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File:Badlands of Aram Chaos.jpg

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Badlands of Aram Chaos This observation shows erosional features on light-toned rocks in Aram Chaos, a crater near the equator of Mars that has been nearly filled with sedimentary rocks. In enhanced color, the sediments are very distinctive. The rocks show a sharp change in color partway down the slope, indicating a change in the properties of the rock, probably to a different composition.

The erosional features have alcoves with aprons downslope, and in some cases have hints of channels, potentially due to abrasion by falling debris. These morphologies bear some resemblance to gullies commonly found in the mid-latitudes, which are often thought to have formed due to erosion by liquid water from melting snow. Near the equator, however, snowmelt in Mars' recent climate is less likely.
来源

https://mars.jpl.nasa.gov/multimedia/images/index.cfm?ImageID=5310

https://mars.nasa.gov/images/33_Badlands_of_Aram_Chaos-full.jpg
作者 w:NASA

许可协议

Public domain 本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zhNASA版权方针页面JPL图片使用方针。)
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The original description page was here. All following user names refer to en.wikipedia.
日期/时间 大小 用户 备注
2017-07-28 06:08:38 2020 × 1488 Dr.K. higher res.
2017-07-28 06:00:57 1024 × 754 Dr.K. {{Information |Description = Badlands_of_Aram_Chaos |Source = https://mars.jpl.nasa.gov/multimedia/images/index.cfm?ImageID=5310 |Date = ~~~~~ |Author = [[NASA]] |Permission = |other_versions = }}

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当前2018年4月5日 (四) 04:002018年4月5日 (四) 04:00版本的缩略图2,020 × 1,488(1.12 MB)OgreBot(BOT): Reverting to most recent version before archival
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