Sun Machine – Wikipedia

This article is ready the Sun and its planetary system. For different similar structures, see Planetary machine. For solar strength structures, see Photovoltaic gadget.

The Solar System[b] is the gravitationally bound machine SOLAR SYSTEM SOLAR SYSTEM of the Sun and the items that orbit it, either immediately or circuitously.[c] Of the items that orbit the Sun at once, the largest are the eight planets,[d] with the the rest being smaller items, the dwarf planets and small Solar System our bodies. Of the objects that orbit the Sun indirectly—the herbal satellites— are large than the smallest planet, Mercury.[e]

The Solar System fashioned 4.6 billion years in the past from the gravitational fall apart of a giant interstellar molecular cloud. The vast majority of the machine’s mass is within the Sun, with the majority of the last mass contained in Jupiter. The 4 smaller internal planets, Mercury, Venus, Earth and Mars, are terrestrial planets, being usually composed of rock and steel. The four outer planets are large planets, being considerably more massive than the terrestrials. Thebiggest planets, Jupiter and Saturn, are gas giants, being composed mainly of hydrogen and helium; the two outermost planets, Uranus and Neptune, are ice giants, being composed commonly of materials with particularly high melting factors in comparison with hydrogen and helium, known as volatiles, which includes water, ammonia and methane. All 8 planets have almost round orbits that lie inside a nearly flat disc called the ecliptic.

The Solar System also contains smaller gadgets. The asteroid belt, which lies between the orbits of Mars and Jupiter, typically consists of objects composed, like the terrestrial planets, of rock and metallic. Beyond Neptune’s orbit lie the Kuiper belt and scattered disc, that are populations of trans-Neptunian items composed usually of ices, and beyond them a newly determined population of sednoids. Within those populations, some items are huge enough to have rounded underneath their personal gravity, even though there may be massive debate as to how many there’ll prove to be.[nine][10] Such items are labeled as dwarf planets. The handiest sure dwarf planet is Pluto, with some other trans-Neptunian object, Eris, expected to be, and the asteroid Ceres at the least close to being a dwarf planet. In addition to thoseareas, numerous other small-frame populations, which include comets, centaurs and interplanetary dirt clouds, freely journey among areas. Six of the planets, the six largest possible dwarf planets, and the various smaller our bodies are orbited through natural satellites, usually termed “moons” after the Moon. Each of the outer planets is encircled via planetary rings of dust and different small objects.

The solar wind, a flow of charged debris flowing outwards from the Sun, creates a bubble-like area in the interstellar medium called the heliosphere. The heliopause is the point at which stress from the solar wind is same to the opposing stress of the interstellar medium; it extends out to the threshold of the scattered disc. The Oort cloud, that is notion to be the supply for long-duration comets, can also exist at a distance kind of one thousand instances in addition than the heliosphere. The Solar System is placed within the Orion Arm, 26,000 mild-years from the center of the Milky Way galaxy.

Discovery and exploration

Andreas Cellarius’s illustration of the Copernican gadget, from the Harmonia Macrocosmica (1660)

For maximum of records, humanity did not recognize or recognize the concept of the Solar System. Most human beings as much as the Late Middle Ages–Renaissance believed Earth to be desk bound at the centre of the universe and categorically extraordinary from the divine or airy gadgets that moved through the sky. Although the Greek philosopher Aristarchus of Samos had speculated on a heliocentric reordering of the cosmos, Nicolaus Copernicus was the primary to broaden a mathematically predictive heliocentric system.[eleven][12]

In the 17th century, Galileo found that the Sun turned into marked with sunspots, and that Jupiter had 4 satellites in orbit round it.[thirteen] Christiaan Huygens accompanied on from Galileo’s discoveries by means of discovering Saturn’s moon Titan and the shape of the jewelry of Saturn.[14] Around 1677, Edmond Halley discovered a transit of Mercury across the Sun, main him to recognize that observations of the sun parallax of a planet (greater ideally the usage of the transit of Venus) may be used to trigonometrically decide the distances between Earth, Venus, and the Sun.[15] In 1705, Halley realised that repeated sightings of a comet have been of the identical item, returning frequently as soon as every seventy five–seventy six years. This become the primary evidence that anything aside from the planets orbited the Sun,[16] even though this had been theorized approximately comets in the 1st century by means of Seneca.[17] Around 1704, the term “Solar System” first appeared in English.[18] In 1838, Friedrich Bessel successfully measured a stellar parallax, an apparent shift inside the position of a celeb created through Earth’s movement around the Sun, supplying the primary direct, experimental proof of heliocentrism.[19] Improvements in observational astronomy and using uncrewed spacecraft have given that enabled the detailed investigation of different bodies orbiting the Sun.

Comprehensive assessment of the Solar System. The Sun, planets, dwarf planets and moons are at scale for his or her relative sizes, now not for distances. A separate distance scale is at the bottom. Moons are listed near their planets via proximity of their orbits; best the largest moons are proven.

Structure and composition

The principal aspect of the Solar System is the Sun, a G2 foremost-collection megastar that incorporates 99.86% of the machine’s recognized mass and dominates it gravitationally.[20] The Sun’s 4 largest orbiting bodies, the large planets, account for ninety nine% of the last mass, with Jupiter and Saturn together comprising more than ninety%. The final items of the Solar System (which includes the four terrestrial planets, the dwarf planets, moons, asteroids, and comets) together incorporate less than zero.002% of the Solar System’s overall mass.

Most big gadgets in orbit around the Sun lie near the plane of Earth’s orbit, referred to as the ecliptic. The planets are very near the ecliptic, while comets and Kuiper belt objects are regularly at considerably more angles to it.[24][25] As a result of the formation of the Solar System, planets (and maximum other gadgets) orbit the Sun in the same direction that the Sun is rotating (counter-clockwise, as considered from above Earth’s north pole).[26] There are exceptions, inclusive of Halley’s Comet. Most of the larger moons orbit their planets in this prograde route (with Triton being the most important retrograde exception) and most large items rotate themselves in the same route (with Venus being a great retrograde exception).

The average structure of the charted areas of the Solar System consists of the Sun, 4 distinctly small inner planets surrounded with the aid of a belt of broadly speaking rocky asteroids, and four giant planets surrounded by using the Kuiper belt of typically icy objects. Astronomers every so often informally divide this structure into separate areas. The inner Solar System includes the 4 terrestrial planets and the asteroid belt. The outer Solar System is beyond the asteroids, such as the 4 massive planets.[27] Since the discovery of the Kuiper belt, the outermost components of the Solar System are taken into consideration a awesome place together with the gadgets past Neptune.[28]

Most of the planets in the Solar System have secondary structures of their very own, being orbited by using planetary items referred to as natural satellites, or moons ( of which, Titan and Ganymede, are large than the planet Mercury). The four giant planets have planetary earrings, skinny bands of tiny particles that orbit them in unison. Most of the biggest natural satellites are in synchronous rotation, with one face completely became towards their parent.[29]

All planets of the Solar System lie very near the ecliptic. The nearer they may be to the Sun, the faster they travel (inner planets at the left, all planets besides Neptune at the proper).

Kepler’s laws of planetary movement describe the orbits of gadgets approximately the Sun. Following Kepler’s legal guidelines, every object travels along an ellipse with the Sun at one focus. Objects towards the Sun (with smaller semi-major axes) travel more fast because they are extra tormented by the Sun’s gravity. On an elliptical orbit, a body’s distance from the Sun varies over the route of its 12 months. A body’s closest approach to the Sun is referred to as its perihelion, while its most distant factor from the Sun is known as its aphelion. The orbits of the planets are nearly circular, but many comets, asteroids, and Kuiper belt gadgets observe incredibly elliptical orbits. The positions of the our bodies within the Solar System may be expected the usage of numerical fashions.

Although the Sun dominates the gadget with the aid of mass, it accounts for most effective approximately 2% of the angular momentum.[30][31] The planets, dominated by means of Jupiter, account for maximum of the rest of the angular momentum because of the mixture in their mass, orbit, and distance from the Sun, with a probable giant contribution from comets.[30]

The Sun, which comprises almost all of the matter within the Solar System, consists of roughly ninety eight% hydrogen and helium.[32] Jupiter and Saturn, which include nearly all the final be counted, also are mainly composed of hydrogen and helium.[33][34] A composition gradient exists inside the Solar System, created by means of warmness and light strain from the Sun; the ones objects towards the Sun, that are greater suffering from warmness and light stress, are composed of factors with excessive melting factors. Objects further from the Sun are composed largely of materials with lower melting factors.[35] The boundary in the Solar System beyond which the ones risky substances could condense is known as the frost line, and it lies at kind of five AU from the Sun.[4]

The items of the inner Solar System are composed typically of rock,[36] the collective call for compounds with excessive melting factors, consisting of silicates, iron or nickel, that remained strong beneath almost all conditions inside the protoplanetary nebula.[37] Jupiter and Saturn are composed specially of gases, the astronomical time period for materials with extremely low melting points and excessive vapour pressure, which includes hydrogen, helium, and neon, which were continually in the gaseous phase in the nebula.[37] Ices, like water, methane, ammonia, hydrogen sulfide, and carbon dioxide,[36] have melting factors up to a few hundred kelvins.[37] They can be discovered as ices, beverages, or gases in diverse places in the Solar System, whereas within the nebula they were either in the strong or gaseous segment.[37] Icy substances incorporate the majority of the satellites of the large planets, in addition to most of Uranus and Neptune (the so-called “ice giants”) and the severa small objects that lie past Neptune’s orbit.[36][38] Together, gases and ices are called volatiles.[39]

Distances and scales

Size evaluation of the Sun and the planets (clickable)

The distance from Earth to the Sun is 1 astronomical unit [AU] (one hundred fifty,000,000 km; ninety three,000,000 mi). For evaluation, the radius of the Sun is 0.0047 AU (700,000 km). Thus, the Sun occupies zero.00001% (10−five %) of the volume of a sphere with a radius the dimensions of Earth’s orbit, whereas Earth’s extent is roughly one millionth (10−6) that of the Sun. Jupiter, the largest planet, is five.2 astronomical gadgets (780,000,000 km) from the Sun and has a radius of seventy one,000 km (0.00047 AU), while the most distant planet, Neptune, is 30 AU (four.five×109 km) from the Sun.

