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Alphonsus (crater): Difference between revisions

Coordinates: 13°23′S 2°51′W / 13.39°S 2.85°W / -13.39; -2.85
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{{Short description|Crater on the Moon}}
{{more footnotes|date=October 2012}}
{{Infobox Lunar crater
{{Infobox Lunar crater
| image = [[File:Alphonsus (LRO) 1.png|350px]]
| image = Alphonsus (LRO) 1.png
| image_size =
| caption = [[Lunar Reconnaissance Orbiter|LRO]] image
| caption = [[Lunar Reconnaissance Orbiter|LRO]] image
| coordinates = {{coord|13.4|S|2.8|W|globe:moon_type:landmark|display=inline,title}}
| coordinates = {{coord|13.39|S|2.85|W|globe:moon_type:landmark|display=inline,title}}
| diameter = 119 km
| diameter = 110.54 km
| depth = 2.7 km
| depth = 2.7 km
| colong = 4
| colong = 4
| eponym = [[Alfonso X of Castile|Alfonso X]]
| eponym = [[Alfonso X of Castile|Alfonso X]]
}}
}}
[[File:Ptolemaeus trium area Si.jpg|thumb|The crater area in a Selenochromatic format Image (Si)|381x381px]]
[[Image:Ranger7 PIA02975.jpg|thumb|300px|right|Alphonsus crater appears in the right half of this image taken by [[Ranger 7]]. ''[[NASA]] photo.'']]
[[File:Ranger7 PIA02975.jpg|thumb|right|Alphonsus crater appears in the right half of this image taken by [[Ranger 7]]. ''[[NASA]] photo.'']]
'''Alphonsus''' is an ancient [[impact crater]] on the [[Moon]] that dates from the pre-Nectarian era.<ref>{{cite web|last=Ambrose
'''Alphonsus''' is an ancient [[impact crater]] on the [[Moon]] that dates from the pre-Nectarian era.<ref>{{cite web|last=Ambrose
|first= W.A.|title=ORIGIN, DISTRIBUTION, AND CHRONOSTRATIGRAPHY OF ASYMMETRIC SECONDARY CRATERS ASSOCIATED WITH NEARSIDE LUNAR BASINS|url=http://www.lpi.usra.edu/meetings/lpsc2008/pdf/1019.pdf|work=Bureau of Economic Geology|publisher=University of Texas at Austin, TX|accessdate=25 September 2013}}</ref> It is located on the lunar highlands on the eastern end of [[Mare Nubium]], west of the [[Imbrian Highlands]], and slightly overlaps the crater [[Ptolemaeus (lunar crater)|Ptolemaeus]] to the north. To the southwest is the smaller [[Alpetragius (crater)|Alpetragius]].
|first= W.A.|title=ORIGIN, DISTRIBUTION, AND CHRONOSTRATIGRAPHY OF ASYMMETRIC SECONDARY CRATERS ASSOCIATED WITH NEARSIDE LUNAR BASINS|url=http://www.lpi.usra.edu/meetings/lpsc2008/pdf/1019.pdf|work=Bureau of Economic Geology|publisher=University of Texas at Austin, TX|access-date=25 September 2013}}</ref> (Older sources state that it is [[Nectarian]] in age.<ref>[https://pubs.er.usgs.gov/publication/pp1348 The geologic history of the Moon]. [[USGS]] Professional Paper 1348. By [[Don Wilhelms|Don E. Wilhelms]], John F. McCauley, and Newell J. Trask. U.S. Government Printing Office, Washington: 1987. Table 9-4.</ref>) It is located on the lunar highlands on the eastern end of [[Mare Nubium]], west of the [[Imbrian Highlands]], and slightly overlaps the crater [[Ptolemaeus (lunar crater)|Ptolemaeus]] to the north. To the southwest is the smaller [[Alpetragius (crater)|Alpetragius]]. The crater name was approved by the [[International Astronomical Union|IAU]] in 1935.<ref>[http://planetarynames.wr.usgs.gov/Feature/206 Alphonsus], Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)</ref>


==Description==
== Description ==
The surface of Alphonsus is broken and irregular along its boundary with Ptolemaeus. The outer walls are slightly distorted and possess a somewhat hexagonal form.
The surface of Alphonsus is broken and irregular along its boundary with Ptolemaeus. The outer walls are slightly distorted and possess a somewhat hexagonal form.


