The rover Curiosity landed on August 6, 2012 near the base of Aeolis Mons (or "Mount Sharp").
|Location||Gale Crater on Mars|
|Peak||Aeolis Mons - 5.5 km (18,000 ft) high|
|Discoverer||NASA in the 1970s|
|Eponym||Aeolis Mons - Aeolis albedo feature
Mount Sharp - Robert P. Sharp (1911-2004)
Gale Crater Mound - Gale Crater
Aeolis Mons (IPA: [ˈiːəlɨs ˈmɒnz]), also unofficially known as Mount Sharp, is a mountain on Mars. It forms the central peak within Gale Crater and is located around , rising 5.5 km (18,000 ft) high from the valley floor. It is feature ID 15000.
Curiosity (the Mars Science Laboratory rover) landed in "Yellowknife" Quad 51 of Aeolis Palus, next to the mountain, on August 6, 2012. NASA named the landing site Bradbury Landing on August 22, 2012. Aeolis Mons is a primary goal for scientific study. On June 5, 2013, NASA announced that Curiosity will soon begin a 8 km (5.0 mi) journey from the Glenelg area to the base of Aeolis Mons. On November 13, 2013, NASA announced that an entryway Curiosity will traverse on its way to Aeolis Mons will be named "Murray Buttes", in honor of planetary scientist Bruce C. Murray (1931-2013). The trip is expected to take nine months to a year with stops along the way to study the local terrain.
The mountain appears to be an enormous mound of eroded sedimentary layers sitting on the central peak of Gale. It rises 5.5 km (18,000 ft) above the northern crater floor and 4.5 km (15,000 ft) above the southern crater floor, higher than the southern crater rim. The sediments may have been laid down over an interval of 2 billion years, and may have once completely filled the crater. Some of the lower sediment layers may have originally been deposited on a lake bed, while observations of possibly cross-bedded strata in the upper mound suggest aeolian processes. However, this issue is debated, and the origin of the lower layers remains unclear. If katabatic wind deposition played the predominant role in the emplacement of the sediments, as suggested by reported 3 degree radial slopes of the mound's layers, erosion would have come into play largely to place an upper limit on the mound's growth.
Mount Everest rises to 8.8 km (29,000 ft) altitude above sea level but is only 4.6 km (15,000 ft) (base-to-peak). Africa's Mount Kilimanjaro is about 5.9 km (19,000 ft) altitude above sea level to the Uhuru peak; also 4.6 km base-to-peak. America's Mt. McKinley, also known as Denali, has a base-to-peak of 5.5 km (18,000 ft). Italy's Monte Bianco is 4.8 km (16,000 ft) in altitude above sea level, Mount Fuji (富士山), which overlooks Tokyo, Japan is about 3.8 km (12,000 ft) altitude. Compared to the Andes, Aeolis Mons would rank outside the hundred tallest peaks, being roughly the same height as Argentina's Cerro Pajonal; the peak is higher than any above sea level in Oceania above sea level, but base-to peak it is considerably shorter than Hawaii's Mauna Kea and its neighbors.
Discovered in the 1970s, the mountain remained nameless for perhaps 40 years. When it became a likely landing site, it was given various labels; for example, in 2010 a NASA photo caption called it "Gale crater mound". In March 2012, NASA unofficially named it "Mount Sharp", for American geologist Robert P. Sharp.
The International Astronomical Union, which is responsible for planetary nomenclature for its participants, names large Martian mountains after the Classical albedo feature in which it is located, not for people. In May 2012 the IAU thus named the mountain Aeolis Mons, and gave the name Aeolis Palus to the crater floor plain between the northern wall of Gale Crater and the northern foothills of the mountain. In recognition of NASA and in honour of Sharp, the IAU gave the name "Robert Sharp" to a large crater (150 km (93 mi) in diameter), located about 260 km (160 mi) west of Gale Crater, following its standard practice of naming large craters after scientists.
