Lunae Palus Quadrangle - Craters

Craters

Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. The peak is caused by a rebound of the crater floor following the impact. Sometimes craters will display layers. Craters can show us what lies deep under the surface.

  • Fesenkov Crater Central Peak, as seen by HiRISE.

  • Santa Fe Crater, as seen by HiRISE.

  • Close up of gullies in previous image, as seen by HiRISE.

  • Canso Crater

  • Canso Crater North Wall and Floor, as seen by HiRISE.

  • Montevallo Crater, as seen by THEMIS. Image shows a landslide on the north rim.

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