- Marius Hills
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The Marius Hills are a set of volcanic domes located in Oceanus Procellarum on Earth's Moon. The domes are thought to have formed from lavas fairly more viscous than those that formed the Lunar mare. These domes average approximately 200–500 m (656.17-1640.43 ft) in height.[1][2][3] The Marius Hills take their name from the nearby 41 km (25 mi) diameter crater Marius.[4] These hills represent the highest concentration of volcanic features on the Moon.[5]
Contents
Geography and geology
An abundance of domes, cones, and volcanic rilles and channels is characteristic of the Marius Hills. The Lunar Reconnaissance Orbiter photographed a pit that could be a skylight in an underground lava tube, indicating that part of its roof has collapsed, as what often happens after lava tubes cease to be active.[3][6]
Data from the Lunar Reconnaissance Orbiter has been used to identify two different varieties of domes among the Marius Hills: (1) large, irregularly shaped domes and (2) smaller domes with steep sides and diameters of about 1–2 km (0.62-1.24 mi). Another feature, possibly pyroclastic, or primarily volcanic in composition, has a roughly circular shape and steep sides. Bright, high albedo boulders have been shown to be characteristic of lava flows in the Marius Hills. This suggests blocky lava with a high silica content formed these features. This hypothesis, however, is not supported by data obtained from the Clementine lunar orbiter. Analysis of lower albedo, or less reflective boulders suggest that many domes in the area may contain two layers of material: (1) an upper layer of thin, dark material covering (2) a layer of thick, bright material.[5]
The Marius Hills region was at one time considered a possible landing site for a lunar landing mission during the American Apollo program (eventually becoming the alternative site for Apollo 15), with the possibility of gaining insight about the volcanic history of the Moon from domes in the area.[7]
Marius Hills "pit"
The pit discovered by the Lunar Reconnaissance Orbiter (LRO) has been the subject of much research and speculation. There is a possibility that this feature could be a skylight in an underground lava tube.[8] The depth of this pit is estimated to be 80 and 88 m (260 and 289 ft) and it's width is estimated to be several hundreds of meters.[9]
See also
References
- ^ "Marius Hills". Lunar Reconnaissance Orbiter. National Aeronautics and Space Administration. http://www.nasa.gov/mission_pages/LRO/multimedia/lroimages/lola-20100319-maurius.html. Retrieved 13 December 2010.
- ^ "Marius Hills, Moon". Lunar and Planetary Institute. http://www.lpi.usra.edu/publications/slidesets/hawaiivolcanoes/slidespages/slide_11.html. Retrieved 13 December 2010.
- ^ a b Greeley, Ronald (1971). "Lava Tubes and Channels in the Lunar Marius Hills". Earth, Moon, and Planets 3 (3): 289–314. Bibcode 1971Moon....3..289G. doi:10.1007/BF00561842. http://www.springerlink.com/content/v50634825un8561l/. Retrieved 13 December 2010.
- ^ "Oblique view of the Marius Hills and Oceanus Procellarum on the Moon". The Moon - Lunar Orbiter 2. National Aeronautics and Space Administration. http://nssdc.gsfc.nasa.gov/imgcat/html/object_page/lo2_m213.html. Retrieved 13 December 2010.
- ^ a b LROC Observations of the Marius Hills. http://meteorites.wustl.edu/abstracts/lpsc41/a_l10r01.pdf. Retrieved 13 December 2010.
- ^ "Marius Hills Pit - Lava Tube Skylight?". Lunar Reconnaissance Orbiter Camera. Arizona State University. http://lroc.sese.asu.edu/news/index.php?/archives/184-Marius-Hills-Pit-Lava-Tube-Skylight.html. Retrieved 13 December 2010.
- ^ "Lunar Orbiter: Prospective Apollo Landing Sites". Lunar and Planetary Institute. http://www.lpi.usra.edu/expmoon/orbiter/orbiter-sites.html. Retrieved 18 June 2011.
- ^ "The Marius Hills pit is a possible skylight". Photojournal. Jet Propulsion Laboratory. http://photojournal.jpl.nasa.gov/catalog/PIA12954. Retrieved 28 June 2011.
- ^ "Marius Hills Flyover". Lunar and Planetary Institute. http://www.lpi.usra.edu/lunar/lunar_flyovers/marius_hills/. Retrieved 28 June 2011.
Categories:- Geological features on the Moon
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