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Matabei's Unusual Dark Rays
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Matabei's Unusual Dark Rays
Release Date: September 14, 2010
Topics: Crater Rays, Craters with Dark Material, HD Resolution Images, Mercury Flyby 2, NAC, Named Craters



Date Acquired: October 6, 2008
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Scale: Matabei is 24 kilometers (15 miles) in diameter

Of interest: When a meteoroid strikes the surface of a planet, material from the target area is ejected outward at high velocity, often creating rays that extend over distances far greater than the size of the crater formed by the impact. During MESSENGERís second Mercury flyby, MDIS captured images of many impressive rays on Mercury, such as the ejecta prominent around Kuiper crater and the extensive ray system associated with the northerly Hokusai crater. For both of those examples, the rays appear bright, which is characteristic of freshly pulverized rock and indicates that the rays are younger than much of Mercuryís surface. In contrast, in the center of this image, a set of dark rays can be seen emanating from the small crater Matabei. Dark rays are rare on Mercury, but other occurrences have been identified, such as at Mozart crater. Mozart is interpreted to have excavated dark material from depth during the impact event, creating dark streamers. The dark rays from Matabei may have a similar origin, and color images to be obtained during MESSENGER's orbital mission phase will be used to explore further the nature of these unusual dark rays.

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington


For information regarding the use of MESSENGER images, see the image use policy.


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