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Shoreline retreat at Titan’s Ontario Lacus and Arrakis Planitia from Cassini Imaging Science Subsystem observations |
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| Authors: | E.P. Turtle J.E. Perry A.S. McEwen |
| Affiliation: | a Johns Hopkins Univ. Applied Physics Lab., 11100 Johns Hopkins Rd., Laurel, MD 20723, United States b Lunar and Planetary Lab., Univ. of Arizona, 1541 E. University Blvd., Tucson, AZ 85721, United States c California Inst. of Technology, 1200 E. California Blvd., Pasadena, CA 91125, United States |
| Abstract: | Recent observations by Cassini’s Imaging Science Subsystem reveal that part of the shoreline of Titan’s Ontario Lacus has retreated by several kilometers and may indicate that the dark area that appeared at Arrakis Planitia (80°S, 120°W) in late 2004 has subsequently faded. These changes provide constraints on aspects of Titan’s methane cycle, as well as on the properties of Titan’s surface materials. |
| Keywords: | Titan Meteorology Satellites, Surfaces |
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