Syrtis Major as the Source Region of the Nakhlite/Chassigny Group of Martian Meteorites: Implications for the Geological History of Mars

Details Syrtis Major as the Source Region of the Nakhlite/Chassigny Group of Martian Meteorites: Implications for the Geological History of Mars Syrtis Major as the Source Region of the Nakhlite/Chassigny Group of Martian Meteorites: Implications for the Geological History of Mars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1019h&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1019

Computer Science

2

Scientific paper

The observed geology and spectroscopy of Syrtis Major is a compelling
match to the mineralogy and hypothesized setting of the Nakhlite /
Chassigny group of martian meteorites. If this connection is real, it
solves many interesting timescale-based problems in martian geology.

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