extremely low wear even with continuous slewing applications
  • Worms made with high-strength alloy eliminates wear during long periods of slewing, especially useful for remote setups that do survey work
  • All worms are tested to meet stringent periodic error specs. Error is measured with PEMPro and the resultant compensating curve is loaded into the servo controller so you can use the PEM function to remove 90% of the variability even in non-encoder mounts

Why a Mach1GTO?

There is much to admire in the Astro-Physics Mach1GTO. It is beautifully machined, intelligently designed, precisely fabricated and assembled, and it has sophisticated electronics and servo drive controls. But the bottom line is performance and results. In February 2007, Roland posted results of a very cold imaging session to the the Yahoo ap-gto group. The mount performed beautifully, and the results posted here prove it.

Whether your Astro-Physics Mach1GTO makes a permanent home in your observatory, explores your favorite observing sites or travels to the ends of the earth with you, it will allow you to optimize your observing sessions to the max. Ideal instruments include: Astro-Physics and similar fast refractors up to our 160 mm f7.5 StarFire EDF, 8-11" SCTs, 6-8" Maks or any scopes of a similar size.

As Roland Christen, founder of Astro-Physics, has stated many times: "The single most important item for the imager is the mount. Next comes the mount. Then comes the mount.... Get the picture?"

Versatility of the Astro-Physics Mach1 GTO

Portable Enough for Airline Travel
Transport this rigid observing platform to your dream destination. The entire mount will fit into a single rugged case that will roll easily through airports or to your car. If needed, the R.A. and Dec. axes split easily into two pieces to fit into a more compact case.

Operate with 12V battery or Regulated Power Supply
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.

Image Past the Meridian
The mount will track and guide well past the meridian in either direction if the object is located such 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.Dennis di Cicco had this to say about the "powerful meridian delay feature" in his 2007 review:

". . . makes it easy to set up photographs that track across the meridian without interruption. It may sound like a small feature on paper, but I found it extremely useful in the field . . ."



Easy Alignment for Non-critical Observing
You can align the Astro-Physics Mach1GTO using setup routines in the keypad to quickly zero in on the pole for most non-critical observing or to get close before tweaking in for imaging. 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. Optional polar alignment scopes, discussed below, are available for more critical alignment

Multiple Options for Controlling your Mount in the Field or Your Observatory
You have your choice of the GTO Keypad (now 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).

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.

Although the Astro-Physics Mach1GTO is very light for its size and load rating, it has been machined out of solid aluminum to withstand the high axial and thrust loads that a medium-sized telescope places on the mount under real-world observing conditions. The mount is solidly built and will withstand gusting winds without excessive shake or vibration. We used high-quality machine tool bearings, rated in excess of 400 lb. static and dynamic load, on the main axis shafts. Both worm wheels turn smoothly with no runout throughout their 360 degree range.

Dennis di Cicco had this to say about the Mach1GTO's performance:

"The mount’s tracking and Go To pointing are among the most accurate I’ve ever tested. At the end of each night I’d park the scope and turn off the power. Whether an hour, day, or week elapsed until I’d power up the mount again and “resume from park," it would have perfect sync with the sky — even to the point of “hiding" stars behind my finderscope’s crosshairs when I’d check the alignment by slewing to them in a bright twilight sky . . .

Such Go To pointing precision comes in handy when shooting photographic mosaics, making a sequence of deep exposures of the same field on multiple nights, or hunting difficult targets by eye."



Precision-Adjust Rotating Pier Base / Hi-Res Azimuth Adjuster
The Precision-Adjust Rotating Pier Base / Hi-Res Azimuth Adjuster offers the same smooth and precise rotation as experienced when using the precision-adjust rotating pier adapters with our larger mounts. Regardless of the mount's load, hi-res adjustments can be made in azimuth with no lockdown needed, which could shift your position.

The azimuth adjuster knobs are now at the rear of the R.A. axis, which provides easier access and nearly doubles the precision of their adjustments. An etched line on the adjuster housing corresponds with the ridges of the knobs to provide a measured adjustment of 0.7021 degrees (42 arcminutes) per rotation or 0.05 degrees (3 arcminutes) per ridge.
 

Clutches and Interchangeable Motor / Gear Boxes
Clutches allow manual operation if power is not available. The R.A. and Dec. Motor / Gear Boxes are interchangeable.

Easy to Adjust and Maintain
The design of the Astro-Physics Mach1GTO is straightforward with modular construction and no complicated internal wiring. We provide information in the Technical Support section of our website pertaining to typical adjustment issues. All electronics including the GTOCP3 control box, motors, gearbox or cables can be removed for servicing. The R.A. and Dec. axes can be shipped separately, if needed.

