This small crater displays a beautiful ejecta pattern resembling a starburst. Looking at this image you can almost imagine the shower of ejecta falling to the ground. The pattern formed out of high and low reflectance areas is due to the freshness of the ejecta. Notice in the second image that as you move away from the center of the crater, the overall reflectance of the ejecta gets lower (darker). This is because the ejecta is less continuous as you get further away from the crater.



Same NAC frame but with a larger view to show context. Notice the bouldery center of this fresh crater and the two low albedo spots that represent secondary impacts. This image is 2.2 km across [NASA/GSFC/Arizona State University].

There are two low reflectance (darker) spots in the ejecta, one just south of the main crater and another just west of it. If you look closely, these spots are actually small craters with their own ejecta, probably secondaries from the primary impact. They excavated material from beneath the ejecta blanket and that material has a lower albedo compared to the ejecta.

Explore the entire NAC Frame!

Posted by: Soderman/NLSI Staff

Source: http://lroc.sese.asu.edu/news/index.php?/archives/380-Action-Shot.html

Posted: Apr 26, 10:43 am

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Lunar Science Forum

The NASA Lunar Science Institute is pleased to announce the 5th annual NASA Lunar Science Forum, to be held July 17-19, 2012. This year's forum will feature sessions on in-depth scientific results from the Lunar Reconnaissance Orbiter, ARTEMIS, LADEE, and the GRAIL satellites, a dedicated side-conference for graduate students and young lunar professionals, as well as the annual Shoemaker Award ceremony and associated keynote lecture.

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If you weigh 120 pounds, you would weigh only 20 pounds on the moon.

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