With some exceptions, the farther a planet or belt is from the Sun, the larger the gap between its orbit and the orbit of the following nearer item to the Sun. For instance, Venus is about zero.33 AU farther out from the Sun than Mercury, while Saturn is four.3 AU out from Jupiter, and Neptune lies 10.five AU out from Uranus. Attempts had been made to decide a relationship among these orbital distances (as an example, the Titius–Bode regulation),[forty] however no such idea has been time-honored.

Some Solar System models try and convey the relative scales worried in the Solar System on human terms. Some are small in scale (and may be mechanical—called orreries)—whereas others extend throughout cities or regional areas.[41] The biggest such scale version, the Sweden Solar System, uses the one hundred ten-metre (361 ft) Ericsson Globe in Stockholm as its substitute Sun, and, following the size, Jupiter is a 7.5-metre (25-foot) sphere at Stockholm Arlanda Airport, 40 km (25 mi) away, while the farthest contemporary object, Sedna, is a ten cm (four in) sphere in Luleå, 912 km (567 mi) away.[42][43]

If the Sun–Neptune distance is scaled to 100 metres, then the Sun might be about three cm in diameter (roughly -thirds the diameter of a golfing ball), the massive planets would be all smaller than about 3 mm, and Earth’s diameter at the side of that of the other terrestrial planets would be smaller than a flea (0.3 mm) at this scale.[forty four]

The Solar System. Distances are to scale, items are not.

Distances of decided on our bodies of the Solar System from the Sun. The left and right edges of each bar correspond to the perihelion and aphelion of the frame, respectively, therefore long bars denote excessive orbital eccentricity. The radius of the Sun is 0.7 million km, and the radius of Jupiter (the largest planet) is 0.07 million km, both too small to clear up on this photo.

Formation and evolution

The Solar System fashioned 4.568 billion years ago from the gravitational fall apart of a place inside a big molecular cloud.[h] This initial cloud changed into possibly numerous mild-years across and probably birthed numerous stars.[forty six] As is standard of molecular clouds, this one consisted basically of hydrogen, with some helium, and small amounts of heavier factors fused by using previous generations of stars. As the place that could come to be the Solar System, known as the pre-solar nebula,[47] collapsed, conservation of angular momentum triggered it to rotate quicker. The centre, in which most of the mass amassed, have become increasingly hotter than the encompassing disc.[forty six] As the contracting nebula rotated quicker, it commenced to flatten into a protoplanetary disc with a diameter of approximately 200 AU[46] and a warm, dense protostar on the centre.[forty eight][49] The planets formed through accretion from this disc,[50] in which dust and gasoline gravitationally attracted each different, coalescing to form ever larger bodies. Hundreds of protoplanets may additionally have existed within the early Solar System, but they either merged or were destroyed, leaving the planets, dwarf planets, and leftover minor bodies.[fifty one]

The geology of the contact binary object Arrokoth (nicknamed Ultima Thule), the first undisturbed planetesimal visited by means of a spacecraft, with comet 67P to scale. The 8 subunits of the bigger lobe, categorized ma to mh, are idea to have been its building blocks. The two lobes came together later, forming a contact binary. Objects which includes Arrokoth are believed in flip to have shaped protoplanets.[fifty two]

Due to their higher boiling points, best metals and silicates may want to exist in solid form within the warm internal Solar System close to the Sun, and these would sooner or later form the rocky planets of Mercury, Venus, Earth, and Mars. Because metal elements most effective comprised a very small fraction of the solar nebula, the terrestrial planets couldn’t develop very massive. The giant planets (Jupiter, Saturn, Uranus, and Neptune) shaped similarly out, beyond the frost line, the factor between the orbits of Mars and Jupiter where cloth is cool sufficient for risky icy compounds to remain stable. The ices that fashioned those planets were extra abundant than the metals and silicates that shaped the terrestrial inner planets, permitting them to grow large sufficient to seize large atmospheres of hydrogen and helium, the lightest and most ample factors. Leftover particles that by no means have become planets congregated in regions such as the asteroid belt, Kuiper belt, and Oort cloud.[51] The Nice model is an reason behind the advent of those regions and the way the outer planets may want to have fashioned in one of a kind positions and migrated to their cutting-edge orbits via diverse gravitational interactions.[53]

Within 50 million years, the stress and density of hydrogen inside the centre of the protostar became awesome sufficient for it to start thermonuclear fusion.[54] The temperature, reaction fee, pressure, and density increased till hydrostatic equilibrium became accomplished: the thermal stress equalled the force of gravity. At this factor, the Sun have become a primary-collection superstar.[fifty five] The essential-sequence section, from beginning to cease, will closing approximately 10 billion years for the Sun in comparison to roundbillion years for all different levels of the Sun’s pre-remnant existence blended.[fifty six] Solar wind from the Sun created the heliosphere and swept away the remaining fuel and dust from the protoplanetary disc into interstellar space, finishing the planetary formation method. The Sun is developing brighter; early in its essential-collection existence its brightness turned into 70% that of what it’s miles today.[fifty seven]

The Solar System will remain roughly as we comprehend it today until the hydrogen in the middle of the Sun has been absolutely transformed to helium, as a way to arise roughly 5 billion years from now. This will mark the stop of the Sun’s primary-sequence existence. At that time, the center of the Sun will agreement with hydrogen fusion going on alongside a shell surrounding the inert helium, and the strength output could be an awful lot more than at present. The outer layers of the Sun will make bigger to roughly 260 instances its present day diameter, and the Sun turns into a crimson giant. Because of its massively multiplied floor area, the surface of the Sun may be considerably cooler (2,600 K at its coolest) than it’s miles on the main sequence.[fifty six] The expanding Sun is anticipated to vaporize Mercury and render Earth uninhabitable. Eventually, the middle might be hot enough for helium fusion; the Sun will burn helium for a fragment of the time it burned hydrogen inside the middle. The Sun is not huge enough to commence the fusion of heavier elements, and nuclear reactions inside the middle will dwindle. Its outer layers will circulate away into area, leaving a white dwarf, an exceptionally dense item, half of the original mass of the Sun however only the dimensions of Earth.[58] The ejected outer layers will form what’s referred to as a planetary nebula, returning some of the fabric that fashioned the Sun—but now enriched with heavier factors like carbon—to the interstellar medium.


Main article: Sun

The Sun is the Solar System’s megastar and by a ways its maximum big element. Its big mass (332,900 Earth masses),[fifty nine] which incorporates ninety nine.86% of all of the mass inside the Solar System,[60] produces temperatures and densities in its core excessive sufficient to sustain nuclear fusion of hydrogen into helium, making it a prime-sequence superstar.[sixty one] This releases an enormous quantity of strength, primarily radiated into space as electromagnetic radiation peaking in visible light.[62]

The Sun is a G2-type most important-collection star. Hotter main-series stars are more luminous. The Sun’s temperature is intermediate among that of the hottest stars and that of the coolest stars. Stars brighter and warmer than the Sun are rare, whereas significantly dimmer and cooler stars, called pink dwarfs, make up eighty five% of the stars in the Milky Way.[sixty three][64]

The Sun is a populace I celebrity; it has a better abundance of factors heavier than hydrogen and helium (“metals” in astronomical parlance) than the older populace II stars.[65] Elements heavier than hydrogen and helium have been formed within the cores of historical and exploding stars, so the first generation of stars had to die earlier than the universe may be enriched with these atoms. The oldest stars contain few metals, while stars born later have more. This excessive metallicity is idea to have been vital to the Sun’s improvement of a planetary machine because the planets form from the accretion of “metals”.[sixty six]

Interplanetary medium

The big majority of the Solar System consists of a close to-vacuum known as the interplanetary medium. Along with mild, the Sun radiates a continuous circulate of charged particles (a plasma) known as the sun wind. This circulate of particles spreads outwards at roughly 1.5 million kilometres in step with hour,[sixty seven] growing a tenuous environment that permeates the interplanetary medium out to at least a hundred AU (see § Heliosphere).[sixty eight] Activity on the Sun’s surface, consisting of solar flares and coronal mass ejections, disturbs the heliosphere, growing space weather and causing geomagnetic storms.[sixty nine] The biggest shape inside the heliosphere is the heliospheric present day sheet, a spiral form created by means of the moves of the Sun’s rotating magnetic discipline on the interplanetary medium.[70][seventy one]

Earth’s magnetic discipline stops its ecosystem from being stripped away by using the sun wind.[seventy two] Venus and Mars do no longer have magnetic fields, and as a end result the solar wind is inflicting their atmospheres to steadily bleed away into space.[seventy three] Coronal mass ejections and comparable events blow a magnetic field and big portions of fabric from the surface of the Sun. The interaction of this magnetic subject and cloth with Earth’s magnetic area funnels charged particles into Earth’s upper environment, where its interactions create aurorae visible close to the magnetic poles.

The heliosphere and planetary magnetic fields (for the ones planets which have them) in part shield the Solar System from excessive-power interstellar particles referred to as cosmic rays. The density of cosmic rays inside the interstellar medium and the power of the Sun’s magnetic field change on very long timescales, so the level of cosmic-ray penetration within the Solar System varies, although with the aid of how plenty is unknown.[seventy four]

The interplanetary medium is home to as a minimum two disc-like regions of cosmic dirt. The first, the zodiacal dust cloud, lies in the internal Solar System and causes the zodiacal mild. It become probably formed with the aid of collisions inside the asteroid belt delivered on with the aid of gravitational interactions with the planets.[seventy five] The 2d dirt cloud extends from about 10 AU to approximately 40 AU, and became probable created through comparable collisions within the Kuiper belt.[76][seventy seven]

SOLAR SYSTEM Inner Solar System

The internal Solar System is the place comprising the terrestrial planets and the asteroid belt.[seventy eight] Composed in particular of silicates and metals, the objects of the inner Solar System are rather close to the Sun; the radius of this entire place is much less than the distance between the orbits of Jupiter and Saturn. This place is likewise inside the frost line, that’s a touch much less than five AU (about seven hundred million km) from the Sun.

Inner planets

Orrery displaying the motions of the internal 4 planets. The small spheres constitute the location of each planet on everyJulian days, starting August 3, 2020 and ending June 21, 2022 (Mars at perihelion).

The 4 terrestrial or internal planets have dense, rocky compositions, few or no moons, and no ring structures. They are composed in large part of refractory minerals along with the silicates—which shape their crusts and mantles—and metals which includes iron and nickel which form their cores. Three of the 4 inner planets (Venus, Earth and Mars) have atmospheres enormous sufficient to generate climate; all have impact craters and tectonic floor capabilities, such as rift valleys and volcanoes. The term internal planet need to now not be stressed with inferior planet, which designates those planets that are closer to the Sun than Earth is (i.e. Mercury and Venus).


