Characterizing the Surface Elemental Composition of 4 Vesta Based on HED Meteorites: Prospective Study of Gamma-Ray and Neutron Spectrometer for the DAWN Mission

Details Characterizing the Surface Elemental Composition of 4 Vesta Based on HED Meteorites: Prospective Study of Gamma-Ray and Neutron Spectrometer for the DAWN Mission Characterizing the Surface Elemental Composition of 4 Vesta Based on HED Meteorites: Prospective Study of Gamma-Ray and Neutron Spectrometer for the DAWN Mission

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1407u&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1407

Computer Science

Scientific paper

the DAWN mission will explore two of the largest main-belt asteroids,
Ceres and Vesta. We compile 42 whole-rock compositions of HED meteorites
and present two diagnostic compositional diagrams to characterize the
surface type of Vesta from GR/NS data.

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