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lroc.sese.asu.edu
Most of the craters on the Moon formed through impact processes. However, some craters, like the one visible in this portion of LROC NAC frame M131488521R, may be a volcano summit pit crater. Crater diameter is ~400 m, the image width is 923 m, and illumination is from the right [NASA/GSFC/Arizona State University]. |
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lroc.sese.asu.edu
Sunrise image of the Eratosthenes central peak summit. LROC NAC image M131725388L; width is 600 m [NASA/GFSC/Arizona State University]. |
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lroc.sese.asu.edu
An asymmetric impact crater (14.349°S, 350.977°E) on the Lassell Massif revealing low reflectance material. NAC frame M152939732L, illumination is from the northwest, north is up, image is ~820 m wide [NASA/GSFC/Arizona State University]. |
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science.nasa.gov
NASA's Lunar Discovery and Exploration program establishes and facilitates science research that is important to the lunar science community. |
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