Mercury (0.four AU from the Sun) is the nearest planet to the Sun and on SOLAR SYSTEM common, all seven different planets.[seventy nine][80] The smallest planet within the Solar System (zero.0.5 M⊕), Mercury has no herbal satellites. Besides impact craters, its most effective recognized geological features are lobed ridges or rupes that had been probably produced by a duration of contraction early in its records.[eighty one] Mercury’s very tenuous ecosystem consists of atoms blasted off its floor through the solar wind.[eighty two] Its highly large iron center and skinny mantle have no longer yet been competently defined. Hypotheses include that its outer layers were stripped off with the aid of a giant effect, or that it become averted from absolutely accreting by way of the younger Sun’s electricity.[eighty three][84]


Venus (zero.7 AU from the Sun) is near in size to Earth (0.815 M⊕) and, like Earth, has a thick silicate mantle round an iron middle, a considerable environment, and evidence of internal geological activity. It is a great deal drier than Earth, and its ecosystem is ninety times as dense. Venus has no natural satellites. It is the most up to date planet, with floor temperatures over 400 °C (752 °F), maximum in all likelihood due to the amount of greenhouse gases within the environment.[85] No definitive evidence of modern-day geological interest has been detected on Venus, but it has no magnetic subject that could save you depletion of its widespread ecosystem, which indicates that its atmosphere is being replenished by means of volcanic eruptions.[86]


Earth (1 AU from the Sun) is the most important and densest of the internal planets, the best one regarded to have current geological pastime, and the most effective region in which life is known to exist.[87] Its liquid hydrosphere is unique most of the terrestrial planets, and it is the best planet in which plate tectonics has been located. Earth’s surroundings is greatly distinctive from the ones of the other planets, having been altered through the presence of existence to include 21% loose oxygen.[88] It has one natural satellite tv for pc, the Moon, the handiest massive satellite of a terrestrial planet within the Solar System.


Main article: Mars

Mars (1.5 AU from the Sun) is smaller than Earth and Venus (0.107 M⊕). It has an surroundings of more often than not carbon dioxide with a floor pressure of 6.1 millibars (kind of zero.6% of that of Earth).[89] Its floor, peppered with enormous volcanoes, together with Olympus Mons, and rift valleys, together with Valles Marineris, shows geological activity which can have persevered until as these days as 2 million years in the past.[ninety] Its red shade comes from iron oxide (rust) in its soil.[ninety one] Mars hastiny herbal satellites (Deimos and Phobos) concept to be either captured asteroids,[92] or ejected particles from a large effect early in Mars’s history.[93]

Asteroid belt

Asteroids except for the biggest, Ceres, are categorized as small Solar System bodies and are composed specifically of refractory rocky and metal minerals, with some ice.[94][ninety five] They range from a few metres to loads of kilometres in length. Asteroids smaller than one meter are normally known as meteoroids and micrometeoroids (grain-sized), depending on distinctive, quite arbitrary definitions.

The asteroid belt occupies the orbit between Mars and Jupiter, among 2.3 and three.3 AU from the Sun. It is concept to be remnants from the Solar System’s formation that did not coalesce due to the gravitational interference of Jupiter.[96] The asteroid belt carries tens of heaps, probable thousands and thousands, of items over one kilometre in diameter.[ninety seven] Despite this, the entire mass of the asteroid belt is not likely to be more than a thousandth of that of Earth.[23] The asteroid belt may be very moderately populated; spacecraft routinely skip through without incident.[98]


Ceres – map of gravity fields: purple is excessive; blue, low.

Ceres (2.seventy seven AU) is the biggest asteroid, a protoplanet, and a dwarf planet. It has a diameter of slightly under 1000 km, and a mass huge sufficient for its very own gravity to pull it right into a round form. Ceres turned into taken into consideration a planet whilst it became discovered in 1801 and was reclassified to asteroid inside the 1850s as in addition observations revealed extra asteroids.[ninety nine] It changed into classified as a dwarf planet in 2006 whilst the definition of a planet turned into created.

Asteroid agencies

Asteroids in the asteroid belt are divided into asteroid companies and households primarily based on their orbital traits. Asteroid moons are asteroids that orbit larger asteroids. They are not as without a doubt outstanding as planetary moons, occasionally being nearly as big as their companions. The asteroid belt also includes principal-belt comets, which may additionally have been the supply of Earth’s water.[a hundred]

Jupiter trojans are placed in both of Jupiter’s L4 or L5 points (gravitationally strong regions main and trailing a planet in its orbit); the term trojan is likewise used for small bodies in another planetary or satellite Lagrange factor. Hilda asteroids are in a 2:3 resonance with Jupiter; that is, they move across the Sun 3 instances for every two Jupiter orbits.[one hundred and one]

The inner Solar System also incorporates near-Earth asteroids, many of which cross the orbits of the inner planets.[102] Some of them are probably hazardous gadgets.

Outer Solar System

The outer location of the Solar System is home to the large planets and their big moons. The centaurs and lots of short-period comets also orbit on this place. Due to their extra distance from the Sun, the solid items within the outer Solar System contain a higher proportion of volatiles, which includes water, ammonia, and methane than the ones of the inner Solar System due to the fact the lower temperatures allow those compounds to remain stable.[fifty one]

Outer planets

Orrery displaying the motions of the outer 4 planets. The small spheres represent the location of every planet on every 2 hundred Julian days, beginning November 18, 1877 and ending September 3, 2042 (Neptune at perihelion).

The four outer planets, or giant planets (once in a while known as Jovian planets), together make up 99% of the mass regarded to orbit the Sun. Jupiter and Saturn are collectively greater than four hundred instances the mass of Earth and consist overwhelmingly of the gases hydrogen and helium, therefore their designation as fuel giants.[103] Uranus and Neptune are a ways much less large—much less than 20 Earth loads (M⊕) each—and are composed by and large of ices. For these motives, some astronomers endorse they belong in their personal class, ice giants.[104] All 4 massive planets have rings, although simplest Saturn’s ring system is without problems determined from Earth. The term superior planet designates planets out of doors Earth’s orbit and as a consequence includes each the outer planets and Mars.


Jupiter (5.2 AU), at 318 M⊕, is 2.five instances the mass of all the other planets prepare. It is composed in large part of hydrogen and helium. Jupiter’s sturdy internal warmth creates semi-everlasting functions in its atmosphere, consisting of cloud bands and the Great Red Spot. Jupiter has 79 known satellites. The four largest, Ganymede, Callisto, Io, and Europa, show similarities to the terrestrial planets, such as volcanism and inner heating.[one zero five] Ganymede, the most important satellite tv for pc inside the Solar System, is bigger than Mercury.


Saturn (9.5 AU), outstanding via its large ring machine, has several similarities to Jupiter, consisting of its atmospheric composition and magnetosphere. Although Saturn has 60% of Jupiter’s quantity, it is less than a 3rd as large, at ninety five M⊕. Saturn is the most effective planet of the Solar System that is less dense than water.[106] The jewelry of Saturn are made of small ice and rock debris. Saturn has 82 showed satellites composed largely of ice. Two of those, Titan and Enceladus, display signs of geological activity.[107] Titan, the second-biggest moon inside the Solar System, is larger than Mercury and the simplest satellite tv for pc within the Solar System with a giant surroundings.


Uranus (19.2 AU), at 14 M⊕, is the lightest of the outer planets. Uniquely many of the planets, it orbits the Sun on its side; its axial tilt is over ninety levels to the ecliptic. It has a far colder core than the alternative giant planets and radiates little or no warmth into area.[108] Uranus has 27 known satellites, the biggest ones being Titania, Oberon, Umbriel, Ariel, and Miranda.[109]


Neptune (30.1 AU), though slightly smaller than Uranus, is extra massive (17 M⊕) and therefore greater dense. It radiates greater internal heat, but no longer as a whole lot as Jupiter or Saturn.[one hundred ten] Neptune has 14 regarded satellites. The largest, Triton, is geologically lively, with geysers of liquid nitrogen.[111] Triton is the simplest big satellite tv for pc with a retrograde orbit. Neptune is accompanied in its orbit through numerous minor planets, termed Neptune trojans, which can be in 1:1 resonance with it.


The centaurs are icy comet-like our bodies whose orbits have semi-important axes extra than Jupiter’s (five.5 AU) and less than Neptune’s (30 AU). The largest known centaur, 10199 Chariklo, has a diameter of about 250 km.[112] The first centaur located, 2060 Chiron, has additionally been categorised as a comet (95P) because it develops a coma just as comets do after they method the Sun.[113]


Comets are small Solar System bodies, typically just a few kilometres throughout, composed largely of unstable ices. They have especially eccentric orbits, normally a perihelion in the orbits of the inner planets and an aphelion a ways beyond Pluto. When a comet enters the inner Solar System, its proximity to the Sun reasons its icy surface to sublimate and ionise, growing a coma: a long tail of fuel and dust regularly visible to the bare eye.

