请输入您要查询的百科知识:

 

词条 Lunar dome
释义

  1. Examples

  2. References

  3. External links

A lunar dome is a type of shield volcano that is found on the surface of the Earth's Moon. They are typically formed by highly viscous, possibly silica-rich lava, erupting from localized vents followed by relatively slow cooling. Lunar domes are wide, rounded, circular features with a gentle slope rising in elevation a few hundred meters to the midpoint. They are typically 8–12 km in diameter, but can be up to 20 km across. Some of the domes contain a small craterlet at the peak.

Some of the domes have been shown to consist of the same materials as the lunar maria. Thus they could be created by some mechanism that differs from the mare-forming flows. It is thought that these domes are formed from a smaller magma chamber that is closer to the surface than is the case for a mare. This results in a lower pressure, and so the lava flows more slowly. The magma wells up through a crack in the surface, but the flow eventually concentrates through one primary vent. This concentration can then result in a vent crater at the peak of the dome.

The cluster of lunar domes at the Marius Hills was considered as a possible landing site of Apollo 15. There are concentrations of lunar domes near the craters Hortensius, and T. Mayer, across the top of Mons Rümker, and in Mare Fecunditatis. Solitary lunar domes are also found, including Kies Pi (π), Milichius Pi (π), Mons Gruithuisen Gamma (γ) and Delta (δ), and domes near the craters Gambart C, Beer, and Capuanus. Omega Cauchy (ω) and Tau Cauchy (τ) form a pair of domes near the crater Cauchy. Likewise near Arago are the domes Arago Alpha (α) and Arago Beta (β). There are two domes south of Mons Esam.

The IAU does not currently have rules that establish the naming of lunar domes, but the practice in the professional literature and in lunar sciences is to name the dome with the name of the nearest crater followed by a number that denotes the order of discovery.

Examples

References

  • Lionel Wilson and James W. Head, "Lunar Gruithuisen and Mairan domes: Rheology and mode of emplacement", Journal of Geophysical Research, vol. 108, 2003.
  • Lena, R., Wöhler, C., Phillips, J., Chiocchetta, M.T., "Lunar Domes:Properties and Formation Processes", "Springer Praxis Books", 2013, "[https://www.springer.com/astronomy/astrophysics+and+astroparticles/book/978-88-470-2636-0]".

External links

  • [https://www.webcitation.org/query?url=http://www.geocities.com/kc5lei/lunar_dome.html&date=2009-10-26+01:15:34 Marvin W. Huddleston, ALPO Lunar Dome Survey Coordinator's web page on Lunar Domes]
  • [https://web.archive.org/web/20070517134848/http://www.lpl.arizona.edu/~rhill/alpo/lunar.html Association of Lunar & Planetary Observers, Lunar Section]
  • GLR Group Website
  • [https://web.archive.org/web/20060510090402/http://luna.uai.it/domi/lunar_domes.htm UAI Lunar Dome Introduction]
{{The Moon}}

5 : Geological features on the Moon|Shield volcanoes|Lava domes|Extraterrestrial volcanoes|Geologic domes

随便看

 

开放百科全书收录14589846条英语、德语、日语等多语种百科知识,基本涵盖了大多数领域的百科知识,是一部内容自由、开放的电子版国际百科全书。

 

Copyright © 2023 OENC.NET All Rights Reserved
京ICP备2021023879号 更新时间:2024/11/12 10:10:47