Difference between revisions of "Arsia Mons"
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− | [[Image:Valentine Cave.JPG|thumb|280px|Valentine Cave in | + | [[Image:Valentine Cave.JPG|thumb|280px|Valentine Cave in Lava Beds National Monument, California. This shows the classic tube shape; the grooves on the wall mark former flow levels. Pits near volcanic regions of Mars may be openings to caves like this.]] |
===References:=== | ===References:=== |
Revision as of 15:28, 8 February 2019
Arsia Mons is an extinct shield volcano in the Tharsis region near the equator. It is part of the Tharsis Montes group of volcanos. Its location is 8.35 S and 120.09 W (239.91 E) in the Phoenicis Lacus quadrangle. Its name is a classical feature name and comes from a corresponding albedo feature on a map by Giovanni Schiaparelli, which he named in turn after the legendary Roman forest of Arsia Silva.[1] Researchers have found much evidence for glaciers on Arsia Mons.[2] [3]
Caves
Seven cave entrances have been discovered on the sides of Arsia Mons. These caves could contain reserves of water ice or even life. They are possible locations for a cave settlement. With the low gravity of Mars, lava tubes may be over 800 feet in width. A lava tube on Mars could protect colonists from meteorites and radiation. Because of the lack of a magnetic field at present, Mars has a fair amount of radiation, especially from cosmic ray sources.[4] A mini-series produced by National Geographic in 2016 depicted how people could establish a base in a cave.[5] [6]
Clouds
Repeated Clouds over Arsia Mons [7] there is some debate about the nature of the clouds whether they are dust particles or water vapor [8] If this is in fact Water Vapor, that indicates the presence of Water Ice around Arsia Mons. [9] [10]
References:
- ↑ https://planetarynames.wr.usgs.gov/Page/MARS/target
- ↑ Scanlon, K., J. Head, D. Marchant. 2015. REMNANT BURIED ICE IN THE ARSIA MONS FAN-SHAPED DEPOSIT, MARS. 46th Lunar and Planetary Science Conference. 2266.pdf
- ↑ "Recent glaciation at high elevations on Arsia Mons, Mars: Implications for the formation and evolution of large tropical mountain glaciers" (PDF) (2007). Journal of Geophysical Research 112 (E3). doi: .
- ↑ https://www.sciencedaily.com/releases/2017/09/170925112842.htm
- ↑ https://www.nationalgeographic.org/education/mars
- ↑ https://www.leonarddavid.com/underground-caves-on-moon-mars-protected-habitats-for-explorers/
- ↑ Jet Propulshion Lab, California Institute of Technology Repeated Clouds over Arsia Mons , https://www.jpl.nasa.gov/spaceimages/details.php?id=PIA04294
- ↑ THEMIS: Ice-rich clouds over Arsia Mons’ caldera, ASU, R Burnham THEMIS: Ice-rich clouds over Arsia Mons’ caldera , http://redplanet.asu.edu/?p=30885, Sep 2018.
- ↑ 43rd Lunar and Planetary Science Conference, USRA - Universities Space Research Association VOLCANO-ICE INTERACTIONS RECORDED IN THE ARSIA MONS FAN-SHAPED GLACIAL DEPOSITS , https://www.lpi.usra.edu/meetings/lpsc2012/pdf/2183.pdf, 2012.
- ↑ LAPL HIRISE, Kelly Kolb, University of Arizona Glacier-Like Flow on Arsia Mons Flank , https://www.uahirise.org/PSP_002922_1725, 4 April 2007.
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