Short-duration comets have orbits lasting less than two hundred years. Long-length comets have orbits lasting lots of years. Short-length comets are concept to originate within the Kuiper belt, whereas long-period comets, along with Hale–Bopp, are concept to originate within the Oort cloud. Many comet organizations, together with the Kreutz Sungrazers, formed from the breakup of a single determine.[114] Some comets with hyperbolic orbits may originate out of doors the Solar System, but figuring out their specific orbits is tough.[a hundred and fifteen] Old comets whose volatiles have normally been pushed out through sun warming are often classified as asteroids.[116]

Trans-Neptunian place

Beyond the orbit of Neptune lies the area of the “trans-Neptunian place”, with the doughnut-fashioned Kuiper belt, domestic of Pluto and numerous different dwarf planets, and an overlapping disc of scattered items, which is tilted toward the aircraft of the Solar System and reaches lots in addition out than the Kuiper belt. The whole place continues to be largely unexplored. It seems to consist overwhelmingly of many heaps of small worlds—the biggest having a diameter most effective a fifth that of Earth and a mass far smaller than that of the Moon—composed specially of rock and ice. This vicinity is every so often described as the “0.33 region of the Solar System”, enclosing the internal and the outer Solar System.[117]

Kuiper belt

The Kuiper belt is a exceptional ring of particles much like the asteroid belt, but consisting in particular of objects composed generally of ice.[118] It extends among 30 and 50 AU from the Sun. Though it’s far anticipated to contain something from dozens to hundreds of dwarf planets, it is composed mainly of small Solar System our bodies. Many of the larger Kuiper belt objects, such as Quaoar, Varuna, and Orcus, can also show to be dwarf planets with similarly records. There are anticipated to be over a hundred,000 Kuiper belt objects with a diameter extra than 50 km, however the overall mass of the Kuiper belt is idea to be simplest a tenth or maybe a hundredth the mass of Earth.[22] Many Kuiper belt gadgets have more than one satellites,[119] and maximum have orbits that take them outside the aircraft of the ecliptic.[120]

The Kuiper belt can be kind of divided into the “classical” belt and the resonances.[118] Resonances are orbits connected to that of Neptune (e.g. twice for every three Neptune orbits, or once for every ). The first resonance starts offevolved inside the orbit of Neptune itself. The classical belt includes gadgets having no resonance with Neptune, and extends from more or less 39.4 AU to 47.7 AU.[121] Members of the classical Kuiper belt are classified as cubewanos, after the primary of their type to be discovered, 15760 Albion (which previously had the provisional designation 1992 QB1), and are nevertheless in close to primordial, low-eccentricity orbits.[122]

Pluto and Charon

The dwarf planet Pluto (with a mean orbit of 39 AU) is the biggest recognized item inside the Kuiper belt. When determined in 1930, it become considered to be the 9th planet; this changed in 2006 with the adoption of a formal definition of planet. Pluto has a incredibly eccentric orbit willing 17 stages to the ecliptic aircraft and starting from 29.7 AU from the Sun at perihelion (in the orbit of Neptune) to forty nine.5 AU at aphelion. Pluto has a 3:2 resonance with Neptune, which means that Pluto orbits twice spherical the Sun for each 3 Neptunian orbits. Kuiper belt items whose orbits percentage this resonance are known as plutinos.[123]

Charon, the biggest of Pluto’s moons, is every so often described as part of a binary device with Pluto, as the 2 our bodies orbit a barycentre of gravity above their surfaces (i.e. they appear to “orbit each other”). Beyond Charon, 4 an awful lot smaller moons, Styx, Nix, Kerberos, and Hydra, orbit within the machine.

Makemake and Haumea

Makemake (45.seventy nine AU average), although smaller than Pluto, is the most important acknowledged item in the classical Kuiper belt (that is, a Kuiper belt object not in a showed resonance with Neptune). Makemake is the brightest item inside the Kuiper belt after Pluto. It became assigned a naming committee under the expectancy that it’d show to be a dwarf planet in 2008.[6] Its orbit is far extra inclined than Pluto’s, at 29°.[124]

Haumea (forty three.thirteen AU average) is in an orbit similar to Makemake, except that it’s far in a brief 7:12 orbital resonance with Neptune.[one hundred twenty five]

It turned into named below the equal expectation that it would show to be a dwarf planet, although next observations have indicated that it is able to no longer be a dwarf planet in any case.[126]

Scattered disc

The scattered disc, which overlaps the Kuiper belt however extends out to approximately two hundred AU, is notion to be the supply of brief-period comets. Scattered-disc gadgets are concept to have been ejected into erratic orbits by using the gravitational influence of Neptune’s early outward migration. Most scattered disc objects (SDOs) have perihelia in the Kuiper belt but aphelia far beyond it (a few greater than one hundred fifty AU from the Sun). SDOs’ orbits also are enormously willing to the ecliptic aircraft and are often nearly perpendicular to it. Some astronomers recall the scattered disc to be simply every other region of the Kuiper belt and describe scattered disc items as “scattered Kuiper belt gadgets”.[127] Some astronomers also classify centaurs as inward-scattered Kuiper belt items along with the outward-scattered residents of the scattered disc.[128]


Eris (with an average orbit of 68 AU) is the largest recognised scattered disc object, and brought on a debate about what constitutes a planet, because it’s miles 25% more massive than Pluto[129] and about the equal diameter. It is the maximum large of the acknowledged dwarf planets. It has one regarded moon, Dysnomia. Like Pluto, its orbit is incredibly eccentric, with a perihelion of 38.2 AU (more or less Pluto’s distance from the Sun) and an aphelion of ninety seven.6 AU, and steeply inclined to the ecliptic aircraft.

Farthest areas

The factor at which the Solar System ends and interstellar space starts offevolved isn’t exactly defined because its outer barriers are shaped by usingforces, the solar wind and the Sun’s gravity. The limit of the solar wind’s affect is more or less 4 times Pluto’s distance from the Sun; this heliopause, the outer boundary of the heliosphere, is considered the start of the interstellar medium.[sixty eight] The Sun’s Hill sphere, the powerful range of its gravitational dominance, is notion to extend up to 1000 times farther and encompasses the hypothetical Oort cloud.[a hundred thirty]


The heliosphere is a stellar-wind bubble, a place of area dominated by way of the Sun, wherein it radiates its solar wind at about 400 km/s, a stream of charged debris, till it collides with the wind of the interstellar medium.

The collision occurs on the termination surprise, that’s more or less eighty–a hundred AU from the Sun upwind of the interstellar medium and roughly two hundred AU from the Sun downwind.[131] Here the wind slows dramatically, condenses and becomes greater turbulent,[131] forming a extraordinary oval structure referred to as the heliosheath. This structure is notion to appearance and behave very similar to a comet’s tail, extending outward for a further 40 AU on the upwind aspect but tailing frequently that distance downwind; evidence from the Cassini and Interstellar Boundary Explorer spacecraft has suggested that it’s miles compelled right into a bubble form by using the constraining movement of the interstellar magnetic subject.[132]

The outer boundary of the heliosphere, the heliopause, is the point at which the solar wind subsequently terminates and is the start of interstellar space.[sixty eight] Voyager 1 and Voyager 2 are said to have surpassed the termination shock and entered the heliosheath, at 94 and eighty four AU from the Sun, respectively.[133][134] Voyager 1 is pronounced to have crossed the heliopause in August 2012.[135]

The form and shape of the outer edge of the heliosphere is probable laid low with the fluid dynamics of interactions with the interstellar medium in addition to sun magnetic fields winning to the south, e.g. it’s far bluntly formed with the northern hemisphere extending nine AU farther than the southern hemisphere.[131] Beyond the heliopause, at around 230 AU, lies the bow surprise, a plasma “wake” left by means of the Sun as it travels through the Milky SOLAR SYSTEM Way.[136]

Zooming out the Solar System:

internal Solar System and Jupiterouter Solar System and Plutoorbit of Sedna (indifferent object)internal a part of the Oort Cloud

Due to a loss of statistics, situations in local interstellar space aren’t regarded for positive. It is expected that NASA’s Voyager spacecraft, as they pass the heliopause, will transmit treasured information on radiation levels and solar wind to Earth.[137] How properly the heliosphere shields the Solar System from cosmic rays is poorly understood. A NASA-funded team has advanced a idea of a “Vision Mission” dedicated to sending a probe to the heliosphere.[138][139]

Detached objects

90377 Sedna (with a mean orbit of 520 AU) is a massive, reddish object with a massive, exceedingly elliptical orbit that takes it from about seventy six AU at perihelion to 940 AU at aphelion and takes eleven,400 years to finish. Mike Brown, who observed the item in 2003, asserts that it can not be a part of the scattered disc or the Kuiper belt due to the fact its perihelion is too remote to were affected by Neptune’s migration. He and different astronomers don’t forget it to be the primary in a completely new population, from time to time termed “distant indifferent objects” (DDOs), which also may include the object 2000 CR105, which has a perihelion of forty five AU, an aphelion of 415 AU, and an orbital period of 3,420 years.[140] Brown phrases this population the “internal Oort cloud” because it can have fashioned via a comparable procedure, even though it is far toward the Sun.[141] Sedna could be very probably a dwarf planet, though its form has but to be decided. The 2d unequivocally detached item, with a perihelion farther than Sedna’s at more or less eighty one AU, is 2012 VP113, discovered in 2012. Its aphelion is most effective half that of Sedna’s, at four hundred–500 AU.[142][143]

Oort cloud

Schematic of the hypothetical Oort cloud, with a round outer cloud and a disc-shaped inner cloud

The Oort cloud is a hypothetical spherical cloud of as much as one trillion icy gadgets this is notion to be the supply for all long-period comets and to surround the Solar System at roughly 50,000 AU (around 1 light-yr (ly)), and likely to as a ways as a hundred,000 AU (1.87 ly). It is notion to be composed of comets that have been ejected from the internal Solar System by means of gravitational interactions with the outer planets. Oort cloud gadgets move very slowly, and can be perturbed through rare occasions, including collisions, the gravitational consequences of a passing star, or the galactic tide, the tidal pressure exerted with the aid of the Milky Way.[one hundred forty four][145]


Much of the Solar System is still unknown. The Sun’s gravitational discipline is estimated to dominate the gravitational forces of surrounding stars out to about two light-years (a hundred twenty five,000 AU). Lower estimates for the radius of the Oort cloud, via evaluation, do no longer location it farther than 50,000 AU.[146] Despite discoveries consisting of Sedna, the region among the Kuiper belt and the Oort cloud, a place tens of heaps of AU in radius, is still definitely unmapped. There are also ongoing studies of the place among Mercury and the Sun.[147] Objects might also but be found in the Solar System’s uncharted regions.

Currently, the furthest regarded objects, which includes Comet West, have aphelia around 70,000 AU from the Sun, but because the Oort cloud turns into higher acknowledged, this could exchange.

