Spectral Observations of a Non-Chondritic 951 Gaspra

Details Spectral Observations of a Non-Chondritic 951 Gaspra Spectral Observations of a Non-Chondritic 951 Gaspra

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1002g&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1002

Physics

Scientific paper

An updated analysis of NASA Galileo spacecraft observations indicate
that 951 Gaspra has been subjected to igneous processes. This is derived
from an observed relative abundance of olivine that is higher than
measured in ordinary chondrites.

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