CERAVOLO Optical Systems - Astrograph

Mechanical Design - Mirror Cells

Mirror Cell The primary mirror is precisely aligned with the corrector lenses and permanently bonded in the six-point flotation cell/backplate. This extra care and attention in assembly means you have less trouble collimating the telescope in the field. The heavy-duty, but light-weighted cell/backplate and OTA cradle allow astro-imagers to bolt heavy cameras and filter wheels to the OTA without inducing flexure. Five fans minimize the cool down time of the primary mirror.
Mirror Cell with Fans The mirror rests on a six-point cell arrangement, optimized to support the mirror without imparting stress. The five rear fans are removable so the primary can be cleaned while still in the cell.
Backplate CNC-Machined heavy-duty backplate. Bulkhead-inspired construction, with ribs for strength, and milled pockets to reduce weight.
Front end assembly The entire front end of the astrograph, seen here, can be easily removed from the tube as a single assembly. To avoid flexure of the carbon fiber tube, the robust spider attaches to a heavy-duty aluminum front end ring.