Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10 5/3/83; site ucf-cs.UUCP Path: utzoo!linus!decvax!duke!ucf-cs!giles From: giles@ucf-cs.UUCP (Bruce Giles) Newsgroups: net.space Subject: Re: Deuterium on Venus Message-ID: <1145@ucf-cs.UUCP> Date: Tue, 10-Jan-84 19:29:28 EST Article-I.D.: ucf-cs.1145 Posted: Tue Jan 10 19:29:28 1984 Date-Received: Wed, 11-Jan-84 05:36:19 EST References: <14945@sri-arpa.UUCP> 3 January 1984, <730@ssc-vax.UUCP> Organization: University of Central Florida Lines: 26 Let us say you wanted to raise the temperature by a factor of 4. This requires 64 times as much incident intensity. Assume that this is gotten from solar sails in Venus vicinity. They need a total surface area of 7.24 billion km**2. If their thickness is .15 microns, then the volume of material required is only 1.1 km**3, not an unreasonable quantity. And we wave a fond farewell to the lightsails as they accelerate into the darkness of interstellar space. (may not make too much sense towards the end, but it sounds good) (hint: divide 7.24 billion km**2 light pressure at Venus by the mass of 1.1 km**3 of material, and use F = ma). Bruce Giles --------------------------------------------- UUCP: decvax!ucf-cs!giles cs-net: giles@ucf ARPA: giles.ucf-cs@Rand-Relay Snail: University of Central Florida Dept of Math, POB 26000 Orlando Fl 32816 ---------------------------------------------