A low ridge system of deposited ejecta bisects the crater floor, and includes the steep central peak designated Alphonsus Alpha (α). This [[pyramid]]-shaped formation rises to a height of 1.5&nbsp;km above the interior surface. It is not volcanic in origin, but rather is made of [[anorthosite]] like the lunar highlands.
A low ridge system of deposited ejecta bisects the crater floor, and includes the steep central peak designated Alphonsus Alpha (α). This [[pyramid]]-shaped formation rises to a height of 1.5&nbsp;km above the interior surface. It is not volcanic in origin, but rather is made of [[anorthosite]] like the lunar highlands.


The floor is fractured by an elaborate system of [[rille]]s and contains three smaller craters surrounded by a symmetric darker halo. These dark-halo craters are [[Volcanic cone|cinder cone]]-shaped and are believed by some to be [[volcanic]] in origin, although others think they were caused by impacts that excavated darker mare material from underneath the lighter lunar [[regolith]].
The floor is fractured by an elaborate system of [[rille]]s and contains four or five smaller craters surrounded by a symmetric darker halo. These dark-halo craters are [[Volcanic cone|cinder cone]]-shaped and are believed by some to be [[volcanic]] in origin, although others think they were caused by impacts that excavated darker mare material from underneath the lighter lunar [[regolith]].


==Exploration==
==Exploration==
The [[Ranger 9]] probe impacted in Alphonsus, a short distance to the northeast of the central peak. [[Harold Urey]] said of a close-up photograph of Alphonsus:
The [[Ranger 9]] probe impacted in Alphonsus, a short distance to the northeast of the central peak. [[Harold Urey]] said of a close-up photograph of Alphonsus:


{{cquote|The floor is covered with many craters of various sizes, some sharp and hence new, others less distinct and partly filled with fragmented material. The walls have fewer craters, and this probably means that slumping of the wall has filled them. Crevasses are evident, and evidence for slumping exists. The larger crater near the top is undoubtedly collisional in origin. Three craters are surrounded by dark halos and were produced by eruptions from the lunar interior. Exceptionally bright, sharp peaks can be seen on certain mountain tops.<ref>EXPLORING SPACE WITH A CAMERA, [https://history.nasa.gov/SP-168/section2a.htm Section 2, To The Moon and Beyond], NASA Special Pulication 168 (SP-168)</ref>}}
{{cquote|The floor is covered with many craters of various sizes, some sharp and hence new, others less distinct and partly filled with fragmented material. The walls have fewer craters, and this probably means that slumping of the wall has filled them. Crevasses are evident, and evidence for slumping exists. The larger crater near the top is undoubtedly collisional in origin. Three craters are surrounded by dark halos and were produced by eruptions from the lunar interior. Exceptionally bright, sharp peaks can be seen on certain mountain tops.<ref>EXPLORING SPACE WITH A CAMERA, [https://history.nasa.gov/SP-168/section2a.htm Section 2, To The Moon and Beyond], NASA Special Publication 168 (SP-168)</ref>}}


==Apollo Landing Site==
Alphonsus was one of the primary alternative landing sites considered for both the [[Apollo 16]] and the [[Apollo 17]] missions.{{citation needed|date=October 2012}}
The dark-haloed craters along some of the rilles in the crater are thought to be volcanic vents, and during the [[Apollo program]] Alphonsus was considered as a possible landing site in order to possibly sample [[xenoliths]] of the lunar mantle from the vents.<ref>To a Rocky Moon: A Geologist's History of Lunar Exploration. Don E. Wilhelms, University of Arizona Press (1993). {{ISBN|978-0816510658}} Chapter 16.</ref> It was considered for [[Apollo 16]] but the Descartes area was selected. It was one of the three final possible sites for [[Apollo 17]], together with [[Gassendi (crater)|Gassendi]] crater and the [[Taurus-Littrow]] valley, but it was considered possibly "contaminated" with younger material from the nearby [[Mare Imbrium|Imbrium basin]].<ref>To a Rocky Moon: A Geologist's History of Lunar Exploration. Don E. Wilhelms, University of Arizona Press (1993). {{ISBN|978-0816510658}} Chapter 17.</ref>


