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File:Oblique View of Warm Season Flows in Newton Crater.jpg

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Revision as of 18:58, 12 September 2018 by Suitupandshowup (talk | contribs) (Recurrent slope lineae, as seen by HiRISE Location is Newton Crater. The flow features are narrow (one-half to five yards or meters wide), relatively dark markings on steep (25 to 40 degree) slopes at several southern hemisphere locations. Repeat im...)
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Oblique_View_of_Warm_Season_Flows_in_Newton_Crater.jpg (525 × 599 pixels, file size: 95 KB, MIME type: image/jpeg)

Summary

Recurrent slope lineae, as seen by HiRISE Location is Newton Crater. The flow features are narrow (one-half to five yards or meters wide), relatively dark markings on steep (25 to 40 degree) slopes at several southern hemisphere locations. Repeat imaging by HiRISE shows the features appear and incrementally grow during warm seasons and fade in cold seasons.


Source: http://photojournal.jpl.nasa.gov/catalog/PIA14479


Image credit: NASA/JPL-Caltech/Univ. of Arizona

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current18:58, 12 September 2018Thumbnail for version as of 18:58, 12 September 2018525 × 599 (95 KB)Suitupandshowup (talk | contribs)Recurrent slope lineae, as seen by HiRISE Location is Newton Crater. The flow features are narrow (one-half to five yards or meters wide), relatively dark markings on steep (25 to 40 degree) slopes at several southern hemisphere locations. Repeat im...

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