Moon

Moon
Designations
Designation
Earth I
Adjectives
Symbol or
Orbital characteristics
Epoch J2000
Uncertainty parameter 0
Perigee362600 km
(356400370400 km)
Apogee405400 km
(404000406700 km)
384399 km  (1.28 ls; 1/389 AU; 1 LD)
Mean orbit radius
384784 km  
(1.28 ls; 1/384 AU; 1.001 LD)
Eccentricity0.0549
27.321661 d
(27d 7h 43min 11.5s)
29.530589 d
(29d 12h 44min 2.9s)
1.022 km/s
Inclination5.145° to the ecliptic
Regressing by one revolution in 18.61 years
Progressing by one
revolution in 8.85 years
Satellite ofEarth
Physical characteristics
1737.4 km  
(0.2727 of Earth's)
Equatorial radius
1738.1 km  
(0.2725 of Earth's)
Polar radius
1736.0 km  
(0.2731 of Earth's)
Flattening0.0012
Circumference10921 km  (equatorial)
3.793×107 km2  
(0.074 of Earth's)
Volume2.1958×1010 km3  
(0.02 of Earth's)
Mass7.346×1022 kg  
(0.0123 of Earth's)
Mean density
3.344 g/cm3
0.606 × Earth
1.622 m/s2 (5.32 ft/s2)
0.1654 g0
0.3929±0.0009
2.38 km/s
(8600 km/h; 5300 mph)
29.530589 d
(29d 12h 44min 2.9s; synodic; solar day) (spin-orbit locked)
27.321661 d  (spin-orbit locked)
Equatorial rotation velocity
4.627 m/s
North pole right ascension
  • 17h 47m 26s
  • 266.86°
North pole declination
65.64°
Albedo0.136
Surface temp. min mean max
Equator 100 K 250 K 390 K
85°N  150 K 230 K
Surface absorbed dose rate13.2 μGy/h
(during lunar daytime)
Surface equivalent dose rate57.0 μSv/h
(during lunar daytime)
  • −2.5 to −12.9
  • −12.74  (mean full moon)
0.2
29.3 to 34.1 arcminutes
Atmosphere
Surface pressure
  • 10−7 Pa (1 picobar)  (day)
  • 10−10 Pa (1 femtobar)   
    (night)
Composition by volume

    The Moon is Earth's only natural satellite. It orbits around Earth at an average distance of 384399 km (238,854 mi; about 30 times Earth's diameter). The Moon is tidally locked to Earth. This makes the Moon's near side face Earth always the same way, and synchronizes its rotation period (lunar day) to its orbital period (lunar month) of 29.5 Earth days. Conversley, the Moon's gravitation causes tidal forces on Earth, which are the main driver 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 contiguous United States). Within the Solar System, it is the largest and most massive satellite in relation to its parent planet, the fifth-largest and fifth-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 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 no significant hydrosphere, atmosphere, or magnetic field. 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 lava. These maria were formed when molten lava flowed into ancient impact basins. The Moon 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 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 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. 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 and the intentional impact of Luna 2. In 1966, the first soft landing (by Luna 9) and orbital insertion (by Luna 10) followed. On July 20, 1969, humans for the first time stepped on an extraterrestrial body, landing on the Moon 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.