File:Inverted channels Mars PIA08070.jpg
本预览的尺寸：254 × 598像素。 其他分辨率：102 × 240像素 | 204 × 480像素 | 651 × 1,533像素。
原始文件 （651 × 1,533像素，文件大小：147 KB，MIME类型：image/jpeg）
摘要
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English: Original Caption Released with Image:
13 April 2006 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows ridges exposed by erosion in the Aeolis region of Mars. The curved and crisscrossing ridges were once channels in a fan of sediment deposited in the Aeolis lowlands. The channels were more resistant to wind erosion than the surrounding materials, so today they are left standing as ridges rather than valleys. Location near: 6.1°S, 209.0°W Image width: ~3 km (~1.9 mi) Illumination from: lower left Season: Southern Summer Image Credit: NASA/JPL/Malin Space Science Systems Original image found at: [1] |
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许可协议
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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/zh、NASA版权方针页面或JPL图片使用方针。） |  |
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原始上传日志
The original description page was here. All following user names refer to en.wikipedia.
- 2006-07-11 15:34 Cuppysfriend 651×1533× (150950 bytes) Original Caption Released with Image: 13 April 2006 This [[Mars Global Surveyor]] (MGS) Mars Orbiter Camera (MOC) image shows ridges exposed by erosion in the Aeolis region of [[Mars]]. The curved and crisscrossing ridges were once channels in a fan of s
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| 当前 | 2009年5月28日 (四) 22:11 | | 651 × 1,533（147 KB） | File Upload Bot (Magnus Manske) | {{BotMoveToCommons|en.wikipedia|year={{subst:CURRENTYEAR}}|month={{subst:CURRENTMONTHNAME}}|day={{subst:CURRENTDAY}}}} {{Information |Description={{en|Original Caption Released with Image: 13 April 2006 This en:Mars Global Surveyor (MGS) Mars Orbi |
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