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Montes
Apenninus forms a sharp, rugged rise at the edge of the Mare Imbrium. The total length of the range is about 600 km (370 mi), with some of the peaks rising as high as 5 km (3.1 mi). The entire area to the southeast of Montes Apenninus - its backslopes - is shaped by ejecta
274:
mission made its landing. This landing was considered one of the most scientifically successful missions of the Apollo program and started the last three J-Series missions that included the lunar rover and 3-day stays. Apollo 15 explored smaller peak Mons Hadley Delta (δ) and Rima Hadley
283:
deposited during the violent uplift of the mountains. Sections of the Montes
Apenninus front are also rubbly, a result of both fallback ejecta and landslides from the newly formed peaks.
415:
Spudis, P. D. (November 10–12, 1980). Merrill, R.B.; Schultz, P. H. (eds.). "Petrology of the
Apennine Front, Apollo 15: Implications for the Geology of the Imbrium Impact Basin".
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244:
509:
645:
216:
From
Eratosthenes, the mountains form an arcing chain that gradually bends from east to northeast, ending at Promontorium Fresnel at about
201:, which abuts against the southern face of the range. To the west of these mountains is a narrow gap where Mare Imbrium in the north joins
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327:
landing site left of center. Mons Hadley, Mons Hadley Delta, and Mons
Bradley are visible. The large crater at right edge is
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This range contains several mountains that have received names, listed below ranging from west to northeast:
763:
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Montes
Apenninus is the most prominent remnant of the outer ring of the Imbrium basin, which also includes
323:
Oblique view of the northern Montes
Apenninus facing east from 105 km altitude, with Hadley Rille and the
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Montes
Apenninus area in selenochromatic image (Si) with some landmarks (yellow/normal, red/pyroclastic).
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Abstracts of Papers
Presented to the Conference on Multi-ring Basins: Formation and Evolution
167:. With their formation dating back about 3.9 billion years, Montes Apenninus are fairly old.
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475:. L&PI Lunar Map series (1st ed.). Lunar and Planetary Institute. December 1976
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Oblique view of the southern Montes
Apenninus facing south from 115 km altitude, with
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279:. This was considered the most geologically diverse landing site of the program.
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This article is about the Lunar mountain range. For other uses of Apennine, see
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88:
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Bussey, B.J.; Spudis, P.D.; Hawke, B.R.; Lucey, P.G.; Taylor, G.J. (1998).
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29.5° N. Here is another gap where the Mare Imbrium to the west joins the
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359:: M. Gålfalk, G. Olofsson, and H.-G. Florén, taken with the SIRCA camera.
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444:"Geology and composition of the Apennine mountains, lunar Imbrium basin"
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347:
186:
The Montes Apenninus range forms the southeastern border of the large
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to the south. Further to the west are the Montes Carpatus mountains.
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highland region. It begins just to the west of the prominent crater
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to the east. At the north end of this gap lie the Montes Caucasus.
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View of the limb of the Moon showing Montes Apenninus (left),
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Montes Apenninus in the infrared. Image courtesy of
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144:'s features. Montes Apenninus is marked with a "K".
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379:"Eratosthenes, Archimedes, Montes Apenninus"
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311:. The large crater at the top center is
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159:'s near side. They are named after the
423:. Lunar and Planetary Institute: 83.
7:
646:International Lunar Research Station
193:and the northwestern border of the
473:"LM-41 Montes Apenninus Lunar Map"
243:, often incorrectly listed as the
155:range on the northern part of the
14:
578:
377:Hungeling, Andreas (2006–2009).
34:
247:(though not the highest point)
1:
664:Man Will Conquer Space Soon!
603:KLE Complex Lunar Expedition
266:The last two peaks form the
245:highest mountain on the Moon
234:Mons Serao (unofficial name)
615:Lunar Expeditionary Complex
381:(in German). Archived from
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343:in upper right (Apollo 15)
18:
16:Mountain range on the Moon
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21:Apennine (disambiguation)
621:Energia Lunar Expedition
519:Colonization of the Moon
764:Exploration of the Moon
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790:Mountains on the Moon
404:The Mons Huygens Myth
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769:Tourism on the Moon
429:1980LPICo.414...83S
303:(top), and western
110:English translation
85: /
682:Chinese Lunar Base
676:Human Lunar Return
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161:Apennine Mountains
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114:Apennine Mountains
49:Highest point
777:
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569:Artemis Base Camp
545:Apollo Lunar Base
526:American projects
299:(right), eastern
256:Mons Hadley Delta
179:to its south and
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720:Montes Apenninus
590:Russian projects
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305:Mare Serenitatis
222:Mare Serenitatis
149:Montes Apenninus
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29:Montes Apenninus
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385:on 18 July 2011
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307:(bottom), from
297:Montes Caucasus
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181:Montes Caucasus
177:Montes Carpatus
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60:Lunar mountains
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698:Proposed sites
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656:Other projects
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466:External links
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203:Mare Insularum
183:to its north.
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140:Detail map of
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627:Lunny Poligon
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563:Lunar Outpost
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151:are a rugged
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710:Eratosthenes
648:(late 2020s)
477:. Retrieved
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420:
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387:. Retrieved
383:the original
372:
341:Eratosthenes
301:Mare Imbrium
281:
265:
251:Mons Bradley
241:Mons Huygens
226:
215:
199:Eratosthenes
195:Terra Nivium
188:Mare Imbrium
185:
174:
148:
147:
142:Mare Imbrium
715:Sinus Medii
705:Sinus Roris
637:Chinese and
479:15 February
389:15 February
261:Mons Hadley
237:Mons Ampère
171:Description
92: /
67:Coordinates
730:Shackleton
588:Soviet and
364:References
313:Archimedes
270:where the
231:Mons Wolff
191:lunar mare
666:" (1950s)
325:Apollo 15
309:Apollo 11
272:Apollo 15
120:Geography
784:Category
751:Moonbase
218:latitude
153:mountain
125:Location
89:20°N 3°W
744:Related
690:(2030s)
684:(2030s)
678:(1990s)
672:(1990s)
629:(2030s)
623:(1980s)
617:(1970s)
611:(1970s)
605:(1970s)
599:(1960s)
571:(2030s)
565:(2000s)
559:(1990s)
553:(1980s)
547:(1970s)
541:(1960s)
535:(1960s)
425:Bibcode
55:Listing
725:Kepler
451:LPSC98
268:valley
105:Naming
94:20; -3
735:Peary
557:Lunox
447:(PDF)
329:Conon
287:Views
277:rille
165:Italy
43:image
481:2010
455:1352
391:2010
355:and
157:Moon
129:Moon
77:20°N
609:L3M
421:414
353:NOT
163:in
80:3°W
41:LRO
786::
453:.
449:.
419:.
357:SO
662:"
511:e
504:t
497:v
483:.
457:.
431:.
427::
393:.
331:.
315:.
23:.
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.