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that flows over other deposits (debris-covered glacial ice). The ice could have been deposited when the tilt of Mars changed the climate, thereby causing more moisture to be present in the atmosphere. Studies suggest the glaciation happened in the Late
Amazonian period, the most recent period in Mars chronology. Multiple stages of glaciation probably occurred. The ice present today represents one more resource for possible future colonization of the planet.
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297:. The northern flanks of the volcano are highly faulted with grabens and normal faults concentric to the volcano's summit caldera. To its lower east flank, there is a chain of elliptical, or oval-shaped, pits, lined up down the center of a shallow trough. These features were formed by faulting and associated collapse; the scarp on each side of the trough is a fault line.
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data, combined with developments in the study of glaciers, scientists suggest that glaciers once existed on
Pavonis Mons and probably still do to some extent. Evidence for this includes concentric ridges (moraines "dropped" by glaciers), a knobby area (caused by ice sublimating), and a smooth section
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Pavonis Mons is the middle of three volcanos (collectively known as
Tharsis Montes) on the Tharsis bulge near the equator of the planet Mars. The other Tharsis volcanoes are Ascraeus Mons and Arsia Mons. The three Tharsis Montes, together with some smaller volcanoes to the north, form a fairly
471:
273:). The dust forms a mantle over the surface that obscures or mutes much of the fine-scale topography and geology of the region. Tharsis is probably dusty because of its high elevations. The summit experiences an atmospheric pressure of around 130
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that is 47 km in diameter and almost 5 km deep. A larger, shallower depression lies immediately northeast of the smaller caldera. The large depression is about 90 km in diameter and structurally more complex than the small caldera.
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238:(the southernmost member of the chain). The Tharsis Montes volcanoes lie along the crest of a northeast-trending rise (Tharsis bulge) that extends more than 3,000 km across the western equatorial region of Mars.
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Pavonis Mons is the name of a
Settlement Defense Front destroyer in the game Call of Duty: Infinite Warfare in the mission "Operation Deep Execute", Captain Khosi Siyada was the ship's commander.
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spacecraft in 1971, and was originally called Middle Spot. Its name formally became
Pavonis Mons in 1973. The equatorial location of its peak and its height make it the ideal terminus for a
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daytime IR mosaic of
Pavonis Mons. A large fan-shaped expanse of knobby deposits (the Pavonis Sulci) believed left by past glaciation extends northwestward from the mountain.
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Pavonis Mons is the smallest of the
Tharsis Montes volcanoes, measuring about 375 km across and standing 14 km above Mars' mean surface level. As a
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is used as the anchor, having been shifted from its current orbit. Pavonis Mons also hosts a space elevator in other GURPS settings, including
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277:(1.3 mbar), about 21% of Mars' mean surface pressure. The atmospheric density is too low to mobilize and remove dust once it is deposited.
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straight line. It has been proposed that this straight line of volcanoes is the result of the sort of plate motion which on Earth makes
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Mouginis-Mark, P.J.; Harris, A.J.L.; Rowland, S.K. (2007). Terrestrial
Analogs to the Calderas of the Tharsis Volcanoes on Mars in
202:, and it has often been proposed as a space elevator location, especially in science fiction. It is also an ideal location for a
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has its base on the southern rim of
Pavonis – the highest place on the equator – and the city of Sheffield is built around it.
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253:, Pavonis Mons has an extremely low profile with flank slopes that average only 4°. The summit contains a deep, circular
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Pavonis Mons provides the putative setting for the song "Approaching
Pavonis Mons by Balloon (Utopia Planitia)" by
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996:"Origin and evolution of a cold-based tropical mountain glacier on Mars: The Pavonis Mons fan-shaped deposit"
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921:"Origin and Evolution of Cold-Based Tropical Mountain Glacier on Mars: the Pavonis Mons Fan-Shaped Deposit"
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194:) that straddle the Martian equator between longitudes 235°E and 259°E. The volcano was discovered by the
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roleplaying game setting. The city of New Shanghai, the largest on Mars, is built around the elevator.
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Geologic Map of Pavonis Mons Volcano, Mars, available as 16.3 Mb PDF file, U.S. Geological Survey 1998
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Scott, D.H.; Dohm, J.M.; Zimbleman, J.R. (1998). Geologic Maps of Pavonis Mons, Mars. USGS, I-2561.
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image showing mantle of dust near summit of Pavonis Mons. The dust makes the image look blurry.
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190:. It is the middle member of a chain of three volcanic mountains (collectively known as the
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lies at the edge of the Tharsis bulge, about 1,200 km northwest of Pavonis Mons.
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Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) wide angle color composite image
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HiRISE image of a 180 m wide lava tube skylight on the volcano's southeast flank
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835:"Surface Properties of Ascraeus Mons: Dust Deposits on a Tharsis Volcano"
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A Traveller's Guide to Mars: The Mysterious Landscapes of the Red Planet
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The bulk of the volcano's surface consists of lava flows of the early
234:(the northernmost of the Tharsis Montes) and 400 km northeast of
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The Martian Surface: Composition, Mineralogy and Physical Properties
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M. Chapman, Ed.; Cambridge University Press: Cambridge, UK, p. 76.
