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PIA11355: Bright Ejecta Rays of Kuiper
Target Name: Mercury
Is a satellite of: Sol (our sun)
Mission: MESSENGER
Spacecraft: MESSENGER
Instrument: Mercury Dual Imaging System - Narrow Angle
Product Size: 1018 samples x 1024 lines
Produced By: Johns Hopkins University/APL
Full-Res TIFF: PIA11355.tif (1.044 MB)
Full-Res JPEG: PIA11355.jpg (129.4 kB)

Click on the image to download a moderately sized image in JPEG format (possibly reduced in size from original).

Original Caption Released with Image:

During Monday’s flyby of Mercury, MESSENGER’s NAC captured a new view of the bright, radial ejecta rays of Kuiper crater that were previously imaged by Mariner 10 at a lower Sun angle. Kuiper crater is named for Gerard Kuiper, a Dutch-American astronomer who was also a member of the Mariner 10 team. Bright ejecta rays such as these are produced as impacts excavate and eject relatively unweathered subsurface material. The ejecta rays of Kuiper and other large craters are observed to extend for hundreds of kilometers across the cratered terrain of Mercury, as seen on the full planet image from MESSENGER’s Wide Angle Camera (WAC) released previously (PIA11245).

Date Acquired: October 6, 2008
Image Mission Elapsed Time (MET): 131774036
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Resolution: 530 meters/pixel (0.33 miles/pixel)
Scale: Kuiper crater is 62 kilometers in diameter (39 miles)
Spacecraft Altitude: 21,000 kilometers (13,000 miles)

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


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