File:Rachmaninoff crater.png

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English: Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)

Scale: The diameter of Rachmaninoff is 290 kilometers (180 miles) Projection: This image is a portion of the NAC approach mosaic acquired during Mercury flyby 3. Shown here is an orthographic reprojection of that mosaic with a resolution of 500 meters/pixel (0.3 miles/pixel).

Of Interest: The International Astronomical Union (IAU) recently approved the name Rachmaninoff for an intriguing double-ring basin on Mercury. This basin, first imaged in its entirety during MESSENGER's third Mercury flyby, was quickly identified as a feature of high scientific interest, because of its fresh appearance, its distinctively colored interior plains, and the extensional troughs on its floor. At the NASA science update to the media on November 3, 2009, this then-unnamed basin featured prominently in the imaging results presented, with both an enhanced-color image and a reprojected mosaic released and discussed. The basin’s name honors the Russian composer, pianist, and conductor, Sergei Rachmaninoff (1873-1943). Rachmaninoff joins ten other names for Mercury craters approved this month.
Date
Source RACHMANINOFF IN CONCERT WITH RECENTLY NAMED CRATERS ON MERCURY
Author NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current17:00, 2 May 2010Thumbnail for version as of 17:00, 2 May 20101,908 × 1,391 (1.94 MB)Bryan Derksen (talk | contribs){{Information |Description={{en|1=Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS) Scale: The diameter of Rachmaninoff is 290 kilometers (180 miles) Projection: This image is a portion of the NAC approach mosaic acquired dur

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