Modeling of Layers of Micron Sized Water Ice Over Enceladus Surface to Fit the 1 to 5 Micron Spectra from the Cassini VIMS Instrument

Details Modeling of Layers of Micron Sized Water Ice Over Enceladus Surface to Fit the 1 to 5 Micron Spectra from the Cassini VIMS Instrument Modeling of Layers of Micron Sized Water Ice Over Enceladus Surface to Fit the 1 to 5 Micron Spectra from the Cassini VIMS Instrument

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2625h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2625

Physics

Scientific paper

We are modeling Enceladus surface as larger grained (>5 µm) ice
covered by a fine-grained ice with a roughly monolayer depth. This
accurately fits the >3 µm VIMS spectrum and provides a more
accurate estimate of the underlying grain size.

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