==Transient lunar phenomena==
==Transient lunar phenomena==
Alphonsus is one of the sites noted for [[transient lunar phenomenon|transient lunar phenomena]], as glowing red-hued clouds have been reported emanating from the crater. On October 26, 1956, the lunar [[astronomer]] [[Dinsmore Alter]] noted some blurring of the rilles on the floor of Alphonsus in the [[photographs]] he took in [[violet (color)|violet]] light. The same blurring did not occur in the [[infrared]] photographs he took at the same time. However, few professional astronomers found this evidence of [[volcanic]] activity on the Moon very convincing.<ref>Dinsmore (1957), '''69''': 158</ref>
Alphonsus is one of the sites noted for [[transient lunar phenomenon|transient lunar phenomena]], as glowing red-hued clouds have been reported emanating from the crater. On October 26, 1956, the lunar [[astronomer]] [[Dinsmore Alter]] noted some blurring of the rilles on the floor of Alphonsus in the [[photographs]] he took in [[violet (color)|violet]] light. The same blurring did not occur in the [[infrared]] photographs he took at the same time. However, few professional astronomers found this evidence of [[volcanic]] activity on the Moon very convincing.<ref>Dinsmore (1957), '''69''': 158</ref>


One astronomer who was intrigued by Alter's observations was [[Nikolai Alexandrovich Kozyrev|Nikolai A. Kozyrev]], from the [[Soviet Union]]. In 1958 while Kozyrev was looking for volcanic phenomenon on the moon, he observed the formation of a mist-like cloud within Alphonsus.<ref>{{cite web|last=Oepik|first=E.J.|title=Cratering and the moon's surface|url=http://hdl.handle.net/2060/19690007782|work=Armagh Observatory|publisher=Department of Physics and Astronomy, University of Maryland|accessdate=20 September 2011}}</ref> The spectrum of the area had been measured at this time, and displayed indications of [[carbon]] matter, possibly C<sub>2</sub> gas. He believed this to be the result of volcanic or related activity. However no evidence for this phenomenon has been found from lunar missions, and the emission results have never been confirmed.<ref>Dinsmore (1957), '''71''': 46</ref>
One astronomer who was intrigued by Alter's observations was [[Nikolai Alexandrovich Kozyrev|Nikolai A. Kozyrev]], from the [[Soviet Union]]. In 1958 while Kozyrev was looking for volcanic phenomenon on the moon, he observed the formation of a mist-like cloud within Alphonsus.<ref>{{cite journal|last=Oepik|first=E.J.|title=Cratering and the moon's surface|work=Armagh Observatory|date=January 1968 |publisher=Department of Physics and Astronomy, University of Maryland|hdl=2060/19690007782}}</ref> The spectrum of the area had been measured at this time, and displayed indications of [[carbon]] matter, possibly C<sub>2</sub> gas. He believed this to be the result of volcanic or related activity. However no evidence for this phenomenon has been found from lunar missions, and the emission results have never been confirmed.<ref>Dinsmore (1957), '''71''': 46</ref>


==Names==
==Names==
Alphonsus is named after King [[Alfonso X of Castile]] (known as "Alfonso the Wise"), who had an interest in astronomy. Like many of the craters on the Moon's near side, it was given its name by [[Giovanni Battista Riccioli|Giovanni Riccioli]], whose 1651 nomenclature system has become standardized; Riccioli originally named it "Alphonsus Rex" ('King Alfonso'), but the 'Rex' was later dropped.<ref>Ewen A. Whitaker, ''Mapping and Naming the Moon'' (Cambridge University Press, 1999), p.210.</ref> Earlier lunar cartographers had given the feature different names. [[Michael van Langren]]'s 1645 map calls it "Ludovici XIV, Reg. Fran.", after [[Louis XIV of France]],<ref>Ewen A. Whitaker, ''Mapping and Naming the Moon'' (Cambridge University Press, 1999), p. 198.</ref> and [[Johannes Hevelius]] called it "Mons Masicytus" after [[List of Lycian place names#M|a range of mountains in Lycia]].<ref>Ewen A. Whitaker, ''Mapping and Naming the Moon'' (Cambridge University Press, 1999), p. 205.</ref>
Alphonsus is named after King [[Alfonso X of Castile]] (known as "Alfonso the Wise"), who had an interest in astronomy.<ref>{{gpn|206}}</ref> Like many of the craters on the Moon's near side, it was given its name by [[Giovanni Battista Riccioli|Giovanni Riccioli]], whose 1651 nomenclature system has become standardized; Riccioli originally named it "Alphonsus Rex" ('King Alfonso'), but the 'Rex' was later dropped.<ref>Ewen A. Whitaker, ''Mapping and Naming the Moon'' (Cambridge University Press, 1999), p.210.</ref> Earlier lunar cartographers had given the feature different names. [[Michael van Langren]]'s 1645 map calls it "Ludovici XIV, Reg. Fran.", after [[Louis XIV of France]],<ref>Ewen A. Whitaker, ''Mapping and Naming the Moon'' (Cambridge University Press, 1999), p. 198.</ref> and [[Johannes Hevelius]] called it "Mons Masicytus" after [[List of Lycian place names#M|a range of mountains in Lycia]].<ref>Ewen A. Whitaker, ''Mapping and Naming the Moon'' (Cambridge University Press, 1999), p. 205.</ref>


