The Compositional Profile of Enceladus Icy Dust Plume from Cassini In-Situ Measurements

Details The Compositional Profile of Enceladus Icy Dust Plume from Cassini In-Situ Measurements The Compositional Profile of Enceladus Icy Dust Plume from Cassini In-Situ Measurements

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1849p&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1849

Computer Science

1

Scientific paper

Measurements by Cassini’s dust detector during Enceladus plume
crossings show strong variations in structure and composition. Salt-rich
ice grains clearly dominate Enceladus’ solid emissions strongly
favoring an abundant liquid water source close to the icy surface.

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