NASA and the ESA continue to refer to the mountain as "Mount Sharp" in press conferences and press releases. This is similar to other informal names, such as the Columbia Hills near one of the Mars Exploration Rover landing sites. Sky & Telescope explained the rationales of the two names to their readers in August 2012, and held an informal poll to newsletter readers. Over 2700 voted and picked Aeolis Mons over Mount Sharp by 57% to 43%. The official name, Aeolis mons, is recorded by the United States Geological Survey.
Aeolis Mons may have formed from the erosion of sediment layers that once filled Gale Crater.
Curiosity's landing site (green dot) - blue dot marks Glenelg Intrigue - blue spot marks the base of Mount Sharp - a planned area of study.
Comparison of color versions (raw, natural, white balance) of Aeolis Mons (August 23, 2012).
Aeolis Mons as viewed by Curiosity (August 8, 2012) (white balanced image).
Layers at the base of Aeolis Mons - dark rock in inset is same size as Curiosity (white balanced image).
"Murray Buttes" - steep knobs Curiosity will pass on its way to Aeolis Mons (November 13, 2013).
- Aeolis quadrangle/Gale Crater
- Composition of Mars
- Geology of Mars
- List of craters on Mars
- List of mountains on Mars
- List of mountains on Mars by height
- List of rocks on Mars
- List of tallest mountains in the Solar System
- ""Mount Sharp" on Mars Compared to Three Big Mountains on Earth". NASA. 27 March 2012. Retrieved 31 March 2012.
- Aeolis Mons
- NASA Staff (August 10, 2012). "Curiosity's Quad - IMAGE". NASA. Retrieved August 11, 2012.
- Agle, DC; Webster, Guy; Brown, Dwayne (August 9, 2012). "NASA's Curiosity Beams Back a Color 360 of Gale Crate". NASA. Retrieved August 11, 2012.
- Amos, Jonathan (August 9, 2012). "Mars rover makes first colour panorama". BBC News. Retrieved August 9, 2012.
- Halvorson, Todd (August 9, 2012). "Quad 51: Name of Mars base evokes rich parallels on Earth". USA Today. Retrieved August 12, 2012.
- NASA Staff (6AUG2012). "NASA Lands Car-Size Rover Beside Martian Mountain". NASA. Retrieved 6AUG2012-1.
- Brown, Dwayne; Cole, Steve; Webster, Guy; Agle, D.C. (August 22, 2012). "NASA Mars Rover Begins Driving at Bradbury Landing". NASA. Retrieved August 22, 2012.
- NASA Staff (6 August 2012). "NASA Lands Car-Size Rover Beside Martian Mountain". NASA/JPL. Retrieved 2012-08-07.
- Webster, Guy; Brown, Dwayne (November 13, 2013). "Mars Rover Teams Dub Sites In Memory of Bruce Murray". NASA. Retrieved November 14, 2013.
- Staff (June 5, 2013). "From 'Glenelg' to Mount Sharp". NASA. Retrieved June 6, 2013.
- Chang, Alicia (June 5, 2013). "Curiosity rover to head toward Mars mountain soon". AP News. Retrieved June 7, 2013.
- Chang, Kenneth (June 7, 2013). "Martian Rock Another Clue to a Once Water-Rich Planet". New York Times. Retrieved June 7, 2013.
- "Gale Crater's History Book". Mars Odyssey THEMIS web site. Arizona State University. Retrieved 2012-12-07.
- Anderson, R. B.; Bell III, J. F. (2010). "Geologic mapping and characterization of Gale Crater and implications for its potential as a Mars Science Laboratory landing site". International Journal of Mars Science and Exploration 5: 76–128. Bibcode:2010IJMSE...5...76A. doi:10.1555/mars.2010.0004.
