Jump to content

Peary (crater): Difference between revisions

Coordinates: 88°38′N 24°24′E / 88.63°N 24.4°E / 88.63; 24.4
From Wikipedia, the free encyclopedia
Content deleted Content added
+image, minor edits
Inserted Si
Tags: nowiki added Visual edit
 
(35 intermediate revisions by 22 users not shown)
Line 1: Line 1:
{{Short description|Crater on the Moon}}
{{lunar crater data
{{Infobox Lunar crater
| image = <div style="position: relative">[[File:The Moon's North Pole.jpg|220px|alt=The lunar north pole]]
| image = Peary (LOLA).png
<div style="position: absolute; left: 45.5%; top: 46.4%;">[[File:Cercle jaune 100%.svg|24px]]</div>
| caption = Shaded relief map, based on the LRO laser altimetry data. Peary is the large crater at center; north pole is situated on its northern (upper) rim
</div>
| coordinates = {{coord|88.63|N|24.4|E|globe:moon_type:landmark|display=inline,title}}
| caption = Location of Peary crater (center) as seen from above the lunar north pole
| diameter = 79 km
| latitude=88.63
| depth = 1.5 km
| N_or_S=N
| colong = 25
| longitude=24.4
| eponym = [[Robert Peary]]
| E_or_W=E
}}
| diameter=79 km
[[File:Goldschmidt Si - Aldo Ferruggia.jpg|left|thumb|The crater area (at the top) in selenochromatic Image (Si). More infos here : <nowiki>https://www.gawh.it/main/selenocromatica</nowiki>]]
| depth=''Unknown''
| colong=25
| eponym=[[Robert Peary]] }}
[[File:Peary crater 4128 h3.jpg|thumb|right|240px|[[Lunar Orbiter 4]] image]]
[[File:Peary crater 4128 h3.jpg|thumb|right|240px|[[Lunar Orbiter 4]] image]]
[[Image:Peary (LOLA).png|thumb|right|240px|Map constructed from [[laser altimetry]] data. Peary is the large crater at center; north pole is situated on its northern (upper) rim]]
[[File:LOLA Peary Crater.jpg|thumb|right|240px|[[False color]] elevation map of Peary Crater, based on topographical data from the [[Lunar Reconnaissance Orbiter]] (LRO) [[Lidar|laser altimeter]].]]
'''Peary''' is the closest large [[Moon|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 remains permanently cloaked in shadow. From the [[Earth]] the crater appears on the northern lunar limb, and is seen from the side.
'''Peary''' is the closest large [[Lunar craters|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==
==Overview==
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.<ref>[https://nssdc.gsfc.nasa.gov/nmc/spacecraft/display.action?id=1967-041A Lunar Orbiter 4], NSSDCA/COSPAR ID: 1967-041A, NSSDC archive, NASA.</ref> Since it is located nearly at the lunar north pole, it was named after the polar explorer [[Robert Peary]].<ref>{{cite web| last = Blue| first = Jennifer| date = July 25, 2007| title = Peary| work = Gazetteer of Planetary Nomenclature |publisher=[[United States Geological Survey]]| url = http://planetarynames.wr.usgs.gov/Feature/4627|access-date = 2014-12-08}}</ref>
The crater is nearly circular, with an outward bulge along the northeast rim. There is a gap in the southwestern rim, where it joins a slightly smaller worn crater [[Florey (crater)|Florey]]. The outer rim of Peary is worn and eroded, creating a rugged mountainous ring that produces long shadows across the crater floor.


==Physical features==
The crater floor is relatively flat, but marked by several small craterlets, particularly in the southeastern half. The southern third of the interior remains cloaked in shadows, and so its features can be readily discerned only by means of ranging methods (for example, [[laser altimetry]]).


