Illumination conditions at the Asteroid 4 Vesta: Implications for the presence of water ice

Details Illumination conditions at the Asteroid 4 Vesta: Implications for the presence of water ice Illumination conditions at the Asteroid 4 Vesta: Implications for the presence of water ice

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012icar..217..272s&link_type=abstract

Icarus, Volume 217, Issue 1, p. 272-276.

Physics

1

Scientific paper

The mean illumination conditions and surface temperatures over one orbital period are calculated for the Asteroid 4 Vesta using a coarse digital elevation model produced from Hubble Space Telescope images. Even with the anticipated effects of finer-scale topography taken into account, it is unlikely that any significant permanently shadowed regions currently exist on Vesta due to its large axial tilt (≈27°). However, under present day conditions, it is predicted that about half of Vesta's surface has an average temperature of less than 145 K, which, based on previous thermal modeling of main belt asteroids, suggests that water ice could survive in the top few meters of the vestal regolith on billion-year timescales.

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