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Portal:Solar System

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The Solar System Portal

TheSun and planets of the Solar System(distances not to scale)

TheSolar System is thegravitationally bound system of theSun and the masses thatorbit it, most prominently its eightplanets, of whichEarth is one. The systemformed about 4.6 billion years ago when a dense region of amolecular cloud collapsed, creating the Sun and aprotoplanetary disc from which the orbiting bodies assembled. Inside theSun's core hydrogenis fused into helium for billions of years, releasing energy which is over even longer periods of time emitted through the Sun's outer layer, thephotosphere. This creates theheliosphere and a decreasing temperaturegradient across the Solar System.

The mass of the Solar System is by 99.86% almost completely made up of the Sun's mass. The nextmost massive objects of the system are the eight planets, which by definition dominate the orbits they occupy. Closest to the Sun in order of increasing distance are the fourterrestrial planetsMercury,Venus, Earth andMars. These are the planets of theinner Solar System. Earth and Mars are the only planets in the Solar System which orbit within the Sun'shabitable zone, in which the sunlight can make surface water under atmospheric pressure liquid. Beyond thefrost line at about fiveastronomical units (AU), are twogas giantsJupiter andSaturn – and twoice giantsUranus andNeptune. These are the planets of theouter Solar System. Jupiter and Saturn possess nearly 90% of the non-stellar mass of the Solar System.

Additionally to the planets there are in the Solar System otherplanetary-mass objects, but which do not dominate their orbits, such asdwarf planets andplanetary-mass moons. TheInternational Astronomical Union's Minor Planet Center listsCeres,Pluto,Eris,Makemake, andHaumea as dwarf planets. Four otherSolar System objects are generally identified as such:Orcus,Quaoar,Gonggong, andSedna.Natural satellites, which are commonly called 'moons', can be found throughout the Solar System and in sizes from planetary-mass moons to much less massivemoonlets at their smallest. The largest two moons (Ganymede of Jupiter andTitan of Saturn) are larger than the smallest planet (Mercury), while the seven most massive, which includes Earth'sMoon, are more massive and larger than any of the dwarf planets.Less massive than these planetary-mass objects are the vast number ofsmall Solar System bodies, such asasteroids,comets,centaurs,meteoroids, andinterplanetary dust clouds. All dwarf planets and many of the smaller bodies are within theasteroid belt (between Mars's and Jupiter's orbit) and theKuiper belt (just outside Neptune's orbit).

The Solar System is within the heliosphere constantly flooded by the chargedplasma particles of thesolar wind, which forms with the interplanetary dust, gas andcosmic rays between the bodies of the Solar System aninterplanetary medium. At around70–90 AU from the Sun, the solar wind is halted by theinterstellar medium, resulting in theheliopause and the border of the interplanetary medium tointerstellar space. Further out somewhere beyond2,000 AU from the Sun extends the outermost region of the Solar System, the theorizedOort cloud, the source forlong-period comets, stretching to the edge of the Solar System, the edge of itsHill sphere, at 178,000–227,000 AU (2.81–3.59 ly), where its gravitational potential becomes equal to the galactic potential. The Solar System currently moves through a cloud of interstellar medium called theLocal Cloud. Theclosest star to the Solar System,Proxima Centauri, is 269,000 AU (4.25 ly) away. Both are within theLocal Bubble, a relatively small 1,000 light-years (ly) wide region of theMilky Way. (Full article...)

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Venus
Venus
Venus is the secondplanet from theSun. It is often calledEarth's "twin" or "sister" among the planets of theSolar System for its orbit being the closest to Earth's, both beingterrestrial planets, and having the most similar and nearly equal size, mass, andsurface gravity. Venus, though, is significantly different, especially as it has noliquid water, andits atmosphere is far thicker and denser than that of any other rocky body in the Solar System. The atmosphere is composed mostly ofcarbon dioxide and has a thick cloud layer ofsulfuric acid that spans the whole planet. At the mean surface level, the atmosphere reaches a temperature of 737 K (464 °C; 867 °F) and apressure 92 times greater than Earth's at sea level, turning the lowest layer of the atmosphere into asupercritical fluid. From Earth, Venus is visible as a star-like point of light,appearing brighter than any other natural point of light in the sky, and as aninferior planet it is always relatively close to the Sun, either as the brightest "morning star" or "evening star".

