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photo credits: Wikimedia Commons
The Moon is the only natural satellite orbiting Earth. It orbits around Earth at an average distance of 384,399 kilometres (238,854 mi), a distance roughly 30 times the width of Earth, and completes an orbit (lunar month) in relation to Earth and the Sun (synodically) every 29.5 days. The Moon and Earth gravitationally pull on each other. The resulting tidal forces are the main drivers of Earth's tides, and have forced the Moon to face Earth with always the same near side, effectively synchronizing the Moon's rotation period (lunar day) to its orbital period (lunar month). This makes the Moon tidally locked to Earth. 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 contiguous United States). Within the Solar System, it is larger and more massive than any known dwarf planet, and the fifth-largest and fifth-most massive moon, as well as the largest and most massive in relation to its parent planet. Its surface gravity is about one-sixth of Earth's, about half that of Mars, and the second-highest among all moons in the Solar System after Jupiter's moon Io. The body of the Moon is differentiated and terrestrial, with only a minuscule hydrosphere, atmosphere, and magnetic field. The lunar surface is covered in regolith dust, which mainly consists of the fine material ejected from the lunar crust by impact events. The lunar crust is marked by impact craters, with some younger ones featuring bright ray-like streaks. The Moon was volcanically active until 1.2 billion years ago, surfacing lava mostly on the thinner near side of the Moon, filling ancient craters, which through cooling formed the today prominently visible dark plains of basalt called maria ('seas'). The Moon formed out of material from Earth, ejected by a giant impact into Earth of a hypothesized Mars-sized body named Theia 4.51 billion years ago, not long after Earth's formation. From a distance, the day and night phases of the lunar day are visible as the lunar phases, and when the Moon passes through Earth's shadow a lunar eclipse is observable. The Moon's apparent size in Earth's sky is about the same as that of the Sun, which causes it to cover the Sun completely during a total solar eclipse. The Moon is the brightest celestial object in Earth's night sky because of its large apparent size, while the reflectance (albedo) of its surface is comparable to that of asphalt. About 59% of the surface of the Moon is visible from Earth owing to the different angles at which the Moon can appear in Earth's sky (libration), making parts of the far side of the Moon visible. The Moon has been an important source of inspiration and knowledge in human history, having been crucial to cosmography, mythology, religion, art, time keeping, natural science and spaceflight. The first human-made objects to fly to an extraterrestrial body were sent to the Moon, starting in 1959 with the flyby of the Soviet Union's Luna 1 probe and the intentional impact of Luna 2. In 1966, the first soft landing (by Luna 9) and orbital insertion (by Luna 10) followed. Humans arrived for the first time at the Moon, or any extraterrestrial body, in orbit on December 24, 1968, with Apollo 8 of the United States, and on the surface at Mare Tranquillitatis on July 20, 1969, with the lander Eagle of Apollo 11. By 1972, six Apollo missions had landed twelve humans on the Moon and stayed up to three days. Renewed robotic exploration of the Moon, in particular to confirm the presence of water on the Moon, has fueled plans to return humans to the Moon, starting with the Artemis program in the late 2020s. Source: Wikipedia (en)
Works about Moon 80
Les Champs de la Lune
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
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?
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
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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The Apollo 15 coarse fines (4-10 mm)
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Workshop on Moon in Transition : Apollo 14, KREEP, and Evolved Lunar Rocks
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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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