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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 |
Implications of these properties for a telescope's mirrorRefractive index: This is a measure of how much the material can slow down light (compared to a vacuum). It's a critical property for lens design, but is unimportant for reflective optics. Density: This is how heavy the material is for a given volume. We usually want our optics as lightweight as possible, so a lower value is better. Young's modulus: This is how stiff the material is. To minimize flexure in the optical cell, or to permit the thinnest possible optic for a given cell design, a higher value is better. Hardness: Harder materials generally polish smoother at the microscopic scale, so a higher value is better. Coefficient of thermal expansion: This describes how much the material will grow (volumetrically) with an increase in temperature. Since we want the shape of our mirror to remain the same while it's changing temperature, a low value is desired. Thermal conductivity: This describes how quickly heat can be transported through the material. Since we want the mirror to cool quickly and track the falling ambient temperature closely, a higher value is better. Specific heat: This is how much heat energy the material can store. A low value is desired, since this will help the mirror to adapt to a change in temperature more quickly. Cost: This property isn't in the table above, but it certainly can be important! Return to Telescope Optics Topics. |
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Copyright 1997-2024 Bryan Greer
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