Eminescu crater is 125 kilometers (78 miles) in diameter and can be seen just at the top of the image previously released on January 30. The image shown here was acquired by the Mercury Dual Imaging System (MDIS) on January 14, 2008, and shows a portion of Mercury's surface unseen by spacecraft prior to MESSENGER's historic flyby. Eminescu is a particularly interesting crater for several reasons. Eminescu formed more recently than most of the craters on Mercury, on the grounds that there are very few later craters superposed on it. Moreover, impressive chains of secondary craters, formed by material ejected by the impact explosion that formed the crater, radiate away from Eminescu. The central peaks within the crater are arranged in a circular pattern; geologists call this a “peak ring.” The bright peaks inside Eminescu exhibit unusual color characteristics in the 11-color Wide Angle Camera (WAC) images, which the MESSENGER Science Team is currently studying. They show up with a bluish tinge in the previously released false-color image of the entire planet; Eminescu is just north of the equator, near the day/night “terminator” in that image.
Image Mission Elapsed Time (MET): 108828468
Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
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