Solar Illumination Conditions at 4 Vesta: Predictions Using the Digital Elevation Model Derived from HST Images

Details Solar Illumination Conditions at 4 Vesta: Predictions Using the Digital Elevation Model Derived from HST Images Solar Illumination Conditions at 4 Vesta: Predictions Using the Digital Elevation Model Derived from HST Images

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2506s&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2506

Physics

Scientific paper

The illumination/shadowing conditions at 4 Vesta are predicted using the
Thomas et al. (1997) HST-derived DEM. Due to the coarse resolution and
large axial tilt, no permanently shadowed regions are predicted.

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