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Natural satellite of Earth, 3,476 km/2,160 mi in diameter, with a mass 0.012 (approximately one-eightieth) that of Earth.
Its surface gravity is only 0.16 (one-sixth) that of Earth. Its average distance from Earth is 384,400 km/238,855 mi, and it orbits in a west-to-east direction every 27.32 days (the sidereal month). It spins on its axis with one side permanently turned towards Earth. The Moon has no atmosphere and was thought to have no water until ice was discovered on its surface in 1998.
Phases The Moon is illuminated by sunlight, and goes through a cycle of phases of shadow, waxing from new (dark) via first quarter (half Moon) to full, and waning back again to new every 29.53 days (the synodic month, also known as a lunation). On its sunlit side, temperatures reach 110°C/230°F, but during the two-week lunar night the surface temperature drops to −170°C/−274°F.
Origins The origin of the Moon is still open to debate. Scientists suggest the following theories: that it split from the Earth; that it was a separate body captured by Earth's gravity; that it formed in orbit around Earth; or – the theory most widely favoured currently – that it was formed from debris thrown off when a body the size of Mars struck Earth.
Research 70% of the far side of the Moon was photographed from the Soviet Lunik 3 in October 1959. Much of our information about the Moon has been derived from this and other photographs and measurements taken by US and Soviet Moon probes, from geological samples brought back by US Apollo astronauts and by Soviet Luna probes, and from experiments set up by US astronauts 1969–72. The US probe Lunar Prospector, launched in January 1998, examined the composition of the lunar crust, recorded gamma rays, and mapped the lunar magnetic field. It also discovered the ice on the Moon in March 1998.
During the 21st century, probes have been sent to the Moon by the European Space Agency, China, Japan, India, and the USA. NASA's Lunar Reconnaissance Orbiter is mapping the Moon from its polar orbit. A pair of GRAIL spacecraft began orbiting the Moon in tandem at the beginning of 2012, travelling just 50 km/30 mi high and about 200 km/120 mi apart. For nearly a year, before being deliberately crashed on the Moon, they measured their varying spacing in order to produce extraordinarily detailed maps of the Moon's gravitational field from which the satellite's inner structure can be deduced.
A joint Indian-Russian mission is planned to include an orbiter, a lander, and a rover, and is due to be launched in 2016. In the longer term, Russia plans an uncrewed lunar ‘colony’, with its own power station, laboratory, long-range rover, and associated satellite in orbit. The Google corporation is offering a prize of $30 million for any privately funded team that can send a rover to the Moon that travels more than 500 m/1,640 ft across the surface. Twenty-two teams registered for the contest and they have until 2015 to accomplish the feat.
In January 2004 US president George W Bush announced a plan to put astronauts back on the Moon by 2020. However, the successor administration of President Barack Obama cancelled the plan, turning its attention to crewed trips to Mars and the asteroids instead. Japan and India have announced their intention to send crewed missions to the Moon.
Composition The Moon is rocky, with a surface heavily scarred by meteorite impacts that have formed craters up to 240 km/150 mi across. Seismic observations indicate that the Moon's surface extends downwards for tens of kilometres; below this crust is a solid mantle about 1,100 km/688 mi thick, and below that a silicate core, part of which may be molten. Rocks brought back by astronauts show that the Moon is 4.6 billion years old, the same age as Earth. It is made up of the same chemical elements as Earth, but in different proportions, and differs from Earth in that most of the Moon's surface features were formed within the first billion years of its history when it was hit repeatedly by meteorites.
The youngest craters are surrounded by bright rays of ejected rock. The largest scars have been filled by dark lava to produce the lowland plains called seas, or maria (plural of mare). These dark patches form the so-called ‘man-in-the-Moon’ pattern. Inside some craters that are permanently in shadow is up to 300 million tonnes/330 million tons of ice existing as a thin layer of crystals.
One of the Moon's easiest features to observe is the crater Plato, which is about 100 km/62 mi in diameter and 2,700 m/8,860 ft deep, and at times is visible with the naked eye.
The US lunar probe Clementine discovered an enormous crater on the far side of the Moon in 1994. The South Pole-Aitken crater is 2,500 km/1,563 mi across and 13 km/8 mi deep, making it the largest known crater in the Solar System.
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