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 [[Florey (crater)|Florey]]. The outer rim of Peary is worn and eroded, creating a rugged mountainous ring that produces long shadows across the crater floor. The crater floor itself is relatively flat, but is marked by several small craterlets, particularly in the southeastern half. The southern third of the interior remains cloaked in shadows, and so its features can be readily discerned only by means of ranging methods (for example, [[laser altimetry]]).
The worn and [[lava]]-flooded crater [[Byrd (lunar crater)|Byrd]] lies close to the southern rim of Peary. To the northwest, about a quarter the way around the lunar pole, is the larger crater [[Hermite (crater)|Hermite]]. On the opposite side of the pole, on the [[Far side (Moon)|far side]] of the Moon, lies the still-larger [[Rozhdestvenskiy (crater)|Rozhdestvenskiy]].


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.<ref>"[https://svs.gsfc.nasa.gov/10595 Ten Cool Things Seen in the First Year of LRO"],
In 2004, a team led by Dr. [[Ben Bussey]] of [[Johns Hopkins University]] using images taken by the [[Clementine mission]] determined that four mountainous regions on the rim of Peary appeared to remain illuminated for the entire lunar day.<ref>{{cite news
NASA Goddard Space Center, June 23, 2010. Retrieved 22 May 2018.</ref>
| last=McKee | first=Maggie | date=April 13, 2005
| title=Sunny spot picked out for future lunar base
| publisher=New Scientist
| url=http://www.newscientist.com/article/dn7263-sunny-spot-picked-out-for-future-lunar-base.html
| accessdate=2007-09-11 }}</ref> These unnamed "[[Peak of Eternal Light|mountains of eternal light]]" are possible due to the Moon's extremely small axial tilt, which also gives rise to permanent shadow at the bottoms of many polar craters. No similar regions of eternal light exist at the less-mountainous [[lunar south pole|south pole]]. Clementine's images were taken during the northern lunar hemisphere's summer season, and it remains unknown whether these four mountains are shaded at any point during their local winter season.


===Illumination===
The northern rim of Peary is considered a likely site for a future [[Moon base]] due to this steady illumination, which would provide both a relatively stable temperature and an uninterrupted solar power supply. It is also near permanently shadowed areas that may contain some quantity of frozen [[water]].
In 2004, a team led by Dr [[Ben Bussey]] of [[Johns Hopkins University]], using images taken by the [[Clementine mission]], determined that four mountainous regions on the rim of Peary appeared to remain illuminated for the entire lunar day.<ref>{{cite magazine| last=McKee | first=Maggie | date=April 13, 2005| title=Sunny spot picked out for future lunar base| magazine=[[New Scientist]]| url=https://www.newscientist.com/article/dn7263-sunny-spot-picked-out-for-future-lunar-base.html| access-date=2007-09-11 }}</ref> These unnamed "[[Peak of Eternal Light|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.<ref name="Speyerer2013">Emerson J. Speyerer and Mark S. Robinson, "[https://www.sciencedirect.com/science/article/pii/S0019103512004174 Persistently illuminated regions at the lunar poles: Ideal sites for future exploration"], ''[[Icarus (journal)|Icarus]]''
Vol. 222, No. 1, January 2013, pp. 122-136 https://doi.org/10.1016/j.icarus.2012.10.010 . Retrieved 21 May 2018.</ref>

The northern rim of Peary is considered a likely site for a future [[Moon base]],<ref>[http://www.cnn.com/2005/TECH/space/04/13/nasa.moon.base/ Researchers find ideal spot for moon base], CNN, April 18, 2005 (accessed 2010 August 22)</ref> 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.<ref name="Gläser2017">P. Gläser, J. Oberst, G.A. Neumann, E. Mazarico, E.J. Speyerer, and M.S. Robinson, "[https://www.sciencedirect.com/science/article/pii/S0032063317300478?via%3Dihub 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</ref>


