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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 |
The consequence of changing the secondary mirror size in a Newtonian telescope is that it affects the size of the fully illuminated region at the focal plane. A given spot on the focal plane is said to be "fully illuminated" if it receives 100% of the light gathered by the primary mirror. Outside this region, the illumination level gradually drops off. As logic suggests, when the size of the secondary increases, so does the size of the fully illuminated region. If the secondary is too small, no place on the focal plane will be fully illuminated, and the telescope will behave like it has a smaller aperture. 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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