File:208500main Vivaldi crater.jpg

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English: As MESSENGER approached Mercury on January 14, 2008, the spacecraft’s Narrow-Angle Camera on the Mercury Dual Imaging System (MDIS) instrument captured this view of the planet’s rugged, cratered landscape illuminated obliquely by the Sun. The large, shadow-filled, double ringed crater to the upper right was glimpsed by Mariner 10 more than three decades ago and named Vivaldi, after the Italian composer. Its outer ring has a diameter of about 200 kilometers (about 125 miles). MESSENGER’s modern camera has revealed detail that was not well seen by Mariner 10, including the broad ancient depression overlapped by the lower-left part of the Vivaldi crater. The MESSENGER science team is in the process of evaluating later images snapped from even closer range showing features on the side of Mercury never seen by Mariner 10. It is already clear that MESSENGER’s superior camera will tell us much that could not be resolved even on the side of Mercury viewed by Mariner’s vidicon camera in the mid-1970s. This MESSENGER image was taken from a distance of about18,000 kilometers (11,000 miles), about 56 minutes before the spacecraft's closest encounter with Mercury. It shows a region roughly 500 kilometers (300 miles) across, and craters as small as 1 kilometer (0.6 mile) can be seen in this image.
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来源 http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?gallery_id=2&image_id=118
作者 NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

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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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当前2008年1月16日 (三) 19:392008年1月16日 (三) 19:39版本的缩略图1,024 × 1,024(725 KB)Bryan Derksen留言 | 贡献{{Information |Description={{en|As NASA's MESSENGER spacecraft approached Mercury on January 14, 2008, it captured this view of the planet's rugged, cratered landscape illuminated obliquely by the sun. This image was taken from a distance of approximately

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