Bahram Vallis
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Bahram Vallis
Bahram Vallis is an ancient river valley in the Lunae Palus quadrangle of Mars at 20.7° north latitude and 57.5° west longitude. It is about 302 km long and was named after the word for 'Mars' in Persian. Bahram Vallis is located midway between Vedra Valles and lower Kasei Valles. It is basically a single trunk valley, with scalloped walls in some places. The presence of streamlined erosional features on its floor shows that fluid was involved with its formation.Baker, V. 1982. The Channels of Mars. University of Texas Press. Austin Image:Kasei Valles topolabled.JPG, Area around Northern Kasei Valles, showing relationships among Kasei Valles, Bahram Vallis, Vedra Valles, Maumee Valles, and Maja Valles. Map location is in Lunae Palus quadrangle and includes parts of Lunae Planum and Chryse Planitia. Image:Bahram Vallis.JPG, Bahram Vallis, as seen by HiRISE. Rotational landslides (slumps) are visible at the base of north wall. File:ESP 056904 2015valley.jpg, Close ...
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Bahram Vallis Based On Day THEMIS
Bahrām ( fa, بهرام) is a male given name. Other variants Behram, Bahran, Vahran, and Vahram ( uz, Баҳром, Bahrom and Tajik: Баҳром, Bahrom) The older form is Vahrām ( pal, 𐭥𐭫𐭧𐭫𐭠𐭭, in la, Varrames), also spelled Wahrām, literally meaning "smiting of resistance" or "victorious". It is name of several prominent figures in pre-Islamic Persia. In the Pahlavi language (Middle Persian), Bahram is another name of the Zoroastrian divinity Verethragna in Avestan language, that is the hypostasis of victory and represents the planet Mars. Historic people * One of the Sassanid kings by that name: ** Bahrām I, ''r.'' 273-276 ** Bahrām II, ''r.'' 276-293 ** Bahrām III, ''r.'' 293 ** Ardashir II, ''r.'' 379–383, who also went by the name 'Ardashir Vahram' ** Bahrām IV, ''r.'' 388–399 ** Bahrām V Gōr, ''r.'' 421–438 (often known as Bahram Gur) ** Bahrām VI Čōbīn, ''r.'' 590-591 ** Bahram VII * Bahram Khan, 14th-century governor based ...
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THEMIS
In Greek mythology and Ancient Greek religion, religion, Themis (; grc, Θέμις, Themis, justice, law, custom) is one of the twelve Titans, Titan children of Gaia and Uranus (mythology), Uranus, and the second wife of Zeus. She is the goddess and personification of justice, divine order, fairness, law, and custom, and her symbols include the Scales of Justice (symbol), Scales of Justice. She is also associated with oracles and prophecies, including the Pythia, Oracle of Delphi. Name ''Themis'' means "divine law" rather than human ordinance, literally "that which is put in place", from the Greek verb ''títhēmi'' (wikt:τίθημι, τίθημι), meaning "to put." To the ancient Greeks she was originally the organizer of the "communal affairs of humans, particularly assemblies." Moses Finley remarked of ''themis'', as the word was used by Homer in the 8th century BCE, to evoke the social order of the 10th- and 9th-century Greek Dark Ages: Finley adds, "There was ''them ...
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Lunae Palus Map
Lunae was a short-lived Spanish pop group built upon the success of ''Operación Triunfo'' a reality show talent contest popular on Spain's TVE network. The band was composed by putting together singers that were not given the chance to pursue a solo career after the show, and was composed of Tessa (born 7 November 1982), Elena Gadel (born 11 November 1982) and Marey (born 19 December 1983) In the summer of 2003, their debut single ' Hipnotizadas' (produced by Xenomania) was a minor summertime hit across Spain, and it was used in a Pringles advertisement tie-in. In September, Lunae released their debut album, Olor a Nuevo. It included 13 tracks, with 3 in English. It also included a collaboration with Enrique Anaut, ''Operación Triunfo'' Season 2 fellow finalist. In January 2004, Lunae released their second single Viva Otra Vez. By March 2004, the band members were working on separate projects (Elena Gadel and Tessa moving on to musicals). However, they still were 'Lunae' at ...
