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List Of Mountains On Mars
This is a list of all named mountains on Mars. Most mountains have a name including one of the following elements: * ''Mons'': a large, isolated, mountain. * ''Montes'', plural of ''mons'': a mountain range. * ''Tholus'': a small dome-shaped mountain. * ''Tholi'', plural of ''tholus'': a group of (usually not contiguous) small mountains. * ''Dorsa'', plural of '' dorsum'': a long low range. Not included. See also * List of craters on Mars * List of mountains on Mars by height * List of tallest mountains in the Solar System * Mineralogy of Mars References External links Mars features database distributed with xephem v3.3(Warning, it uses West coordinates, and table should be in East coordinates) IAU, USGS: Martian system nomenclatureIAU, USGS: Mars nomenclature: mountains (planetocentric east longitude)IAU, USGS: Mars nomenclature: tholus (planetocentric east longitude)Peter Grego, Mars and how to Observe it(List of elevations of named Martian mountains) {{DEFAULTSORT:Lis ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Mars
Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, only being larger than Mercury. In the English language, Mars is named for the Roman god of war. Mars is a terrestrial planet with a thin atmosphere (less than 1% that of Earth's), and has a crust primarily composed of elements similar to Earth's crust, as well as a core made of iron and nickel. Mars has surface features such as impact craters, valleys, dunes and polar ice caps. It has two small and irregularly shaped moons, Phobos and Deimos. Some of the most notable surface features on Mars include Olympus Mons, the largest volcano and highest known mountain in the Solar System and Valles Marineris, one of the largest canyons in the Solar System. The Borealis basin in the Northern Hemisphere covers approximately 40% of the planet and may be a large impact feature. Days and seasons on Mars are comparable to those of Earth, as the planets have a similar rotation period ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Arsia Mons
Arsia Mons is the southernmost of three volcanoes (collectively known as Tharsis Montes) on the Tharsis bulge near the equator of the planet Mars. To its north is Pavonis Mons, and north of that is Ascraeus Mons. The tallest volcano in the Solar System, Olympus Mons, is to its northwest. Its name 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. Structure Arsia Mons is a shield volcano with a relatively low slope and a massive caldera at its summit. The southernmost of the three Tharsis Montes volcanoes, it is the only major Tharsis volcano south of the equator. The volcano is in diameter, almost high (more than higher than the surrounding plains), and the summit caldera is 110 km (72 miles) wide. It experiences atmospheric pressure lower than 107 pascals [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Echus Montes
Echus Montes is a large mountain on Mars at . It is located in the Lunae Palus quadrangle The Lunae Palus quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The quadrangle is also referred to as MC-10 (Mars Chart-10). Lunae Planum and parts o .... File:Echus Montes1.jpg, Echus Montes, as seen by CTX. References Mountains on Mars Lunae Palus quadrangle {{Mars-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Coronae Montes
''Coronae Montes'' is a mountain on the planet Mars. The name ''Coronae Montes''is a classical albedo name. It has a diameter of . This was approved by International Astronomical Union in 1991. See also * List of mountains on Mars This is a list of all named mountains on Mars. Most mountains have a name including one of the following elements: * ''Mons'': a large, isolated, mountain. * ''Montes'', plural of ''mons'': a mountain range. * ''Tholus'': a small dome-shaped mount ... References External links Gazetteer of Planetary Nomenclature Mountains on Mars Hellas quadrangle {{mars-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Coprates Montes
The Dez River ( fa, دز), the ancient Coprates (;James Knowles (1835) ''A Pronouncing and Explanatory Dictionary of the English Language'' el, Κοπράτης or Κοπράτας), is a tributary of the Karun River and is 400 km long. It is the site of the Dez Dam ) , image = , image_size = , image_caption = , image_alt = , location_map = Iran , location_map_size = , location_map_caption = , coordinates = , country = I .... References Rivers of Khuzestan Province Landforms of Khuzestan Province {{Iran-river-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Chronius Mons
Chronius Mons is a shield volcano located on Eridania quadrangle of the planet Mars. The name ''Chronius Mons'' is a classical albedo name. This was approved by International Astronomical Union The International Astronomical Union (IAU; french: link=yes, Union astronomique internationale, UAI) is a nongovernmental organisation with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreac ... on September 13, 2006. References Eridania quadrangle Volcanoes of Mars Shield volcanoes {{mars-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Charitum Montes
