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A number of solar-orbiting meteoroids were large enough to be tracked in space before striking Earth.
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Solar System
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It is now widely accepted that collisions in the past have had a significant role in shaping the geological and biological history of Earth.
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Solar System
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Mars-crossing asteroids are those with perhihelia above 1.3 AU which cross the orbit of Mars.
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Solar System
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As of 2024, NASA lists 26,182 confirmed Mars-crossing asteroids.
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Solar System
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Asteroid belt The asteroid belt occupies a torus-shaped region between 2.3 and 3.3 AU from the Sun, which lies between the orbits of Mars and Jupiter.
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Solar System
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It is thought to be remnants from the Solar System's formation that failed to coalesce because of the gravitational interference of Jupiter.
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Solar System
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The asteroid belt contains tens of thousands, possibly millions, of objects over one kilometer in diameter.
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Solar System
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Despite this, the total mass of the asteroid belt is unlikely to be more than a thousandth of that of Earth.
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Solar System
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The asteroid belt is very sparsely populated; spacecraft routinely pass through without incident.
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Solar System
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Below are the descriptions of the three largest bodies in the asteroid belt.
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Solar System
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They are all considered to be relatively intact protoplanets, a precursor stage before becoming a fully-formed planet (see List of exceptional asteroids): Ceres (2.55–2.98 AU) is the only dwarf planet in the asteroid belt.
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Solar System
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It is the largest object in the belt, with a diameter of 940 km (580 mi).
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Solar System
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Its surface contains a mixture of carbon, frozen water and hydrated minerals.
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Solar System
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There are signs of past cryovolcanic activity, where volatile material such as water are erupted onto the surface, as seen in surface bright spots.
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Solar System
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Ceres has a very thin water vapor atmosphere, but practically speaking it is indistinguishable from a vacuum.
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Solar System
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Vesta (2.13–3.41 AU) is the second-largest object in the asteroid belt.
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Solar System
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Its fragments survive as the Vesta asteroid family and numerous HED meteorites found on Earth.
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Solar System
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Vesta's surface, dominated by basaltic and metamorphic material, has a denser composition than Ceres's.
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Solar System
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Its surface is marked by two giant craters: Rheasilvia and Veneneia.
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Solar System
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Pallas (2.15–2.57 AU) is the third-largest object in the asteroid belt.
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Solar System
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It has its own Pallas asteroid family.
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Solar System
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Not much is known about Pallas because it has never been visited by a spacecraft, though its surface is predicted to be composed of silicates.
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Solar System
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Hilda asteroids are in a 3:2 resonance with Jupiter; that is, they go around the Sun three times for every two Jovian orbits.
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Solar System
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They lie in three linked clusters between Jupiter and the main asteroid belt.
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Solar System
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Trojans are bodies located within another body's gravitationally stable Lagrange points: L4, 60° ahead in its orbit, or L5, 60° behind in its orbit.
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Solar System
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Every planet except Mercury is known to possess at least one trojan.
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Solar System
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The Jupiter trojan population is roughly equal to that of the asteroid belt.
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Solar System
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After Jupiter, Neptune possesses the most confirmed trojans, at 28.
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Solar System
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Outer Solar System The outer region of the Solar System is home to the giant planets and their large moons.
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Solar System
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The centaurs and many short-period comets orbit in this region.
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Solar System
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Due to their greater distance from the Sun, the solid objects in the outer Solar System contain a higher proportion of volatiles such as water, ammonia, and methane, than planets of the inner Solar System because their lower temperatures allow these compounds to remain solid, without significant sublimation.
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Solar System
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Outer planets The four outer planets, called giant planets or Jovian planets, collectively make up 99% of the mass orbiting the Sun.
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Solar System
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All four giant planets have multiple moons and a ring system, although only Saturn's rings are easily observed from Earth.
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Solar System
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Jupiter and Saturn are composed mainly of gases with extremely low melting points, such as hydrogen, helium, and neon, hence their designation as gas giants.
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Solar System
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Uranus and Neptune are ice giants, meaning they are largely composed of 'ice' in the astronomical sense (chemical compounds with melting points of up to a few hundred kelvins such as water, methane, ammonia, hydrogen sulfide, and carbon dioxide.)
