Photos • Location


Escalante_(crater) Latitude and Longitude:
0°12′N 244°42′W / 0.2°N 244.7°W / 0.2; -244.7
From Wikipedia, the free encyclopedia
(Redirected from Escalante (crater))
Escalante Crater
Escalante Crater Wall, as seen by HiRISE. Picture on left is enlargement of the one on right. Scale bar is long.
PlanetMars
Coordinates 0°12′N 244°42′W / 0.2°N 244.7°W / 0.2; -244.7
Quadrangle Amenthes
EponymMexican astronomer F. Escalante

Escalante Crater is an impact crater in the Amenthes quadrangle of Mars. It is located at 0.2° N and 244.7° W. It is 79.3 km (49.3 mi) in diameter, and was named after Mexican astronomer (c. 1930) Francisco Javier Escalante Plancarte [ es]. [1]

This topographic map was created using Mars Orbiter Laser Altimeter (MOLA) technology on the Mars Global Surveyor spacecraft. This image is a screenshot of RedMapper's website and shows the rim and center of Escalante crater
  • Map of Amenthes quadrangle. The northwest part is the large impact basin Isidis. The crater Escalante sits right on the equator.
    Map of Amenthes quadrangle. The northwest part is the large impact basin Isidis. The crater Escalante sits right on the equator.
  • CTX camera (on Mars Reconnaissance Orbiter) image of Escalante Crater. Dunes are visible near the bottom of the image.
    CTX camera (on Mars Reconnaissance Orbiter) image of Escalante Crater. Dunes are visible near the bottom of the image.
  • Enlargement of dunes in Escalante Crater from previous photo. Image taken with CTX camera (on Mars Reconnaissance Orbiter).
    Enlargement of dunes in Escalante Crater from previous photo. Image taken with CTX camera (on Mars Reconnaissance Orbiter).

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. [2] The peak is caused by a rebound of the crater floor following the impact. [3] 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. [4] 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

References

  1. ^ "Gazetteer of Planetary Nomenclature". planetarynames.wr.usgs.gov. Feature 1841. USGS. 17 November 2010. Retrieved 2022-04-15.
  2. ^ "Stones, Wind, and Ice: A Guide to Martian Impact Craters".
  3. ^ Hugh H. Kieffer (1992). Mars. University of Arizona Press. ISBN  978-0-8165-1257-7. Retrieved 7 March 2011.
  4. ^ Garvin, J., et al. 2002. Global geometric properities of martian impact craters. Lunar Planet Sci. 33. Abstract @1255.
Retrieved from " https://en.wikipedia.org/?title=Escalante_(Martian_crater)&oldid=1199102554"