Formations of Martian Plagioclases and Flow Textures by Carbon Dioxides-rich Gas and Fluid Compared with Natural Rocks and Artificial Products on the Earth

Details Formations of Martian Plagioclases and Flow Textures by Carbon Dioxides-rich Gas and Fluid Compared with Natural Rocks and Artificial Products on the Earth Formations of Martian Plagioclases and Flow Textures by Carbon Dioxides-rich Gas and Fluid Compared with Natural Rocks and Artificial Products on the Earth

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1090m&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

1

Scientific paper

Carbon-bearing grains formed in basalts and syntheses are applied to
carbon-fixing on martian plagioclases which are formed by impact
pressures from carbon dioxides gas.

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