Astronomy:Peak ring

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Short description: Roughly circular ring within an impact crater
The Apollo basin is a peak ring crater

A peak ring crater is a type of complex crater, which is different from a multi-ringed basin or central-peak crater. A central peak is not seen; instead, a roughly circular ring or plateau, possibly discontinuous, surrounds the crater's center, with the crater rim still farther out from the center.[1]

Formation

The rings form by different processes, and inner rings may not be formed by the same processes as outer rings.[2]

It has long been the view that peak rings are formed in the stage subsequent to central peak formation in craters, with the stage being dependent on the crater diameter and planetary gravity. The central peaks of craters are believed to originate from hydrodynamic flow of material lifted by inward-collapsing crater walls, while impact-shattered rock debris is briefly turned to fluid by strong vibrations that develop during crater formation. The peak-ring structure of Chicxulub crater was probably formed as inward-collapsing material struck the over-steepened central peak, to form a hydraulic jump at the location where the peak ring was located.[3]

Other hypotheses have been formulated. Perhaps, in the case of Chicxulub crater, an over-high central peak collapsed into the peak ring.[4][5]

Chicxulub is Earth's only crater to have an intact peak ring structure.[6] The Carswell crater in Saskatchewan, Canada, may also be an eroded peak ring crater.[7]

Examples

See also

On Mercury:

  • Ahmad Baba
  • Caravaggio
  • Chekhov
  • Eminescu
  • Holst
  • Homer
  • Michelangelo
  • Mozart
  • Nabokov
  • Polygnotus
  • Rachmaninoff
  • Raditladi
  • Renoir
  • Vivaldi

On Venus:

  • Barton
  • Isabella
  • Meitner
  • Mona Lisa
  • Wheatley
  • Yablochkina

On Earth:

References

  1. Baker, David M. H. (August 2011). "The transition from complex crater to peak-ring basin on the Moon: New observations from the Lunar Orbiter Laser Altimeter (LOLA) instrument". Icarus 214 (2): 377–393. doi:10.1016/j.icarus.2011.05.030. Bibcode2011Icar..214..377B. 
  2. Geology Page: www.geologypage.com/2016/10/research-helps-explain-formation-ringed-crater-moon.html, accessdate: February 5, 2017
  3. H. J. Melosh (2015). "Peak-ring Craters and Multiring Basins". http://www.hou.usra.edu/meetings/gap2015/pdf/1003.pdf. 
  4. H. J. Melosh (2016). "Drilling into Chicxulub's formation". Science 354 (6314): 878–882. doi:10.1126/science.aah6561. PMID 27856906. http://eprints.gla.ac.uk/131793/1/131793.pdf. 
  5. "The formation of large meteorite craters is unraveled". Geology Page. October 29, 2018. http://www.geologypage.com/2018/10/the-formation-of-large-meteorite-craters-is-unraveled.html#ixzz5VVkNl3Vz. 
  6. Thomas Sumner (Nov 17, 2016). "How a ring of mountains forms inside a crater". https://www.sciencenews.org/article/how-ring-mountains-forms-inside-crater. 
  7. Genest, Serge; Robert, Francine; Duhamel, Isabelle (2010). "The Carswell impact event, Saskatchewan, Canada: Evidence for a pre-Athabasca multiring basin?". Large Meteorite Impacts and Planetary Evolution IV. doi:10.1130/2010.2465(26). ISBN 978-0-8137-2465-2.