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12.5"Motorized&Computer ControlledAltAz Telescopeclick on image for larger version
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Lessons learned after two years with the AltAz driven scope.
This was the second telescope that I built. I saw Mel Bartels' plans for the motorized dobsonian and knew I just had to build one of these - I knew it was the wave of the future!
The scope is a 12.5" F5.9 reflector with an AltAz (dobsonian-style) mount. I decided on a truss-tube design so that the scope could be disassembled to make transport a bit easier.
I began grinding the primary mirror during the summer of 1995. Grinding and polishing were completed within a few weeks. I used commercial polishing pads w/cerium oxide to speed up the polishing process. Final figuring was done with red optical rouge. The rouge gave a very smooth surface, but the stuff is really messy.
A pitch lap of Gugolz 64 was used on a dental plaster tool. The final surface figure as measured with a basic focault test and calculated by tex.exe was about 1/14 wave. Star testing has shown the mirror to be excellent (doesn't everyone say that?). Under good seeing, the scope yields razor sharp detail. Planetary contrast is quite good despite the fact that the optical system is 21% obstructed.
The mirror was shipped to P.A. Clausing where it received a Beral coating.
The 2.6"(MA) secondary mirror was interferogram tested at 0.122 wave P-V maximum error. The secondary support was fabricated from 3/8" wall fiber-resin tubing. A resistor bridge was glued to the back of the secondary (inside the holder) to provide heating for dew removal. The spider was totally fabricated from scratch and made from aluminum.
Birch plywood was used as the main construction material. The upper cage assy rings were cut out with a router to 14" inside diameter. Truss tubes are .055" wall 1" aluminum covered with foam pipe insulation. Clamp blocks for both the mirror box and upper cage were fabricated from hardwood maple.
The mirror cell frame was welded up from 1" box section steel tubing. The mirror support itself uses a 9 point floatation system on a 14.5" diameter birch backing plate. The backing plate is attached to the steel frame with three large adjustment screws. The adjustment screws pass through bushings in the box frame and are terminated with large "T" handles for easy collimation adjustments. Heavy duty die-springs are used to keep constant tension on the mirror cell backing plate.
Both the altitude and azimuth axis run on ball-bearing races instead of the usual teflon pads that are commonly used on dobsonian mounts. Ball bearings were chosen to minimize friction and to increase the accuracy of the stepper motor drive system.
The stepper motors are coupled to the drive wheels via hollow shafts with set screws. The set screws can be loosened to permit both axis of the scope to be disengaged from the drive motors.
Mel's AltAz software uses a common PC (a 486 notebook in my case) to directly control the stepper motors of each axis via the PC's parallel port.
Because the dobsonian style mount of the telescope is alt-az, both axis of the scope need to move at once in order to track an object across the sky. The computer constantly drives each stepper motor at the proper rate to maintain a fix on any RA/DEC position on the sky. In addition to tracking, the system also has "goto" slewing capability. A user programmable internal database can be used, or coordinates can be passed to the software from many of the commercially sold planetarium programs.
The full documentation on Mel's altaz scope control system can be found on this page. I originally chose Hurst stepper motors w/600:1 reduction gearboxes, which are of the same type used by Tech 2000 on their "dob-driver" product. The Hurst SAS series motors are available with a variety of reduction gear ratios and are 48 steps/rev. After a short time, I discovered (with a little help from Jerry Pinter) that the Hurst SAS series steppers had a serious flaw. Both Jerry and myself found that these motors had alternating FULL step sizes. In my case, I was measuring 5 deg for one step followed by 10 deg for the next step, followed by 5 degrees once again. In actual use, a wagging motion was seen in the eyepiece at high magnification as the drive went through a series of 10 small micro-steps, and then 10 larger micro-steps.
Jerry had mentioned that he had success with switching to another brand of stepper motor - which he mated to the original Hurst gearbox. I decided to try the same approach. I was fortunate enough to find a friend with 150:1 gearboxes that was willing to swap for my 600:1 units. I then purchased a set of AstroSyn 200 step/rev motors from C&H distributing for $20 each. In order to adapt the new motors to the Hurst gearboxes, I had to remove the rotor and shaft from the housing. I then put each shaft in a lathe and turned down the diameter to match the spur gears from the original Hurst motors. I allowed about .050" space between the motor and gearbox which I later filled with RTV and rubber washers to reduce vibration. The motors are now secured to the gearboxes with nylon screws.
Mel mentions in his documentation that he uses 5 volt motors and runs them on 12 or 24 volts in order to attain a higher maximum slew speed. I also used this approach with the original Hurst motors (which were 12v) by running them on 24 volts. The new AstroSyn motors are rated for 10 volts, but didn't like being run on 24 volts directly. During the speed ramp-up, the motor was hitting several speeds where a resonance was occuring. At these points, the motor would get very rough and would usually stall. I tried starting the ramp at a higher initial speed, but that didn't help. It was becoming obvious that the windings were simply drawing to much current during the ramp-up, so I was forced to drop the supply to 12 volts.
I was determined to get the new motors to run faster, so I tried installing a set of current limiting resistors in series with the motors. My calculated values for the limiting resistors weren't quite optimal at first, so I hooked up a decade resistor box and dialed in values until the motors smoothed out. With the resistors set to the proper value, the motors now run happily across their entire speed range on 24 volts, and the max slew speed that I can now attain is much higher. The scope is able to slew at about 1.8 degrees/second now. (with gearing that yields 0.23 arcsec/microstep resolution)
A small voltmeter enclosure is mounted on the base of the scope to monitor battery condition. Three switches are mounted on this enclosure to control power to the motor drive system, the primary mirror cooling fan, and the secondary mirror dew heater.
I have recently installed a heater on the telrad. Severe dewing at recent starparties was showing that something more than a passive dew-shield was needed. A switch on the upper cage was added to turn the telrad heater on and off.
The handpad unit for slewing control and alignment functions plugs into this same enclosure. The handpad cabling permits the laptop computer to be located approx 12 feet from the telescope.
A few people have asked me what the little black box was that the altitude stepper motor is plugged into. Well, there are actually two of those little black boxes - one for each motor. They each house a custom designed P.C. board for the drive electronics. I chose to split the drive circuitry for each axis so that the cabling between the motors and the drive transistors would be as short as possible.
If anyone is interested in making their own boards from the PCB artwork, you can download a gif file of the artwork here. I can provide additional information if you need it.
Here is a picture of the boards installed in the boxes...
The addition of encoders to the scope make a significant improvement in pointing accuracy. The neatest feature made possible by the encoders is the ability of the mount to automatically return to the proper position and resume tracking if it gets disturbed or moved by accident. The 4000 count encoders are interfaced to the computer via a serial cable and David Lanes Micro guider III.
Here are some close-ups of various parts of the scope.
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| In the image directly above, you can see the 1/4 inch thick aluminum plate which is the driving surface for the azimuth axis roller.
The image to the right shows the altitude encoder mounting. Also note the mirror cell design, in the picture to the above right, which incorporates a light baffle and mounting plate for the floatation triangles. The actual contact points to the back of the mirror are the heads of three nylon screws on each triangle |
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