Space weathering and the suface composition of Phobos

Details Space weathering and the suface composition of Phobos Space weathering and the suface composition of Phobos

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..148k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.148

Physics

Scientific paper

The most of the observed Phobos area is characterized by redder spectral unit (PRU), while bluer spectral unit (PBU) is being generally associated with the interior and the ejecta of Stickney crater. We present a model that is based on laboratory experiments and using which we try to explain the difference in spectral slopes of the two parts of Phobos surface.

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