Rotationally Resolved Spectroscopy of Vesta in the 2-3 µm Region

Details Rotationally Resolved Spectroscopy of Vesta in the 2-3 µm Region Rotationally Resolved Spectroscopy of Vesta in the 2-3 µm Region

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1811r&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1811

Physics

Scientific paper

We present spectra from 2001-2004, and show that the northern and
southern hemispheres of Vesta are distinct. The northern hemisphere
shows evidence of a ~1% band at 3 µm, while the southern
hemisphere does not. We suggest the band is due to contamination from
carbonaceous impactors.

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