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Bohr (crater)

Lunar surface depression

Bohr (crater)
Summary

Lunar surface depression

FieldValue
imageBohr crater Vallis Bohr 4188_h2.jpg
captionLunar Orbiter 4 image, with Bohr crater in upper right and Vallis Bohr in lower left
coordinates
diameter71 km
depthUnknown
colong87
eponymNiels Bohr
LRO]] mosaic

Bohr is a lunar impact crater that is located near the western lunar limb, in the area that is affected by librations. It is attached to the southwestern rim of the larger, eroded Vasco da Gama formation, and to the southeast of the crater Einstein. The crater was observed for the first time in 1963, by Arthus and Ewen Whitaker in the book Rectified Lunar Atlas.http://host.planet4589.org/astro/lunar/ https://planetarynames.wr.usgs.gov/

The rim of Bohr is worn and eroded, and a pair of small, bowl-shaped craters lies across the western rim. The rim to the northeast has been shored up by the adjacent Vasco da Gama, but the remainder forms an irregular ring of rugged ground. To the southwest of Bohr is Vallis Bohr, a valley trending in a north–south direction. This long cleft is most likely associated with the formation of the Mare Orientale farther to the south.

References

  • {{cite book | author-link2 = Ewen Whitaker
  • {{cite web | access-date = 2007-08-05
  • {{cite book | author-link1 = Ben Bussey | author-link2 = Paul Spudis
  • {{cite book
  • {{cite web | access-date = 2007-10-24 | archive-date = 2012-02-08 | archive-url = https://web.archive.org/web/20120208141804/http://host.planet4589.org/astro/lunar/ | url-status = dead
  • {{cite book | author-link = Patrick Moore
  • {{cite book
  • {{cite book | author-link = Antonín Rükl
  • {{cite book | author-link = Thomas William Webb
  • {{cite book | author-link = Ewen Whitaker
  • {{cite book
Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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