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Solar System
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Icy substances comprise the majority of the satellites of the giant planets and small objects that lie beyond Neptune's orbit.
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Solar System
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Jupiter (4.95–5.46 AU) is the biggest and most massive planet in the Solar System.
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Solar System
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On its surface, there are orange-brown and white cloud bands moving via the principles of atmospheric circulation, with giant storms swirling on the surface such as the Great Red Spot and white 'ovals'.
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Solar System
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Jupiter possesses a strong enough magnetosphere to redirect ionizing radiation and cause auroras on its poles.
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Solar System
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As of 2025, Jupiter has 97 confirmed satellites, which can roughly be sorted into three groups: The Amalthea group, consisting of Metis, Adrastea, Amalthea, and Thebe.
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Solar System
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They orbit substantially closer to Jupiter than other satellites.
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Solar System
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Materials from these natural satellites are the source of Jupiter's faint ring.
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Solar System
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The Galilean moons, consisting of Ganymede, Callisto, Io, and Europa.
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Solar System
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They are the largest moons of Jupiter and exhibit planetary properties.
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Solar System
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Irregular satellites, consisting of substantially smaller natural satellites.
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Solar System
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They have more distant orbits than the other objects.
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Solar System
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Saturn (9.08–10.12 AU) has a distinctive visible ring system orbiting around its equator composed of small ice and rock particles.
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Solar System
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Like Jupiter, it is mostly made of hydrogen and helium.
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Solar System
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At its north and south poles, Saturn has peculiar hexagon-shaped storms larger than the diameter of Earth.
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Solar System
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Saturn has a magnetosphere capable of producing weak auroras.
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Solar System
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As of 2025, Saturn has 274 confirmed satellites, grouped into: Ring moonlets and shepherds, which orbit inside or close to Saturn's rings.
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Solar System
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A moonlet can only partially clear out dust in its orbit, while the ring shepherds are able to completely clear out dust, forming visible gaps in the rings.
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Solar System
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Inner large satellites Mimas, Enceladus, Tethys, and Dione.
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Solar System
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These satellites orbit within Saturn's E ring.
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Solar System
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They are composed mostly of water ice and are believed to have differentiated internal structures.
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Solar System
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Trojan moons Calypso and Telesto (trojans of Tethys), and Helene and Polydeuces (trojans of Dione).
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Solar System
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These small moons share their orbits with Tethys and Dione, leading or trailing either.
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Solar System
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Outer large satellites Rhea, Titan, Hyperion, and Iapetus.
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Solar System
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Titan is the only satellite in the Solar System to have a substantial atmosphere.
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Solar System
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Irregular satellites, consisting of substantially smaller natural satellites.
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Solar System
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They have more distant orbits than the other objects.
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Solar System
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Phoebe is the largest irregular satellite of Saturn.
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Solar System
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Uranus (18.3–20.1 AU), uniquely among the planets, orbits the Sun on its side with an axial tilt >90°.
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Solar System
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This gives the planet extreme seasonal variation as each pole points alternately toward and then away from the Sun.
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Solar System
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Uranus's outer layer has a muted cyan color, but underneath these clouds are many mysteries about its climate, such as unusually low internal heat and erratic cloud formation.
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Solar System
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As of 2025, Uranus has 28 confirmed satellites, divided into three groups: Inner satellites, which orbit inside Uranus's ring system.
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Solar System
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They are very close to each other, which suggests that their orbits are chaotic.
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Solar System
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Large satellites, consisting of Titania, Oberon, Umbriel, Ariel, and Miranda.
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Solar System
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Most of them have roughly equal amounts of rock and ice, except Miranda, which is made primarily of ice.
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Solar System
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Irregular satellites, having more distant and eccentric orbits than the other objects.
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Solar System
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Neptune (29.9–30.5 AU) is the furthest planet known in the Solar System.
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Solar System
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Its outer atmosphere has a slightly muted cyan color, with occasional storms on the surface that look like dark spots.
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Solar System
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Like Uranus, many atmospheric phenomena of Neptune are unexplained, such as the thermosphere's abnormally high temperature or the strong tilt (47°) of its magnetosphere.
