This rayed crater was given the name Bek
in March 2010
October 6, 2008
Image Mission Elapsed Time (MET):
Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
240 meters/pixel (0.15 miles/pixel)
Image is approximately 240 kilometers (150 miles) wide
9,500 kilometers (5,900 miles)
This NAC image from MESSENGER's second Mercury flyby shows a crater with a set of light-colored rays radiating outward from it. Such rays are formed when an impact excavates material from below the surface and throws it outward from the crater. These bright rays, consisting both of ejecta and the secondary craters that form when the ejected material re-impacts the surface, slowly begin to fade as they are exposed to the harsh space environment. Mercury and other airless planetary bodies are constantly being bombarded with micrometeorites and energetic ions, an effect known as space weathering. Craters with bright rays are thought to be relatively young because the rays are still visible, suggesting that they have had less exposure to weathering processes. The crater in the center of this image has rays that have already begun to fade, implying that it is older than some other rayed craters on Mercury's surface. Images of younger craters with much brighter and more striking rays
have been previously released.
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.