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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 the diameter of Earth. Tidal forces between Earth and the Moon have synchronized the Moon's orbital period (lunar month) with its rotation period (lunar day) at 29.5 Earth days, causing the same side of the Moon to always face Earth. The Moon's gravitational pull—and, to a lesser extent, the Sun's—are the main drivers of Earth's tides. In geophysical terms, the Moon is a planetary-mass object or satellite planet. Its mass is 1.2% that of the Earth, and its diameter is 3,474 km (2,159 mi), roughly one-quarter of Earth's (about as wide as the United States from coast to coast). Within the Solar System, it is the largest and most massive satellite in relation to its parent planet, the fifth largest and most massive moon overall, and larger and more massive than all known dwarf planets. Its surface gravity is about one sixth of Earth's, about half of that of Mars, and the second highest among all Solar System moons, after Jupiter's moon Io. 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, rilles and, mostly on the near side of the Moon, by dark maria ("seas"), which are plains of cooled magma. These maria were formed when molten lava flowed into ancient impact basins. The Moon is, except 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 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. The Moon has been an important source of inspiration and knowledge for humans, having been crucial to cosmography, mythology, religion, art, time keeping, natural science, and spaceflight. In 1959, the first human-made objects to leave Earth and reach another body arrived at the Moon, with the flyby of the Soviet Union's Luna 1 and the intentional impact of Luna 2. In 1966, the Moon became the first extraterrestrial body with a soft landing by Luna 9 and a orbital insertion by Luna 10 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. Since then, exploration of the Moon has continued robotically, and crewed missions are being planned to return beginning in the late 2020s. Source: Wikipedia (en)
Works about Moon 79
Quiet Night Thought the bully
Selenographia, sive Lunae descriptio
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Théorie de la Lune
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Theoria Motuum Lunae
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The face of the moon
The Man Who Sold the Moon
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Lunar Surface Data Book 5 (00N/20E)
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Lunar Orbiter photographic data
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Proceedings of the Apollo 11 Lunar Science Conference
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Apollo 11 Lunar Science Conference Abstracts
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Guide to Lunar Orbiter photographs
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Proceedings of the Second Lunar Science Conference, Houston, Texas, January 11-14, 1971
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On the Moon with Apollo 15: A Guidebook to Hadley Rille and the Apennine Mountains
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1971 Lunar Science Conference Abstracts
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Proceedings of the Third Lunar Science Conference, Houston, Texas, January 10-13, 1972
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Lunar Science III: Revised Abstracts of Papers Presented at the Third Lunar Science Conference Houston, 10-13 January 1972
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Lunar Science IV : abstracts of papers
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Proceedings of the Fourth Lunar Science Conference Houston, Texas, March 5-8, 1973
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COSPAR - IAU - LSI Colloquium on Lunar Dynamics and Observational Coordinate Systems, Revised Abstracts
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Geophysical and Geochemical Exploration of the Moon and Planets. Proceedings of a Symposium Held at the Lunar Science Institute, Houston, Texas, January 10 - 12, 1973
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Proceedings of the Fifth Lunar Science Conference, Houston, Texas, March 1974
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Abstracts of Papers Presented at the Conference on Interactions of the Interplanetary Plasma with the Modern and Ancient Moon
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Lunar Science V: Abstracts of Papers Submitted to the Fifth Lunar Science Conference
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Proceedings of the Sixth Lunar Science Conference, Houston, Texas, March 17-21, 1975
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Papers Presented to the Conference on Origins of Mare Basalts and Their Implications for Lunar Evolution: November 17-19, 1975
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Lunar Science VI: Abstracts of Papers Submitted to the Sixth Lunar Science Conference
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User Guide to 1:250,000 Scale Lunar Maps
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Lunar stratigraphy and sedimentology
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Proceedings of the Seventh Lunar Science Conference Houston, Texas, March 15-19, 1976
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Papers Presented to the Conference on Comparisons of Mercury and the Moon: Houston, Texas 15-17 November 1976
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7th Lunar Science Conference Abstracts for Special Symposium on Recent Activity in the Moon
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Lunar Science VII: Abstracts of Papers Submitted to the Seventh Lunar Science Conference
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