Planet
Planet
A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.
Definition[edit | edit source]
The term planet is ancient, with ties to history, astrology, science, mythology, and religion. Several planets in the Solar System can be seen with the naked eye. These were regarded by many early cultures as divine, or as emissaries of deities. As scientific knowledge advanced, human perception of the planets changed, incorporating a number of disparate objects. In 2006, the International Astronomical Union (IAU) officially adopted a resolution defining planets within the Solar System.
History[edit | edit source]
The idea of planets has evolved over its history, from the divine lights of antiquity to the earthly objects of the scientific age. The concept has expanded to include worlds not only in the Solar System, but in hundreds of other extrasolar systems. The ambiguities inherent in defining planets have led to much scientific controversy.
Planetary attributes[edit | edit source]
Planets are generally divided into two main types: large low-density giant planets, and smaller rocky terrestrials. Under IAU definitions, there are eight planets in the Solar System. In order of increasing distance from the Sun, they are the four terrestrials, Mercury, Venus, Earth, and Mars, then the four giant planets, Jupiter, Saturn, Uranus, and Neptune.
Extrasolar planets[edit | edit source]
In the 21st century, the discovery of extrasolar planets (planets that orbit stars other than the Sun) has become a key part of astronomical research. With the discovery of planets in other star systems, the field of planetary science has expanded to include these extrasolar planets.
See also[edit | edit source]
- Star
- Solar System
- Extrasolar planet
- International Astronomical Union
- Mercury (planet)
- Venus
- Earth
- Mars
- Jupiter
- Saturn
- Uranus
- Neptune
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