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Isis (lunar Crater)
Isis is a tiny lunar volcanic crater in the southeastern part of the Mare Serenitatis. It is located to the northeast of the small crater Dawes, and to the west of the Montes Taurus range. To the east-northeast of this position is the landing site of the Apollo 17 mission, in the Taurus–Littrow valley. Isis and nearby Osiris are located on conical uprises situated along a rille and are interpreted as small volcanic cones. The name of the crater was approved by the IAU in 1976, and refers to an Egyptian female given name. Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) References * * * * * * *External links {{Commons category[...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Apollo 17
Apollo 17 (December 7–19, 1972) was the final mission of NASA's Apollo program, the most recent time humans have set foot on the Moon or traveled beyond low Earth orbit. Commander Gene Cernan and Lunar Module Pilot Harrison Schmitt walked on the Moon, while Command Module Pilot Ronald Evans orbited above. Schmitt was the only professional geologist to land on the Moon; he was selected in place of Joe Engle, as NASA had been under pressure to send a scientist to the Moon. The mission's heavy emphasis on science meant the inclusion of a number of new experiments, including a biological experiment containing five mice that was carried in the command module. Mission planners had two primary goals in deciding on the landing site: to sample lunar highland material older than that at Mare Imbrium and to investigate the possibility of relatively recent volcanic activity. They therefore selected Taurus–Littrow, where formations that had been viewed and pictured from orbi ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Isis (given Name)
Isis is a female first name. Meaning The initial popularity of the name derived from its association with the goddess Isis of the Egyptian pantheon. Her strong character has subsequently been adopted as an axiom among feminists. Popularity The name's popularity in the United States peaked in 2005, where it was the 522nd most popular name for baby girls. Since 2014, the name Isis has decreased significantly in the United States, Canada, United Kingdom and Australia, due to the name being associated with the jihadist terrorist organization Islamic State of Iraq and Syria (ISIS). Many name changes have been recorded as well. By 2015, the name had completely dropped off the top 1000 list of most popular names for baby girls. Given name * Isis Anchalee (b. 1993), creator of the ''#ilooklikeanengineer'' gender equality campaign * Isis Casalduc (born 1981), Puerto Rican beauty pageant titleholder and model * Isis Finlay (1934–2007), 1954 Miss Cuba * Isis Gaston (born 2000), rap ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Isis Crater AS15-P-9305
Isis (; ''Ēse''; ; Meroitic: ''Wos'' 'a''or ''Wusa''; Phoenician: 𐤀𐤎, romanized: ʾs) was a major goddess in ancient Egyptian religion whose worship spread throughout the Greco-Roman world. Isis was first mentioned in the Old Kingdom () as one of the main characters of the Osiris myth, in which she resurrects her slain brother and husband, the divine king Osiris, and produces and protects his heir, Horus. She was believed to help the dead enter the afterlife as she had helped Osiris, and she was considered the divine mother of the pharaoh, who was likened to Horus. Her maternal aid was invoked in healing Spell (paranormal), spells to benefit ordinary people. Originally, she played a limited role in royal rituals and temple rites, although she was more prominent in funerary practices and magical texts. She was usually portrayed in art as a human woman wearing a throne-like hieroglyph on her head. During the New Kingdom (), as she took on traits that originally belon ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Catena Brigitte AS17-M-0597 LTVT
Catena (Latin for chain) or catenae (plural) may refer to: Science * ''Catena'' (fly), a genus in the family Tachinidae *Catena (linguistics) is a unit of syntax and morphology, closely associated with dependency grammars *Catena (computing), number of bits transferred in one cycle * Catenary, a type of curve in mathematics * Crater chain, a line of craters along the surface of an astronomical body *Farmacia Catena, a trade name of the drug idebenone *Catena (soil) in pedology, a sequence of soil profiles down a slope *Catena (cryptography), a cryptographic algorithm used as a key derivation function Publishing *''CATENA'' (), a journal of soil sciences published by Elsevier *''Catena Paperback'', published by E. Schweizerbart *''Catena Supplements'', published by E. Schweizerbart *'' CATENA: Magazine of the Catenian Association'' * Catena Media, an online media company in Malta Other uses *Catena (surname) * Catena (biblical commentary), a verse-by-verse biblical commentary *C ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Lunar Craters
Lunar craters are impact craters on Earth's Moon. The Moon's surface has many craters, all of which were formed by impacts. The International Astronomical Union currently recognizes 9,137 craters, of which 1,675 have been dated. History The word ''crater'' was adopted from the Greek word for "vessel" (, a Greek vessel used to mix wine and water). Galileo built his first telescope in late 1609, and turned it to the Moon for the first time on November 30, 1609. He discovered that, contrary to general opinion at that time, the Moon was not a perfect sphere, but had both mountains and cup-like depressions. These were named craters by Johann Hieronymus Schröter (1791), extending its previous use with volcanoes. Robert Hooke in '' Micrographia'' (1665) proposed two hypotheses for lunar crater formation: one, that the craters were caused by projectile bombardment from space, the other, that they were the products of subterranean lunar volcanism. Scientific opinion as to the ori ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Volcanic Crater
A volcanic crater is an approximately circular depression in the ground caused by volcanic activity. It is typically a bowl-shaped feature containing one or more vents. During volcanic eruptions, molten magma and volcanic gases rise from an underground magma chamber, through a conduit, until they reach the crater's vent, from where the gases escape into the atmosphere and the magma is erupted as lava. A volcanic crater can be of large dimensions, and sometimes of great depth. During certain types of explosive eruptions, a volcano's magma chamber may empty enough for an area above it to subside, forming a type of larger depression known as a caldera. Geomorphology In most volcanoes, the crater is situated at the top of a mountain formed from the erupted volcanic deposits such as lava flows and tephra. Volcanoes that terminate in such a summit crater are usually of a conical form. Other volcanic craters may be found on the flanks of volcanoes, and these are commonly referred ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Mare Serenitatis
