Investigating the Origin of Dark Material on Vesta: Locations and Geological Context

Details Investigating the Origin of Dark Material on Vesta: Locations and Geological Context Investigating the Origin of Dark Material on Vesta: Locations and Geological Context

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1807j&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1807

Physics

1

Scientific paper

Deposits of dark material (DM) appear on Vesta’s surface as
lower-albedo features in the visible wavelength. DM are distributed
unevenly and are often associated with impact craters as outcrops in
walls and mass-wasting deposits as well as ejecta.

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