Exploring Surface and Shallow Subsurface Volatile Presence on Vesta Using a Bistatic Radar Experiment

Details Exploring Surface and Shallow Subsurface Volatile Presence on Vesta Using a Bistatic Radar Experiment Exploring Surface and Shallow Subsurface Volatile Presence on Vesta Using a Bistatic Radar Experiment

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2685p&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2685

Physics

Scientific paper

An interesting topic of concern for Vesta is the presence or lack of
volatiles. A bistatic radar experiment may help address this question,
where data interpretation relies on dielectric models of the surface and
shallow subsurface.

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