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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 of Xanthe Terra and Chryse Planitia are found in the Lunae Palus quadrangle. The Lunae Palus quadrangle contains many ancient river valleys. The quadrangle covers the area from 45° to 90° west longitude and 0° to 30° north latitude on Mars. The ''Viking 1'' Lander (part of Viking program) landed in the quadrangle on July 20, 1976, at . It was the first robot spacecraft to successfully land on the Red Planet. Results from ''Viking I'' mission What would it look like walking around the landing site The sky would be a light pink. The dirt would also appear pink. Rocks of many sizes would be spread about. One large rock, named Big Joe, is as big as a banquet table. Some boulders would show erosion due to the wind. There would be ...
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Mars
Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, only being larger than Mercury (planet), Mercury. In the English language, Mars is named for the Mars (mythology), 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 (moon), Phobos and Deimos (moon), Deimos. Some of the most notable surface features on Mars include Olympus Mons, the largest volcano and List of tallest mountains in the Solar System, highest known mountain in the Solar System and Valles Marineris, one of the largest canyons in the Solar System. The North Polar Basin (Mars), Borealis basin in the Northern Hemisphere covers approximately 40% of the planet and may be a la ...
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Astrogeology Research Program
The Astrogeology Science Center is the entity within the United States Geological Survey concerned with the study of planetary geology and planetary cartography. It is housed in the Shoemaker Building in Flagstaff, Arizona. The Center was established in 1963 by Eugene Merle Shoemaker to provide lunar geologic mapping and to assist in training astronauts destined for the Moon as part of the Apollo program. Since its inception, the Astrogeology Science Center has participated in processing and analyzing data from various missions to the planetary bodies in the Solar System, assisting in finding potential landing sites for exploration vehicles, mapping our neighboring planets and their moons, and conducting research to better understand the origins, evolutions, and geologic processes operating on these bodies. The Early Days Gene Shoemaker founded the Astrogeology Research Program August 25, 1960. The research program started out as the ''Astrogeologic Studies Group'' at the Uni ...
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United States Geological Survey
The United States Geological Survey (USGS), formerly simply known as the Geological Survey, is a scientific agency of the United States government. The scientists of the USGS study the landscape of the United States, its natural resources, and the natural hazards that threaten it. The organization's work spans the disciplines of biology, geography, geology, and hydrology. The USGS is a fact-finding research organization with no regulatory responsibility. The agency was founded on March 3, 1879. The USGS is a bureau of the United States Department of the Interior; it is that department's sole scientific agency. The USGS employs approximately 8,670 people and is headquartered in Reston, Virginia. The USGS also has major offices near Lakewood, Colorado, at the Denver Federal Center, and Menlo Park, California. The current motto of the USGS, in use since August 1997, is "science for a changing world". The agency's previous slogan, adopted on the occasion of its hundredt ...
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Vedra Valles
The Vedra Valles are a set of channels in an ancient river valley in the Lunae Palus quadrangle of Mars, located at 19.4° N and 55.6° W. They are 115 km long and were named after an ancient river in Great Britain. Together with other ancient river valleys, they have provided strong evidence for a great deal of running water on the surface of Mars.Moore, P. et al. 1990. The Atlas of the Solar System. Mitchell Beazley Publishers NY, NY. Image:Kasei Valles topolabled.JPG, Area around the Northern Kasei Valles, showing relationships among Bahram Vallis and the Kasei Valles, Vedra Valles, Maumee Valles, and Maja Valles. Map location is in Lunae Palus quadrangle and includes parts of Lunae Planum and Chryse Planitia. Vallesmaumeevedrabox.jpg, Map showing relative positions of several channel systems in the Lunae Palus quadrangle, including the Vedra Valles, Maumee Valles, and Maja Valles. Box indicates their location; colors designate elevation. See also * Geology of Mars ...
