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Water on MarsIt is reported that the SNC meteorites are a factor of 2 richer in moderately volatile elements (Na, K, P, etc.) and some volatile elements (Cl, Br, I, S) compared to the Earth and Mars. It is proposed that Mars accreted homogeneously, with the result that all the water except trace amounts (on reaction with metallic Fe) was converted to H(sub 2) and escaped. This model predicts a total Mars H(sub 2)O inventory of 18 ppm (equivalent to an ocean 80 m deep on the planet), and a value for Earth of 300 ppm, close to the actual abundance.
Document ID
19890001451
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Waenke, H.
(Max-Planck-Inst. fuer Chemie Mainz, Germany)
Dreibus, G.
(Max-Planck-Inst. fuer Chemie Mainz, Germany)
Date Acquired
September 5, 2013
Publication Date
January 1, 1987
Publication Information
Publication: Lunar and Planetary Inst., MECA Symposium on Mars: Evolution of its Climate and Atmosphere
Subject Category
Lunar And Planetary Exploration
Accession Number
89N10822
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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