Jump to content

Chincoteague (crater)

Coordinates: 41°30′N 236°00′W / 41.5°N 236.0°W / 41.5; -236.0
From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Fgnievinski (talk | contribs) at 06:20, 30 November 2019. The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Chincoteague Crater
Chincoteague Crater, as seen by HiRISE.
PlanetMars
Coordinates41°30′N 236°00′W / 41.5°N 236.0°W / 41.5; -236.0
QuadrangleCebrenia
Diameter37 km
EponymChincoteague, Virginia, USA

Chincoteague Crater is an impact crater in the Cebrenia quadrangle of Mars, located at 41.5° N and 236.0° W. It is 37.0 km in diameter and was named after Chincoteague, a town in Virginia, USA.[1] Chincoteague Crater has a small central mound. Along the wall of Chincoteague Crater a number of gullies are visible.

  • Close-up of Chincoteague Crater, as seen by HiRISE. Image close up view of previous image. Note the gullies and associated landforms.
    Close-up of Chincoteague Crater, as seen by HiRISE. Image close up view of previous image. Note the gullies and associated landforms.
  • Chincoteague Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter).
    Chincoteague Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter).
  • Gullies on western wall of Chincoteague Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter). Note: this is an enlargement of the previous image.
    Gullies on western wall of Chincoteague Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter). Note: this is an enlargement of the previous image.
  • A topographic map created using Mars Orbiter Laser Altimeter (MOLA) data. This map show the relative elevation in 100 meter elevation contour lines (dashed) and 500 meter elevation contour lines (bold) with an average accuracy of each point is originally ~100 meters in horizontal position and ~1 meter in radius (Neumann and others, 2001). However, the total elevation uncertainty is at least ±3 m due to the global error in the areoid.
    A topographic map created using Mars Orbiter Laser Altimeter (MOLA) data. This map show the relative elevation in 100 meter elevation contour lines (dashed) and 500 meter elevation contour lines (bold) with an average accuracy of each point is originally ~100 meters in horizontal position and ~1 meter in radius (Neumann and others, 2001). However, the total elevation uncertainty is at least ±3 m due to the global error in the areoid.

Gullies

Main article: Martian Gullies

Chincoteague Crater displays gullies on its wall. Many ideas have been put forth to explain them. For many years, many researchers thought they were made by recent liquid water.[2] However, with more observations, other mechanisms became possible. It was observed that new gullies were forming today during the Martian spring when dry ice was able to sublimate (turn from a solid to a gas). Chunks of dry ice could accumulate in the cold winter months and then slide down when warmed. In the thin atmosphere of the planet they would ride on a cushion of gas that was coming off the pieces of dry ice.[3][4][5]

See also

References

  1. ^ "Chincoteague (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. ^ Malin, M., Edgett, K. 2000. Evidence for recent groundwater seepage and surface runoff on Mars. Science 288, 2330–2335.
  3. ^ http://www.jpl.nasa.gov/news/news.php?release=2014-226
  4. ^ http://hirise.lpl.arizona.edu/ESP_032078_1420
  5. ^ http://www.space.com/26534-mars-gullies-dry-ice.html
Retrieved from "https://en.wikipedia.org/w/index.php?title=Chincoteague_(crater)&oldid=928576995"