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NASA Astronomy Picture of the Day: A Hole in Mars (18 July 2012)
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Mars: An Introduction to its Interior, Surface and Atmosphere
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image of channels and pits on southern flank of Pavonis Mons.
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Shean, David E.; Head, James W.; Marchant, David R. (2005).
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Like most of the Tharsis region, Pavonis Mons has a high
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NASA MGS data 0.7 degrees N 245.9 degrees E 13368 meters
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The Geology of Mars: Evidence from Earth-based Analogs,
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8.7 km (5.4 mi) 28,543 ft (8,700 m)
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skylight surrounded by a collapse pit on Pavonis Mons
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skylight surrounded by a collapse pit on Pavonis Mons
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Pavonis Mons hosts a space elevator to Deimos in the
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1061:
Sleep, Norman H. (1994). "Martian plate tectonics".
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1151:"Tectonic implications of Mars crustal magnetism"
226:Pavonis Mons stands at the southern edge of the
1214:Hypothetical Spacecraft and Interstellar Travel
1155:Proceedings of the National Academy of Sciences
222:. Pavonis Mons is located at the southern edge.
743:"Morphometric Properties of Martian Volcanoes"
617:Carr, Michael H. (1973). "Volcanism on Mars".
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289:MOLA colorized topography of Pavonis Mons
230:- approximately 400 km southwest of
366:Pavonis Mons is also the base of Mars's
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18:
1211:Nygren, Ezekial (February 28, 2015).
656:"Gazetteer of Planetary Nomenclature"
573:. USGS Astrogeology Research Program.
7:
318:Possible evidence of plate tectonics
571:Gazetteer of Planetary Nomenclature
542:List of mountains on Mars by height
702:Morton, Oliver (October 4, 2002).
464:on southern flank of Pavonis Mons.
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340:, released as part of the album
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1063:Journal of Geophysical Research
1003:Journal of Geophysical Research
925:Journal of Geophysical Research
747:Journal of Geophysical Research
619:Journal of Geophysical Research
391:Buck Rogers in the 25th Century
343:Yoshimi Battles the Pink Robots
1110:. Cambridge University Press.
1040:. Cambridge University Press.
966:. Cambridge University Press.
325:chains of "hot spot" volcanoes
1:
1106:Barlow, Nadine (2008-01-10).
894:. New York: Workman. p.
886:Hartmann, W.K. (2003-01-01).
658:. planetarynames.wr.usgs.gov.
495:image (color) of a 35 m wide
242:, the tallest volcano in the
1689:Recurring slope lineae (RSL)
1149:Connerney, J. E. P. (2005).
2123:Inspiration Mars Foundation
867:Martian Weather Observation
842:Lunar and Planetary Science
2330:
2309:Phoenicis Lacus quadrangle
2158:Artificial objects on Mars
793:Cambridge University Press
2227:
2175:List of films set on Mars
1990:C/2013 A1 (Siding Spring)
1787:Classical albedo features
1289:
783:Carr, Michael H. (2006).
679:10.1007/978-3-319-44311-9
673:. Switzerland: Springer.
669:Genta, Giancarlo (2017).
603:Dictionary.com Unabridged
590:Dictionary.com Unabridged
24:
2093:List of missions to Mars
1036:Bell, Jim (2008-06-05).
960:Michael H. Carr (2006).
919:Shean, David E. (2005).
833:Zimbleman, J.R. (1985).
708:. Picador. p. 296.
2251:Solar System portal
1176:10.1073/pnas.0507469102
741:Plescia, J. B. (2004).
639:10.1029/JB078i020p04049
265:(reflectivity) and low
1865:Solar eclipses on Mars
1724:"Swiss cheese" feature
1580:Concentric crater fill
290:
223:
178:mountain") is a large
514:image of a 35 m wide
288:
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186:region of the planet
2065:Permanent settlement
1023:10.1029/2004JE002360
946:10.1029/2004JE002360
768:10.1029/2002JE002031
428:Mars Global Surveyor
351:Kim Stanley Robinson
2207:Timekeeping on Mars
1884:Planetary transits
1869:Satellite transits
1782:Observation history
1630:Lobate debris apron
1167:2005PNAS..10214970C
1161:(42): 14970–14975.
1075:1994JGR....99.5639S
1015:2005JGRE..110.5001S
963:The surface of Mars
937:2005JGRE..110.5001S
854:1985LPI....16..934Z
787:The Surface of Mars
759:2004JGRE..109.3003P
631:1973JGR....78.4049C
210:General description
65: /
21:
2314:Tharsis quadrangle
1136:2011-06-03 at the
872:2007-03-11 at the
547:Tharsis quadrangle
331:In popular culture
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228:Tharsis quadrangle
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220:Tharsis quadrangle
2304:Volcanoes of Mars
2294:Mountains on Mars
2259:
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2212:Sol (day on Mars)
2180:Martian scientist
2163:Memorials on Mars
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2117:The Case for Mars
2014:
2013:
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1729:Terrain softening
1694:Ring mold craters
1662:North Polar Basin
1585:Dark slope streak
1430:Vastitas Borealis
1327:Dust devil tracks
1131:dsc.discovery.com
1117:978-0-521-85226-5
1093:10.1029/94JE00216
1069:(E3): 5639–5655.
