Aeolis Mensae

Aeolis Mensae is tableland feature in the Aeolis quadrangle of Mars. Its location is centered at 2.9° south latitude and 219.6° west longitude. It is 820 kilometres (510 mi) long and was named after a classical albedo feature name.[1]

Aeolis Mensae
Aeolis Mensae yardangs, as seen by HiRISE. Scale bar is 500 meters long. Click on image for better view of yardangs.
Coordinates2.9°S 219.6°W / -2.9; -219.6
Aeolis Mensae

Inverted relief

Some places on Mars show inverted relief, in which a stream bed may be a raised feature, instead of a valley. The inversion may be caused by the deposition of large rocks or by cementation. In either case erosion lowered the surrounding land, but left the old channel as a raised ridge because the stream bed is more resistant to erosion. An image taken by HiRISE shows a ridge that may be old channels that have become inverted.[2]

A study from 2019 showed that the area of Aeolis Mensae is the most likely source of methane which was previously detected by Curiosity.[3]

References
  1. "Planetary Names: Welcome". Planetarynames.wr.usgs.gov. Retrieved 2013-03-17.
  2. "HiRISE | Sinuous Ridges Near Aeolis Mensae". Hiroc.lpl.arizona.edu. 2007-01-31. Archived from the original on 2016-03-05. Retrieved 2013-03-17.
  3. Amoroso, Marilena; Merritt, Donald; Parra, Julia Marín-Yaseli de la; Cardesín-Moinelo, Alejandro; Aoki, Shohei; Wolkenberg, Paulina; Formisano, Vittorio; Oehler, Dorothy; Etiope, Giuseppe; Neary, Lori; Daerden, Frank; Viscardy, Sébastien; Giuranna, Marco (1 April 2019). "Independent confirmation of a methane spike on Mars and a source region east of Gale Crater". Nature Geoscience. 12 (5): 326–332. Bibcode:2019NatGe..12..326G. doi:10.1038/s41561-019-0331-9. ISSN 1752-0908. S2CID 134110253.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.