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File:Rachmaninoff crater (closeup).jpg

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English: This spectacular 290-kilometer-diameter double-ring basin seen in detail for the first time during MESSENGER's third flyby of Mercury bears a striking resemblance to Raditladi basin, observed during the first flyby. This basin, now named Rachmaninoff, is remarkably well preserved and appears to have formed relatively recently, compared with most basins on Mercury. The low numbers of superposed impact craters and marked differences in color across the basin (seen in this enhanced color image released earlier this week) suggest that the smooth area within the innermost ring may be the site of some of the most recent volcanism on Mercury.
Date Acquired: September 29, 2009
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Scale: This double-ring basin is 290 kilometers (180 miles) in diameter
(original caption, edited to include the name)
日期
來源 http://photojournal.jpl.nasa.gov/catalog/PIA12368
作者 NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

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目前2010年7月17日 (六) 16:58於 2010年7月17日 (六) 16:58 版本的縮圖791 × 780(86 KB)Ruslik0{{Information |Description={{en|1=This spectacular 290-kilometer-diameter double-ring basin seen in detail for the first time during MESSENGER's third flyby of Mercury bears a striking resemblance to Raditladi basin, observed during the first flyby. This

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