Difference between revisions of "File:ESP 055530 2180channels.jpg"
(Channels on the edge of a crater's ejecta. The heat form the impact ejecta may have melted ice in the ground and formed the channels we see. Source: http://hirise.lpl.arizona.edu/ESP_055530_2180 Image credit: NASA/JPL/University of Arizona) |
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Latest revision as of 08:57, 21 April 2020
Summary
Channels on the edge of a crater's ejecta. The heat form the impact ejecta may have melted ice in the ground and formed the channels we see.
Source: http://hirise.lpl.arizona.edu/ESP_055530_2180
Image credit: NASA/JPL/University of Arizona
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 08:57, 21 April 2020 |  | 2,048 × 4,468 (3.4 MB) | Suitupandshowup (talk | contribs) | Channels on the edge of a crater's ejecta. The heat form the impact ejecta may have melted ice in the ground and formed the channels we see. Source: http://hirise.lpl.arizona.edu/ESP_055530_2180 Image credit: NASA/JPL/University of Arizona |
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