Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/5/84; site philabs.UUCP Path: utzoo!watmath!clyde!bonnie!akgua!gatech!ut-sally!seismo!cmcl2!philabs!ams From: ams@philabs.UUCP (Ali Shaik) Newsgroups: net.physics,net.space Subject: Telescopes and parabolic mirrors Message-ID: <532@philabs.UUCP> Date: Mon, 9-Dec-85 11:14:12 EST Article-I.D.: philabs.532 Posted: Mon Dec 9 11:14:12 1985 Date-Received: Wed, 11-Dec-85 04:09:16 EST Reply-To: ams@philabs.UUCP (Ali Shaik) Organization: Philips Labs, Briarcliff Manor, NY Lines: 22 Keywords: mirror using pressurized sheet Xref: watmath net.physics:3676 net.space:4921 One way to figure out if a thin circular sheet would deform to a paraboloid when pressurized is to set up the differential equations of deformation and solve them. Intuitive analogies to soap bubbles, etc may not always work. I looked up "Theory of plates and shells" by Timoshenko and Woinowsky-Kreiger, and sure enough, they had done all the dirty work for me! (see eq. 67 on page 57). The deflection contains the square of the radius multiplied by a large constant plus radius to the fourth power. The surface is a paraboloid to within 6% upto half the radius of the sheet. Thus darkening the area beyond 0.5r looks as if it would give close approximation to a paraboloid. I don't know how much this means in terms of image quality. It looks promising for manufacture of cheap telescopes. - Ali "Bangalore" Shaik ihnp4!philabs!ams