Initial Water Compositions: Aqueous Alteration of Planetesimals

Details Initial Water Compositions: Aqueous Alteration of Planetesimals Initial Water Compositions: Aqueous Alteration of Planetesimals

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1850f&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1850

Computer Science

Scientific paper

Oxygen isotope data for sulfate and carbonate minerals (alteration
products) point to an initial water-ice oxygen isotope composition
closer to that proposed by Clayton and Mayeda than to that of Young. The
implication being that water-ice does not lie on an extension of the
slope 1 CCAM line.

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