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Two-toned Impact Crater in Balmer Basin A Reflection of the
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Two-toned Impact Crater in Balmer Basin: A Reflection of the Target?

November 29, 2012
The Balmer Basin Constellation Region of Interest lies within the Balmer Crater, centered at about 20°S latitude and 70°E longitude. Balmer is an old, highly degraded crater some 110 km across and is part of a larger basin structure called the Balmer-Kapteyn Basin, which has 225 km and 450 km diameter rings. Scientifically, this area is interesting because it contains a type of 'light plains deposit' that appears to lie on top of an ancient basaltic surface. Building on earlier studies of these deposits, Hawke et al. [2005] concluded that the deposits formed by the deposition of material ejected by later-formed impact basins that mixed with regolith that had developed on the old Balmer volcanic lava flows. This conclusion was based on the occurrence of numerous 'dark haloed' impact craters, such as one shown as an LROC featured image on August 31, 2009. Perhaps dark-haloed craters are not the only types that reflect this dichotomy. Two-toned deposits are evident in the crater shown in today's featured image. This distinctive two-toned appearance is seen in some other similar-size craters in Balmer, but is not common. The regolith here is probably fairly thick, perhaps 50 to 100 m in many places. The regolith is a zone of mixing between the light-toned basin ejecta deposits and the underlying basalts. This crater appears to have excavated both types of materials. Materials excavated during formation of this ~450 m diameter impact crater have an unusual two-toned character, likely a reflection of heterogeneity in the target materials. This crater occurs in Balmer Basin, an area thought to harbor a type of 'cryptomare' - an old volcanic surface covered by later light-toned impact deposits. The dark materials may be basaltic rock excavated from deeper parts of the crater. The crater is located at 18.341°S latitude and 69.950°E longitude. The scene is 540 m across, a subset of NAC M111138159LE. Credit: NASA/GSFC/Arizona State University


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