File:Inverted channels Mars PIA08070.jpg
預覽大小：254 × 598 像素。 其他解析度：102 × 240 像素 | 204 × 480 像素 | 651 × 1,533 像素。
原始檔案 （651 × 1,533 像素，檔案大小：147 KB，MIME 類型：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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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/zh，NASA版權政策或JPL圖像使用政策） |  |
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原始上傳日誌
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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