PIA13476: Matabei's Unusual Dark Rays
 Target Name:  Mercury
 Is a satellite of:  Sol (our sun)
 Mission:  MESSENGER
 Spacecraft:  MESSENGER
 Instrument:  MDIS - Narrow Angle
 Product Size:  1920 x 1080 pixels (w x h)
 Produced By:  Johns Hopkins University/APL
 Full-Res TIFF:  PIA13476.tif (2.076 MB)
 Full-Res JPEG:  PIA13476.jpg (278.5 kB)

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Original Caption Released with Image:

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 MESSENGER's 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 Mercury's 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.

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

These images are from MESSENGER, a NASA Discovery mission to conduct the first orbital study of the innermost planet, Mercury. For information regarding the use of images, see the MESSENGER image use policy.

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

Image Addition Date: