Hydrous Magmatism on Mars: A Source for Water on the Ancient Martian Surface and the Current Martian Subsurface?

Details Hydrous Magmatism on Mars: A Source for Water on the Ancient Martian Surface and the Current Martian Subsurface? Hydrous Magmatism on Mars: A Source for Water on the Ancient Martian Surface and the Current Martian Subsurface?

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2207m&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

Water was analyzed in amphibole and biotite from melt inclusions in the
Chassigny meteorite. The measured values are much higher than previous
analyses and may allow for a much wetter martian interior than has been
previously postulated.

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