File:Flow-like features in Dunes on Richardson Crater, Mars - example 2.jpg
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Summary
[edit]DescriptionFlow-like features in Dunes on Richardson Crater, Mars - example 2.jpg |
English: The dark material at the end of the flows moves at between 0.1
and 1.4 m/day in late spring / summer on Mars. Most models for it favour liquid water as a cause. Either interfacial layers, or else layers of water created through the solid state greenhouse effect. http://www.lpi.usra.edu/meetings/lpsc2008/pdf/1555.pdf |
Date | |
Source | Detail from http://www.uahirise.org/PSP_003597_1080 obtained using HiView |
Author | NASA/JPL/University of Arizona |
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[edit]Public domainPublic domainfalsefalse |
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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current | 01:07, 15 April 2015 | 844 × 868 (177 KB) | Robertinventor (talk | contribs) | User created page with UploadWizard |
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