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Copernicus (lunar crater)
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The terrain along the bottom is hilly in the southern half while the north is relatively smooth. The central peaks consist of three isolated mountainous rises climbing as high as 1. These peaks are separated from each other by valleys, and they form a rough line along an east-west axis.
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Infrared observations of these peaks during the s determined that they were primarily composed of the mafic form of olivine. Based on high-resolution images from Lunar Orbiter 5Terry W. Offield of the U. Sets of parallel fracturesaligned with the lunar structure grid, formed after the crater wall took its present form, but before the smoothest floor materials were emplaced.
The smooth floor materials show a swirling pattern of cracks like those seen on terrestrial lava flows. These materials are associated with numerous hills that have summit craters and are probably small volcanoes. Several low places on the rim and wall are partly filled by what appears to be ponded volcanic material, or possibly fluidized impact debris. The rays are less distinct than the long, linear rays extending from Tychoinstead forming a nebulous pattern with plumy markings.
In multiple locations the rays lie at glancing angles, instead of forming a true radial dispersal.
An extensive pattern of smaller secondary craters can also be observed surrounding Copernicus, a detail that was depicted in a map by Giovanni Cassini in Some of these secondary craters form sinuous chains in the ejecta.