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Seasonal variability on Saturn’s Moons Mimas and Tethys

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dc.contributor.author Hendrix, A. R.
dc.contributor.author Cassidy, T. A.
dc.contributor.author Paranicas, C.
dc.contributor.author Teolis, B.
dc.contributor.author Hansen, C. J.
dc.date.accessioned 2013-07-08T16:44:03Z
dc.date.available 2013-07-08T16:44:03Z
dc.date.issued 2012-09-28
dc.identifier.citation European Planetary Science Congress (EPSC) 2012, Madrid, Spain, September 23-29, 2012 en_US
dc.identifier.clearanceno 12-3382
dc.identifier.uri http://hdl.handle.net/2014/43335
dc.description.abstract We present far-ultraviolet (FUV) observations of Mimas and Tethys, which show evidence for likely seasonal variation in UV albedo across their surfaces. The ultraviolet is an important wavelength regime for studying the effects of photolytic and radiolytic processes, because primarily the uppermost layers of the regolith and grains are sensed in this range. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2012. en_US
dc.subject Cassini Ultraviolet Imaging Spectrograph (UVIS) en_US
dc.subject far-ultraviolet (FUV) en_US
dc.title Seasonal variability on Saturn’s Moons Mimas and Tethys en_US
dc.type Preprint en_US


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