Route your cables through the mount for tangle-free operation and peace of mind.
Both axes have 2 inch clearance holes down the center with no shafts protruding into the holes. Wires from CCD cameras and accessories can be inserted from the bottom of the RA axis to emerge from the top of the Dec axis. Channels have been machined to allow the cables to be routed under the mounting plates. There is no restriction of rotation with the wires inserted - one can rotate both axes more than 360 degrees without catching the wires on any parts. The mounts shipped starting in June 2011, have a larger cable channel at the top of the Dec. axis.


Use Accessories you May Already Own
If you already own our previous 400 or 600E German Equatorials or other Astro-Physics mounts, you will be pleased to learn that many of the same accessories can be used with the Astro-Physics Mach1GTO. These include counterweights, mounting plates, polar alignment scope (PASILL4L or the prior PASILL4 or PASILL3 models are preferred), piers and tripods.

Fast and Precise Polar Alignment
The optional CNC machined Right Angle Polar Alignment Scope (RAPAS) allows you to polar align the Astro-Physics Mach1GTO in record time and with a precision that permits you to quickly begin imaging. Its revolutionary right-angle design will immediately win you over. No longer will you be kneeling on the ground, straining your neck to polar align. Instead you will comfortably look down into the scope. Polaris, a 2nd magnitude star, is the only one that you need to position on the circular grid pattern of the reticle, so it is possible to align in light polluted skies. No other stars are needed.

There are several ways to determine where Polaris should be positioned on the circular reticle grid. The Astro-Physics ASCOM V2 driver includes the Astro-Physics Polar Alignment Scope Utility that duplicates the grid and provides a continuously updated positioning of Polaris. Custom apps are available for your iPhone/iPad/iPod Touch and Android or Windows devices. Those of you who wish to do it the old-fashioned way can calculate Polaris' position in local sidereal time.

Note: All Mach1GTO mounts shipped beginning in 2014 (serial number M10670 and later) will have the adapter for the Right-Angle Polar Alignment Scope built in. Mounts shipped in prior years must purchase the Right-Angle Polar Alignment Scope Adapter for Mach1GTO (RAPM1) separately.

If you already own the earlier PASILL4L, PASILL4 or PASILL3 versions of the Losmandy Polar Alignment Scope and wish to use it on a Mach1GTO mount that already has the adapter for the Right-Angle Polar Alignment scope (1.79" thread diameter on the backplate), you will need to purchase the Losmandy Polar Alignment Scope Adapter for 1100GTO, 1600GTO and some Mach1GTO Mounts (Q16030).

Mechanical Specifications

ConstructionAll CNC machined aluminum bar stock, stainless steel, brass; stainless steel fasteners
Finishing and AssemblyEvery part is hand-finished and inspected. All assembly is done by hand, by highly skilled mount assembly staff.
Worm wheel - R.A./Dec.5.9" (150 mm), 225 tooth aluminum
Worm gear - R.A./Dec.Brass, 0.705" (17.9 mm) diameter
Axis shaft - R.A./Dec.2.36" (60 mm) diameter
Shaft axis bearings - R.A./Dec.3.1" (78 mm) diameter, 2 per axis
Latitude range0 to 70 degrees with or without the polar scope attached, engraved scale
Azimuth adjustmentApproximately 13 degrees (+/- 6.5 degrees from center)
Counterweight shaft1.125" (29 mm) diameter x 14.5" (368 mm) long [13.625" (346.1 mm) useable length], incl. washer and safety knob.
Optional counterweight shaft (M1053-A) available: 1.875" (48 mm) diameter x 10.7" (272 mm) long; fits inside Dec. axis for transport.
Weight of mountTotal: 32.1 lb. (14.6 kg)
R.A. axis/polar fork: 16.5 lb. (7.5 kg)
Dec. axis: 11.5 lb. (5.2 kg)
Counterweight shaft: 4.1 lb. (1.9 kg)
CapacityApproximately 45 lb. (20 kg) scope and accessories (not including counterweights), depending on length. Recommended for: Astro-Physics and similar fast refractors up to our 160 mm f7.5 Starfire EDF, 8-11" SCTs and 6-8" Maks.
These are only guidelines. Some telescopes are very long for their weight or heavy for their size and will require a larger mount. Remember also that imaging requirements are more rigid than visual observation.