==Interior craters==
==Interior craters==
[[File:Alphonsus small craters AS16-P-4661 ASU.jpg|thumb|right|240px|Oblique view of the five small named craters: C = Chang-Ngo, R = Ravi, M = Monira, J = Jose, S = Soraya. Facing south with sun illuminating from left.]][[File:1965 74994L.jpg|thumb|243px|right|Ranger 9 image showing [[rille]]s on the floor of the crater]]
[[File:Alphonsus small craters AS16-P-4661 ASU.jpg|thumb|right|300px|Oblique view of the five small named craters: C = Chang-Ngo, R = Ravi, M = Monira, J = Jose, S = Soraya. Facing south with sun illuminating from left. North on the photo is on the bottom]][[File:1965 74994L.jpg|thumb|300px|right|Ranger 9 image showing [[rille]]s on the floor of the crater]]
Five tiny craters in the northeastern part of Alphonsus' interior floor have been assigned names by the [[International Astronomical Union|IAU]]. These are listed in the table below.
Five tiny craters in the northeastern part of Alphonsus' interior floor have been assigned names by the [[International Astronomical Union|IAU]]. These are listed in the table below.


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==Notes==
==References==
{{Reflist}}
{{Reflist}}

==References==
{{refbegin}}
{{refbegin}}
* {{cite book
* {{cite book
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| 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
}}
* {{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/
| accessdate = 2007-08-05
| ref = harv
}}
}}
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| authorlink2 = Paul Spudis
| author-link2 = Paul Spudis
| date = 2004
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| title = The Clementine Atlas of the Moon
| title = The Clementine Atlas of the Moon
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| location = New York
| location = New York
| isbn = 978-0-521-81528-4
| isbn = 978-0-521-81528-4
| ref = harv
}}
}}
* {{cite book
* {{cite book
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| 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
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| 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}}
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| author-link = Patrick Moore
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| publisher = Sterling Publishing Co
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| url = https://archive.org/details/patrickmooreonmo00patr
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}}
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| publisher = Cambridge University Press
| publisher = Cambridge University Press
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}}
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| author-link = Antonín Rükl
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| title = Atlas of the Moon
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| publisher = Dover
| publisher = Dover
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* {{cite book
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| first = Ewen A.
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| last = Whitaker
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| author-link = Ewen Whitaker
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| date = 1999
| title = Mapping and Naming the Moon
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{{refend}}
{{refend}}
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|title=Micro-Topo
|title=Micro-Topo
|publisher=Lunar Photo of the Day
|publisher=Lunar Photo of the Day
|accessdate=2006-07-21
|access-date=2006-07-21
|deadurl=yes
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|archiveurl=https://web.archive.org/web/20060514140245/http://www.lpod.org/?m=20060406
|archive-url=https://web.archive.org/web/20060514140245/http://www.lpod.org/?m=20060406
|archivedate=2006-05-14
|archive-date=2006-05-14
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}}
* {{cite book
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| chapter = Rangers Bring the Moon Up Close | pages= 48
| chapter = Rangers Bring the Moon Up Close | pages= 48
| url = https://history.nasa.gov/SP-168/sp168.htm
| url = https://history.nasa.gov/SP-168/sp168.htm
| chapterurl = https://history.nasa.gov/SP-168/section2a.htm#46 }}
| chapter-url = https://history.nasa.gov/SP-168/section2a.htm#46 }}
* {{cite journal
* {{cite journal
| last = Alter | first = Dinsmore
| last = Alter | first = Dinsmore
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| journal=Publications of the Astronomical Society of the Pacific
| journal=Publications of the Astronomical Society of the Pacific
| date=1957 | volume=69
| date=1957 | volume=69
| issue = 407
| bibcode=1957PASP...69..158A
| bibcode=1957PASP...69..158A
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| doi=10.1086/127036
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* {{cite journal
* {{cite journal
| last = Alter | first = Dinsmore
| last = Alter | first = Dinsmore
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| journal=Publications of the Astronomical Society of the Pacific
| journal=Publications of the Astronomical Society of the Pacific
| date=1959 | volume=71
| date=1959 | volume=71
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| bibcode=1959PASP...71...46A
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* {{cite web
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| publisher = NASA | accessdate = 2007-02-09 }}
| publisher = NASA | access-date = 2007-02-09 }}


