Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!watmath!clyde!rutgers!seismo!ll-xn!cit-vax!oddhack!jon From: jon@oddhack.Caltech.Edu (Jon Leech) Newsgroups: sci.space Subject: Re: Martian surface chemical composition. Message-ID: <1103@cit-vax.Caltech.Edu> Date: Fri, 31-Oct-86 12:38:00 EST Article-I.D.: cit-vax.1103 Posted: Fri Oct 31 12:38:00 1986 Date-Received: Sat, 1-Nov-86 04:30:48 EST Sender: news@cit-vax.Caltech.Edu Reply-To: jon@cit-vax.UUCP (Jon Leech) Organization: California Institute of Technology Lines: 13 In article <8610310817.AA15131@s1-b.arpa> ESG7@DFVLROP1.BITNET writes: > My question is, how hard is it to extract useful stuff from the surface material? Taking oxygen out of the various iron oxides and the like it's locked up in sounds very energy-consuming. Also, it would be interesting to compare the composition of exposed surface material and areas further down which haven't been radiated for billions of years. Of course I refer to molecular composition, not atomic abundance which should be much the same as the exposed surface. -- Jon Leech (jon@csvax.caltech.edu || ...seismo!cit-vax!jon) Caltech Computer Science Graphics Group __@/