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Kasei Valles
The Kasei Valles are a giant system of canyons in Mare Acidalium and Lunae Palus quadrangles on Mars, centered at 24.6° north latitude and 65.0° west longitude. They are long and were named for the word for "Mars" in Japanese. This is one of the largest outflow channel systems on Mars. Geography This huge system is 300 miles wide in some places. In contrast, Earth's Grand Canyon is only 18 miles wide. It is one of the longest continuous outflow channel systems on Mars. The Kasei Valles system begins in Echus Chasma, near Valles Marineris. It runs initially northward, then turns eastward and appears to empty into Chryse Planitia, not far from where Viking 1 landed. At around 20° north latitude the system splits into two channels, called Kasei Vallis Canyon and North Kasei Channel. These branches recombine at around 63° west longitude, forming a large island between the channels known as Sacra Mensa. Some parts of the Kasei Valles are 2–3 km deep. Like other ...
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Maumee Valles
The Maumee Valles are a set of channels in an ancient river valley in the Lunae Palus quadrangle of Mars, located at 19.7° N and 53.2° W. They are 350 km long and were named after a North American river in Indiana and Ohio. Together with other ancient river valleys, they have provided strong evidence for a great deal of running water on the surface of Mars.Moore, P. et al. 1990. The Atlas of the Solar System. Mitchell Beazley Publishers NY, NY. Image:Kasei Valles topolabled.JPG, Area around the Northern Kasei Valles, showing relationships among Bahram Vallis and the Kasei Valles, Vedra Valles, Maumee Valles, and Maja Valles. Map location is in Lunae Palus quadrangle and includes parts of Lunae Planum and Chryse Planitia. Vallesmaumeevedrabox.jpg, Map showing relative positions of several channel systems in Lunae Palus quadrangle, including the Vedra Valles, Maumee Valles, and Maja Valles. Box indicates where these valleys can be found. Colors show elevation. See also ...
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Maja Valles
The Maja Valles are a large system of ancient outflow channels in the Lunae Palus quadrangle on Mars. Their location is 12.6° north latitude and 58.3° west longitude. The name is a Nepali word for "Mars". The Maja Valles begin at Juventae Chasma. Parts of the system have been partially buried by thin volcanic debris. The channels end at Chryse Planitia. Huge outflow channels were found in many areas by the Viking Orbiters. They showed that floods of water broke through dams, carved deep valleys, eroded grooves into bedrock, and traveled thousands of kilometers. The Maja Valles show evidence of lava flows in the northern section. Studies with HiRISE and CTX images suggest that the lava flows did not reach the turbulence necessary to erode large channels. So, the Maja Valles are believed to be have formed through water erosion.Keske, A., P. Christensen. 2017. MAJA VALLES: A MULTI-SOURCE FLUVIO-VOLCANIC OUTFLOW CHANNEL SYSTEM. Lunar and Planetary Science XLVIII (2017). 2985pdf. ...
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Chryse Planitia
Chryse Planitia (Greek, "''Golden Plain''") is a smooth circular plain in the northern equatorial region of Mars close to the Tharsis region to the west, centered at . Chryse Planitia lies partially in the Lunae Palus quadrangle, partially in the Oxia Palus quadrangle, partially in the Mare Acidalium quadrangle. It is 1600 km or 994 mi in diameter and with a floor 2.5 km below the average planetary surface altitude, and has been suggested to be an ancient buried impact basin, though this is contested. It has several features in common with lunar maria, such as Wrinkle-ridge, wrinkle ridges. The density of impact craters in the range is close to half the average for lunar maria. Chryse Planitia shows evidence of water erosion in the past, and is the bottom end for many outflow channels from the southern highlands as well as from Valles Marineris and the flanks of the Tharsis bulge. It is one of the lowest regions on Mars ( below the mean surface elevation of Mars) ...
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