Galactic context

Diagram of the Milky Way with the position of the Solar System marked by using a SOLAR SYSTEM yellow arrow

The Solar System is located in the Milky Way, a barred spiral galaxy with a diameter of about 100,000 light-years containing more than 100 billion stars.[148] The Sun resides in one of the Milky Way’s outer spiral palms, called the Orion–Cygnus Arm or Local Spur.[149] The Sun lies approximately 26,660 mild-years from the Galactic Centre,[150] and its speed across the center of the Milky Way is ready 247 km/s, so that it completes one revolution each 210 million years. This revolution is called the Solar System’s galactic yr.[151] The solar apex, the direction of the Sun’s direction thru interstellar area, is near the constellation Hercules inside the route of the contemporary location of the bright big name Vega.[152] The plane of the ecliptic lies at an perspective of approximately 60° to the galactic plane.[i]

The Solar System’s region in the Milky Way is a factor within the evolutionary history of existence on Earth. Its orbit is close to circular, and orbits close to the Sun are at more or less the same speed as that of the spiral arms.[154][one hundred fifty five] Therefore, the Sun passes thru hands only not often. Because spiral hands are home to a much large attention of supernovae, gravitational instabilities, and radiation that would disrupt the Solar System, this has given Earth lengthy periods of stability for lifestyles to adapt.[154] However, the changing position of the Solar System relative to other parts of the Milky Way may want to provide an explanation for periodic extinction events on Earth, according to the Shiva hypothesis or related theories.The Solar System lies well outdoor the superstar-crowded environs of the galactic centre. Near the centre, gravitational tugs from nearby stars may want to perturb our bodies in the Oort cloud and send many comets into the internal Solar System, producing collisions with doubtlessly catastrophic implications for lifestyles on Earth. The severe radiation of the galactic centre can also intrude with the development of complicated lifestyles.[154] Even on the Solar System’s modern-day place, some scientists have speculated that latest supernovae might also have adversely affected lifestyles within the closing 35,000 years, with the aid of flinging portions of expelled stellar center toward the Sun, as radioactive dirt grains and larger, comet-like our bodies.[156]


Beyond the heliosphere is the interstellar medium, such as various clouds of gases. The Solar System presently moves through the Local Interstellar Cloud.

The Solar System is in the Local Interstellar Cloud or Local Fluff. It is concept to be near the neighbouring G-Cloud but it is not recognised if the Solar System is embedded inside the Local Interstellar Cloud, or if it’s miles in the vicinity where the Local Interstellar Cloud and G-Cloud are interacting.[157][158] The Local Interstellar Cloud is a place of denser cloud in an in any other case sparse place referred to as the Local Bubble, an hourglass-fashioned cavity in the interstellar medium more or less 300 light-years (ly) throughout. The bubble is suffused with high-temperature plasma, that shows it is the product of several latest supernovae.[159]

There are noticeably few stars within ten mild-years of the Sun. The closest is the triple celebrity gadget Alpha Centauri, which is set 4.4 mild-years away. Alpha Centauri A and B are a carefully tied pair of Sun-like stars, while the small pink dwarf, Proxima Centauri, orbits the pair at a distance of zero.2 light-year. In 2016, a potentially habitable exoplanet changed into confirmed to be orbiting Proxima Centauri, known as Proxima Centauri b, the nearest confirmed exoplanet to the Sun.[one hundred sixty] The stars next closest to the Sun are the purple dwarfs Barnard’s Star (at five.nine ly), Wolf 359 (7.eight ly), and Lalande 21185 (8.3 ly).

The largest nearby famous person is Sirius, a vivid major-sequence big name more or less 8.6 mild-years away and more or less twice the Sun’s mass and this is orbited via a white dwarf, Sirius B. The nearest brown dwarfs are the binary Luhman sixteen gadget at 6.6 light-years. Other structures inside ten light-years are the binary red-dwarf gadget Luyten 726-eight (eight.7 ly) and the solitary pink dwarf Ross 154 (9.7 ly).[161] The closest solitary Sun-like famous person to the Solar System is Tau Ceti at 11.9 light-years. It has roughly eighty% of the Sun’s mass however most effective 60% of its luminosity.[162] The closest acknowledged free-floating planetary-mass object to the Sun is WISE 0855−0714,[163] an item with a mass less than 10 Jupiter masses kind of 7 light-years away.

Compared to many different planetary systems, the Solar System stands out in lacking planets indoors to the orbit of Mercury.[164][one hundred sixty five] The known Solar System also lacks outstanding-Earths (Planet Nine will be a super-Earth beyond the recognized Solar System).[164] Uncommonly, it has best small rocky planets and large gasoline giants; somewhere else planets of intermediate size are common—each rocky and gas—so there is no “gap” as seen between the scale of Earth and of Neptune (with a radius three.eight instances as large). Also, those amazing-Earths have closer orbits than Mercury.[164] This led to the speculation that every one planetary systems start with many near-in planets, and that normally a series in their collisions causes consolidation of mass into few large planets, but in case of the Solar System the collisions precipitated their destruction and ejection.[166][167]

The orbits of Solar System planets are nearly circular. Compared to different systems, they’ve smaller orbital eccentricity.[164] Although there are tries to provide an explanation for it in part with a bias inside the radial-speed detection method and partly with long interactions of a quite high variety of planets, the precise causes continue to be undetermined.[164][168]

Visual summary

This phase is a sampling of Solar System our bodies, decided on for length and exceptional of images, and looked after through volume. Some large gadgets are omitted here (extensively Eris, Haumea, Makemake, and Nereid) because they’ve not been imaged in high excellent.

See alsoNotes^ a b As of August 27, 2019.

^ Capitalization of the call varies. The International Astronomical Union, the authoritative frame regarding astronomical nomenclature, specifies capitalizing the names of all individual astronomical objects but uses mixed “Solar System” and “solar device” systems in their naming hints file. The name is generally rendered in decrease case (“solar machine”), as, for instance, in the Oxford English Dictionary and Merriam-Webster’s eleventh Collegiate Dictionary.

^ The herbal satellites (moons) orbiting the Solar System’s planets are an example of the latter.

^ Historically, several different bodies were as soon as taken into consideration planets, along with, from its discovery in 1930 till 2006, Pluto. See Former planets.

^ Themoons larger than Mercury are Ganymede, which orbits Jupiter, and Titan, which orbits Saturn. Although bigger than Mercury, both moons have much less than half of its mass. In addition, the radius of Jupiter’s moon Callisto is over ninety eight% that of Mercury.

^ The date is based totally on the oldest inclusions found to this point in meteorites, 4568.2+0.2−zero.four million years, and is notion to be the date of the formation of the primary solid fabric within the collapsing nebula.[45]

^ If is the angle between the north pole of the ecliptic and the north galactic pole then:

in which = 27° 07′ forty two.01″ and = 12h 51m 26.282 are the declination and right ascension of the north galactic pole,[153] while = 66° 33′ 38.6″ and = 18h 0m 00 are the ones for the north pole of the ecliptic. (Both pairs of coordinates are for J2000 epoch.) The result of the calculation is 60.19°.

References^ “How Many Solar System Bodies”. NASA/JPL Solar System Dynamics. Retrieved 20 April 2018.

^ Wm. Robert Johnston (15 September 2019). “Asteroids with Satellites”. Johnston’s Archive. Retrieved 28 September 2019.

^ a b “Latest Published Data”. The International Astronomical Union Minor Planet Center. Retrieved 28 September 2019.

^ a b Mumma, M.J.; Disanti, M.A.; Dello Russo, N.; Magee-Sauer, K.; Gibb, E.; Novak, R. (2003). “Remote infrared observations of figure volatiles in comets: A window at the early sun system”. Advances in Space Research. 31 (12): 2563–2575. Bibcode:2003AdSpR..31.2563M. CiteSeerX doi:10.1016/S0273-1177(03)00578-7.

^ a b c “The Final IAU Resolution on the definition of “planet” prepared for vote casting”. IAU. 24 August 2006. Archived from the original on 7 January 2009. Retrieved 2 March 2007.

^ a b “Dwarf Planets and their Systems”. Working Group for Planetary System Nomenclature (WGPSN). U.S. Geological Survey. 7 November 2008. Retrieved thirteen July 2008.

^ Ron Ekers. “IAU Planet Definition Committee”. International Astronomical Union. Archived from the authentic on 3 June 2009. Retrieved 13 October 2008.

^ “Plutoid selected as name for Solar System gadgets like Pluto”. International Astronomical Union, Paris. eleven June 2008. Archived from the authentic on 13 June 2008. Retrieved eleven June 2008.

^ Grundy, W.M.; Noll, K.S.; Buie, M.W.; Benecchi, S.D.; Ragozzine, D.; Roe, H.G. (December 2018). “The Mutual Orbit, Mass, and Density of Transneptunian Binary Gǃkúnǁʼhòmdímà ((229762) 2007 UK126)” (PDF). Icarus. 334: 30–38. doi:10.1016/j.icarus.2018.12.037. Archived from the unique on 7 April 2019.

^ Mike Brown (23 August 2011). “Free the dwarf planets!”. Mike Brown’s Planets.

^ WC Rufus (1923). “The astronomical machine of Copernicus”. Popular Astronomy. Vol. 31. p. 510. Bibcode:1923PA…..31..510R.

^ Weinert, Friedel (2009). Copernicus, Darwin, & Freud: revolutions within the history and philosophy of technological know-how. Wiley-Blackwell. p. 21. ISBN 978-1-4051-8183-nine.

^ Eric W. Weisstein (2006). “Galileo Galilei (1564–1642)”. Wolfram Research. Retrieved 27 October 2010.

^ “Discoverer of Titan: Christiaan Huygens”. ESA Space Science. 2005. Retrieved 27 October 2010.

^ Jeremiah Horrocks, William Crabtree, and the Lancashire observations of the transit of Venus of 1639, Allan Chapman 2004 Cambridge University Press doi:10.1017/S1743921305001225

^ “Comet Halley”. University of Tennessee. Retrieved 27 December 2006.

^ Sagan, Carl & Druyan, Ann (1997). Comet. New York: Random House. pp. 26–27, 37–38. ISBN 978-zero-3078-0105-zero.

^ “Etymonline: Solar System”. Retrieved 24 January 2008.

^ “1838: Friedrich Bessel Measures Distance to a Star”. Observatories of the Carnegie Institution for Science. Archived from the authentic on 1 October 2018. Retrieved 22 September 2018.

^ M Woolfson (2000). “The foundation and evolution of the solar gadget”. Astronomy & Geophysics. 41 (1): 1.12–1.19. Bibcode:2000A&G….41a..12W. doi:10.1046/j.1468-4004.2000.00012.x.

^ Alessandro Morbidelli (2005). “Origin and dynamical evolution of comets and their reservoirs”. arXiv:astro-ph/0512256.

^ a b Audrey Delsanti & David Jewitt (2006). “The Solar System Beyond The Planets” (PDF). Institute for Astronomy, University of Hawaii. Archived from the authentic (PDF) on 29 January 2007. Retrieved three January 2007.

