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.
來源

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

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Public domain 本作品由NASA創作,屬於公有領域。根據NASA的版權政策:“NASA的創作除非另有聲明否則不受版權保護。”(參見:Template:PD-USGov/zhNASA版權政策JPL圖像使用政策
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The original description page was here. All following user names refer to en.wikipedia.
日期/時間 尺寸 用戶 備⁠註
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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目前2018年4月5日 (四) 04:00於 2018年4月5日 (四) 04:00 版本的縮圖2,020 × 1,488(1.12 MB)OgreBot(BOT): Reverting to most recent version before archival
2018年4月5日 (四) 04:00於 2018年4月5日 (四) 04:00 版本的縮圖1,024 × 754(205 KB)OgreBot(BOT): Uploading old version of file from en.wikipedia; originally uploaded on 2017-07-28 06:00:57 by Dr.K.
2018年4月4日 (三) 19:24於 2018年4月4日 (三) 19:24 版本的縮圖2,020 × 1,488(1.12 MB)IazygesTransferred from en.wikipedia (MTC!) (1.1.0)

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