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Dave Shouldice's Low Profile Equatorial Table |
| Dave Shouldice built this platform to drive his
15" Dob-mounted telescope. He recently bought this telescope, replacing
his equatorially mounted clock driven telescope. This is his solution to the
tracking problem with the new Dob. This platform won 3rd place in the ATM Walkaround at the Colorado Springs Astronomical Society's Rocky Mountain Star Stare, 1999.
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Being a planetary observer, and having been accustomed to tracking, the purchase of a Dob left me wanting. My goals for tracking:
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References:In my research I found 4 articles of note:
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DesignThe key to a low profile table was to try and make all the forces (weight) from the scope supported as directly as possible by the feet and structure, not the baseboard. IE keep the horizontal distance from the bottom Teflon pads to the feet to a minimum. This will minimize the need for a top or bottom structural baseboard. Most equatorial tables that I reviewed seemed justly concerned with the cantilevered loads, and opted for ¾" or 1" plywood for the top and bottom boards. Due to my eyepiece height issue, I tried to use structure only where needed.. The forces:The 3 Teflon pads that compose the azimuth bearing on the dob carry all the weight. The desire was to place 2 feet to the North of the table with one to the South. North Feet:
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The 2 North support tracks attach to the bottom of the baseboard. Per D'Autumn, this baseboard rotates around a virtual axis that points to the North pole, but, passes through the center of Mass of the telescope (centered between the 2 altitude bearing axis). This is important. If you don't rotate the table around both your center of mass and the pole, your motor torque needs will greatly increase, and it will be much harder to purchase. The power is needed as the motor will have to lift your scope. Also, the imbalance will make your scope tippy. The curved tracks attached to the baseboard mark D'Autumn's conic sections. As there is only 15 degrees (1 hour) worth of tracking, you can make the bearing track from a vertical board, like the one the "Equatorial Platform" design. The weight is directly supported. My tracks have, at the farthest ends of its rotation, a 2.5" distance between the Teflon pad and the roller that supports the curved track. Only after it was functional, and knew where the ground board moved, I added a brace behind the tracks on the baseboard to minimize the droop of the baseboard when it is at the end of travel. I lined the tracks with a piece of rolled stainless to reduce friction and prevent denting of the track.
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A pair of cam rollers is attached to the ground board with an angle bracket that hold the threaded insert for the adjustable feet. As the forces at the roller bearing is almost vertical, only minimum support is needed from the ground board for these feet. South Foot:
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The South pad sits over a conventional cylindrical bearing section bolted to the South end of the baseboard. This is held up by 3 bearings, 2 supporting the radial force, with 1 supporting the axial. This holds the base board from moving N. or S. of the design position. Gravity holds it from moving E or W. As the 3 bearings attach to the ground board support the S. load, and as the table moves E. or W. shifts East or West of centerline. The South foot of the table is held by a threaded insert near the S. bearing holder (angle bracket). To deal with the force that moves on either side of center, you either need a bottom plate that doesn't twist (I added a ¾" brace), or you could add 2 South feet. Forces from below:
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The first time I set up on my lawn, I learned of another force, the grass,
that pushed up on the center, between the feet, bowing my base. Most of
the weight (hopefully) is supported by the feet, but short of making the
feet higher than the grass (and raising my eyepiece) I reinforced the
bottom board with a ¾" plywood with holes to decrease weight. This also
stopped the twisting of the S. baseboard.
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The DriveThis too took a lot of research. I decided that I was only interested in a tracking drive, not a hand controller for fine tuning, or slow motion axes. These would have driven the design to steppers with controllers, computers etc. To add complexity, failure modes stress etc. The result, however was to make a synchronous worm gear drive like Shaw chose. Designs like those made by D'Autumn and Ken Florentino of CSAS show how to use threaded rod for the worm and rack. The motor and worm are located on a bracket mounted on a spring loaded hinge. When the hinge is moved, the table can be reset to the beginning of travel. This project took me 4 months of obsessing to design and build, with most of the time in calculations and drawings. I assume you will only take a fraction of this. On first use I saw the central star in the Cat's eye and have tracked the planets for 45 minutes. I still use my DSC (digital setting circles), with the DSC aligned with the table at the beginning of travel. To find an object by the DSC, I first reset the drive. If it is a struggle to locate, or at setup of the DSC, I turn off the drive. Actually I tend to run the drive mainly when I am with the public, when using high power, or for long stares.
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ConstructionYou should download all the pictures, graphs, and perform calculations from Peters' and Shaw's article mentioned above in the references.
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This needs to be quite solid, but easily removable. You will have this on and off the top board several times before and after you are done. After making this, take it outside at night, level the top surface, point it North, and see if your polar axis points to Polaris. Fix (re cut or shim it if it doesn't.)
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The motor will need a gear to drive a gear on the threaded rod. This keeps the motor from hitting the rack. This drives the location of the rack. It is advisable to make the hinged motor support and rack before attaching the rack. I cut a hole in my ground board to allow for more space. At end of travel, ensure that the rail does not hit the motor. Mine clears by ¼". Also, to avoid need for an end of travel limit switch, I offset my motor W so that at end of travel it runs off the end of the rack.
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The rigidity of this
plate is important as it will define the stiffness of the drive. Bolt the
bracket to a solid hinge. I used a gate hinge that I had taken apart and
hammered on the hinge to take out the slop. I also inserted a washer in
series with the hinge to take out lateral movement. Don't bolt this to the
ground board yet.
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Important details to consider: I am at 40 degrees latitude, so the polar axis splits the loads between radial and axial forces. Also, my scope weighs 100 +lbs. ,there is 14.5" between my scope's Teflon foot pads, the height from the Teflon pads to the center of the horizontal scope bearings is 18". If you are building for a different lattitude, or other dimensions of your telescope are very different, you should carefully consider the changes you must make for this mount to work for you. Clear skies - david.shouldice@cobe.com |