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Not Your Average Complex Crater
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Not Your Average Complex Crater

November 30, 2012
By comparing photographs from past eras of lunar exploration with the high resolution data being returned by the Lunar Reconnaissance Orbiter Narrow Angle Camera, we can identify new craters that have formed in the last four decades. In this case, bright ejecta and rays extend from an impact site that is not present in the previous image from the Apollo 15 panoramic camera. The Apollo image (AS15-9527) was taken in August 1971 with the sun 64° above the horizon. The LROC image (M108971316L) was taken September 30, 2009 when the sun was 72° above the horizon. Images taken under similar lighting conditions like these are the most useful for identifying and comparing surface features. Using these two images as "before" and "after" views, we can conclude that a natural object (asteroid or comet) about 0.5 m (~20 inches) in diameter must have impacted the Moon here within the last 38 years. Note that this location (16.92° N latitude, 40.50° E longitude) does not correspond to a known impact site for past spacecraft, nor is it near any of the Apollo landing sites, where the Lunar Module ascent stages impacted and created craters. The impact exposed fresh material from underneath the surface. Rays of this bright material extend far outward from the central crater, helping us to clearly identify it. The rays are actually more than 3x more reflective than the underlying basalts! Thus, even though the crater itself is only ~10 meters (30 feet) across, the bright markings would have been prominent in the high-sun Apollo image if the crater had existed in 1971. Discoveries of recent, datable impact craters like these establish the present-day impact cratering rate on the Moon, which will lead to better understanding of the bombardment rate in the inner solar system. Meteorites of this size are a potential hazard to future explorers on the Moon or anywhere in the inner Solar System where there is no shielding atmosphere. If we have a better sense of the current impact rate for this size of impactor, we can more effectively design habitats and hardware to protect human explorers. A crater this young has also not been modified by other processes, so we can study the appearance of features we know are extremely fresh. In addition, since ages are estimated using the number of craters present on planetary surfaces, knowing how many craters are currently being produced will improve our understanding of the geologic history of the Moon, Mars, and other planets. In particular, we must rely on small craters like this to date small areas and/or geologically recent terrains. The small, irregular terraces on the walls of Bürg Crater and the debris piles and outcropping wall material, with strong variations in reflectance, only hint at the geologic diversity of this complex crater. Bürg's crater rim is on the upper left, with downslope direction toward the lower right. Illumination is from the right, image width is 870 m, LROC NAC M116139887R. Credit: NASA/GSFC/Arizona State University