==References==
==References==
Line 40: Line 38:
| last2 = Whitaker
| last2 = Whitaker
| first2 = E. A.
| first2 = E. A.
| authorlink2 = Ewen Whitaker
| author-link2 = Ewen Whitaker
| date = 1982
| date = 1982
| title = [[NASA]] Catalogue of Lunar Nomenclature
| title = NASA Catalogue of Lunar Nomenclature
| publisher = NASA RP-1097
| publisher = NASA RP-1097
| ref = harv
| title-link = NASA
}}
}}
* {{cite web
| last = Blue
| first = Jennifer
| date = July 25, 2007
| title = Gazetteer of Planetary Nomenclature
| publisher = [[United States Geological Survey|USGS]]
| url = http://planetarynames.wr.usgs.gov/Feature/4627
| accessdate = 2014-12-08
| ref = harv
}}
* {{cite book
* {{cite book
| last1 = Bussey
| last1 = Bussey
| first1 = B.
| first1 = B.
| authorlink1 = Ben Bussey
| author-link1 = Ben Bussey
| last2 = Spudis
| last2 = Spudis
| first2 = P.
| first2 = P.
| authorlink2 = Paul Spudis
| author-link2 = Paul Spudis
| date = 2004
| date = 2004
| title = The Clementine Atlas of the Moon
| title = The Clementine Atlas of the Moon
| publisher = Cambridge University Press
| publisher = [[Cambridge University Press]]
| location = New York
| location = New York
| isbn = 978-0-521-81528-4
| isbn = 978-0-521-81528-4
| ref = harv
}}
}}
* {{cite book
* {{cite book
Line 79: Line 66:
| publisher = Tudor Publishers
| publisher = Tudor Publishers
| isbn = 978-0-936389-27-1
| isbn = 978-0-936389-27-1
| url = https://archive.org/details/isbn_9780936389271
| ref = harv
}}
}}
* {{cite web
* {{cite web
Line 87: Line 74:
| url = http://host.planet4589.org/astro/lunar/
| url = http://host.planet4589.org/astro/lunar/
| title = Lunar Nomenclature
| title = Lunar Nomenclature
| publisher = Jonathan's Space Report
| publisher = [[Jonathan's Space Report]]
| accessdate = 2007-10-24
| access-date = 2007-10-24
| ref = harv
}}
}}
* {{cite journal| last1 = Menzel| first1 = D. H.| last2 = Minnaert| first2 = M.| last3 = Levin| first3 = B.| last4 = Dollfus| first4 = A.| last5 = Bell| first5 = B.| title = Report on Lunar Nomenclature by the Working Group of Commission 17 of the IAU| doi = 10.1007/BF00171763| journal = Space Science Reviews| volume = 12| issue = 2| pages = 136–186| year = 1971| pmid = | pmc =| bibcode = 1971SSRv...12..136M| ref = harv}}
* {{cite journal| last1 = Menzel| first1 = D. H.| last2 = Minnaert| first2 = M.| last3 = Levin| first3 = B.| last4 = Dollfus| first4 = A.| last5 = Bell| first5 = B.| title = Report on Lunar Nomenclature by the Working Group of Commission 17 of the IAU| doi = 10.1007/BF00171763| journal = Space Science Reviews| volume = 12| issue = 2| pages = 136–186| year = 1971| bibcode = 1971SSRv...12..136M| s2cid = 122125855}}
* {{cite book
* {{cite book
| first = Patrick
| first = Patrick
| last = Moore
| last = Moore
| authorlink = Patrick Moore
| author-link = Patrick Moore
| date = 2001
| date = 2001
| title = On the Moon
| title = On the Moon
| publisher = Sterling Publishing Co
| publisher = [[Sterling Publishing Co]]
| isbn = 978-0-304-35469-6
| isbn = 978-0-304-35469-6
| url = https://archive.org/details/patrickmooreonmo00patr
| ref = harv
}}
}}
* {{cite book
* {{cite book
Line 109: Line 95:
| publisher = Cambridge University Press
| publisher = Cambridge University Press
| isbn = 978-0-521-33500-3
| isbn = 978-0-521-33500-3
| ref = harv
}}
}}
* {{cite book
* {{cite book
| last = Rükl
| last = Rükl
| first = Antonín
| first = Antonín
| authorlink = Antonín Rükl
| author-link = Antonín Rükl
| date = 1990
| date = 1990
| title = Atlas of the Moon
| title = Atlas of the Moon
| publisher = Kalmbach Books
| publisher = [[Kalmbach Books]]
| isbn = 978-0-913135-17-4
| isbn = 978-0-913135-17-4
| ref = harv
}}
}}
* {{cite book
* {{cite book
| last = Webb
| last = Webb
| first = Rev. T. W.
| first = Rev. T. W.
| authorlink = Thomas William Webb
| author-link = Thomas William Webb
| date = 1962
| date = 1962
| title = Celestial Objects for Common Telescopes
| title = Celestial Objects for Common Telescopes
Line 130: Line 114:
| publisher = Dover
| publisher = Dover
| isbn = 978-0-486-20917-3
| isbn = 978-0-486-20917-3
| url = https://archive.org/details/celestialobjects00webb
| ref = harv
}}
}}
* {{cite book
* {{cite book
| first = Ewen A.
| first = Ewen A.
| last = Whitaker
| last = Whitaker
| authorlink = Ewen Whitaker
| author-link = Ewen Whitaker
| date = 2003
| date = 2003
| title = Mapping and Naming the Moon
| title = Mapping and Naming the Moon
| publisher = Cambridge University Press
| publisher = Cambridge University Press
| isbn = 978-0-521-54414-6
| isbn = 978-0-521-54414-6
| url = https://books.google.com/books?id=aV1i27jDYL8C
| ref = harv
| url = http://books.google.com/books?id=aV1i27jDYL8C
}}
}}
* {{cite book
* {{cite book
Line 150: Line 133:
| publisher = Springer
| publisher = Springer
| isbn = 978-1-85233-193-1
| isbn = 978-1-85233-193-1
| ref = harv
}}
}}
{{refend}}
{{refend}}


