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HomeTelescope ThermodynamicsSept. 2000 Sky & Telescope magazine companion web siteMay & June 2004 Sky & Telescope magazine companion web siteUsing fans with a Newtonian telescopeTips on attaching a temperature probe to your telescopeOptical MiscellanyTry this at home!How atmospheric seeing affects telescopes with different focal ratiosAnimated focal plane illumination mapProperties of various mirror substrate materialsAdventures in collimation |
This animated plot depicts the illumination level of a 1.5 by 1.5 inch portion of the focal plane as the secondary size is varied. The secondary mirror size goes from being drastically too small (0.8" minor axis size) to excessively large (3.10" minor axis size). The color red represents a fully illuminated area, while deep blue regions are receiving almost no light at all. This animation is based on the formulas published by William T. Peters and Robert Pike (Sky & Telescope; March 1977, pgs. 220-223). Notes:
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Copyright 1997-2024 Bryan Greer
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