Lacus Oblivionis
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Lacus Oblivionis
Lacus Oblivionis (Latin ''oblīviōnis'', "Lake of Forgetfulness") is a small lunar mare on the surface of the Moon The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet, with a diameter about one-quarter that of Earth (comparable to the width of .... It is located at 21.0° S, 168.0° W and is 50 km in diameter. The name was adopted by the IAU in 1976.Lacus Oblivionis
Feature 3213, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) The crater Mohorovičić R (satellite of Mohorovičić) lies to the northeast, and the crater Sniadec ...
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Lacus Oblivionis (LRO)
Lacus Oblivionis (Latin ''oblīviōnis'', "Lake of Forgetfulness") is a small lunar mare on the surface of the Moon The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet, with a diameter about one-quarter that of Earth (comparable to the width of .... It is located at 21.0° S, 168.0° W and is 50 km in diameter. The name was adopted by the IAU in 1976.Lacus Oblivionis
Feature 3213, Gazetteer of Planetary Nomenclature, International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN) The crater Mohorovičić R (satellite of Mohorovičić) lies to the northeast, and the crater Sniadec ...
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Lunar Reconnaissance Orbiter
The Lunar Reconnaissance Orbiter (LRO) is a NASA robotic spacecraft currently orbiting the Moon in an eccentric polar mapping orbit. Data collected by LRO have been described as essential for planning NASA's future human and robotic missions to the Moon. Its detailed mapping program is identifying safe landing sites, locating potential resources on the Moon, characterizing the radiation environment, and demonstrating new technologies. Launched on June 18, 2009, in conjunction with the Lunar Crater Observation and Sensing Satellite (LCROSS), as the vanguard of NASA's Lunar Precursor Robotic Program, LRO was the first United States mission to the Moon in over ten years. LRO and LCROSS were launched as part of the United States's Vision for Space Exploration program. The probe has made a 3-D map of the Moon's surface at 100-meter resolution and 98.2% coverage (excluding polar areas in deep shadow), including 0.5-meter resolution images of Apollo landing sites. The first images f ...
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Lacus Oblivionis AS17-151-23192-93
The Latin word ''lacus'' means "opening, hole, pool, lake," and was also the word for a distribution point in the public water supply of ancient Rome. It can refer to: Geography *Lucrinus Lacus, a lake in Campania *Albanus Lake, Lake Albano in Lazio, Italy *Alsietinus Lacus, the ancient name of a lake in Etruria today known as Lake Martignano * Lacus Curtius, a topographical feature in ancient Rome *Lacus Juturnae, a spring and man-made religious structure in ancient Rome Extraterrestrial ''Lacus'' may also refer to a lunar mare; see List of maria on the Moon: *Lacus Aestatis *Lacus Autumni *Lacus Bonitatis * Lacus Excellentiae *Lacus Felicitatis * Lacus Mortis *Lacus Solitudinis *Lacus Somniorum *Lacus Spei *Lacus Temporis ''Lacus'' may refer to similar features on other celestial bodies: * Ontario Lacus on Titan, a moon of Saturn *Solis Lacus on Mars Fictional characters * Lacus Clyne from ''Mobile Suit Gundam SEED'' and '' Mobile Suit Gundam SEED Destiny'' anime. Asso ...
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Latin
Latin (, or , ) is a classical language belonging to the Italic branch of the Indo-European languages. Latin was originally a dialect spoken in the lower Tiber area (then known as Latium) around present-day Rome, but through the power of the Roman Republic it became the dominant language in the Italian region and subsequently throughout the Roman Empire. Even after the fall of Western Rome, Latin remained the common language of international communication, science, scholarship and academia in Europe until well into the 18th century, when other regional vernaculars (including its own descendants, the Romance languages) supplanted it in common academic and political usage, and it eventually became a dead language in the modern linguistic definition. Latin is a highly inflected language, with three distinct genders (masculine, feminine, and neuter), six or seven noun cases (nominative, accusative, genitive, dative, ablative, and vocative), five declensions, four verb conjuga ...
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Lunar Mare
The lunar maria (; singular: mare ) are large, dark, basaltic plains on Earth's Moon, formed by ancient asteroid impacts on the far side on the Moon that triggered volcanic activity on the opposite (near) side. They were dubbed , Latin for 'seas', by early astronomers who mistook them for actual seas. They are less reflective than the "highlands" as a result of their iron-rich composition, and hence appear dark to the naked eye. The maria cover about 16% of the lunar surface, mostly on the side visible from Earth. The few maria on the far side are much smaller, residing mostly in very large craters. The traditional nomenclature for the Moon also includes one (ocean), as well as features with the names ('lake'), ('marsh'), and ('bay'). The last three are smaller than maria, but have the same nature and characteristics. The names of maria refer to sea features (Mare Humorum, Mare Imbrium, Mare Insularum, Mare Nubium, Mare Spumans, Mare Undarum, Mare Vaporum, Oceanus Procellarum ...
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Moon
The Moon is Earth's only natural satellite. It is the fifth largest satellite in the Solar System and the largest and most massive relative to its parent planet, with a diameter about one-quarter that of Earth (comparable to the width of Australia). The Moon is a planetary-mass object with a differentiated rocky body, making it a satellite planet under the geophysical definitions of the term and larger than all known dwarf planets of the Solar System. It lacks any significant atmosphere, hydrosphere, or magnetic field. Its surface gravity is about one-sixth of Earth's at , with Jupiter's moon Io being the only satellite in the Solar System known to have a higher surface gravity and density. The Moon orbits Earth at an average distance of , or about 30 times Earth's diameter. Its gravitational influence is the main driver of Earth's tides and very slowly lengthens Earth's day. The Moon's orbit around Earth has a sidereal period of 27.3 days. During each synodic period ...
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Mohorovičić (crater)
Mohorovičić is a Lunar craters, lunar impact crater that is located on the Far side (Moon), far side of the Moon. It lies to the southwest of the larger crater Doppler (crater), Doppler and the huge walled plain Korolev (lunar crater), Korolev. To the southwest of Mohorovičić is a small lunar mare that has been named Lacus Oblivionis. Due south of it is an unnamed mountain that formed during the impact that created the South Pole-Aitken Basin. This is a circular crater that has undergone some wear from subsequent impacts. The satellite crater Mohorovičić Z lies on the northern interior floor, adjacent to the northern inner wall and rim. A small, cup-shaped crater is intruding into the western rim. Satellite craters By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Mohorovičić. References

* * * * * * * * * * * * {{DEFAULTSORT:Mohorovicic (crater) Impact craters on th ...
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Sniadecki (crater)
Sniadecki is a lunar impact crater on the far side of the Moon. This is a circular, bowl-shaped feature that is not overlain by any significant impacts. However the larger satellite crater Sniadecki Q is attached to the southwestern outer rim and has disrupted the rim edge somewhat. There is also a small crater attached to the western outer rim. To the northeast of Sniadecki is a small lunar mare feature that has been designated Lacus Oblivionis. To the northwest of Sniadecki is the crater Bok. Satellite craters By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Sniadecki. See also * 1262 Sniadeckia 1262 Sniadeckia, provisional designation , is a carbonaceous background asteroid from the asteroid belt's outer regions, approximately 54 kilometers in diameter. It was discovered on 23 March 1933, by Belgian astronomer Sylvain Arend at the Royal ..., asteroid References * * * * * * * ...
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