==External links==
==External links==
{{Commons category}}
{{Commonscat}}
*[https://the-moon.us/wiki/Alphonsus Alphonsus at The Moon Wiki] {{Webarchive|url=https://web.archive.org/web/20151109125101/http://the-moon.wikispaces.com/Alphonsus |date=2015-11-09 }}
* {{cite web | last = Wood | first = Chuck | date = 2006-04-06 | url = http://www2.lpod.org/wiki/April_6,_2006 | title = Micro-Topo | publisher = Lunar Photo of the Day | accessdate = 2006-07-21 }}
*[https://the-moon.us/wiki/Rimae_Alphonsus Rimae Alphonsus at The Moon Wiki]
*[http://lroc.sese.asu.edu/posts/1 Alphonsus crater mantled floor fracture], from [[Lunar Reconnaissance Orbiter|LROC]]
*[http://lroc.sese.asu.edu/posts/1 Alphonsus crater mantled floor fracture], from [[Lunar Reconnaissance Orbiter|LROC]]
*[http://www.lpi.usra.edu/resources/lunar_orbiter/bin/info.shtml?285 Lunar Orbiter map and photo of Alphonsus]
*[http://www.lpi.usra.edu/resources/lunar_orbiter/bin/info.shtml?285 Lunar Orbiter map and photo of Alphonsus]

===Other related articles===
* {{cite web | last = Wood | first = Chuck | date = May 15, 2004 | url = http://www.lpod.org/archive/archive/2004/05/LPOD-2004-05-15.htm | title = The Golden Triad | publisher = Lunar Photo of the Day | access-date = September 16, 2017 | archive-url = https://web.archive.org/web/20180530165228/http://www.lpod.org/archive/archive/2004/05/LPOD-2004-05-15.htm | archive-date = May 30, 2018 | url-status = dead }}
* {{cite web | last = Wood | first = Chuck | date = May 21, 2004 | url = http://www.lpod.org/archive/archive/2004/05/LPOD-2004-05-21.htm | title = Volcanic Craters on the Moon | publisher = Lunar Photo of the Day | access-date = September 16, 2017 | archive-url = https://web.archive.org/web/20180530202019/http://www.lpod.org/archive/archive/2004/05/LPOD-2004-05-21.htm | archive-date = May 30, 2018 | url-status = dead }}
* {{cite web | last = Wood | first = Chuck | date = October 31, 2004 | url = http://www.lpod.org/archive/LPOD-2004-10-31.htm | title = Sunrise and Sunset on the Triade | publisher = Lunar Photo of the Day | access-date = October 14, 2017 | archive-url = https://web.archive.org/web/20171014150747/http://www.lpod.org/archive/LPOD-2004-10-31.htm | archive-date = October 14, 2017 | url-status = dead }} - one of three craters making up a ''Triad'' which includes Alphonsus
* {{cite web| last = Wood | first = Chuck | date = July 10, 2006 | url = http://www.lpod.org/?m=20060710 | title = Craters and Papers | publisher = Lunar Photo of the Day |url-status=dead|archive-url=https://web.archive.org/web/20110614233616/http://www.lpod.org/?m=20060710|archive-date=June 14, 2011}}
* {{cite web| last = Wood | first = Chuck | date = September 16, 2006 | url = http://www.lpod.org/?m=20060916 | title = Just Another Glorious Image | publisher = Lunar Photo of the Day |url-status=dead|archive-url=https://web.archive.org/web/20110614233616/http://www.lpod.org/?m=20060916|archive-date=June 14, 2011}}
* {{cite web| last = Wood | first = Chuck | date = November 27, 2006 | url = http://www.lpod.org/?m=20061127 | title = A Long Line in the Matter of Confidence | publisher = Lunar Photo of the Day |url-status=dead|archive-url=https://web.archive.org/web/20110614233616/http://www.lpod.org/?m=20061127|archive-date=June 14, 2011}}
*{{APOD |date=9 February 2007|title=Ptolemaeus, Alphonsus and Arzachel}}
* {{cite web| last = Wood | first = Chuck | date = February 13, 2007| url = http://www.lpod.org/?m=20070213 | title = New Observations of a Well-Known Area | publisher = Lunar Photo of the Day |url-status=dead|archive-url=https://web.archive.org/web/20110614233616/http://www.lpod.org/?m=20070213|archive-date=June 14, 2011}}

