Resolved ultraviolet surface reflectance spectroscopy of Mercury from MESSENGER

Details Resolved ultraviolet surface reflectance spectroscopy of Mercury from MESSENGER Resolved ultraviolet surface reflectance spectroscopy of Mercury from MESSENGER

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1444h&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1444

Physics

Scientific paper

The MESSENGER spacecraft successfully entered orbit around Mercury on March 18, 2011. Although no clear diagnostic absorption features were found from the surface reflectance spectra collected during the earlier Mercury flybys, an inflection in the middle-ultraviolet, not seen in spectra from the Moon, was identified. Ultraviolet spectra have now been acquired from several locations on the planet, and we search for and interpret any variability.

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