Constraints on Martian Global Surface Mineralogical Composition, Albedo, and Thermal Inertia from Hubble Space Telescope Extended-Visible Multispectral Data

Details Constraints on Martian Global Surface Mineralogical Composition, Albedo, and Thermal Inertia from Hubble Space Telescope Extended-Visible Multispectral Data Constraints on Martian Global Surface Mineralogical Composition, Albedo, and Thermal Inertia from Hubble Space Telescope Extended-Visible Multispectral Data

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1913m&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1913

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Scientific paper

We are using 12-band (255 to 1042 nm) multispectral data of Mars from
observations made by the Hubble Space Telescope (HST) in 1999
(Ls ~ 130°) to globally map mineralogical compositions
and albedo at spatial scales of ~20 to 50 km/pixel.

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