Photometric determination of crater's depth on Enceladus

Details Photometric determination of crater's depth on Enceladus Photometric determination of crater's depth on Enceladus

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..726d&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.726

Physics

Scientific paper

We show here that it is possible to overcome the difficulty at determining the crater's depth of planetary bodies without radar or laser altimetry, by the use of the multi-angle geometry of imaging data. We present here for Enceladus the adaptation of a macroscopic surface roughness model, developed by [4] and well documented by [1,2]. This model allows reproducing the average photometric behavior of a crater and constraining its aspect ratio with a very good accuracy.

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