Charitum Montes is a large group of mountains in the Argyre quadrangle of Mars, located at 58.4° south latitude and 40.29° west longitude. It is 850 km across and was named after a classical albedo feature name. Charitum Montes has gullies A gully is a landform created by running water, mass movement, or commonly a combination of both eroding sharply into soil or other relatively erodible material, typically on a hillside or in river floodplains or terraces. Gullies resemble lar ... in some areas. References External links''Charitum Montes: a cratered winter wonderland''- ESA {{Portal bar, Solar System Argyre quadrangle Mountains on Mars ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Chalce Montes
Chalce Montes is a mountain range on the planet Mars. The name refers to the Martian albedo feature ''Chalce'', that was named after the Greek island Chalki. It has a diameter of ; its elevation is . See also * List of mountains on Mars This is a list of all named mountains on Mars. Most mountains have a name including one of the following elements: * ''Mons'': a large, isolated, mountain. * ''Montes'', plural of ''mons'': a mountain range. * ''Tholus'': a small dome-shaped mount ... References Mountain ranges on Mars {{mars-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Cerberus Tholi
In Greek mythology, Cerberus (; grc-gre, Κέρβερος ''Kérberos'' ), often referred to as the hound of Hades, is a multi-headed dog that guards the gates of the Underworld to prevent the dead from leaving. He was the offspring of the monsters Echidna and Typhon, and was usually described as having three heads, a serpent for a tail, and snakes protruding from multiple parts of his body. Cerberus is primarily known for his capture by Heracles, the last of Heracles' twelve labours. Descriptions Descriptions of Cerberus vary, including the number of his heads. Cerberus was usually three-headed, though not always. Cerberus had several multi-headed relatives. His father was the multi snake-headed Typhon, and Cerberus was the brother of three other multi-headed monsters, the multi-snake-headed Lernaean Hydra; Orthrus, the two-headed dog who guarded the Cattle of Geryon; and the Chimera, who had three heads: that of a lion, a goat, and a snake. And, like these close relative ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Ceraunius Tholus
Ceraunius Tholus is a volcano on Mars located in the Tharsis quadrangle at 24.25° north latitude and 262.75° east longitude, part of the Uranius group of volcanoes. It is across, approximately high and is named after a classical albedo feature name. It is generally believed to be a basaltic shield with the lower part buried beneath plain forming lavas. Earlier interpretations suggested that it is a stratovolcano. The slopes on Ceraunius Tholus are quite steep with an average slope of 8° with many radial erosion channels and pitted valleys extending from just below the rim of the caldera toward the base of the volcano. The current view is that the valleys were eroded by water. Interesting features on Ceraunius Tholus are three large canyons at the northwest flank of Ceraunius Tholus which are up to 2.5 km wide and 300 m deep. The biggest of these three also appears to be the youngest and protrude from the lowest point of the volcanic caldera and ends at the interesting ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Centauri Montes
Centauri Montes is a group of mountains in the Hellas quadrangle The Hellas quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Hellas quadrangle is also referred to as MC-28 (Mars Chart-28). The Hellas quadrangle c ... of Mars, located at . It is 270 km across and was named after the albedo feature Centauri Lacus. According to NASA, there are light-sediment gulley deposits that have formed in a crater around the Centauri Montes. References Hellas quadrangle Mountains on Mars {{Mars-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Biblis Tholus
Biblis Tholus is an extinct Martian volcano located at , one of two volcanoes near the center of the Tharsis volcanism. Along with Ulysses Tholus, it is almost midway between Olympus Mons and the Tharsis Montes. Biblis Tholus lies in the Tharsis quadrangle. It is approximately long and wide, rising about from its surroundings. In the middle of the volcano is a caldera, named Biblis Patera, believed to have formed as the result of collapse of the magma chamber during eruptions of the volcano. The caldera is in diameter and four kilometers (2.5 miles) in depth. Image:Biblis Patera - topography map.png, Topography and location in Tharsis using MOLA data set. Image:Biblis Patera from Mars Odyssey.JPG, Close-up of Biblis Patera taken with Mars Odyssey. Rim of crater shows multiple episodes of collapse. Image:Ulysses Patera.JPG, Nearby Ulysses Tholus, showing its location in relation to other volcanoes (photo by THEMIS). Image:Biblis Patera Pedestal Crater.JPG, Biblis Pa ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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