Peary (crater)

Coordinates: 88°38′N 24°24′E / 88.63°N 24.4°E / 88.63; 24.4
Source: Wikipedia, the free encyclopedia.
Peary
Colongitude
25° at sunrise
EponymRobert Peary
Lunar Orbiter 4 image
False color elevation map of Peary Crater, based on topographical data from the Lunar Reconnaissance Orbiter (LRO) laser altimeter.

Peary is the closest large lunar impact crater to the lunar north pole. At this latitude the crater interior receives little sunlight, and portions of the southernmost region of the crater floor remain permanently cloaked in shadow. From the Earth the crater appears on the northern lunar limb, and is seen from the side.

Observation and Etymology

Since Peary is located nearly on the limb of the Moon as viewed from Earth, high-quality images of the crater were not available until space probes started photographing the Moon; the first high-quality images came from the US

Lunar Orbiter 4 spacecraft.[1] Since it is located nearly at the lunar north pole, it was named after the polar explorer Robert Peary.[2]

Physical features

Peary is nearly circular, with an outward bulge along the northeast rim. There is a gap in the southwestern rim, where it joins the slightly smaller crater

laser altimetry
).

Because of the low sun angle, the average temperature on the crater floor or Peary is between 30 and 40 K, one of the coldest locations in the Solar System.[3]

Illumination

In 2004, a team led by Dr

peaks of eternal light" are due to the Moon's extremely small axial tilt, which also gives rise to permanent shadow at the bottoms of many polar craters. Clementine's images were taken during the northern lunar hemisphere's summer season, and more detailed lunar topography collected by the Lunar Reconnaissance Orbiter (LRO) showed that no points on the Moon receive perpetual light during both winter and summer.[5]

The northern rim of Peary is considered a likely site for a future

Moon base,[6] due to this near-constant illumination, which would provide both a relatively stable temperature and a nearly uninterrupted solar power supply. It is also near permanently shadowed areas that may contain some quantity of frozen water.[7]

References

  1. ^ Lunar Orbiter 4, NSSDCA/COSPAR ID: 1967-041A, NSSDC archive, NASA.
  2. ^ Blue, Jennifer (July 25, 2007). "Peary". Gazetteer of Planetary Nomenclature, USGS. Retrieved 2014-12-08.
  3. ^ "Ten Cool Things Seen in the First Year of LRO", NASA Goddard Space Center, June 23, 2010. Retrieved 22 May 2018.
  4. ^ McKee, Maggie (April 13, 2005). "Sunny spot picked out for future lunar base". New Scientist. Retrieved 2007-09-11.
  5. ^ Emerson J. Speyerer and Mark S. Robinson, "Persistently illuminated regions at the lunar poles: Ideal sites for future exploration", Icarus Vol. 222, No. 1, January 2013, pp. 122-136 https://doi.org/10.1016/j.icarus.2012.10.010 . Retrieved 21 May 2018.
  6. ^ Researchers find ideal spot for moon base, CNN, April 18, 2005 (accessed 2010 August 22)
  7. ^ P. Gläser, J. Oberst, G.A. Neumann, E. Mazarico, E.J. Speyerer, and M.S. Robinson, "Illumination conditions at the lunar poles: Implications for future exploration", Planetary and Space Science, 2017. https://doi.org/10.1016/j.pss.2017.07.006

External links