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

The Solar System is the gravitationally bound system of the Sun and the objects that orbit it. It was formed 4.6 billion years ago when a dense region of a molecular cloud collapsed, forming the Sun and a protoplanetary disc. The Sun is an ordinary main sequence star that maintains a balanced equilibrium by the fusion of hydrogen into helium at its core, releasing this energy from its outer photosphere.

The largest objects that orbit the Sun are the eight planets. In order from the Sun, they are four terrestrial planets ( Mercury, Venus, Earth and Mars); two gas giants ( Jupiter and Saturn); and two ice giants ( Uranus and Neptune). All terrestrial planets have solid surfaces. Inversely, all giant planets do not have a definite surface, as they are mainly composed of gases and liquids. Over 99.86% of the Solar System's mass is in the Sun and nearly 90% of the remaining mass is in Jupiter and Saturn.

There is a strong consensus among astronomers that the Solar System has at least eight dwarf planets: Ceres, Pluto, Haumea, Quaoar, Makemake, Gonggong, Eris, and Sedna. There are a vast number of small Solar System bodies, such as asteroids, comets, centaurs, meteoroids, and interplanetary dust clouds. Some of these bodies are in the asteroid belt (between Mars's and Jupiter's orbit) and the Kuiper belt (just outside Neptune's orbit). Six planets, six dwarf planets, and other bodies have orbiting natural satellites, which are commonly called 'moons'.

The Solar System is constantly flooded by the Sun's charged particles, the solar wind, forming the heliosphere. Around 75–90 astronomical units, the solar wind is halted, resulting in the heliopause. This is the boundary of the Solar System to interstellar space. The outermost region of the Solar System is the theorized Oort cloud, the source for long-period comets, extending 2,000–200,000 astronomical units (0.032–3.2 light-years). The closest star to the Solar System, Proxima Centauri, is 4.25 light-years away. Both stars belong to the Local Group and the Milky Way galaxy. ( Full article...)

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Galileo image of 243 Ida. The tiny dot to the right is its moon, Dactyl.
Galileo image of 243 Ida. The tiny dot to the right is its moon, Dactyl.
243 Ida is an asteroid in the Koronis family of the main belt. It was discovered on 29 September 1884 by Johann Palisa and named after a nymph from Greek mythology. Later telescopic observations categorized Ida as an S-type asteroid, the most numerous type in the inner asteroid belt. On 28 August 1993, Ida was visited by the spacecraft Galileo, bound for Jupiter. It was the second asteroid to be visited by a spacecraft and the first found to possess a satellite. Like all main-belt asteroids, Ida's orbit lies between the planets Mars and Jupiter. Its orbital period is 4.84 years, and its rotation period is 4.63 hours. Ida has an average diameter of 31.4 km (19.5 mi). It is irregularly shaped and elongated, and apparently composed of two large objects connected together in a shape reminiscent of a croissant. Its surface is one of the most heavily cratered in the Solar System, featuring a wide variety of crater sizes and ages. Ida's moon, Dactyl, was discovered by mission member Ann Harch in images returned from Galileo. It was named after creatures which inhabited Mount Ida in Greek mythology. Data returned from the flyby pointed to S-type asteroids as the source for the ordinary chondrite meteorites, the most common type found on the Earth's surface. ( Full article...)

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

Sun: Sunspot · Solar wind · Solar flare · Solar eclipse
Mercury: Geology · Exploration ( Mariner 10 · MESSENGER · BepiColombo· Transit
Venus: Geology · Atmosphere · Exploration ( Venera · Mariner program 2/ 5/ 10 · Pioneer · Vega 1/ 2ˑ Magellan · Venus Express· Transit
Earth: History · Geology · Geography · Atmosphere · Rotation
Moon: Geology · Selenography · Atmosphere · Exploration ( Luna · Apollo 8/ 11· Orbit · Lunar eclipse
Mars: Moons ( Phobos · Deimos) · Geology · Geography · Atmosphere · Exploration ( Mariner · Mars · Viking 1/ 2 · Pathfinder · MER)
Ceres: Exploration ( Dawn)
Jupiter: Moons ( Amalthea, Io · Europa · Ganymede · Callisto) · Rings · Atmosphere · Magnetosphere · Exploration ( Pioneer 10/ 11 · Voyager 1/ 2 · Ulysses · Cassini · Galileo · New Horizons)
Saturn: Moons ( Mimas · Enceladus · Tethys · Dione · Rhea · Titan · Iapetus) · Rings · Exploration ( Pioneer 11 · Voyager 1/ 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) · Exploration ( New Horizons)
Haumea: Moons ( Hi'iaka, Namaka)
Makemake
Eris: Dysnomia
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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The planet Saturn, see here eclipsing the sun
The planet Saturn, see here eclipsing the sun

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