Instrument mounting interface

Please call
Diameter of base5.800" (147.32 mm) diameter

GTOCP4 Servo Drive System

Like the previous GTO mounts, the GTOCP4 servo 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 motor. The system can be accurately 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 only 0.4 amps when tracking the stars, 2 amps with both motors slewing and requires only 12 volts to operate. The servo drive will satisfy the requirements of the sophisticated, advanced astrophotographer, yet is easy for the casual, visual observer to use.

Gear Accuracy and PE Performance
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 7 arc seconds (+/- 3.5 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 integral 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 7 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.


Pre-loaded PEMPro Curve
As mentioned above, the spec of 7 arc seconds (+/- 3.5 arc sec.) is the maximum native mechanical error inherent in the mount's RA axis WITHOUT any software correction. In order to optimize performance even further, we use a special version of Ray Gralak's PEMPro (described below) developed specifically for our test equipment. We generate a unique PE curve for each mount that we program into each GTOCP4 Control Box. Simply use the optional Keypad or your Astro-Physics software (ASCOM V2 driver, PulseGuide or APCC) to turn the PE Correction "on" and you will see results significantly better than our published 7 arc second spec without additional PEMPro runs! However, you may use PEMPro to further refine your PE, if you chose to do so.

PEMPro (available from CCDWare) is a very powerful program that allows the user to characterize the periodic error to a high degree of accuracy and to reduce it dramatically for long unguided exposures. It is especially useful for this mount since the average worm rotation error is already quite low, and the short term ripple error is almost nonexistent. If you are a serious imager, you may wish to consider purchasing PEMPro, especially down the road as your worm gear runs in. Depending on usage, re-measuring error and re-loading periodic error correction from one to four times a year is a good practice, especially if you do some unguided images from time to time. Additional PEMPRo runs are not necessary for visual observers.


GTOCP4 Control Box
The GTOCP4 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 Astro-Physics Mach1GTO uses the same GTOCP4 Control Box (with the exception of the completely black-anodized exterior), as its big brothers - the 1100GTO and 1600GTO mounts. In fact, the control boxes for all three mounts are interchangeable with one another in an emergency. 

GTO Keypad (optional purchase)

The Keypad is a self-contained computer that allows you to control all essential telescope functions and includes an extensive database of objects. 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.

Prior to mid-October 2015, the Keypad was included as part of the mount. However, some of our customers own multiple AP mounts, but only use one at a time. For them, one keypad is sufficient. Others only control their AP mounts with their computer and do not use their Keypad. So, we decided to offer the Keypad as an option. As a result, we were able to reduce the price of the mount accordingly.

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. They will choose to purchase the Keypad.

GTO Servo Drive System Specifications

Electronic componentsRated for industrial and automotive applications
MotorsZero-cogging Swiss DC servo motors, enclosed in machined, aluminum housing
Motor encoder2000 tic quadrature yielding an effective resolution of 0.050 arcseconds per tic
Motor reduction gear train57.6:1 gear reduction through a custom built set of large diameter, fine-toothed, precision, spur gears for vastly superior performance
Servo Motor Control Box

GTOCP4 Control Box; black-anodized to match the mount
Included: machined aluminum Control Box Adapter

Hand-held computerGTO Keypad to control all mount functions. Includes extensive databases and tour features in a simple, intuitive interface. Firmware updates via the internet
Power consumption~ 0.3 to 0.5 amps at 13.8 volts - tracking
~ 1.0 to 2.2 amps at 13.8 volts - both motors slewing at 1200x
Power requirementsNominal 12 volt DC supply at minimum of 5 amps continuous
Periodic error

7 arc seconds peak-to-peak (+/- 3.5 arc seconds) or less in one worm cycle (6.4 minutes); native, prior to any error correction

Maximum slew speed5 degrees / second

Astro-Physics Keypad for GTO mounts. Compatible with all of the Astro-Physics mount with GTO electronics.

Please include mount serial number during purchase phase of the keypad.

The Keypad is a self-contained handheld computer that allows you to control all essential telescope functions and includes an extensive database of objects. We have designed this unit to be as intuitive and easy to use as possible, while filling it with terrific features to make your observing session productive and pleasurable.

Most buttons are assigned to one function only. You do not have to remember shift key patterns or complex keystroke sequences. The directional buttons are shaped like arrows to help you find them in the dark without looking at your keypad. The stop button is readily accessible if you need to cancel any slewing request immediately.

The menu system is very easy to navigate. Each 4-line screen will display several choices which correspond to a number button. Simply press the number button to initiate the command, e.g. "1=M, 2=NGC." When you press "1" the Messier entry screen will display and you can enter the number of the object that you wish to see. Press GOTO, which will cause the mount to slew. The <PREV and NEXT> buttons will allow you to scroll quickly through the lists of common names or from one menu to another.

