Bernard (crater) explained

Bernard (crater) should not be confused with Barnard (Martian crater).

Titlecolor:
  1. FA8072
Bernard
Coordinate Title:Coordinates
Globe:Mars
Coordinates:-23.4°N -154.2°W
Diameter:128 km
Eponym:P. Bernard, a French atmospheric scientist

Bernard is a large crater in the Memnonia quadrangle of Mars, located at 23.4° south latitude and 154.2° west longitude. It is 128 km in diameter and was named after P. Bernard, a French atmospheric scientist. The floor of the crater contains large cracks, which may be due to erosion.

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.[1] The peak is caused by a rebound of the crater floor following the impact.[2] If one measures the diameter of a crater, the original depth can be estimated with various ratios. Because of this relationship, researchers have found that many Martian craters contain a great deal of material; much of it is believed to be ice deposited when the climate was different.[3] Sometimes craters expose layers that were buried. Rocks from deep underground are tossed onto the surface. Hence, craters can show us what lies deep under the surface.

See also

Notes and References

  1. Web site: Stones, Wind, and Ice: A Guide to Martian Impact Craters.
  2. Book: Hugh H. Kieffer. Mars. 7 March 2011. 1992. University of Arizona Press. 978-0-8165-1257-7.
  3. Garvin, J., et al. 2002. Global geometric properities of martian impact craters. Lunar Planet Sci. 33. Abstract @1255.