^ a b Krasinsky, G.A.; Pitjeva, E.V.; Vasilyev, M.V.; Yagudina, E.I. (July 2002). “Hidden Mass within the Asteroid Belt”. Icarus. 158 (1): ninety eight–one hundred and five. Bibcode:2002Icar..158…98K. doi:10.1006/icar.2002.6837.

^ Levison, H.F.; Morbidelli, A. (27 November 2003). “The formation of the Kuiper belt via the outward delivery of our bodies at some stage in Neptune’s migration”. Nature. 426 (6965): 419–421. Bibcode:2003Natur.426..419L. doi:10.1038/nature02120. PMID 14647375. S2CID 4395099.

^ Harold F. Levison; Martin J Duncan (1997). “From the Kuiper Belt to Jupiter-Family Comets: The Spatial Distribution of Ecliptic Comets”. Icarus. 127 (1): thirteen–32. Bibcode:1997Icar..127…13L. doi:10.1006/icar.1996.5637.

^ Grossman, Lisa (13 August 2009). “Planet determined orbiting its celebrity backwards for first time”. New Scientist. Retrieved 10 October 2009.

^ “The Solar System”. Nine Planets. Retrieved 15 February 2007.

^ Amir Alexander (2006). “New Horizons Set to Launch on nine-Year Voyage to Pluto and the Kuiper Belt”. The Planetary Society. Archived from the unique on 22 February 2006. Retrieved eight November 2006.

^ Bennett, Jeffrey O. (2020). “Chapter four.5”. The cosmic attitude (Ninth ed.). Hoboken, NJ. ISBN 978-0-134-87436-four.

^ a b Marochnik, L. & Mukhin, L. (1995). “Is Solar System Evolution Cometary Dominated?”.In Shostak, G.S. (ed.). Progress within the Search for Extraterrestrial Life. Astronomical Society of the Pacific Conference Series. 74. p. eighty three. Bibcode:1995ASPC…seventy four…83M. ISBN 0-937707-ninety three-7.

^ Bi, S.L.; Li, T.D.; Li, L.H.; Yang, W.M. (2011). “Solar Models with Revised Abundance”. The Astrophysical Journal. 731 (2): L42. arXiv:1104.1032. Bibcode:2011ApJ…731L..42B. doi:10.1088/2041-8205/731/2/L42. S2CID 118681206.

^”The Sun’s Vital Statistics”. Stanford Solar Center. Retrieved 29 July 2008., citing Eddy, J. (1979). A New Sun: The Solar Results From Skylab. NASA. p. 37. NASA SP-402.

^ Williams, David R. (7 September 2006). “Saturn Fact Sheet”. NASA. Archived from the authentic on 4 August 2011. Retrieved 31 July 2007.

^ Williams, David R. (sixteen November 2004). “Jupiter Fact Sheet”. NASA. Archived from the authentic on 26 September 2011. Retrieved 8 August 2007.

^ Paul Robert Weissman; Torrence V. Johnson (2007). Encyclopedia of the sun machine. Academic Press. p. 615. ISBN 978-zero-12-088589-three.

^ a b c Podolak, M.; Weizman, A.; Marley, M. (December 1995). “Comparative fashions of Uranus and Neptune”. Planetary and Space Science. forty three (12): 1517–1522. Bibcode:1995P&SS…43.1517P. doi:10.1016/0032-1/3(95)00061-five.

^ a b c d Podolak, M.; Podolak, J.I.; Marley, M.S. (February 2000). “Further investigations of random fashions of Uranus and Neptune”. Planetary and Space Science. 48 (2–3): 143–151. Bibcode:2000P&SS…forty eight..143P. doi:10.1016/S0032-third(99)00088-four.

^ Michael Zellik (2002). Astronomy: The Evolving Universe (9th ed.). Cambridge University Press. p. 240. ISBN 978-zero-521-80090-7. OCLC 223304585.

^ Placxo, Kevin W.; Gross, Michael (2006). Astrobiology: a brief creation. JHU Press. p. sixty six. ISBN 978-zero-8018-8367-five.

^ “Dawn: A Journey to the Beginning of the Solar System”. Space Physics Center: UCLA. 2005. Archived from the unique on 24 May 2012. Retrieved three November 2007.

^ Guy Ottewell (1989). “The Thousand-Yard Model identity=”cite_note-49″>^ “Tours of Model Solar Systems”. University of Illinois. Archived from the unique on 12 April 2011. Retrieved 10 May 2012.

^ “Luleå är Sedna. I alla fall om vår sol motsvaras av Globen i Stockholm”. Norrbotten Kuriren (in Swedish). Archived from the unique on 15 July 2010. Retrieved 10 May 2010.

^ See, for example, Office of Space Science (9 July 2004). “Solar System Scale”. NASA Educator Features. Retrieved 2 April 2013.

^ Bouvier, A.; Wadhwa, M. (2010). “The age of the Solar System redefined by way of the oldest Pb–Pb age of a meteoritic inclusion”. Nature Geoscience. 3 (nine): 637–641. Bibcode:2010NatGe…3..637B. doi:10.1038/NGEO941. S2CID 56092512.

^ a b c “Lecture thirteen: The Nebular Theory of the origin of the Solar System”. University of Arizona. Retrieved 27 December 2006.

^ Irvine, W.M. (1983). “The chemical composition of the pre-solar nebula”. Cometary exploration; Proceedings of the International Conference. 1. p. three. Bibcode:1983coex….1….3I.

^ Greaves, Jane S. (7 January 2005). “Disks Around Stars and the Growth of Planetary Systems”. Science. 307 (5706): sixty eight–71. Bibcode:2005Sci…307…68G. doi:10.1126/science.1101979. PMID 15637266. S2CID 27720602.

^ Present Understanding of the Origin of Planetary Systems. National Academy of Sciences. 5 April 2000. doi:10.17226/1732. ISBN 978-zero-309-04193-five. Retrieved 19 January 2007.

^ Boss, A.P.; Durisen, R.H. (2005). “Chondrule-forming Shock Fronts within the Solar Nebula: A Possible Unified Scenario for Planet and Chondrite Formation”. The Astrophysical Journal. 621 (2): L137. arXiv:astro-ph/0501592. Bibcode:2005ApJ…621L.137B. doi:10.1086/429160. S2CID 15244154.

^ a b c Bennett, Jeffrey O. (2020). “Chapter 8.2”. The cosmic angle (Ninth ed.). Hoboken, NJ. ISBN 978-0-134-87436-four.

^ Bartels, Meghan (18 March 2019). “NASA’s New Horizons Reveals Geologic ‘Frankenstein’ That Formed Ultima Thule”. Retrieved 18 March 2019.

^ Batygin, Konstantin; Brown, Michael E. (20 June 2010). “Early Dynamical Evolution of the Solar System: Pinning Down the Initial Conditions of the Nice Model”. The Astrophysical Journal. 716 (2): 1323–1331. arXiv:1004.5414. Bibcode:2010ApJ…716.1323B. doi:10.1088/0004-637X/716/2/1323. S2CID 7609851.

^ Sukyoung Yi; Pierre Demarque; Yong-Cheol Kim; Young-Wook Lee; Chang H. Ree; Thibault Lejeune; Sydney Barnes (2001). “Toward Better Age Estimates for Stellar Populations: The Y2 Isochrones for Solar Mixture”. Astrophysical Journal Supplement. 136 (2): 417–437. arXiv:astro-ph/0104292. SOLAR SYSTEM Bibcode:2001ApJS..136..417Y. doi:10.1086/321795. S2CID 118940644.

^ A. Chrysostomou; P.W. Lucas (2005). “The Formation of Stars”. Contemporary Physics. 46 (1): 29–forty. Bibcode:2005ConPh..forty six…29C. doi:10.1080/0010751042000275277. S2CID 120275197.

^ a b Schröder, K.-P.; Connon Smith, Robert (May 2008). “Distant destiny of the Sun and Earth revisited”. Monthly Notices of the Royal Astronomical Society. 386 (1): 155–163. arXiv:0801.4031. Bibcode:2008MNRAS.386..155S. doi:10.1111/j.1365-2966.2008.13022.x. S2CID 10073988.

^ Nir J. Shaviv (2003). “Towards a Solution to the Early Faint Sun Paradox: A Lower Cosmic Ray Flux from a Stronger Solar Wind”. Journal of Geophysical Research. 108 (A12): 1437. arXiv:astroph/0306477. Bibcode:2003JGRA..108.1437S. doi:10.1029/2003JA009997. S2CID 11148141.

^ Pogge, Richard W. (1997). “The Once & Future Sun”. New Vistas in Astronomy. Archived from the unique on 27 May 2005. Retrieved 7 December 2005.

^ “Sun: Facts & Figures”. NASA. Archived from the authentic on 2 January 2008. Retrieved 14 May 2009.

^Woolfson, M. (2000). “The foundation and evolution of the sun machine”. Astronomy & Geophysics. 41 (1): 12. Bibcode:2000A&G….41a..12W. doi:10.1046/j.1468-4004.2000.00012.x.

^ Zirker, Jack B. (2002). Journey from the Center of the Sun. Princeton University Press. pp. 120–127. ISBN 978-zero-691-05781-1.

^ “Why is visible mild visible, but not different elements of the spectrum?”. The Straight Dome. 2003. Retrieved 14 May 2009.

^ Than, Ker (30 January 2006). “Astronomers Had it Wrong: Most Stars are Single”. Retrieved 1 August 2007.

^ Smart, R. L.; Carollo, D.; Lattanzi, M. G.; McLean, B.; Spagna, A. (2001). “The Second Guide Star Catalogue and Cool Stars”.In Hugh R.A. Jones; Iain A. Steele (eds.). Ultracool Dwarfs: New Spectral Types L and T. Springer. p. 119. Bibcode:2001udns.conf..119S.

^ T.S. van Albada; Norman Baker (1973). “On the Two Oosterhoff Groups of Globular Clusters”. The Astrophysical Journal. 185: 477–498. Bibcode:1973ApJ…185..477V. doi:10.1086/152434.

^ Charles H. Lineweaver (nine March 2001). “An Estimate of the Age Distribution of Terrestrial Planets in the Universe: Quantifying Metallicity as a Selection Effect”. Icarus. 151 (2): 307–313. arXiv:astro-ph/0012399. Bibcode:2001Icar..151..307L. CiteSeerX doi:10.1006/icar.2001.6607. S2CID 14077895.

