Designations | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Designation | Earth I | ||||||||||||
Adjectives | |||||||||||||
Symbol | or | ||||||||||||
Orbital characteristics | |||||||||||||
Epoch J2000 | |||||||||||||
Perigee | 362600 km (356400–370400 km) | ||||||||||||
Apogee | 405400 km (404000–406700 km) | ||||||||||||
384399 km (1.28 ls, 0.00257 AU)[1] | |||||||||||||
Eccentricity | 0.0549[1] | ||||||||||||
29.530589 d (29 d 12 h 44 min 2.9 s) | |||||||||||||
Average orbital speed | 1.022 km/s | ||||||||||||
Inclination | 5.145° to the ecliptic[2][a] | ||||||||||||
Regressing by one revolution in 18.61 years | |||||||||||||
Progressing by one revolution in 8.85 years | |||||||||||||
Satellite of | Earth[b][3] | ||||||||||||
Physical characteristics | |||||||||||||
1737.4 km (0.2727 of Earth's)[1][4][5] | |||||||||||||
Equatorial radius | 1738.1 km (0.2725 of Earth's)[4] | ||||||||||||
Polar radius | 1736.0 km (0.2731 of Earth's)[4] | ||||||||||||
Flattening | 0.0012[4] | ||||||||||||
Circumference | 10921 km (equatorial) | ||||||||||||
3.793×107 km2 (0.074 of Earth's) | |||||||||||||
Volume | 2.1958×1010 km3 (0.02 of Earth's)[4] | ||||||||||||
Mass | 7.346×1022 kg (0.0123 of Earth's)[1][4][6] | ||||||||||||
Mean density | 3.344 g/cm3[1][4] 0.606 × Earth | ||||||||||||
1.622 m/s2 (5.32 ft/s2)[4] 0.1654 g0 | |||||||||||||
0.3929±0.0009[7] | |||||||||||||
2.38 km/s (8600 km/h; 5300 mph) | |||||||||||||
27.321661 d (spin-orbit locked) | |||||||||||||
Equatorial rotation velocity | 4.627 m/s | ||||||||||||
| |||||||||||||
North pole right ascension |
| ||||||||||||
North pole declination | 65.64°[10] | ||||||||||||
Albedo | 0.136[11] | ||||||||||||
| |||||||||||||
Surface absorbed dose rate | 13.2 μGy/h (during lunar daytime)[14] | ||||||||||||
Surface equivalent dose rate | 57.0 μSv/h (during lunar daytime)[14] | ||||||||||||
0.2[15] | |||||||||||||
29.3 to 34.1 arcminutes[4][d] | |||||||||||||
Atmosphere[16] | |||||||||||||
Surface pressure | |||||||||||||
Composition by volume | |||||||||||||
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.[17] 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.[18] 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.
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was invoked but never defined (see the help page).Vasavada1999
was invoked but never defined (see the help page).We measured an average total absorbed dose rate in silicon of 13.2 ± 1 μGy/hour ... LND measured an average dose equivalent of 1369 μSv/day on the surface of the Moon
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