File:Mars glacial-like lobe deposit.jpg

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Summary

DescriptionMars glacial-like lobe deposit.jpg	Perspective view of a 5-km-wide, glacial-like lobe deposit sloping up into a box canyon along the crustal dichotomy boundary on Mars. The up-slope geometry of these deposits implies a past thickness of ice on the order of ~920 m at this location. Cessation of glacial conditions caused lowering of the debris-covered glacier surface to the configuration seen today. See “Late Amazonian glaciation at the dichotomy boundary on Mars: Evidence for glacial thickness maxima and multiple glacial phases,” by Dickson et al. (2008), doi:10.1130/G24382A.1
Date	circa 2008 date QS:P,+2008-00-00T00:00:00Z/9,P1480,Q5727902
Source	Geological Society of America
Author	NASA/JPL/MSSS

Licensing

	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.)
	Warnings: Use of NASA logos, insignia and emblems is restricted per U.S. law 14 CFR 1221. The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI.[1] See also {{PD-Hubble}} and {{Cc-Hubble}}. The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. [2] Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. [3] The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	11:21, 28 April 2008		550 × 474 (64 KB)	Bender235	{{Information \|Description=Perspective view of a 5-km-wide, glacial-like lobe deposit sloping up into a box canyon along the crustal dichotomy boundary on Mars. The up-slope geometry of these deposits implies a past thickness of ice on the order of ~920 m

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- Aigua a Mart
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- Presencia de agua en Marte
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- Géologie de Mars
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- Geologija Marsa
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- مریخ اُتے پانی
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- Гидросфера Марса
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- مریخ پر پانی
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