Another suggested terrestrial analog for Tharsis Tholus is the Maderas Volcano in Nicaragua.[d]. Maciejak, F.; Lenat J.-F.; Provost, A. • (480) 727-7956 (Fax) Its origin is still debatable and there are four main models proposed: fluvial action, volcanic flows, valley being a lava channel or some combination of previously mentioned models. Listed Patera elevation is the average elevation of the shallow dish-shaped depression (the actual 'patera') at the summit. A; A; A; A; Language: Mobile Apps: apple; android; For surfers: Free toolbar & extensions; Word of the Day; Help; For webmasters: Free content; Linking; Lookup box; Close. The scale bar is 1000 meters long. Tharsis Tholus is an intermediate-sized shield volcano located in the eastern Tharsis region of the planet Mars. In planetary geology, a Tholus (pl. A large debris avalanche deposit (DAD) is present at the northwestern edge of the western block. Top is a three-dimensional oblique view of the summit caldera of Albor Tholus, a volcano in the Elysium region. The edifice has been modified by at least four distinct episodes of structural deformation. It was named after Russian astronomer Matvey Gusev (1826–1866) in 1976.. Tholus. Thus, Tharsis Tholus may be the result of two volcanoes growing together, with the main one taking up the northern two thirds of the structure. Arsia Mons, the southernmost of the group, has a large summit caldera that is 130 kilometres (81 mi) across and 1.3 kilometres (0.81 mi) deep. 1,410 people follow this. Listed mons elevation is the highest point (at 16 pixels/degree) within the feature. Ceraunius Tholus Na Galipedia, a Wikipedia en galego. References ↑ CHARACTERISTICS OF VALLEYS ON CERAUNIUS THOLUS AND THEIR FORMATION: PART I. Caleb I. Fassett and James W. Head, Dept. Structuris concamerationalibus ex variis rebus factis est historia longissima, cuius memoria ex praehistoria ad tempora nostra venit. Click on image to see dark slope streaks. The volcano was discovered by the Mariner 9 spacecraft in 1972 and originally given the informal name Volcano 7. The DAD appears to be made up of coherent slabs of flank material originating from the down-dropped western flank. Mapping Mars. Wikipedia Encyclopedia; Tools. Albor Tholus je vyhaslá sopka v oblasti Elysium Plantitia na Marsu. Mars in all its glory Answers: 1) mons 2) valles 3) tholus 4) chasma 5) Valles Marineris. Geology of Tharsis Tholus, Mars.  A third, barely visible, caldera is present on the volcano's southern flank. Top is a three-dimensional oblique view of the summit caldera of Albor Tholus, a volcano in the Elysium region. Tharsis Tholus lies on the eastern edge of the Tharsis quadrangle at 13.5°N, 91°W. Venus is classified as a terrestrial planet and it is sometimes called Earth's "sister planet" owing to their similar size, gravity, and bulk composition (Venus is both the closest planet to Earth and the planet closest in size to Earth).  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. tholus Also found in: Dictionary, Wikipedia. Ceraunius Tholus and Uranius Tholus in 3D ESA209220.jpg 1,280 × 770; 399 KB. (1995). It measures approximately 34 kilometers in diameter and was named after Jürgen Rahe, a German-American astronomer and NASA science program director. Volcanic Spreading Induces Flank Collapse at Mauna Loa. From Wikipedia, the free encyclopedia 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. tholus (thoh -lŭs) (plural: tholi) a hill or dome on the surface of a planet or satellite. Along with Ulysses Tholus, it is almost midway between Olympus Mons and the Tharsis Montes. In 1973, the International Astronomical Union (IAU) officially designated it Tharsis … [a] Earlier interpretations suggested that it is a stratovolcano. Robinson, M. (1993) PhD dissertation. Robinson, M. (1993) PhD dissertation cited by Plescia (2003), p. 236. Norton, O. Wikipedia: Instance of: tholus, shield volcano: Located on astronomical location: Mars: Location: Tharsis quadrangle : Diameter: 149 km ; Elevation above sea level: 8,500 ±500 m; 13° 15′ 00″ N, 90° 41′ 24″ W: Authority control Q1548991 BabelNet ID: 01422027n.  It is distinctly bulbous in appearance, and is unique among Martian volcanoes in the degree to which it has been modified by faulting. Landslide debris from the caldera's western and southeastern wall is present on the floor of the caldera. The summit crater of Ceraunius Tholus is just to the right of this picture.  The volcano rises to an elevation of about 9 km (5.6 mi). USGS. The summit crater of Ceraunius Tholus is just to the right of this picture. It is 130 kilometres (81 mi) across, approximately 8,500 metres (27,887 ft) high and is named after a classical albedo feature name. Some researchers have compared the deformation on the flanks of Tharsis Tholus to "sector collapse" observed at Mauna Loa in Hawaii and other terrestrial volcanoes. 16 Aug 2019 The Tharsis quadrangle spans the northern half of the highest region on the surface of Mars. Most of the volcano's surface is mantled with a thick layer of fine dust or ash, giving the volcano's flanks a smooth to slightly hummocky appearance. Biblis Tholus is an extinct Martian volcano located at 2.55°N 235.62°E, one of two volcanoes near the center of the Tharsis volcanism.  The volcano has an elongated central caldera (collapse crater) measuring 36.7 × 38.9 km and about 3 km deep. Gusev is a crater on the planet Mars and is located at and is in the Aeolis quadrangleThe crater is about 166 kilometers in diameter and formed approximately three to four billion years ago. Tholus, en tant que contractant général s’est entouré d’experts dans chaque corps de métiers afin de... See More. Click on image to see dark slope streaks. Uranius Tholus is a volcano on Mars located in the Tharsis quadrangle at 26.52° north latitude and 262.43° east longitude. Characteristics of valleys on Ceraunius Tholus and their formation: Part I. Caleb I. Fassett and James W. Head, Dept. 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