^ “Solar Physics: The Solar Wind”. Marshall Space Flight Center. sixteen July 2006. Retrieved three October 2006.

^ a b c “Voyager Enters Solar System’s Final Frontier”. NASA. Retrieved 2 April 2007.

^ Phillips, Tony (15 February 2001). “The Sun Does a Flip”. NASA–Science News. Archived from the original on 12 May 2009. Retrieved four February 2007.

^ “A Star withNorth Poles”. NASA–Science News. 22 April 2003. Archived from the unique on 18 July 2009.

^ Riley, Pete (2002). “Modeling the heliospheric contemporary sheet: Solar cycle versions” (PDF). Journal of Geophysical Research. 107. Bibcode:2002JGRA.107g.SSH8R. doi:10.1029/2001JA000299. Archived from the authentic (PDF) on 14 August 2009.

^ “Solar Wind blows some of Earth’s environment into area”. Science@NASA Headline News. eight December 1998.

^ Lundin, Richard (nine March 2001). “Erosion by means of the Solar Wind”. Science. 291 (5510): 1909. doi:10.1126/science.1059763. PMID 11245195. S2CID 128505404.

^ Langner, U.W.; M.S. Potgieter (2005). “Effects of the location of the sun wind termination surprise and the heliopause on the heliospheric modulation of cosmic rays”. Advances in Space Research. 35 (12): 2084–2090. Bibcode:2005AdSpR..35.2084L. doi:10.1016/j.asr.2004.12.1/2.

^ “Long-term Evolution of the Zodiacal Cloud”. 1998. Archived from the unique on 29 September 2006. Retrieved 3 February 2007.

^ “ESA scientist discovers a way to shortlist stars that might have planets”. ESA Science and Technology. 2003. Retrieved 3 February 2007.

^ Landgraf, M.; Liou, J.-C.; Zook, H.A.; Grün, E. (May 2002). “Origins of Solar System Dust past Jupiter” (PDF). The Astronomical Journal. 123 (five): 2857–2861. arXiv:astro-ph/0201291. Bibcode:2002AJ….123.2857L. doi:10.1086/339704. S2CID 38710056. Retrieved nine February 2007.

^ “Inner Solar System”. NASA Science (Planets). Archived from the authentic on 11 May 2009. Retrieved nine May 2009.

^ Ryan Whitwam (18 March 2019). “Mercury Is Actually the Closest Planet to Every Other Planet”. Retrieved 25 March 2019.

^ Mercury is the closest planet to all seven other planets on YouTube

^ Schenk P., Melosh H.J. (1994), Lobate Thrust Scarps and the Thickness of Mercury’s Lithosphere, Abstracts of the 25th Lunar and Planetary Science Conference, 1994LPI….25.1203S

^ Bill Arnett (2006). “Mercury”. Nine Planets. Retrieved 14 September 2006.

^ Benz, W.; Slattery, W.L.; Cameron, A.G.W. (1988). “Collisional stripping of Mercury’s mantle”. Icarus (Submitted manuscript). 74 (3): 516–528. Bibcode:1988Icar…seventy four..516B. doi:10.1016/0019-1035(88)90118-2.

^ Cameron, A.G.W. (1985). “The partial volatilization of Mercury”. Icarus. sixty four (2): 285–294. Bibcode:1985Icar…sixty four..285C. doi:10.1016/0019-1035(85)90091-0.

^ Mark Alan Bullock (1997). The Stability of Climate on Venus (PDF) (PhD). Southwest Research Institute. Archived from the original (PDF) on 14 June 2007. Retrieved 26 December 2006.

^ Paul Rincon (1999). “Climate Change as a Regulator of Tectonics on Venus” (PDF). Johnson Space Center Houston, TX, Institute of Meteoritics, University of New Mexico, Albuquerque, NM. Archived from the authentic (PDF) on 14 June 2007. Retrieved 19 November 2006.

^ “What are the traits of the Solar System that cause the origins of existence?”. NASA Science (Big Questions). Archived from the authentic on 8 April 2010. Retrieved 30 August 2011.

^ Anne E. Egger. “Earth’s Atmosphere: Composition and Structure”. Archived from the unique on 21 February 2007. Retrieved 26 December 2006.

^ David C. Gatling; Conway Leovy (2007). “Mars Atmosphere: History and Surface Interactions”.In Lucy-Ann McFadden;et al. (eds.). Encyclopaedia of the Solar System. pp. 301–314.

^ David Noever (2004). “Modern Martian Marvels: Volcanoes?”. NASA Astrobiology Magazine. Retrieved 23 July 2006.

^ “Mars: A Kid’s Eye View”. NASA. Archived from the original on 26 December 2003. Retrieved 14 May 2009.

^ Scott S. Sheppard; David Jewitt & Jan Kleyna (2004). “A Survey for Outer Satellites of Mars: Limits to Completeness” (PDF). Astronomical Journal. Retrieved 26 December 2006.

^ Pascal Rosenblatt; Sébastien Charnoz; Kevin M. Dunseath; Mariko Terao-Dunseath; Antony Trinh; Ryuki Hyodo; Hidenori Genda; Stéven Toupin (2016). “Accretion of Phobos and Deimos in an prolonged debris disc stirred by brief moons” (PDF). Nature Geoscience. nine (8): 581. Bibcode:2016NatGe…nine..581R. doi:10.1038/ngeo2742.

^ “IAU Planet Definition Committee”. International Astronomical Union. 2006. Archived from the original on 3 June 2009. Retrieved 1 March 2009.

^ “Are Kuiper Belt Objects asteroids? Are massive Kuiper Belt Objects planets?”. Cornell University. Archived from the unique on three January 2009. Retrieved 1 March 2009.

^ Petit, J.-M.; Morbidelli, A.; Chambers, J. (2001). “The Primordial Excitation and Clearing of the Asteroid Belt” (PDF). Icarus. 153 (2): 338–347. Bibcode:2001Icar..153..338P. doi:10.1006/icar.2001.6702. Retrieved 22 March 2007.

^ “New examine exhibits twice as many asteroids as previously believed”. ESA. 2002. Retrieved 23 June 2006.

^ “Cassini Passes Through Asteroid Belt”. NASA. Retrieved 1 March 2021.

^ “History and Discovery of Asteroids” (DOC). NASA. Retrieved 29 August 2006.

^ Phil Berardelli (2006). “Main-Belt Comets May Have Been Source of Earths Water”. SpaceDaily. Retrieved 23 June 2006.

^ Barucci, M. A.; Kruikshank, D.P.; Mottola S.; Lazzarin M. (2002). “Physical Properties of Trojan and Centaur Asteroids”. Asteroids III. Tucson, Arizona: University of Arizona Press. pp. 273–87.

^ Morbidelli, A.; Bottke, W.F.; Froeschlé, Ch.; Michel, P. (January 2002).W.F. Bottke Jr.; A. Cellino; P. Paolicchi; R.P. Binzel (eds.). “Origin and Evolution of Near-Earth Objects” (PDF). Asteroids III: 409–422. Bibcode:2002aste.e-book..409M.

^ “Gas Giant identification=”cite_note-112″>^ Jack J. Lissauer; David J. Stevenson (2006). “Formation of Giant Planets” (PDF). NASA Ames Research Center; California Institute of Technology. Archived from the unique (PDF) on 26 March 2009. Retrieved 16 January 2006.

^ Pappalardo, R T (1999). “Geology of the Icy Galilean Satellites: A Framework for Compositional Studies”. Brown University. Archived from the unique on 30 September 2007. Retrieved sixteen January 2006.

^ “Saturn – The Most Beautiful Planet of our solar device”. Preserve Articles. 23 January 2011. Archived from the original on 20 January 2012. Retrieved 24 July 2011.

^ Kargel, J.S. (1994). “Cryovolcanism on the icy satellites”. Earth, Moon, and Planets (Submitted manuscript). sixty seven (1–3): one hundred and one–113. Bibcode:1995EM&P…sixty seven..101K. doi:10.1007/BF00613296. S2CID 54843498.

^ Hawksett, David; Longstaff, Alan; Cooper, Keith; Clark, Stuart (2005). “10 Mysteries of the Solar System”. Astronomy Now. 19 (8): sixty five. Bibcode:2005AsNow..19h..65H.

^ Sheppard, S. S.; Jewitt, D.; Kleyna, J. (2005). “An Ultradeep Survey for Irregular Satellites of Uranus: Limits to Completeness”. The Astronomical Journal. 129 (1): 518. arXiv:astro-ph/0410059. Bibcode:2005AJ….129..518S. doi:10.1086/426329. S2CID 18688556.

^ Podolak, M.; Reynolds, R.T.; Young, R. (1990). “Post Voyager comparisons of the interiors of Uranus and Neptune”. Geophysical Research Letters (Submitted manuscript). 17 (10): 1737–1740. Bibcode:1990GeoRL..17.1737P. doi:10.1029/GL017i010p01737.

^ Duxbury, N.S.; Brown, R.H. (1995). “The Plausibility of Boiling Geysers on Triton”. Beacon eSpace. Archived from the authentic on 26 April 2009. Retrieved sixteen January 2006.

^ John Stansberry; Will Grundy; Mike Brown; Dale Cruikshank; John Spencer; David Trilling; Jean-Luc Margot (2007). “Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope”. The Solar System Beyond Neptune. p. 161. arXiv:astro-ph/0702538. Bibcode:2008ssbn.e-book..161S.

^ Patrick Vanouplines (1995). “Chiron biography”. Vrije Universitiet Brussel. Archived from the original on 2 May 2009. Retrieved 23 June 2006.

^ Sekanina, Zdeněk (2001). “Kreutz sungrazers: the remaining case of cometary fragmentation and disintegration?”. Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic. 89: 78–93. Bibcode:2001PAICz..89…78S.

^ Królikowska, M. (2001). “A have a look at of the authentic orbits of hyperbolic comets”. Astronomy & Astrophysics. 376 (1): 316–324. Bibcode:2001A&A…376..316K. doi:10.1051/0004-6361:20010945.

^ Whipple, Fred L. (1992). “The sports of comets associated with their getting old and beginning”. Celestial Mechanics and Dynamical Astronomy. fifty four (1–three): 1–11. Bibcode:1992CeMDA..54….1W. doi:10.1007/BF00049540. S2CID 189827311.

^ Alan Stern (February 2015). “Journey to the Solar System’s Third Zone”. American Scientist. Retrieved 26 October 2018.

