File:Titan - Rev 181 (37267739732).png
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Summary
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Four frame infrared mosaic of Titan's surface acquired by Cassini as it approached the moon for the T-89 flyby on Februrary 17, 2013. At the time, Cassini was ~625,000 km from the moon. This image captures Titan's southern hemisphere, with the dark equatorial Belet region the primary visible surface feature. This is one of the many large equatorial dune fields present on Titan. The bright Adiri region, which is likely a highlands region of pure water ice crust pokes through the dune fields at the 3 o'clock position. The growing winter polar vortex, which forms over the polar regions during the 14.5-year polar night, is also visible at the 7 o'clock position. Image Credit: NASA / JPL / Cassini-SSI / Justin Cowart |
| Date | |
| Source | Titan - Rev 181 |
| Author | Justin Cowart |
Licensing
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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This image was originally posted to Flickr by jccwrt at https://flickr.com/photos/132160802@N06/37267739732. It was reviewed on 3 December 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
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| current | 12:23, 3 December 2020 | 2,000 × 2,000 (2.5 MB) | Eyes Roger (talk | contribs) | Transferred from Flickr via #flickr2commons |
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