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Solar System
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As of 2025, Neptune has 16 confirmed satellites, divided into two groups: Regular satellites, which have circular orbits that lie near Neptune's equator.
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Solar System
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Irregular satellites, which as the name implies, have less regular orbits.
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Solar System
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One of them, Triton, is Neptune's largest moon.
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Solar System
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It is geologically active, with erupting geysers of nitrogen gas, and possesses a thin, cloudy nitrogen atmosphere.
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Solar System
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Centaurs The centaurs are icy, comet-like bodies whose semi-major axes are longer than Jupiter's and shorter than Neptune's (between 5.5 and 30 AU).
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Solar System
https://en.wikipedia.org/wiki/Solar_System.https://en.wikipedia.org/wiki/Solar_System.https://en.wikipedia.org/wiki/Solar_System.https://en.wikipedia.org/wiki/Solar_System.https://en.wikipedia.org/wiki/Solar_System.https://en.wikipedia.org/wiki/Solar_System.https://en.wikipedia.org/wiki/Solar_System.https://en.wikipedi...
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These are former Kuiper belt and scattered disc objects (SDOs) that were gravitationally perturbed closer to the Sun by the outer planets, and are expected to become comets or be ejected out of the Solar System.
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Solar System
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While most centaurs are inactive and asteroid-like, some exhibit cometary activity, such as the first centaur discovered, 2060 Chiron, which has been classified as a comet (95P) because it develops a coma just as comets do when they approach the Sun.
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The largest known centaur, 10199 Chariklo, has a diameter of about 250 km (160 mi) and is one of the few minor planets possessing a ring system.
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Solar System
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Trans-Neptunian region Beyond the orbit of Neptune lies the area of the "trans-Neptunian region", with the doughnut-shaped Kuiper belt, home of Pluto and several other dwarf planets, and an overlapping disc of scattered objects, which is tilted toward the plane of the Solar System and reaches much further out than the ...
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The entire region is still largely unexplored.
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Solar System
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It appears to consist overwhelmingly of many thousands of small worlds – the largest having a diameter only a fifth that of Earth and a mass far smaller than that of the Moon – composed mainly of rock and ice.
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Solar System
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This region is sometimes described as the "third zone of the Solar System", enclosing the inner and the outer Solar System.
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Solar System
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Kuiper belt The Kuiper belt is a great ring of debris similar to the asteroid belt, but consisting mainly of objects composed primarily of ice.
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Solar System
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It extends between 30 and 50 AU from the Sun.
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Solar System
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It is composed mainly of small Solar System bodies, although the largest few are probably large enough to be dwarf planets.
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Solar System
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There are estimated to be over 100,000 Kuiper belt objects with a diameter greater than 50 km (30 mi), but the total mass of the Kuiper belt is thought to be only a tenth or even a hundredth the mass of Earth.
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Solar System
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Many Kuiper belt objects have satellites, and most have orbits that are substantially inclined (~10°) to the plane of the ecliptic.
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Solar System
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The Kuiper belt can be roughly divided into the "classical" belt and the resonant trans-Neptunian objects.
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Solar System
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The latter have orbits whose periods are in a simple ratio to that of Neptune: for example, going around the Sun twice for every three times that Neptune does, or once for every two.
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Solar System
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The classical belt consists of objects having no resonance with Neptune, and extends from roughly 39.4 to 47.7 AU.
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Members of the classical Kuiper belt are sometimes called "cubewanos", after the first of their kind to be discovered, originally designated 1992 QB1, (and has since been named Albion); they are still in near primordial, low-eccentricity orbits.
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There is strong consensus among astronomers that five members of the Kuiper belt are dwarf planets.
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Solar System
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Many dwarf planet candidates are being considered, pending further data for verification.
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Solar System
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Pluto (29.7–49.3 AU) is the largest known object in the Kuiper belt.
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Pluto has a relatively eccentric orbit, inclined 17 degrees to the ecliptic plane.
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Pluto has a 2:3 resonance with Neptune, meaning that Pluto orbits twice around the Sun for every three Neptunian orbits.
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Kuiper belt objects whose orbits share this resonance are called plutinos.
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Solar System
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