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 if you don't use it for a few months, you will feel at home with the Keypad very quickly.

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

Compatible mounts include: Mach1GTO, 1100GTO, 1600GTO, 3600GTO and the older 400GTO, 600EGTO, 900GTO and 1200GTO,

Features
  • Handheld keypad with red backlit alphanumeric keypad and red 4-line by 20-character data display.
  • Vacumn-fluorescent display rated to -40 degrees F or C (F and C are are equivalent at this temperature) allows hardy observers to view or image on cold winter nights (please contact Astro-Physics if you wish to operate the mount in severe temperatures below -20F). Normal computers and mobile devices cannot be used at these temperatures.
  • Directional N-S-E-W keys provide immediate response when you wish to center an object or cruise the surface of the moon.
  • Set tracking, guiding, centering and slewing rates.
  • Sets R.A. and declination reversal (E-W reversal in R.A. and N-S reversal in Dec.) for correct object orientation and movement in eyepiece.
  • PEM - Periodic Error Memory ( make your correction just once, remains in memory permanently) - turns this feature on and off.
  • Set R.A. and declination backlash control.
  • Stores 9 observing site locations.
  • Quick and easy polar alignment routines, even during daylight!
  • Adjust brightness of the reticle output for your illuminated guiding eyepiece or polar alignment scope.
  • More than 17,000 objects in extensive databases: Messier (110), NGC (7840), IC (5,386), ADS double stars (215), Abell galaxy clusters (2,712), calibration stars by common name (200), Greek star names by constellation (1053), common objects (100), planets (8) , Moon and Sun.
  • Enter catalog or common star number, solar system object, R.A./Dec. (or Alt/Azcoordinates or common name of object; press GO TO and your telescope will automatically slew to the object.
  • Search and tour functions assist you to plan observing session.
  • Display will indicate if object is below horizon and cancel slewing request.
  • STOP button to cancel your slewing request when the telescope is already moving.
  • Display information about objects (object type and magnitude) before slewing.
  • Timer will let you know when the exposure time of your astrophoto is complete.
  • Continuous readout of current position.
  • Select one of three preprogrammed park positions.
  • Activate meridian swap delay function to allow astrophographers to take a series of images for a mosaic near the meridian without the mount swapping sides.
  • SmartGuide control provides variable speed capability to both axes.
  • Altitude/Azimuth display allows you to position the mount for fixed targets to any Alt/Az point. This is great for taking dark frames.
  • What's Up Now function will suggest objects to view based on what is actually above the horizon at the time.
  • External Auto Connect mode allows primary mount control from an external computer and places the GTO Keypad into a secondary role for seamless operation in computer dominated applications like remote imaging.
  • Reference Park allows you to start the mount in the field by placing the telescope in Park1 position for quick daytime polar alignment.
  • Retractable hanger.
  • Future firmware upgrades available through internet downloads.


Specifications of the Keypad

Dimensions7.2 x 4.1 x 1" (181.6x104.1x24.6mm)
Weight1 pound 8 ounces, including cable and KEYPRO (680 grams)

Keypad

Red LED fiber optic backlit, alphanumeric
Display screen4x20 character alphanumeric
Pre-defined Tracking RatesSidereal, solar, lunar and stop (Note: lunar rate is R.A. only, and does not include the moon's movement in declination.)
Rate selections for Auto-guider port0.25x, 0.5x, 1x
Pre-defined Direction Button Rates

0.25x, 0.5x, 1x, 12x, 64x for centering and manual guiding.

600x, 1200x for rapid button movement. (Actual rates will be slower for 3600GTO mounts and for older 400GTO / 600EGTO mounts with the 32:1 gearboxes. Keypad display will still read 600 or 1200 - see below for actual rates)

Pre-defined Rapid GoTo Slew Rates - All 900GTO, 1200GTO and Mach1GTO600x, 900x and 1200x ( top speed - 5 degrees per second)
Pre-defined Rapid GoTo Slew Rates - 3600GTO and 3600GTOPE300x, 450x and 600x ( top speed - 2.5 degrees per second)
Pre-defined Rapid GoTo Slew Rates - 400GTO and 600EGTO with 32:1 gearbox590x, 860x and 980x (Top speed dependent on available voltage from power supply. Note that these rates differ from those in the GTOCP2 - 460x, 580x, and 675x)
Pre-defined Rapid GoTo Slew Rate - 400GTO and 600EGTO with 19.8:1 gearbox600x, 900x and 1200x ( top speed - 5 degrees per second)