Cassini/VIMS Spectra and Time-Evolution of Precipitation-Associated Surface Brightenings on Titan

Details Cassini/VIMS Spectra and Time-Evolution of Precipitation-Associated Surface Brightenings on Titan Cassini/VIMS Spectra and Time-Evolution of Precipitation-Associated Surface Brightenings on Titan

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2762b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2762

Physics

Scientific paper

Large areas of Titan's surface brightened at all wavelengths as seen
from Cassini/VIMS for several months, then faded. The brightenings
occurred after a large storm and rainfall event, and may relate to
volatile refreezing due to evaporative cooling.

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