{{Authority control}}

{{Craters on the Moon: A–B}}
{{Craters on the Moon: C-F}}


[[Category:Impact craters on the Moon]]
[[Category:Impact craters on the Moon]]

Latest revision as of 22:31, 27 August 2024

Alphonsus
LRO image
Coordinates13°23′S 2°51′W / 13.39°S 2.85°W / -13.39; -2.85
Diameter110.54 km
Depth2.7 km
Colongitude4° at sunrise
EponymAlfonso X
The crater area in a Selenochromatic format Image (Si)
Alphonsus crater appears in the right half of this image taken by Ranger 7. NASA photo.

Alphonsus is an ancient impact crater on the Moon that dates from the pre-Nectarian era.[1] (Older sources state that it is Nectarian in age.[2]) It is located on the lunar highlands on the eastern end of Mare Nubium, west of the Imbrian Highlands, and slightly overlaps the crater Ptolemaeus to the north. To the southwest is the smaller Alpetragius. The crater name was approved by the IAU in 1935.[3]

Description

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The surface of Alphonsus is broken and irregular along its boundary with Ptolemaeus. The outer walls are slightly distorted and possess a somewhat hexagonal form.

A low ridge system of deposited ejecta bisects the crater floor, and includes the steep central peak designated Alphonsus Alpha (α). This pyramid-shaped formation rises to a height of 1.5 km above the interior surface. It is not volcanic in origin, but rather is made of anorthosite like the lunar highlands.

The floor is fractured by an elaborate system of rilles and contains four or five smaller craters surrounded by a symmetric darker halo. These dark-halo craters are cinder cone-shaped and are believed by some to be volcanic in origin, although others think they were caused by impacts that excavated darker mare material from underneath the lighter lunar regolith.

Exploration

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The Ranger 9 probe impacted in Alphonsus, a short distance to the northeast of the central peak. Harold Urey said of a close-up photograph of Alphonsus:

The floor is covered with many craters of various sizes, some sharp and hence new, others less distinct and partly filled with fragmented material. The walls have fewer craters, and this probably means that slumping of the wall has filled them. Crevasses are evident, and evidence for slumping exists. The larger crater near the top is undoubtedly collisional in origin. Three craters are surrounded by dark halos and were produced by eruptions from the lunar interior. Exceptionally bright, sharp peaks can be seen on certain mountain tops.[4]

Apollo Landing Site

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The dark-haloed craters along some of the rilles in the crater are thought to be volcanic vents, and during the Apollo program Alphonsus was considered as a possible landing site in order to possibly sample xenoliths of the lunar mantle from the vents.[5] It was considered for Apollo 16 but the Descartes area was selected. It was one of the three final possible sites for Apollo 17, together with Gassendi crater and the Taurus-Littrow valley, but it was considered possibly "contaminated" with younger material from the nearby Imbrium basin.[6]

Transient lunar phenomena

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Alphonsus is one of the sites noted for transient lunar phenomena, as glowing red-hued clouds have been reported emanating from the crater. On October 26, 1956, the lunar astronomer Dinsmore Alter noted some blurring of the rilles on the floor of Alphonsus in the photographs he took in violet light. The same blurring did not occur in the infrared photographs he took at the same time. However, few professional astronomers found this evidence of volcanic activity on the Moon very convincing.[7]

One astronomer who was intrigued by Alter's observations was Nikolai A. Kozyrev, from the Soviet Union. In 1958 while Kozyrev was looking for volcanic phenomenon on the moon, he observed the formation of a mist-like cloud within Alphonsus.[8] The spectrum of the area had been measured at this time, and displayed indications of carbon matter, possibly C2 gas. He believed this to be the result of volcanic or related activity. However no evidence for this phenomenon has been found from lunar missions, and the emission results have never been confirmed.[9]