Mare Serenitatis (Latin ''serēnitātis'', the "Sea of Serenity") is a lunar mare located to the east of Mare Imbrium on the Moon. Its diameter is . Geology Mare Serenitatis is located within the Serenitatis basin, which is of the Nectarian epoch. The material surrounding the mare is of the Lower Imbrian epoch, while the mare material is of the Upper Imbrian epoch. The mare basalt covers a majority of the basin and overflows into Lacus Somniorum to the northeast. The most noticeable feature is the crater Posidonius on the northeast rim of the mare. The ring feature to the west of the mare is indistinct, except for Montes Haemus. Mare Serenitatis connects with Mare Tranquillitatis to the southeast and borders Mare Vaporum to the southwest. Mare Serenitatis is an example of a mascon, an anomalous gravitational region on the moon. A mass concentration (mascon), or gravitational high, was identified in the center of Mare Serenitatis from Doppler tracking of the five Lun ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Dawes (lunar Crater)
Dawes is a lunar impact crater located in the wide straight between Mare Serenitatis and Mare Tranquilitatis. To its southwest lies the larger crater Plinius, and to its northeast sits the Mons Argaeus mountain rise. It is named after British astronomer William Rutter Dawes. Description Dawes is circular with a sharp rim that has a slightly flattened oval perimeter. It has a slight central rise, and a somewhat darker floor that is nearly covered in overlapping swirl-like deposits. Much of the deposits are slumped or fall-back material. The inner walls are steep and free from impact erosion. Northeast of Dawes is a rille known as Rima Dawes. Detailed examination of this crater has located what appear to be alcoves and channels along the inner rim. It is hypothesized that micrometeorite impacts along the rim trigger dry landslides, which produce a gully-like appearance. A similar phenomenon may be responsible for gully-like features along the inner rim of some Martian craters. ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Montes Taurus
Montes Taurus is a rugged, jumbled mountainous region on the Moon. It is located to the east of the Mare Serenitatis, in the northeastern quadrant of the Moon's near side. Coordinates of their center are , and their extent is about 170 km. Montes Taurus are rather unimpressive and indistinct compared to other named lunar mountain systems. It is a broad hilly region without sharp borders. These mountains reach maximal height between craters Kirchhoff and Newcomb (4.9 km above Mare Serenitatis and 2.1 km above mean level of lunar surface). A number of craters lie embedded within this range. At the southwestern edge of the region is the crater Römer, and Newcomb is located in the northeastern section. Several satellite craters also lie throughout the Montes Taurus. Southwestern edge of this region hosts Taurus–Littrow valley, the landing site of the manned Apollo 17 mission. Name The Montes Taurus are named after Taurus Mountains in southern Turkey. This na ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Taurus–Littrow
Taurus–Littrow is a lunar valley located on the near side at the coordinates . It served as the landing site for the American Apollo 17 mission in December 1972, the last crewed mission to the Moon. The valley is located on the southeastern edge of Mare Serenitatis along a ring of mountains formed between 3.8 and 3.9 billion years ago when a large object impacted the Moon, forming the Serenitatis basin and pushing rock outward and upward. Taurus–Littrow is located in the Taurus mountain range and south of Littrow crater, features from which the valley received its name. The valley's name, coined by the Apollo 17 crew, was approved by the International Astronomical Union in 1973. Data collected during Apollo 17 indicate that the valley is composed primarily of feldspar-rich breccia in the large massifs surrounding the valley and basalt underlying the valley floor, covered by an unconsolidated layer of mixed material formed by various geologic events. Taurus–Littrow ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Osiris (lunar Crater)
Osiris is a tiny lunar volcanic crater in the southeastern part of the Mare Serenitatis. It is located to the northeast of the small crater Dawes, and to the west of the Montes Taurus range. To the east-northeast of this position is the landing site of the Apollo 17 mission, in the Taurus–Littrow valley. Osiris and nearby Isis are located on conical uprises situated along a rille and are interpreted as small volcanic cones. Osiris is the biggest of 5 cones on this rille. The name of the crater was approved by the IAU in 1976, and refers to an Egyptian male given name. Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) References * * * * * * * {{cite book , first = Peter T. , last = Wlasuk , date = 2000 , title = Observing ...[...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Rille
Rille (German for 'groove') is typically used to describe any of the long, narrow depressions in the surface of the Moon that resemble channels. The Latin term is ''rima'', plural ''rimae''. Typically, a rille can be several kilometers wide and hundreds of kilometers in length. However, the term has also been used loosely to describe similar structures on a number of planets in the Solar System, including Mars, Venus, and on a number of moons. All bear a structural resemblance to each other. Structures Three types of rille are found on the lunar surface: * Sinuous rilles meander in a curved path like a mature river, and are commonly thought to be the remains of collapsed lava tubes or extinct lava flows. They usually begin at an extinct volcano, then meander and sometimes split as they are followed across the surface. , 195 sinuous rilles have been identified on the Moon. Vallis Schröteri in Oceanus Procellarum is the largest sinuous rille, and Rima Hadley is the on ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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