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Planet
This article is about the astronomical object. For other uses, see Planet (disambiguation).
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.[a][1][2]
Mercury Venus
Earth Mars
Jupiter Saturn
Uranus Neptune
The eight known planets of the Solar System
The terrestrial planets
Mercury, Venus, Earth, and Mars
The giant planets
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. Five planets in the Solar System are visible to 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. This definition is controversial because it excludes many objects of planetary mass based on where or what they orbit. Although eight of the planetary bodies discovered before 1950 remain "planets" under the modern definition, some celestial bodies, such as Ceres, Pallas, Juno and Vesta (each an object in the solar asteroid belt), and Pluto (the first trans-Neptunian object discovered), that were once considered planets by the scientific community, are no longer viewed as such.
The planets were thought by Ptolemy to orbit Earth in deferent and epicycle motions. Although the idea that the planets orbited the Sun had been suggested many times, it was not until the 17th century that this view was supported by evidence from the first telescopic astronomical observations, performed by Galileo Galilei. At about the same time, by careful analysis of pre-telescopic observational data collected by Tycho Brahe, Johannes Kepler found 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 some shared such features as ice caps and seasons. Since the dawn of the Space Age, close observation by space probes has found that Earth and the other planets share characteristics such as volcanism, hurricanes, tectonics, and even hydrology.
Planets are generally divided into two main types: large low-density giant planets, and smaller rocky terrestrials. There are eight planets in the Solar System.[1] 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. Six of the planets are orbited by one or more natural satellites.
Several thousands of planets around other stars ("extrasolar planets" or "exoplanets") have been discovered in the Milky Way. As of 1 January 2019, 3,946 known extrasolar planets in 2,945 planetary systems (including 650 multiple planetary systems), ranging in size from just above the size of the Moon to gas giants about twice as large as Jupiter have been discovered, out of which more than 100 planets are the same size as Earth, nine of which are at the same relative distance from their star as Earth from the Sun, i.e. in the circumstellar habitable zone.[3][4] On December 20, 2011, the Kepler Space Telescope team reported the discovery of the first Earth-sized extrasolar planets, Kepler-20e[5] and Kepler-20f,[6] orbiting a Sun-like star, Kepler-20.[7][8][9] A 2012 study, analyzing gravitational microlensing data, estimates an average of at least 1.6 bound planets for every star in the Milky Way.[10] Around one in five Sun-like[b] stars is thought to have an Earth-sized[c] planet in its habitable[d] zone.
History
Mythology and naming
Formation
Solar System
Exoplanets
Planetary-mass objects
Attributes
See also
Notes
References
External links
Last edited 1 day ago by JeanLucMargot
Wikipedia
Content is available under CC BY-SA 3.0 unless otherwise noted.
Terms of UsePrivacyDesktop
Wikipedia Search
EditWatch this pageRead in another language
Planet
This article is about the astronomical object. For other uses, see Planet (disambiguation).
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.[a][1][2]
Mercury Venus
Earth Mars
Jupiter Saturn
Uranus Neptune
The eight known planets of the Solar System
The terrestrial planets
Mercury, Venus, Earth, and Mars
The giant planets
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. Five planets in the Solar System are visible to 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. This definition is controversial because it excludes many objects of planetary mass based on where or what they orbit. Although eight of the planetary bodies discovered before 1950 remain "planets" under the modern definition, some celestial bodies, such as Ceres, Pallas, Juno and Vesta (each an object in the solar asteroid belt), and Pluto (the first trans-Neptunian object discovered), that were once considered planets by the scientific community, are no longer viewed as such.
The planets were thought by Ptolemy to orbit Earth in deferent and epicycle motions. Although the idea that the planets orbited the Sun had been suggested many times, it was not until the 17th century that this view was supported by evidence from the first telescopic astronomical observations, performed by Galileo Galilei. At about the same time, by careful analysis of pre-telescopic observational data collected by Tycho Brahe, Johannes Kepler found 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 some shared such features as ice caps and seasons. Since the dawn of the Space Age, close observation by space probes has found that Earth and the other planets share characteristics such as volcanism, hurricanes, tectonics, and even hydrology.
Planets are generally divided into two main types: large low-density giant planets, and smaller rocky terrestrials. There are eight planets in the Solar System.[1] 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. Six of the planets are orbited by one or more natural satellites.
Several thousands of planets around other stars ("extrasolar planets" or "exoplanets") have been discovered in the Milky Way. As of 1 January 2019, 3,946 known extrasolar planets in 2,945 planetary systems (including 650 multiple planetary systems), ranging in size from just above the size of the Moon to gas giants about twice as large as Jupiter have been discovered, out of which more than 100 planets are the same size as Earth, nine of which are at the same relative distance from their star as Earth from the Sun, i.e. in the circumstellar habitable zone.[3][4] On December 20, 2011, the Kepler Space Telescope team reported the discovery of the first Earth-sized extrasolar planets, Kepler-20e[5] and Kepler-20f,[6] orbiting a Sun-like star, Kepler-20.[7][8][9] A 2012 study, analyzing gravitational microlensing data, estimates an average of at least 1.6 bound planets for every star in the Milky Way.[10] Around one in five Sun-like[b] stars is thought to have an Earth-sized[c] planet in its habitable[d] zone.
History
Mythology and naming
Formation
Solar System
Exoplanets
Planetary-mass objects
Attributes
See also
Notes
References
External links
Last edited 1 day ago by JeanLucMargot
Wikipedia
Content is available under CC BY-SA 3.0 unless otherwise noted.
Terms of UsePrivacyDesktop
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Mercury
- it is the smallest planet
- it is the closest planet to the sun
- it takes 88 days to go around the sun once
- it takes about 59 days to complete one rotation on its axis
- a year on earth is equal to 4 years on mercury
- it has no natural satellite
- it has no atmosphere
- it becomes very hot during the day and very cold during the night
- its temperature is around 430° C
Venus
- it is the second planet
- it takes nearly 225 days to go around the sun once
- it rotates from east to west
- it takes about 243 days to complete one rotation on its axis
- it has no natural satellite
- it is the hottest and brightest planet in the solar system
- its temperature is 465°C
- it is also known as morning and evening star because it can be seen before sunrise and after sunset
Earth
- it is the planet on which we live
- it is the third planet
- it is located in an ideal distance from the sun
- it is the only planet which support life
- it refers as 'blue planet as it appears blue when seen from space
- it takes 365 days to complete one revolution around the sun
- it takes 24 hours to rotate on its axis
- it has one natural satellite- the moon
plz like the answer
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