Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site ssc-vax.UUCP Path: utzoo!linus!decvax!microsoft!fluke!ssc-vax!eder From: eder@ssc-vax.UUCP (Dani Eder) Newsgroups: net.space Subject: Re: Deuterium on Venus Message-ID: <730@ssc-vax.UUCP> Date: Tue, 3-Jan-84 15:13:16 EST Article-I.D.: ssc-vax.730 Posted: Tue Jan 3 15:13:16 1984 Date-Received: Fri, 6-Jan-84 04:22:13 EST References: <14945@sri-arpa.UUCP> 3 January 1984 Organization: Boeing Aerospace, Seattle Lines: 14 A simpler and more controllable method of terraforming Venus would be to shine more sunlight on it and boil the atmosphere off. 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. DaniEder Boeing Aerospace Company ssc-vax!eder