Infrared spectrometric data of basaltic Martian analogues from Mongolian terranes and the Baikal Rift Zone

Details Infrared spectrometric data of basaltic Martian analogues from Mongolian terranes and the Baikal Rift Zone Infrared spectrometric data of basaltic Martian analogues from Mongolian terranes and the Baikal Rift Zone

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epsc.conf..937g&link_type=abstract

European Planetary Science Congress 2008, Proceedings of the conference held 21-25 September, 2008 in Münster, Germany. Online a

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Infrared spectroscopy has been used to analyse the composition of the rock material of basaltic Martian analogues from Mongolian terranes and the southern part of the Baikal Rift Zone, for comparison of the results with those of Martian missions. Collected samples of basalts derive from various geologic environments (rift zone, island-arc, ophiolite). Microscopic observations in thin sections show diversification of composition and structures of basalts. The most diversified are basalts from the Mandalovoo terrane [1].

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