The Solar System. Our Solar System includes the Sun and the planetary system revolving around it. A “planetary system” is a group of non-stellar objects (planets, dwarf planets, moons, asteroids, meteoroids, comets and cosmic dust) that orbit around a star, the sun is classified as a star. The Solar System includes four terrestrial planets (composed of rock and metal) and four gas giants.
Planets and their moonsThe eight planets can be divided into two distinct categories on the basis of their densities (mass per unit volume). The four inner, or, planets—Mercury, Earth, and Mars—have rocky and densities greater than 3 grams per cubic cm. (Water has a of 1 gram per cubic cm.) In contrast, the four, also called the Jovian, or, planets—Jupiter, and Neptune—are large objects with densities less than 2 grams per cubic cm; they are composed primarily of and (Jupiter and Saturn) or of ice, hydrogen, and helium (Uranus and Neptune). The is unique—an icy, low-density body smaller than Earth’s, more similar to comets or to the large icy moons of the outer planets than to any of the planets themselves. Its acceptance as a member of the Kuiper belt explains these.The relatively small inner planets have solid surfaces, lack ring systems, and have few or no moons. The atmospheres of Venus, Earth, and are composed of a significant percentage of oxidized such as. Among the inner planets, only Earth has a strong, which shields it from the interplanetary medium.
The magnetic field traps some of the electrically charged particles of the interplanetary medium inside a region around Earth known as the. Heavy concentrations of these high-energy particles occur in the in the inner part of the magnetosphere.The four giant outer planets are much more massive than the terrestrial planets and have immense atmospheres composed mainly of hydrogen and helium. They have no solid surfaces, however, and their densities are so low that one of them, Saturn, would actually float in. Each of the outer planets has a magnetic field, a ring system, and many known moons, with more likely to be discovered. Pluto has no known rings and only five known moons.
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Several other Kuiper belt objects and some asteroids also have moons of their own. Jovian planets The Jovian—or gaseous, Jupiter-like—planets. Lunar and Planetary InstituteMost of the known moons move around their respective planets in the same direction that the planets orbit the. They are extremely, representing a wide range of. Is orbited by, a body wracked by intense volcanism, while Saturn’s largest moon, —a body larger than the terrestrial Mercury—exhibits a primitive denser than that of Earth. Moves in a orbit around Neptune—that is, opposite to the direction of the planet’s orbit around the Sun—and features plumes of material rising through its atmosphere from a surface whose temperature is only 37 kelvins (K; −393 °F, −236 °C).
AndThe s and s are remnants of the planet-building process in the inner and outer solar system, respectively. The asteroid belt is home to rocky bodies ranging in size from the largest known asteroid, (also classified by the as a dwarf planet), with a diameter of roughly 940 km (585 miles), to microscopic dust particles that are dispersed throughout the belt. Some asteroids travel in paths that cross the orbit of Earth, providing opportunities for collisions with the planet. The rare collisions of relatively large objects (those with diameters greater than about 1 km 0.6 mile) with Earth can be devastating, as in the case of the asteroid impact that is thought to have been responsible for the massive extinction of species at the end of the 65 million years ago ( see; ).
More commonly, the impacting objects are much smaller, reaching Earth’s surface as s. Asteroid observations from Earth, which have been confirmed by spacecraft flybys, indicate that some asteroids are mainly metal (principally iron), others are stony, and still others are rich in organic compounds, resembling the meteorites. The asteroids that have been visited by spacecraft are irregularly shaped objects pockmarked with craters; some of them have retained very primitive material from the early days of the solar system.
Gaspra, an asteroid of the main belt, in a composite of two images taken by the Galileo spacecraft during its flyby on October 29, 1991. Pocked with numerous small craters, Gaspra measures about 20 km (12 miles) in its longest dimension. Its irregular shape and groovelike linear markings suggest that it was once part of a larger body that experienced one or more shattering collisions.
Colours in the composite image have been enhanced by computer to highlight subtle variations in reflectivity and other surface characteristics. Duelyst forums download. NASA/JPL/CaltechThe physical characteristics of comet nuclei are fundamentally different from those of asteroids. Ices are their main, predominantly frozen water, but frozen, and other ices are also present.
These cosmic ice balls are laced with rock dust and a rich variety of organic compounds, many of which are collected in tiny grains. Some comets may have more such “dirt” than ice. Comet Wild 2 The icy nucleus of Comet Wild 2, in a composite image taken by the U.S. Stardust spacecraft during its close approach to the comet on January 2, 2004. The image consists of a short exposure to resolve fine details of the surface and a longer exposure to capture the faint jets of gas and dust streaming into space.
Wild 2's nucleus is about 5 km (3 miles) across. NASA/JPL/Stardust/University of Washington, SeattleComets can be classified according to their orbital period, the time it takes for them to revolve around the Sun. Comets that have orbital periods greater than 200 years (and usually much greater) are called long-period comets; those that make a return appearance in less time are short-period comets.
Each kind appears to have a distinct source.The nucleus of a typical long-period comet is irregularly shaped and a few kilometres across. It can have an orbital period of millions of years, and it spends most of its life at immense distances from the Sun, as much as one-fifth of the way to the nearest. This is the realm of the. The comet nuclei in this spherical shell are too distant to be visible from Earth. The presence of the cloud is presumed from the highly elliptical orbits—with eccentricities close to 1—in which the long-period comets are observed as they approach and then swing around the Sun.
Their orbits can be inclined in any direction—hence the that the Oort cloud is spherical. In contrast, most short-period comets, particularly those with periods of 20 years or less, move in rounder, prograde orbits near the plane of the solar system. Their source is believed to be the much nearer, which lies in the plane of the solar system beyond the orbit of. Comet nuclei in the Kuiper belt have been photographed from Earth with large telescopes.
Comet debris Learn about comet debris, including meteors (shooting stars). © Open University As comet nuclei trace out the parts of their orbits closest to the Sun, they are warmed through and begin to shed gases and dust, which form the familiar fuzzy-looking comas and long, wispy tails. The gas dissipates into space, but the grains of silicates and organic compounds remain to orbit the Sun along paths very similar to that of the parent comet. When Earth’s path around the Sun intersects one of these dust-populated orbits, a occurs.
During such an event, nighttime observers may see tens to hundreds of so-called shooting stars per hour as the dust grains burn up in the upper atmosphere of Earth. Although many random meteors can be observed nightly, they occur at a much higher rate during a meteor shower.
Even on an average day, Earth’s atmosphere is bombarded with more than 80 tons of dust grains, mostly asteroidal and cometary debris. TheIn addition to particles of debris ( see ), the space through which the planets travel contains s, s, and ions of the abundant elements, all streaming outward from the Sun in the form of the. Occasional giant s, short-lived eruptions on the Sun’s surface, expel matter (along with high-energy radiation) that contributes to this.In 2012 the space probe 1 crossed the boundary between the interplanetary medium and the —a region called the. Since passing through the heliopause, Voyager 1 has been able to measure the properties of interstellar space.