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Sun

The Sun, sometimes called Sol, is the star in our larger image solar system. The planet Observation data Earth and all of her Mean distance from Earth 150,000,000 km sister planets, both the other terrestrial planets Visual brightness (V) -26.8m and the gas giants, orbit Absolute magnitude 4.8m the Sun. Other bodies that orbit the Sun Physical characteristics include asteroids, Diameter 1,392,000 km meteoroids, comets, Trans-Neptunian objects, Relative diameter (dS/dE) 109 and, of course, dust. Surface area 6.09 × 1012 km2 Volume 1.41 × 1027 m3 Physical and other Mass 1.9891 × 1030 kg characteristics Relative mass to Earth 333,400 The Sun is a main Density 1411 kg m-3 sequence star, with a Relative density to Earth 0.26 spectral class of G2, meaning that it is Relative density to water 1.409 somewhat bigger and Surface gravity 274 m s-2 hotter than the average star but far smaller than Relative surface gravity 27.9 g a red giant star. A G2 Surface temperature 5780 K star has a main sequence Temperature of corona 5 × 106 K lifetime of about 10 billion years, and the Luminosity (LS) 3.827 × 1026 J s-1 Sun is probably about 5 billion years old, as Orbital characteristics determined by Period of rotation nucleocosmochronology. At equator: 27d 6h 36m At the center of the Sun, At 30¡ latitude: 28d 4h 48m where its density is 1.5 At 60¡ latitude: 30d 19h 12m × 105 kg m-3, At 75¡ latitude: 31d 19h 12m thermonuclear reactions (nuclear fusion) convert Period of orbit around 2.2 × 108 years hydrogen into helium. 3.9 galactic centre × 1045 atoms Photospheric composition undergo nuclear reactions Hydrogen 73.46 % there every second. This Helium 24.85 % releases energy which escapes from the surface Oxygen 0.77 % of the Sun as light. Carbon 0.29 % Physicists are able to replicate thermonuclear Iron 0.16 % reactions with hydrogen Neon 0.12 % bombs. Sustained nuclear Nitrogen 0.09 % fusion on earth for electricity generation Silicon 0.07 % may be possible in the Magnesium 0.05 % future, with nuclear Sulphur 0.04 % fusion reactors. All matter in the Sun is in the form of plasma due to its extreme temperature. This makes it possible for the sun to rotate faster at its equator than it does at higher latitudes, since the Sun is not a solid body. The differential rotation of the Sun's latitudes causes its magnetic field lines to become twisted together over time, causing magnetic field loops to erupt from the sun's surface and trigger the formation of the Sun's dramatic sunspots and solar prominences. The corona has 1011 atoms/m3, and the photosphere has 1023 atoms/m3. For some time it was thought that the number of neutrinos produced by the nuclear reaction in the Sun was only one third of the number predicted by theory, a result that was termed the solar neutrino problem. When it was recently found that neutrinos had mass, and could therefore transform into harder-to-detect varieties of neutrinos while en route from the Sun to Earth, measurement and theory were reconciled. Observation of the Sun can reveal such phenomena as: * Sunspots * Faculae * Solar flares * Solar prominences o quiescent prominences o eruptive prominences Caution: looking directly at the sun can damage the retina and one's eyesight. There are several newspapers called The Sun. Sun is a shortened name for Sun Microsystems. The Solar System Sun - Mercury - Venus - Earth - Mars - Asteroids - Jupiter - Saturn - Uranus - Neptune - Pluto - Comets - Kuiper belt - Oort cloud

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