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photo credits: Wikimedia Commons
The Moon is Earth's only natural satellite. It orbits at an average distance of 384,400 km (238,900 mi), about 30 times Earth's diameter. The Moon always presents the same side to Earth, because gravitational pull has locked its rotation to the planet. This results in the lunar day of 29.5 Earth days matching the lunar month. The Moon's gravitational pull – and to a lesser extent the Sun's – are the main drivers of the tides. The Moon is in geophysical terms a planetary-mass object or satellite planet. It has a mass that amounts to 1.2% of Earth's, and a diameter that is roughly one-quarter of Earth's or with 3,474 km (2,159 mi) about as wide as Australia. Within the Solar System it is the most massive and largest satellite in relation to its parent planet, the fifth most massive and largest moon overall, and more massive and larger than all known dwarf planets. Its surface gravity is about one sixth of Earth's, about half of that of Mars, and after Jupiter's moon Io the second highest among all Solar System moons. The body of the Moon is differentiated and terrestrial, with no significant hydrosphere, atmosphere, or magnetic field. It formed 4.51 billion years ago, not long after Earth's formation, out of the debris from a giant impact between Earth and a hypothesized Mars-sized body called Theia. The lunar surface is covered in lunar dust and marked by mountains, impact craters, their ejecta, ray-like streaks and, mostly on the near side of the Moon, by dark maria ("seas"), which are plains of cooled magma. These maria formed when large impacts on the far side of the Moon heated up low lying layers of its crust on the near side. The Moon is, beside when passing through Earth's shadow during a lunar eclipse, always illuminated by the Sun, but from Earth the visible illumination shifts during its orbit, producing the lunar phases. The Moon is the brightest celestial object in Earth's night sky. This is mainly due to its large angular diameter, while the reflectance of the lunar surface is comparable to that of asphalt. The apparent size is nearly the same as that of the Sun, allowing it to cover the Sun almost completely during a total solar eclipse. From Earth about 59% of the lunar surface is visible over time due to cyclical shifts in perspective (libration), making parts of the far side of the Moon visible. For humans the Moon has been an important source of inspiration and knowledge, having been crucial to cosmography, mythology, religion, art, time keeping, natural science, and spaceflight. On September 13, 1959, the first human-made object to reach an extraterrestrial body arrived on the Moon, the Soviet Union's Luna 2 impactor. In 1966 the Moon became the first extraterrestrial body where soft landings and orbital insertions were achieved. On July 20, 1969, humans for the first time landed on the Moon and any extraterrestrial body, at Mare Tranquillitatis with the lander Eagle of the United States' Apollo 11 mission. Five more crews were sent between then and 1972, each with two men landing on the surface. The longest stay was 75 hours by the Apollo 17 crew. Thereafter exploration of the Moon has continued robotically, with crewed missions being planned to return starting in the late 2020s. Source: Wikipedia (en)
Works about Moon 68
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Kosmos
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New Views of the Moon 2 -- Asia
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Lunar Polar Volatiles
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New Views of the Moon 2, Europe
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New Views of the Moon 2
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Explore! Marvel Moon: February 25, 2015, Lunar and Planetary Institute
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The Clementine Atlas of the Moon
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Second Conference on the Lunar Highlands Crust
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Ground-Based Geophysics on the Moon: January 21–22, 2010, Tempe, Arizona
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Nördlingen 2010: The Ries Crater, the Moon, and the Future of Human Space Exploration
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Limit
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Lunar Reconnaissance Orbiter Science Targeting Meeting
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The Dead and the Gone
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Joint Annual Meeting of LEAG-ICEUM-SRR: October 28-31, 2008, Cape Canaveral, Florida
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Who Built the Moon?
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Lunar Sourcebook: A User's Guide to the Moon
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Digital Lunar Orbiter Photographic Atlas of the Moon
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The Moon Beyond 2002, Next Steps in Lunar Science and Exploration: September 12-14, 2002, Taos, New Mexico
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Workshop on New Views of the Moon II, Understanding the Moon Through the Integration of Diverse Datasets: Flagstaff, Arizona, September 22-24, 1999
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Workshop on New Views of the Moon, Integrated Remotely Sensed, Geophysical, and Sample Datasets
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The once and future moon
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Workshop on Geology of the Apollo 17 Landing Site.
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Workshop on Mare Volcanism and Basalt Petrogenesis: "Astounding Fundamental Concepts (AFC)" Developed Over the Last Fifteen Years
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Workshop on Moon in Transition : Apollo 14, KREEP, and Evolved Lunar Rocks
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The Apollo 15 coarse fines (4-10 mm)
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Workshop on the Geology and Petrology of the Apollo 15 Landing Site
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Workshop on Pristine Highlands Rocks and the Early History of the Moon
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Catalog of Lunar Mare Basalts Greater Than 40 Grams
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Workshop on Apollo 16
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Papers Presented to the Conference on the Ancient Sun Fossil Record in the Earth, Moon and Meteorites: A Lunar and Planetary Institute Topical Conference Boulder, Colorado 15 - 19 October 1979
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Papers Presented to the Conference on the Lunar Highlands Crust
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Apollo Over the Moon: A View From Orbit
Works based on Moon 1
Narratives set in Moon 17
- ¡En la Luna!
- The Gods Themselves
- A True Story
- Have Space Suit—Will Travel
- A Fall of Moondust
- Paradiso - Canto secondo
- Columbus Was a Dope
- Adolphus Claar
- Chasseurs de chimères
- De la Lune à la Terre
- Le Maître d'armes
- Luna incognita
- Revers de fortune
- Artemis
- Growing Up Weightless
- La nouvelle lune
- Chainsaw Man
Subject - wd:Q405