Secondary Fayalites and Metamorphic Olivine-rich Aggregates in the Yamato-86009 CV3 Carbonaceous Chondrite: Evidence for Complex Formation of CV3 Asteroids

Details Secondary Fayalites and Metamorphic Olivine-rich Aggregates in the Yamato-86009 CV3 Carbonaceous Chondrite: Evidence for Complex Formation of CV3 Asteroids Secondary Fayalites and Metamorphic Olivine-rich Aggregates in the Yamato-86009 CV3 Carbonaceous Chondrite: Evidence for Complex Formation of CV3 Asteroids

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1576j&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

3

Scientific paper

Iron-probe oxygen isotope analysis indicates that secondary fayalite and
magnetite formed at low temperature (<300°C), while a FeO-rich
metamorphic olivine aggregate originated neither a differentiated nor an
R-chondrite parent body.

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