A 5-Micron-Bright Spot on Titan: Evidence for Surface Diversity

Author:

Barnes Jason W.12345,Brown Robert H.12345,Turtle Elizabeth P.12345,McEwen Alfred S.12345,Lorenz Ralph D.12345,Janssen Michael12345,Schaller Emily L.12345,Brown Michael E.12345,Buratti Bonnie J.12345,Sotin Christophe12345,Griffith Caitlin12345,Clark Roger12345,Perry Jason12345,Fussner Stephanie12345,Barbara John12345,West Richard12345,Elachi Charles12345,Bouchez Antonin H.12345,Roe Henry G.12345,Baines Kevin H.12345,Bellucci Giancarlo12345,Bibring Jean-Pierre12345,Capaccioni Fabrizio12345,Cerroni Priscilla12345,Combes Michel12345,Coradini Angioletta12345,Cruikshank Dale P.12345,Drossart Pierre12345,Formisano Vittorio12345,Jaumann Ralf12345,Langevin Yves12345,Matson Dennis L.12345,McCord Thomas B.12345,Nicholson Phillip D.12345,Sicardy Bruno12345

Affiliation:

1. Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.

2. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

3. Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.

4. Laboratoire de Planétologie et Géodynamique, UMR CNRS 6112, Université de Nantes, France.

5. U.S. Geological Survey, Flagstaff, AZ 86001, USA.

Abstract

Observations from the Cassini Visual and Infrared Mapping Spectrometer show an anomalously bright spot on Titan located at 80°W and 20°S. This area is bright in reflected light at all observed wavelengths, but is most noticeable at 5 microns. The spot is associated with a surface albedo feature identified in images taken by the Cassini Imaging Science Subsystem. We discuss various hypotheses about the source of the spot, reaching the conclusion that the spot is probably due to variation in surface composition, perhaps associated with recent geophysical phenomena.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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