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Provided the curve is given an adequate cross sectional area it can be as stiff as aluminium. The image shows the basic idea. Thinner plywood strips are laminated over a former and clamped tight while the glue sets. Normally there is a degree of spring and the radius of the final result may increase. The flange bearings can be placed inside or outside the "arms". A bolt, fitted with load spreading washers or plates will clamp the curve securely to a suitably curved base.
The next step is to be equally adventurous with the design of the declination axis and saddle.
Here a similar, but tighter curve is nested within the polar axis curve to provide twin declination bearing supports. The downside of this arrangement is the severe obstruction of the telescope tube on either side of the mounting. To point at the Pole the telescope must lie alongside the mounting rather than above it.
Since the two axes shafts cannot physically cross each other it is not possible to have the declination shaft perpendicular to the polar axis in the usual sense. [As shown by the red arrow] This would require a stub shaft and plate bearing impaled on the red arrow. A separate Declination counterweight shaft could be attached via a clamp but this adds bulk and complication. The
telescope tube needs to clear the polar axis and large wormwheel.
So the declination overhang/saddle must be extended considerably in the direction of
the arrow.
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The lower image shows a circular declination assembly with a superimposed T-shaped box. All made form plywood laminations. The head of the 'T' provides the declination shaft housing and enough offset to avoid collisions between the OTA and mounting. The advantage here is that the declination assembly lies between the PA bearings and is evenly supported by flanges. So no stress raising cantilevering for the Polar Axis. The saddle is cantilevered but has a plate bearing formed by the wormwheel.
Click on any image for an enlargement.
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