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词条 Elysium Mons
释义

  1. Discovery

  2. Terrestrial analog

  3. Possible source of nakhlites

  4. Gallery

  5. Interactive Mars map

  6. See also

  7. References

  8. External links

{{about|the volcano on Mars|other uses|Elysium (disambiguation)}}{{Infobox feature on celestial object
|name = Elysium Mons
|image =
|caption = 2001 Mars Odyssey THEMIS daytime infrared image mosaic
|coordinates = {{coord|25.02|N|147.21|E|globe:mars_type:landmark|display=inline,title}}
|coordinates_footnotes = [1]
|peak = {{convert|13.9|km|ft}} above plains
{{convert|16|km|ft}} above datum
|discoverer = Mariner 9
}}

Elysium Mons is a volcano on Mars located in the volcanic province Elysium, at {{Coord|25.02|N|147.21|E|globe:Mars_type:mountain_source:gpn}}, in the Martian eastern hemisphere. It stands about {{convert|12.6|km|ft|abbr=on}} above its base,[2] and about {{convert|14.1|km|ft|abbr=on}} above the Martian datum,[2] making it the third tallest Martian mountain in terms of relief and the fourth highest in elevation. Its diameter is about {{convert|240|km|mi|abbr=on}}, with a summit caldera about {{convert|14|km|mi|abbr=on}} across. It is flanked by the smaller volcanoes Hecates Tholus to the northeast, and Albor Tholus to the southeast.

Discovery

Elysium Mons was discovered in 1972 in images returned by the Mariner 9 orbiter.

Terrestrial analog

The terrestrial volcano Emi Koussi (in Chad) has been studied as an analog of Elysium Mons. The two shield volcanoes have summit calderas of similar size, but Elysium Mons is 3.5 times larger in diameter and 6 times higher than its counterpart on Earth.

Possible source of nakhlites

A 6.5 km diameter crater at 29.674 N, 130.799 E, in the volcanic plains to the northwest of Elysium Mons has been identified as a possible source for the nakhlite meteorites, a family of similar basaltic Martian meteorites with cosmogenic ages of about 10.7 Ma, suggesting ejection from Mars by a single impact event. The dates of the igneous rocks of the nakhlites range from 1416 ± 7 Ma to 1322 ± 10 Ma. These dates plus the crater dimensions suggest a growth rate of the source volcano during that interval of 0.4–0.7 m per Ma, far slower than would be expected for a terrestrial volcano. This implies that Martian volcanism had slowed greatly by that point in history.[3]

{{clear}}

Gallery

Interactive Mars map

{{Mars map}}

See also

  • Geography of Mars
  • List of mountains on Mars by height
  • List of tallest mountains in the Solar System

References

1. ^{{gpn|1783|Elysium Mons}}
2. ^{{cite journal|last1=Plescia|first1=J. B.|title=Morphometric properties of Martian volcanoes|journal=Journal of Geophysical Research|volume=109|issue=E3|pages=E03003|date=2004|issn=0148-0227|doi=10.1029/2002JE002031|bibcode = 2004JGRE..109.3003P }}
3. ^{{cite journal|last1= Cohen|first1=B. E.|last2= Mark|first2=D. F.|last3= Cassata|first3=W. S.|last4= Lee|first4=M. R.|last5= Tomkinson|first5= T.|last6= Smith|first6=C. L.|title= Taking the pulse of Mars via dating of a plume-fed volcano|journal= Nature Communications|volume= 8|issue= 1|year= 2017|doi= 10.1038/s41467-017-00513-8|bibcode=2017NatCo...8..640C}}

External links

{{Commons category|Elysium Mons}}
  • Google Mars - zoomable map centered on Elysium Mons
  • "Elysium Mons Volcano" - NASA images of Elysium Mons, from Malin Space Science Systems
{{Mars}}{{portal bar|Mars}}{{Mars-stub}}{{Crater-stub}}

2 : Volcanoes of Mars|Mountains on Mars

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