- Cabrol, N. A.; et al. (1999). "Hydrogeologic evolution of Gale Crater and its relevance in the exobiological exploration of Mars". Icarus 139 (2): 235–245. Bibcode:1999Icar..139..235C. doi:10.1006/icar.1999.6099.
- Irwin, R. P.; Howard, A. D.; Craddock, R. A.; Moore, J. M. (2005). "An intense terminal epoch of widespread fluvial activity on early Mars: 2. Increased runoff and paleolake development". Journal of Geophysical Research 110: E12S15. Bibcode:2005JGRE..11012S15I. doi:10.1029/2005JE002460.
- Wall, M. (2013-05-06). "Bizarre Mars Mountain Possibly Built by Wind, Not Water". Space.com. Retrieved 2013-05-13.
- Kite, E. S.; Lewis, K. W.; Lamb, M. P.; Newman, C. E.; Richardson, M. I. (2013). "Growth and form of the mound in Gale Crater, Mars: Slope wind enhanced erosion and transport". Geology 41 (5): 543–546. doi:10.1130/G33909.1. ISSN 0091-7613.
- Fred W. Price (1988). The Moon observer's handbook. London: Cambridge University Press. ISBN 0-521-33500-0.
- Mount Everest (1:50,000 scale map), prepared under the direction of Bradford Washburn for the Boston Museum of Science, the Swiss Foundation for Alpine Research, and the National Geographic Society, 1991, ISBN 3-85515-105-9
- "Kilimajaro Guide—Kilimanjaro 2010 Precise Height Measurement Expedition". Retrieved 16 May 2009.
- S. Green - Kilimanjaro: Highest Mountain in Africa - About.com
- Adam Helman, 2005. The Finest Peaks : Prominence and Other Mountain Measures, p. 9: "the base to peak rise of Mount McKinley is the largest of any mountain that lies entirely above sea level, some 18000 feet"
- Sumitpostorg - Zugspitze
- "Mont Blanc shrinks by 45cm in two years". Sydney Morning Herald. November 6, 2009.
- NASA - Layers in Lower Formation of Gale Crater Mound
- "Mount Sharp or Aeolis Mons?". Sky & Telescope. 2012-08-14. Retrieved 2012-08-18.
- Space.com staff (29 March 2012). "NASA's New Mars Rover Will Explore Towering "Mount Sharp"". Space.com. Retrieved 30 March 2012.
- Blue, J. (16 May 2012). "Three New Names Approved for Features on Mars". US Geological Survey. Retrieved 28 May 2012.
- Agle, D. C. (28 March 2012). "'Mount Sharp' On Mars Links Geology's Past and Future". NASA. Retrieved 31 March 2012.
- ESA - Mars Express marks the spot for Curiosity landing
- Mars Science Laboratory: Multimedia-Images
- Jürgen Blunck - Mars and its Satellites, A Detailed Commentary on the Nomenclature, 2nd edition. 1982.
|Look up Aeolis Mons in Wiktionary, the free dictionary.|
|Wikimedia Commons has media related to Aeolis Mons.|
- Google Mars scrollable map - centered on Aeolis Mons.
- Aeolis Mons - Curiosity Rover "StreetView" (Sol 2 - 08/08/2012) - NASA/JPL - 360º Panorama
- Aeolis Mons - Curiosity Rover Mission Summary - Video (02:37)
- Aeolis Mons - HiRise (South side of mountain)
- Aeolis Mons - "Mount Sharp" Oblique (19,663px × 1,452px)
- Aeolis Mons - Gale Crater - Image/THEMIS VIS 18m/px Mosaic (Zoomable) (small)
- Aeolis Mons - Gale Crater - Image/HRSCview
- Aeolis Mons - HRSCview (oblique view looking east)
- Aeolis Mons - 7,703px × 2,253px black & white panorama
- Aeolis Mons - Color Panorama by Damien Bouic
- Images - PIA16105 PIA16104
- Video (04:32) - Evidence: Water "Vigorously" Flowed On Mars - September, 2012