File:Frost in the Hellaspontes Montes - Mars Express (44410805372).png

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Mars Express HRSC image of CO2 frost deposits in unnamed midsouthern craters. These craters are located in the western Hellaspontes Montes, a mountain chain composed of jumbled ejecta deposits of the Hellas Basin.

During the winter season, the surface becomes so cold at night that the atmosphere freezes out on the surface. This frost typically sublimates back into the atmosphere during the day, but can last through the winter in shaded alcoves. In the large crater at bottom right, a sand dune reaches high enough above the crater floor that it catches a small amount of sunlight during the winter season, which keeps the peak of the dune frost free.

This image was during Mars Express' 8588th orbit of Mars, Spetember 19, 2010.

Image Credit: ESA/DLR/FU Berlin/J. Cowart, CC BY-SA 3.0 IGO
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Source Frost in the Hellaspontes Montes - Mars Express
Author Justin Cowart

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This file is licensed under the Creative Commons Attribution-ShareAlike 3.0 IGO license.
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This image was originally posted to Flickr by jccwrt at https://flickr.com/photos/132160802@N06/44410805372. 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.

3 December 2020

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current12:18, 3 December 2020Thumbnail for version as of 12:18, 3 December 20208,533 × 2,400 (27 MB)Eyes Roger (talk | contribs)Transferred from Flickr via #flickr2commons

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