Columbus (Martian crater)

Columbus Crater

Columbus crater based on THEMIS day-time image
Planet Mars
Coordinates 29°48′S 166°06′W / 29.8°S 166.1°W / -29.8; -166.1Coordinates: 29°48′S 166°06′W / 29.8°S 166.1°W / -29.8; -166.1
Diameter 119 km
Eponym Christopher Columbus, Italian explorer (1451-1506)

Columbus Crater is a crater in the Memnonia quadrangle of Mars, located at 29.8° south latitude and 166.1° west longitude. It is 119 km in diameter and was named after Christopher Columbus, Italian explorer (1451–1506).[1][2] The discovery of sulfates and clay minerals in sediments within Columbus Crater are strong evidence that a lake once existed in the crater.[3][4] Research with an orbiting near-infrared spectrometer, which reveals the types of minerals present based on the wavelengths of light they absorb, found evidence of layers of both clay and sulfates in Columbus crater. This is exactly what would appear if a large lake had slowly evaporated.[5][6] Moreover, because some layers contained gypsum, a sulfate which forms in relatively fresh water, life could have formed in the crater.[7]

Layers

Columbus Crater contains layers, also called strata. Many places on Mars show rocks arranged in layers. Rock can form layers in a variety of ways. Layers may be formed by volcanoes, wind, or water.[8] Sometimes the layers are of different colors. Light-toned rocks on Mars have been associated with hydrated minerals like sulfates. The Mars Rover Opportunity examined such layers close-up with several instruments. Some layers are probably made up of fine particles because they seem to break up into fine dust. Other layers break up into large boulders so they are probably much harder. Basalt, a volcanic rock, is thought to be in the layers that form boulders. Basalt has been identified on Mars in many places. Instruments on orbiting spacecraft have detected clay (also called phyllosilicates) in some layers. In Columbus Crater, the CRISM instrument on the Mars Reconnaissance Orbiter found kaolinite, hydrated sulfates including alunite and possibly jarosite.[9] Further study concluded that gypsum, polyhydrated and monohydrated Mg/Fe-sulfates were common and small deposits of montmorillonite, Fe/Mg-phyllosilicates, and crystalline ferric oxide or hydroxide were found. Thermal emission spectra suggest that some minerals were in the tens of percent range.[10][11]

Scientists are excited about finding hydrated minerals such as sulfates and clays on Mars because they are usually formed in the presence of water.[12] Places that contain clays and/or other hydrated minerals would be good places to look for evidence of life.[13] Sulfate minerals were found above aluminum-rich clays.[14]

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See also

References

  1. ↑ "Gazetteer of Planetary Nomenclature | Columbus". usgs.gov. International Astronomical Union. Retrieved 4 March 2015.
  2. ↑ http://www.google.com/mars/
  3. ↑ http://www.nasa.gov/mission_pages/msl/multimedia/pia15099.html#.VWyD-c9VhBc
  4. ↑ Wray,J., R. Milliken, C. Dundas, G. Swayze, J. Andrews-Hanna, A. Baldridge, M. Chojnacki, J. Bishop, B. Ehlmann, S. Murchie, R. Clark, F. Seelos, L. Tornabene, and S. Squyres. 2011. Columbus crater and other possible groundwater-fed paleolakes of Terra Sirenum, Mars. Journal of Geophysical Research E: Planets DOI: 10.1029/2010JE003694
  5. ↑ Cabrol, N. and E. Grin (eds.). 2010. Lakes on Mars. Elsevier.NY.
  6. ↑ Wray, J. et al. 2009. Columbus Crater and other possible plaelakes in Terra Sirenum, Mars. Lunar and Planetary Science Conference. 40: 1896.
  7. ↑ http://news.nationalgeographic.com/news/2009/11/091125-mars-crater-lake-michigan-water_2.html
  8. ↑ http://hirise.lpl.arizona.edu?PSP_008437_1750
  9. ↑ Murchie, S. et al. 2009. A synthesis of Martian aqueous mineralogy after 1 Mars year of observations from the Mars Reconnaissance Orbiter. Journal of Geophysical Research: 114.
  10. ↑ https://pubs.er.usgs.gov/publication/70035986
  11. ↑ Wray,J., R. Milliken, C. Dundas, G. Swayze, J. Andrews-Hanna, A. Baldridge, M. Chojnacki, J. Bishop, B. Ehlmann, S. Murchie, R. Clark, F. Seelos, L. Tornabene, and S. Squyres. 2011. Columbus crater and other possible groundwater-fed paleolakes of Terra Sirenum, Mars. Journal of Geophysical Research E: Planets DOI: 10.1029/2010JE003694
  12. ↑ http://themis.asu.edu/features/nilosyrtis
  13. ↑ http://hirise.lpl.arizona.edu/PSP_004046_2080
  14. ↑ https://www.nasa.gov/mission_pages/msl/multimedia/pia15099.html#.VTj_UiFVhBd
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