1047:978-0-521-86698-9
973:978-0-521-87201-0
905:978-0-7611-2606-5
806:978-0-521-87201-0
688:978-3-319-44311-9
625:(20): 4049–4062.
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1380:Planum Australe
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1009:(E5): E05001.
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931:(E5): E05001.
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671:Next Stop Mars
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606:(Online). n.d.
593:(Online). n.d.
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180:shield volcano
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2278:Solar System
2197:Life on Mars
2192:Flag of Mars
2133:Mars Society
2115:
2108:
2075:Terraforming
2070:Colonization
1840:Swift crater
1682:polar wander
1410:Terra Sabaea
1350:Arabia Terra
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977:. Retrieved
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356:Mars Trilogy
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260:
248:
244:Solar System
240:Olympus Mons
225:
117:Pavonis Mons
116:
115:
108:
74:1.48; 247.04
40:Feature type
20:Pavonis Mons
2020:Exploration
1942:5261 Eureka
1610:Groundwater
1575:Composition
1400:Tempe Terra
1390:Quadrangles
1317:Circulation
848:: 934–935.
476:The summit
462:cinder cone
72: /
48:Coordinates
2288:Categories
1677:Polar caps
1657:Mud cracks
1640:Meteorites
1625:Lava tubes
1560:Carbonates
1495:Labyrinthi
1370:Iani Chaos
1309:Atmosphere
795:. p.
753:: E03003.
553:References
394:franchise.
383:GURPS Mars
236:Arsia Mons
93:Discoverer
2202:Sub-Earth
2185:Mythology
2138:Mars race
1905:Asteroids
1801:Astronomy
1772:Hesperian
1767:Amazonian
1739:Volcanism
1714:Spherules
1635:Marsquake
1590:Dichotomy
1505:by height
1500:Mountains
1300:Geography
1079:CiteSeerX
516:lava tube
497:lava tube
359:, Mars's
196:Mariner 9
97:Mariner 9
2238:Category
2102:Advocacy
2085:Missions
2028:Concepts
1857:Transits
1828:Monolith
1777:Noachian
1749:Yardangs
1645:on Earth
1605:Glaciers
1450:"Canals"
1442:features
1440:Physical
1217:. Lulu.
1195:16217034
1134:Archived
979:21 March
870:Archived
773:Table 1.
536:See also
301:Glaciers
204:Sky Ramp
107:Latin -
60:247°02′E
2170:Fiction
2151:Related
2045:Landing
2040:Orbiter
1999:General
1968:2007 NS
1958:1999 UJ
1948:1998 VF
1937:Trojans
1924:2007 WD
1913:Impacts
1893:Mercury
1759:History
1719:Surface
1650:on Mars
1615:Gullies
1600:Geysers
1547:Geology
1537:Gravity
1532:Valleys
1485:Gullies
1475:Craters
1465:Catenae
1460:Canyons
1415:Tharsis
1360:Cydonia
1342:Regions
1332:Methane
1322:Climate
1186:1250232
1163:Bibcode
1071:Bibcode
1011:Bibcode
933:Bibcode
850:Bibcode
755:Bibcode
627:Bibcode
478:caldera
402:Gallery
370:in the
311:Odyssey
281:Geology
255:caldera
218:Map of
184:Tharsis
176:peacock
2264:Portal
2242:
2231:
1983:Comets
1878:Deimos
1873:Phobos
1835:Deimos
1818:Phobos
1522:Plains
1490:Mensae
1480:Fossae
1221:
1193:
1183:
1114:
1081:
1044:
970:
902:
803:
712:
685:
598:"Mons"
585:"Pavo"
512:HiRISE
493:HiRISE
446:THEMIS
379:Deimos
305:Using
263:albedo
104:Eponym
99:(1971)
57:1°29′N
32:THEMIS
2050:Rover
2035:Flyby
2006:Orbit
1888:Earth
1810:Moons
1744:Water
1620:Lakes
1570:Color
1420:Undae
999:(PDF)
838:(PDF)
372:GURPS
174:for "
172:Latin
1709:Soil
1454:list
1283:Mars
1219:ISBN
1191:PMID
1112:ISBN
1042:ISBN
981:2011
968:ISBN
900:ISBN
801:ISBN
710:ISBN
683:ISBN
309:and
188:Mars
85:Peak
1181:PMC
1171:doi
1159:102
1089:doi
1019:doi
1007:110
941:doi
929:110
846:XVI
763:doi
751:109
675:doi
635:doi
431:MOC
353:'s
349:In
307:MGS
2290::
1950:31
1203:^
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724:^
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623:78
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460:A
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275:Pa
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137:oʊ
2266::
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170:(
166:/
163:z
160:n
157:ɒ
154:m
151:ˈ
146:s
143:ɪ
140:n
134:v
131:ˈ
128:ə
125:p
122:/
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