Names

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Alphonsus is named after King Alfonso X of Castile (known as "Alfonso the Wise"), who had an interest in astronomy.[10] Like many of the craters on the Moon's near side, it was given its name by Giovanni Riccioli, whose 1651 nomenclature system has become standardized; Riccioli originally named it "Alphonsus Rex" ('King Alfonso'), but the 'Rex' was later dropped.[11] Earlier lunar cartographers had given the feature different names. Michael van Langren's 1645 map calls it "Ludovici XIV, Reg. Fran.", after Louis XIV of France,[12] and Johannes Hevelius called it "Mons Masicytus" after a range of mountains in Lycia.[13]

Interior craters

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Oblique view of the five small named craters: C = Chang-Ngo, R = Ravi, M = Monira, J = Jose, S = Soraya. Facing south with sun illuminating from left. North on the photo is on the bottom
Ranger 9 image showing rilles on the floor of the crater

Five tiny craters in the northeastern part of Alphonsus' interior floor have been assigned names by the IAU. These are listed in the table below.

Crater Coordinates Diameter Name source
Chang-Ngo 12°42′S 2°06′W / 12.7°S 2.1°W / -12.7; -2.1 3 km Chinese goddess of the moon
José 12°42′S 1°36′W / 12.7°S 1.6°W / -12.7; -1.6 2 km Spanish masculine name
Monira 12°36′S 1°42′W / 12.6°S 1.7°W / -12.6; -1.7 2 km Arabic feminine name
Ravi 12°30′S 1°54′W / 12.5°S 1.9°W / -12.5; -1.9 2.5 km Indian masculine name
Soraya 12°54′S 1°36′W / 12.9°S 1.6°W / -12.9; -1.6 2 km Persian feminine name

Satellite craters

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Alphonsus crater and its satellite craters taken from Earth in 2012 at the University of Hertfordshire's Bayfordbury Observatory with the telescopes Meade LX200 14" and Lumenera Skynyx 2-1

By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Alphonsus.

Alphonsus Latitude Longitude Diameter
A 14.8° S 2.3° W 4 km
B 13.2° S 0.2° W 24 km
C 14.4° S 4.8° W 4 km
D 15.1° S 0.8° W 23 km
G 12.3° S 3.3° W 4 km
H 15.6° S 0.5° W 8 km
J 15.1° S 2.5° W 8 km
K 12.5° S 0.1° W 20 km
L 12.0° S 3.7° W 4 km
R 14.4° S 1.9° W 3 km
X 15.0° S 4.4° W 5 km
Y 14.7° S 1.8° W 3 km

References

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  1. ^ Ambrose, W.A. "ORIGIN, DISTRIBUTION, AND CHRONOSTRATIGRAPHY OF ASYMMETRIC SECONDARY CRATERS ASSOCIATED WITH NEARSIDE LUNAR BASINS" (PDF). Bureau of Economic Geology. University of Texas at Austin, TX. Retrieved 25 September 2013.
  2. ^ The geologic history of the Moon. USGS Professional Paper 1348. By Don E. Wilhelms, John F. McCauley, and Newell J. Trask. U.S. Government Printing Office, Washington: 1987. Table 9-4.
  3. ^ Alphonsus, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN)
  4. ^ EXPLORING SPACE WITH A CAMERA, Section 2, To The Moon and Beyond, NASA Special Publication 168 (SP-168)
  5. ^ To a Rocky Moon: A Geologist's History of Lunar Exploration. Don E. Wilhelms, University of Arizona Press (1993). ISBN 978-0816510658 Chapter 16.
  6. ^ To a Rocky Moon: A Geologist's History of Lunar Exploration. Don E. Wilhelms, University of Arizona Press (1993). ISBN 978-0816510658 Chapter 17.
  7. ^ Dinsmore (1957), 69: 158
  8. ^ Oepik, E.J. (January 1968). "Cratering and the moon's surface". Armagh Observatory. Department of Physics and Astronomy, University of Maryland. hdl:2060/19690007782.
  9. ^ Dinsmore (1957), 71: 46
  10. ^ "Alphonsus (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  11. ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.210.
  12. ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 198.
  13. ^ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 205.

Further reading

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