Planet

A planet is a large astronomical body that is not a star or stellar remnant. There are competing scientific definitions of a 'planet'. In the dynamicist definition adopted by the International Astronomical Union (IAU), a planet is a non-stellar body that is massive enough to be rounded by its own gravity, that directly orbits a star, and that has cleared its orbital zone of competing objects. The IAU has also declared that there are eight planets in the Solar System, independently of the formal definition.[lower-alpha 2][1][2] In the geological definition used by most planetologists, a planet is a rounded sub-stellar body, possibly a satellite. In addition to the eight Solar planets accepted by the IAU, these include dwarf planets such as Eris and Pluto and planetary-mass moons.[3]

The eight known planets[lower-alpha 1] of the Solar System:
Mercury, Venus, Earth, and Mars
Jupiter and Saturn (gas giants)
Uranus and Neptune (ice giants)

Shown in order from the Sun and in true color. Sizes are not to scale.

The term planet is ancient, with ties to history, astrology, science, mythology and religion. Apart from the Moon, five planets are visible to the naked eye in the night sky. Planets were regarded by many early cultures as emissaries of deities or as divine themselves. As scientific knowledge advanced, human perception of the planets changed, and the invention of the telescope enabled the discovery of additional planetary objects that were diverse in size, shape and orbit. In 2006, the IAU adopted a resolution limiting the number of planets within the Solar System, though they are not followed by all astronomers, especially planetologists. The IAU resolution is controversial because it excludes many geologically active objects of planetary mass due to where or what they orbit.

Ptolemy thought that the planets orbited Earth in deferent and epicycle motions. Although the idea that the planets orbited the Sun had been suggested before, it wasn't until the 17th century that this view was supported by the concrete evidence, in the form of telescopic observations performed by Galileo Galilei. About the same time, by careful analysis of pre-telescopic observational data collected by Tycho Brahe, Johannes Kepler discovered that the planets' orbits were elliptical rather than circular. As observational tools improved, astronomers saw that, like Earth, each of the planets rotated around an axis tilted with respect to its orbital pole, and that some shared such features as ice caps and seasons. Since the dawn of the Space Age, close observations by space probes have found that Earth and other planets share additional characteristics such as volcanism, hurricanes, tectonics and even hydrology.

The eight Solar planets in the IAU definition are divided into two divergent types: large low-density giant planets and small rocky terrestrial planets. In order of increasing distance from the Sun, they are the four terrestrials: Mercury, Venus, Earth, and Mars; and the four giants: Jupiter, Saturn, Uranus, and Neptune. Six are orbited by natural satellites, the two exceptions being the innermost planets Mercury and Venus. Under geophysical definitions, the classification is more complex: the Moon and Jupiter's moons Io and Europa[lower-alpha 3] are additional terrestrial planets, but a large number of small icy planets are also added, such as the dwarf planets Ceres and Pluto and the other large giant-planet moons such as Ganymede, Callisto, and Titan.

Beginning at the end of the twentieth century, several thousand planets have been discovered orbiting other stars. These are referred to as "extrasolar planets", or "exoplanets" for short. As of 1 January 2022, 4,905 extrasolar planets have been discovered in 3,629 planetary systems. The count includes 808 multi-planetary systems. Known exoplanets range in size from gas giants about twice as large as Jupiter down to just over the size of the Moon. More than 100 of these planets are approximately the size as Earth, nine of which orbit in the habitable zone of their star.[6][7] In 2011, the Kepler Space Telescope team reported the discovery of the first Earth-sized extrasolar planets orbiting a Sun-like star, Kepler-20e[8] and Kepler-20f.[9][10][11][12] A 2012 study, analyzing gravitational microlensing data, estimates a minimum of 1.6 bound planets on average for every star in the Milky Way.[13] As of 2013, one in five Sun-like[lower-alpha 4] stars is thought to have an Earth-sized[lower-alpha 5] planet in its habitable[lower-alpha 6] zone.[14][15]


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