The orbits of Venus and Earth make the two planets approach each other insynodic periods of 1.6 years. In the course of this, Venus comes closer to Earth than any other planet, in contrast toMercury which stays closer over the course of an orbit to Earth than any other planet, due to its orbit being closer to the Sun. Ininterplanetary spaceflight from Earth, Venus is frequently used as a waypoint forgravity assists, offering a faster and more economical route. Venus has nomoons and a very slowretrograde rotation about its axis, a result of competing forces of solar tidal locking and differential heating of Venus's massive atmosphere. As a result, a Venusian day is 116.75 Earth days long, about half a Venusiansolar year, which is 224.7 Earth days long.(Full article...)

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Great Comet of 1577

  • ...that the passing of theGreat Comet of 1577 (pictured) caused almost century-long debate, during whichGalileo argued that comets were merely optical illusions?

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Solar System:Planets (Definition · Planetary habitability · Terrestrial planets · Gas giants · Rings· Dwarf planets (Plutoid· Colonization · Discovery timelineˑExploration · Moons · Planetariums

Sun:Sunspot · Solar wind · Solar flare · Solar eclipse
Mercury:Geology · Exploration (Mariner 10 · MESSENGER · BepiColombo· Transit
Venus:Geology · Atmosphere · Exploration (Venera · Mariner program2/5/10 · Pioneer · Vega1/2ˑMagellan · Venus Express· Transit
Earth:History · Geology · Geography · Atmosphere · Rotation
Moon:Geology · Selenography · Atmosphere · Exploration (Luna · Apollo8/11· Orbit · Lunar eclipse
Mars:Moons(Phobos · Deimos) · Geology · Geography · Atmosphere · Exploration (Mariner · Mars · Viking1/2 · Pathfinder · MER)
Ceres:Exploration (Dawn)
Jupiter:Moons(Amalthea,Io · Europa · Ganymede · Callisto) · Rings · Atmosphere · Magnetosphere · Exploration (Pioneer10/11 · Voyager1/2 · Ulysses · Cassini · Galileo · New Horizons)
Saturn:Moons(Mimas · Enceladus · Tethys · Dione · Rhea · Titan · Iapetus) · Rings · Exploration (Pioneer 11 · Voyager1/2 · CassiniHuygens)
Uranus:Moons(Miranda · Ariel · Umbriel · Titania · Oberon) · Rings · Exploration (Voyager 2)
Neptune:Moons(Triton) · Rings · Exploration (Voyager 2)
Planets beyond Neptune
Pluto:Moons(Charon,Nix,Hydra,Kerberos,Styx) · Geology · Atmosphere · Exploration (New Horizons)
Haumea:Moons(Hi'iaka,Namaka) · Ring
Quaoar:Weywot · Rings
Makemake:S/2015 (136472) 1
Gonggong:Xiangliu
Eris:Dysnomia
Sedna
Small bodies:Meteoroids · Asteroids (Asteroid belt· Centaurs · TNOs (Kuiper belt · Scattered disc · Oort cloud· Comets (Hale–Bopp · Halley's · Hyakutake · Shoemaker–Levy 9)
Formation and evolution of the Solar System:History of Solar System formation and evolution hypotheses · Nebular hypothesis
See also:Featured content · Featured topic · Good articles · List of objects

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Italicized articles are on dwarf planets or major moons.

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The planet Saturn, see here eclipsing the sun
The planet Saturn, see here eclipsing the sun

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