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WHAT IS SOLAR SYSTEM?


340px-Planets2013
Age4.568 billion years

Location
Local Interstellar Cloud, Local Bubble,
Orion–Cygnus Arm, Milky Way
System mass1.0014 Solar masses
Nearest star


Proxima Centauri(4.22 ly)

Alpha Centaurisystem(4.37 ly)

Nearest known planetary systemAlpha Centauri system(4.37 ly)


Planetary system
Semi-major axisof outer planet( Neptune)30.10 AU(4.503 billion km)


Distance to Kuiper cliff50 AU


Populations

Stars1( Sun)


Planets
8 ( Mercury Venus Earth Mars
Jupiter Saturn Uranus Neptune)



Known dwarf planets
Possibly several hundred; [ 1 ]
five currently recognized by the IAU
( Ceres Pluto Haumea Makemake Eris)



Known natural satellites
450
(173 planetary [ 2 ]277 minor planetary [ 3 ])


Known minor planets688,621(as of 2015-07-18) [ 4 ]



Known comets3,354(as of 2015-07-18) [ 4 ]



Identified rounded satellites19


Orbit about Galactic Center

Invariable-to- galactic

planeinclination60.19°(ecliptic)

Distance to Galactic

Center27,000 ± 1,000 ly


Orbital speed220 km/s


Orbital period225–250 Myr




Star-related properties


Spectral type G2V

THE MEANING AND DEFINITION OF

SOLAR SYSTEM


The Solar System comprises the Sun and the objects that orbit it, either directly or indirectly. Of those objects that orbit the Sun directly, the largest eight are the planets that form the planetary systemaround it, while the remainder are significantly smaller objects, such as dwarf planetsand small Solar System bodiessuch as cometsand asteroids. Of those that orbit the Sun indirectly, two are larger than the smallest planet.


The Solar System formed 4.6 billion years agofrom the gravitational collapse of a giant interstellar molecular cloud. The vast majority of the system's massis in the Sun, with most of the remaining mass contained in Jupiter. The four smaller inner planets, Mercury, Venus, Earthand Mars, are terrestrial planets, being primarily composed of rock and metal. The four outer planets are giant planets, being substantially more massive than the terrestrials. The two largest, Jupiter and Saturn, are gas giants, being composed mainly of hydrogenand helium;the two outermost planets, Uranus and Neptune, are ice giants, being composed largely of substances with relatively high melting points compared with hydrogen and helium, called ices, such as water, ammonia and methane.

All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic.

The Solar System also contains smaller objects. The asteroid belt, which lies between Mars and Jupiter, mostly contains objects composed, like the terrestrial planets, of rock and metal. Beyond Neptune's orbit lie the Kuiper beltand scattered disc, populations of trans-Neptunian objectscomposed mostly of ices, and beyond them a newly discovered population of sednoids. Within these populations are several dozen to possibly tens of thousands of objects large enough to have been rounded by their own gravity. Such objects are categorized as dwarf planets. Identified dwarf planets include the asteroid Ceresand the trans-Neptunian objects Plutoand Eris.

In addition to these two regions, various other small-body populations, including comets, centaursand interplanetary dust, freely travel between regions. Six of the planets, at least three of the dwarf planets, and many of the smaller bodies are orbited by natural satellites, usually termed "moons" after the Moon. Each of the outer planets is encircled by planetary ringsof dust and other small objects.
The solar wind, plasmaflowing outwards from the Sun, creates a bubblein the interstellar mediumknown as the heliosphere. The heliopauseis the point at which pressure from the solar wind is equal to the opposing pressure of interstellar wind; it extends out to the edge of the scattered disc. The Oort cloud, which is believed to be the source for long-period comets, may also exist at a distance roughly a thousand times further than the heliosphere. The Solar System is located in the Orion Arm, 26,000 light-years from the center of the Milky Way.
Solarsystem
Our solar system consists of an average star we call the Sun, the planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto. It includes: the satellites of the planets; numerous comets, asteroids, and meteoroids; and the interplanetary medium. The Sun is the richest source of electromagnetic energy (mostly in the form of heat and light) in the solar system. The Sun's nearest known stellar neighbor is a red dwarf star called Proxima Centauri, at a distance of 4.3 light yearsaway. The whole solar system, together with the local stars visible on a clear night, orbits the center of our home galaxy, a spiral disk of 200 billion stars we call the Milky Way. The Milky Way has two small galaxies orbiting it nearby, which are visible from the southern hemisphere. They are called the Large Magellanic Cloud and the Small Magellanic Cloud. The nearest large galaxy is the Andromeda Galaxy. It is a spiral galaxy like the Milky Way but is 4 times as massive and is 2 million light years away.

Main article: Discovery and exploration of the Solar System
For many thousands of years, humanity, with a few notable exceptions, did not recognize the existence of the Solar System.


220px-HeliocentricPeople believed Earth to be stationary at the centre of the universeand categorically different from the divine or ethereal objects that moved through the sky. Although the Greekphilosopher Aristarchus of Samoshad speculated on a heliocentric reordering of the cosmos, Nicolaus Copernicuswas the first to develop a mathematically predictive heliocentricsystem. In the 17th-century, Galileo Galilei, Johannes Keplerand Isaac Newton, developed an understanding of physicsthat led to the gradual acceptance of the idea that Earth moves around the Sun and that the planets are governed by the same physical laws that governed Earth. The invention of the telescope led to the discovery of further planets and moons. Improvements in the telescope and the use of unmanned spacecrafthave enabled the investigation of geological phenomena, such as mountains, craters, seasonal meteorological phenomena, such as clouds, dust stormsand ice capson the other planets.
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STRUCTURE AND COMPOSITION

300px-Oort cloud Sedna orbit.svgThe orbitsof the bodies in the Solar System to scale (clockwise from top left)
The principal component of the Solar System is the Sun, a G2 main-sequence starthat contains 99.86% of the system's known mass and dominates it gravitationally.The Sun's four largest orbiting bodies, the giant planets, account for 99% of the remaining mass, with Jupiter and Saturn together comprising more than 90%. The remaining objects of the Solar System (including the four terrestrial planets, the dwarf planets, moons, asteroids, and comets) together comprise less than 0.002% of the Solar System's total mass.
Most large objects in orbit around the Sun lie near the plane of Earth's orbit, known as the ecliptic. The planets are very close to the ecliptic, whereas comets and Kuiper beltobjects are frequently at significantly greater angles to it. All the planets and most other objects orbit the Sun in the same direction that the Sun is rotating (counter-clockwise, as viewed from above Earth's north pole). There are exceptions, such as Halley's Comet.
The overall structure of the charted regions of the Solar System consists of the Sun, four relatively small inner planets surrounded by a next belt of mostly rocky asteroids, and four giant planets surrounded by the Kuiper belt of mostly icy objects. Astronomers sometimes informally divide this structure into separate regions. The inner Solar System includes the four terrestrial planets and the asteroid belt. The outer Solar System is beyond the asteroids, including the four giant planets. [ 20 ]Since the discovery of the Kuiper belt, the outermost parts of the Solar System are considered a distinct region consisting of the objects beyond Neptune.

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