Identification of Refractory-rich Asteroids: Evidence for the Earliest Accreted Bodies in the Solar System

Details Identification of Refractory-rich Asteroids: Evidence for the Earliest Accreted Bodies in the Solar System Identification of Refractory-rich Asteroids: Evidence for the Earliest Accreted Bodies in the Solar System

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1613s&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Computer Science

1

Scientific paper

New telescopic data show that spinel-rich asteroids are not rare.
Comparisons to spectra of petrographically controlled CAIs, the oldest
materials in the solar system, demonstrate the role of FeO and
alteration in linking these populations.

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