Combined albedo spectrum of Phobos in UV and Visible with SPICAM and OMEGA on Mars Express

Details Combined albedo spectrum of Phobos in UV and Visible with SPICAM and OMEGA on Mars Express Combined albedo spectrum of Phobos in UV and Visible with SPICAM and OMEGA on Mars Express

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..523b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.523

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Scientific paper

Mars Express made several encounters with Phobos for the last 6 years. Observations with SPICAM and OMEGA on board Mars Express cover the range from UV (190-310 nm) to visible and near IR up to 5 μm. In the following we consider only the visible channel of OMEGA and the UV channel of SPICAM. In the UV channel, there is a dip in the geometrical albedo spectrum centered at 220 nm, similar to the one observed in the interstellar extinction, interpreted of PAH origin. The combined UV/VIS SPICAM/OMEGA spectrum exhibits another strong dip centered at 350 nm. It could tentatively be attributed to the presence of ilmenite.

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