==External links==
==External links==
* [http://planetarynames.wr.usgs.gov/images/Lunar/lac_1_lo.pdf LAC-1 area] - Map of northern lunar pole
* [http://www.cnn.com/2005/TECH/space/04/13/nasa.moon.base/ Researchers find ideal spot for moon base], CNN, April 18, 2005 (accessed 2010 August 22)


{{Moon colonization}}
{{Moon colonization}}

Latest revision as of 19:27, 18 August 2024

Peary
Shaded relief map, based on the LRO laser altimetry data. Peary is the large crater at center; north pole is situated on its northern (upper) rim
Coordinates88°38′N 24°24′E / 88.63°N 24.4°E / 88.63; 24.4
Diameter79 km
Depth1.5 km
Colongitude25° at sunrise
EponymRobert Peary
The crater area (at the top) in selenochromatic Image (Si). More infos here : https://www.gawh.it/main/selenocromatica
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

[edit]

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

[edit]

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 Florey. The outer rim of Peary is worn and eroded, creating a rugged mountainous ring that produces long shadows across the crater floor. The crater floor itself is relatively flat, but is marked by several small craterlets, particularly in the southeastern half. The southern third of the interior remains cloaked in shadows, and so its features can be readily discerned only by means of ranging methods (for example, 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

[edit]

In 2004, a team led by Dr Ben Bussey of Johns Hopkins University, using images taken by the Clementine mission, determined that four mountainous regions on the rim of Peary appeared to remain illuminated for the entire lunar day.[4] These unnamed "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

[edit]
  1. ^ Lunar Orbiter 4, NSSDCA/COSPAR ID: 1967-041A, NSSDC archive, NASA.
  2. ^ Blue, Jennifer (July 25, 2007). "Peary". Gazetteer of Planetary Nomenclature. United States Geological Survey. 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
[edit]