The 2004 Opposition of Ceres Observed with Adaptive Optics on the VLT

Details The 2004 Opposition of Ceres Observed with Adaptive Optics on the VLT The 2004 Opposition of Ceres Observed with Adaptive Optics on the VLT

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1388e&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1388

Computer Science

2

Scientific paper

Ceres has been observed with NACO on the VLT. Imaging and spectroscopy
were performed in the 1.1-4.1 µm range with spatial resolution up
to 50 km. The aim is 1) to provide the first IR map of Ceres 2) to map
compositional variations at the surface.

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