Orcus Patera

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Elevation map centered on Orcus Patera. MOLA elevation map from the Mars Global Surveyor Mars orbiter MOLA orcus patera.jpg
Elevation map centered on Orcus Patera. MOLA elevation map from the Mars Global Surveyor Mars orbiter

Orcus Patera is a region on the surface of the planet Mars first photographed by Mariner 4. Of unknown formation, whether by volcanic, tectonic, or cratering causes, the region includes a depression about 380 kilometres (240 miles) long, 140 kilometres (87 miles) wide, surrounded by a rim up to 1.8 kilometres (1 mile) high.

Contents

Description

Orcus Patera was first imaged by Mariner 4. [1] It is a depression about 380 kilometres (240 miles) long, 140 kilometres (87 miles) wide, and about 0.5 kilometres (13 mile) deep but with a relatively smooth floor. [2] It has a rim up to 1.8 kilometres (1 mile) high. [2]

It has experienced aeolian processes, and has some small craters and graben structures. [2] However, it is not known how the patera originally formed. [2] Theories include volcanic, tectonic, or cratering events. [2] A study in 2000 that incorporated new results from Mars Global Surveyor along with older Viking data, did not come out clearly in favor of either volcanic or cratering processes. [3]

Mars Express observed this region in 2005, yielding a digital terrain model and color pictures. [2]

Images

Viking

OrcusPatera zoom.jpg
Orcus Patera by a Viking Orbiter. Orcus Patera is the elongated crater in the center. This is in the Elysium Planitia region. [4]

Mars Express

Orcus Patera by HRSC.jpg
Mars Express HRSC natural color image of Orcus Patera
Elevation of Orcus Patera and surroundings.jpg
Mars Express HRSC topographic view of Orcus Patera with colors coding for elevation

Location

Orcus Patera is west of Olympus Mons and east of Elysium Mons. [2] It is about halfway between those two volcanoes, and east and north of Gale crater.

Elysium Planitia topo.jpg
In this labeled elevation map (color corresponds to elevation in this view of Elysium Planitia), the location of Orcus Patera can be identified in upper right. Gale crater, where the Curiosity Mars rover landed in 2012 is in the lower left, and InSight landed north of Gale in 2018.
Orcus Patera in a wide view of Elysium Planitia quadrangle USGS-Mars-MC-15-ElysiumRegion-mola.png
Orcus Patera in a wide view of Elysium Planitia quadrangle

See also

Related Research Articles

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Ceraunius Fossae Set of fractures in the northern Tharsis region of Mars

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Ulysses Tholus Martian volcano

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Endeavour (crater)

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Hesperia Planum Broad lava plain in the southern highlands of the planet Mars

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Elysium Planitia Broad plain that straddles the equator of Mars

Elysium Planitia, located in the Elysium and Aeolis quadrangles, is a broad plain that straddles the equator of Mars, centered at 3.0°N 154.7°E. It lies to the south of the volcanic province of Elysium, the second largest volcanic region on the planet, after Tharsis. Elysium contains the major volcanoes Elysium Mons, Albor Tholus and Hecates Tholus. Another more ancient shield volcano, Apollinaris Mons, is situated just to the south of eastern Elysium Planitia. Within the plains, Cerberus Fossae is the only Mars location with recent volcanic eruptions. Lava flows dated no older than 0.2 million years from the present have been found, and evidence has been found that volcanic activity may have occurred as recently as 53,000 years ago. Such activity could have provided the environment, in terms of energy and chemicals, needed to support life forms.

Eden Patera

Eden Patera is a feature located in the Mare Acidalium quadrangle on the planet Mars. In October 2013 the feature gained some attention when it was speculated it may be a supervolcano rather than an impact crater, according to research from the Planetary Science Institute in Tucson, led by Joseph R. Michalski. The research postulated the crater was formed by the volcano's caldera collapsing, rather than from an impact. Some of reasons for suspecting that Eden Patera is a collapsed caldera not an impact crater are its irregular shape, an apparent lack of a raised rim or central peak, and lack of impact ejecta.

Irnini Mons Mons on Venus

Irnini Mons is a volcanic structure on the planet Venus, and is named after the Assyro-Babylonian goddess of cedar-tree mountains. It has a diameter of 475 km (295 mi), a height of 1.75 km (1.09 mi), and is located in Venus' northern hemisphere. More specifically, it is located in the central Eistla Regio region at in the V-20 quadrangle. Sappho Patera, a 225 km (140 mi) diameter wide, caldera-like, depression tops the summit of Irnini Mons. The primary structural features surrounding Irnini Mons are graben, seen as linear depressed sections of rock, radiating from the central magma chamber. Also, concentric, circular ridges and graben outline the Sappho Patera depression at the summit. The volcano is crossed by various rift zones, including the north-south trending Badb Linea rift, the Guor Linea rift extending to the northwest, and the Virtus Linea rift continuing to the southeast.

Patera (planetary nomenclature)

Patera is an irregular crater, or a complex crater with scalloped edges on a celestial body. Paterae can have any origin, although majority of them were created by volcanism. The term comes from Latin language, where it refers to a shallow bowl used in antique culture.

References

  1. Williams, Dave; Friedlander, Jay. "The Orcus Patera region on Mars". Mars - Mariner 4. NASA . Retrieved December 20, 2015.
  2. 1 2 3 4 5 6 7 "HRSC Press Release #471 - Orcus Patera (orbit 2216 & 2238)". 2010-08-27. Archived from the original on 2014-08-07.
  3. Orcus Patera : Impact Crater or Volcanic Caldera? (2000)
  4. "Catalog Page for PIA00175".