^ a b Stephen C. Tegler (2007). “Kuiper Belt Objects: Physical Studies”.In Lucy-Ann McFadden;et al. (eds.). Encyclopedia of the Solar System. pp. 605–620.

^ Brown, M.E.; Van Dam, M.A.; Bouchez, A.H.; Le Mignant, D.; Campbell, R.D.; Chin, J.C.Y.; Conrad, A.; Hartman, S.K.; Johansson, E.M.; Lafon, R.E.; Rabinowitz, D.L. Rabinowitz; Stomski, P.J. Jr.; Summers, D.M.; Trujillo, C.A.; Wizinowich, P.L. (2006). “Satellites of the Largest Kuiper Belt Objects” (PDF). The Astrophysical Journal. 639 (1): L43–L46. arXiv:astro-ph/0510029. Bibcode:2006ApJ…639L..43B. doi:10.1086/501524. S2CID 2578831. Retrieved 19 October 2011.

^ Chiang, E.I.; Jordan, A.B.; Millis, R.L.; Buie, M.W.; Wasserman, L.H.; Elliot, J.L.; Kern, S.D.; Trilling, D.E.; Meech, K.J.;et al. (2003). “Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances” (PDF). The Astronomical Journal. 126 (1): 430–443. arXiv:astro-ph/0301458. Bibcode:2003AJ….126..430C. doi:10.1086/375207. S2CID 54079935. Retrieved 15 August 2009.

^ M.W. Buie; R.L. Millis; L. H. Wasserman; J.L. Elliot; S.D. Kern; K.B. Clancy; E.I. Chiang; A.B. Jordan; K.J. Meech; R.M. Wagner; D.E. Trilling (2005). “Procedures, Resources and Selected Results of the Deep Ecliptic Survey”. Earth, Moon, and Planets. 92 (1): 113–124. arXiv:astro-ph/0309251. Bibcode:2003EM&P…ninety two..113B. doi:10.1023/ S2CID 14820512.

^ E. Dotto1; M. A. Barucci2; M. Fulchignoni (24 August 2006). “Beyond Neptune, the new frontier of the Solar System” (PDF). Retrieved 26 December 2006.

^ Fajans, J.; L. Frièdland (October 2001). “Autoresonant (nonstationary) excitation of pendulums, Plutinos, plasmas, and other nonlinear oscillators” (PDF). American Journal of Physics. sixty nine (10): 1096–1102. Bibcode:2001AmJPh..69.1096F. doi:10.1119/1.1389278. Archived from the original (PDF) on 7 June 2011. Retrieved 26 December 2006.

^ Marc W. Buie (5 April 2008). “Orbit Fit and Astrometric record for 136472”. SwRI (Space Science Department). Retrieved 15 July 2012.

^ Michael E. Brown. “The biggest Kuiper belt objects” (PDF). Caltech. Retrieved 15 July 2012.

^ Ortiz, J. L.; Santos-Sanz, P.; Sicardy, B.;et al. (2017). “The length, form, density and ring of the dwarf planet Haumea from a stellar occultation”. Nature. 550 (7675): 219–223. arXiv:2006.03113. Bibcode:2017Natur.550..219O. doi:10.1038/nature24051. hdl:10045/70230. PMID 29022593. S2CID 205260767.

^ David Jewitt (2005). “The 1,000 km Scale KBOs”. University of Hawaii. Retrieved 16 July 2006.

^ “List of Centaurs and Scattered-Disk Objects”. IAU: Minor Planet Center. Retrieved 2 April 2007.

^ Brown, Michael E.; Schaller, Emily L. (15 June 2007). “The Mass of Dwarf Planet Eris”. Science. 316 (5831): 1585. Bibcode:2007Sci…316.1585B. doi:10.1126/science.1139415. PMID 17569855. S2CID 21468196.

^ Littmann, Mark (2004). Planets Beyond: Discovering the Outer Solar System. Courier Dover Publications. pp. 162–163. ISBN 978-0-486-43602-9.

^ a b c Fahr, H. J.; Kausch, T.; Scherer, H. (2000). “A 5-fluid hydrodynamic technique to version the Solar System-interstellar medium interplay” (PDF). Astronomy & Astrophysics. 357: 268. Bibcode:2000A&A…357..268F. Archived from the authentic (PDF) on eight August 2017. Retrieved 24 August 2008. See Figures 1 and 2.

^ “Cassini’s Big Sky: The View from the Center of Our Solar System”. NASA/JPL. 2009. Archived from the authentic on 6 February 2012. Retrieved 20 December 2009.

^ Stone, E.C.; Cummings, A.C.; McDonald, F.B.; Heikkila, B.C.; Lal, N.; Webber, W.R. (September 2005). “Voyager 1 explores the termination surprise region and the heliosheath beyond”. Science. 309 (5743): 2017–20. Bibcode:2005Sci…309.2017S. doi:10.1126/science.1117684. PMID 16179468. S2CID 34517751.

^ Stone, E.C.; Cummings, A.C.; McDonald, F.B.; Heikkila, B.C.; Lal, N.; Webber, W.R. (July 2008). “An asymmetric sun wind termination shock”. Nature. 454 (7200): seventy one–four. Bibcode:2008Natur.454…71S. doi:10.1038/nature07022. PMID 18596802. S2CID 4431329.

^ Cook, Jia-Rui C.; Agle, D. C.; Brown, Dwayne (12 September 2013). “NASA Spacecraft Embarks on Historic Journey into Interstellar Space”. NASA. Retrieved 12 September 2013.

^ Nemiroff, R.; Bonnell, J., eds. (24 June 2002). “The Sun’s Heliosphere & Heliopause”. Astronomy Picture of the Day. NASA. Retrieved 23 June 2006.

^ “Voyager: Interstellar Mission”. NASA Jet Propulsion Laboratory. 2007. Retrieved eight May 2008.

^ R. L. McNutt Jr.;et al. (2006). “Innovative Interstellar Explorer” (PDF). Physics of the Inner Heliosheath: Voyager Observations, Theory, and Future Prospects. AIP Conference Proceedings. 858. pp. 341–347. Bibcode:2006AIPC..858..341M. doi:10.1063/1.2359348.

^ Anderson, Mark (5 January 2007). “Interstellar space, and step on it!”. New Scientist. Retrieved five February 2007.

^ David Jewitt (2004). “Sedna – 2003 VB12”. University of Hawaii. Retrieved 23 June 2006.

^ Mike Brown (2004). “Sedna”. Caltech. Retrieved 2 May 2007.

^”JPL Small-Body Database Browser: (2012 VP113)” (2013-10-30 ultimate obs). Jet Propulsion Laboratory. Retrieved 26 March 2014.

^”A new object at the edge of our Solar System discovered”. 26 March 2014.

^ Stern SA, Weissman PR (2001). “Rapid collisional evolution of comets in the course of the formation of the Oort cloud”. Nature. 409 (6820): 589–591. Bibcode:2001Natur.409..589S. doi:10.1038/35054508. PMID 11214311. S2CID 205013399.

^ Bill Arnett (2006). “The Kuiper Belt and the Oort Cloud”. Nine Planets. Retrieved 23 June 2006.

^ T. Encrenaz; JP. Bibring; M. Blanc; MA. Barucci; F. Roques; PH. Zarka (2004). The Solar System: Third edition. Springer. p. 1.

^ Durda D.D.; Stern S.A.; Colwell W.B.; Parker J.W.; Levison H.F.; Hassler D.M. (2004). “A New Observational Search for Vulcanoids in SOHO/LASCO Coronagraph Images”. Icarus. 148 (1): 312–315. Bibcode:2000Icar..148..312D. doi:10.1006/icar.2000.6520.

^English, J. (2000). “Exposing the Stuff Between the Stars” (Press release). Hubble News Desk. Retrieved 10 May 2007.

^ R. Drimmel; D.N. Spergel (2001). “Three Dimensional Structure of the Milky Way Disk”. The Astrophysical Journal. 556 (1): 181–202. arXiv:astro-ph/0101259. Bibcode:2001ApJ…556..181D. doi:10.1086/321556. S2CID 15757160.

^ GRAVITY Collaboration: A geometric distance size to the Galactic center black hole with 0.three% uncertainty. Astronomie & Astrophysics 625, 2019, doi:10.1051/0004-6361/201935656.

^ Leong, Stacy (2002). “Period of the Sun’s Orbit around the Galaxy (Cosmic Year)”. The Physics Factbook. Retrieved 2 April 2007.

^ C. Barbieri (2003). “Elementi di Astronomia e Astrofisica in keeping with il Corso di Ingegneria Aerospaziale V settimana”. Archived from the original on 14 May 2005. Retrieved 12 February 2007.

^ Reid, M.J.; Brunthaler, A. (2004). “The Proper Motion of Sagittarius A*”. The Astrophysical Journal. 616 (2): 872–884. arXiv:astro-ph/0408107. Bibcode:2004ApJ…616..872R. doi:10.1086/424960. S2CID 16568545.

^ a b c Leslie Mullen (18 May 2001). “Galactic Habitable Zones”. Astrobiology Magazine. Retrieved 1 June 2020.

^ O. Gerhard (2011). “Pattern speeds in the Milky Way”. Mem. S.A.It. Suppl. 18: 185. arXiv:1003.2489. Bibcode:2011MSAIS..18..185G.

^ “Supernova Explosion May Have Caused Mammoth Extinction”. 2005. Retrieved 2 February 2007.

^ “Our Local Galactic Neighborhood”. NASA. five June 2013. Archived from the unique on 21 November 2013.

^ Into the Interstellar Void, Centauri Dreams, five June 2013

^ “Near-Earth Supernovas”. NASA. Archived from the unique on 13 August 2006. Retrieved 23 July 2006.

^ Anglada-Escudé, Guillem; Amado, Pedro J.; Barnes, John; Berdiñas, Zaira M.; Butler, R. Paul; Coleman, Gavin A. L.; de la Cueva, Ignacio; Dreizler, Stefan; Endl, Michael; Giesers, Benjamin; Jeffers, Sandra V.; Jenkins, James S.; Jones, Hugh R. A.; Kiraga, Marcin; Kürster, Martin; López-González, Marίa J.; Marvin, Christopher J.; Morales, Nicolás; Morin, Julien; Nelson, Richard P.; Ortiz, José L.; Ofir, Aviv; Paardekooper, Sijme-Jan; Reiners, Ansgar; Rodríguez, Eloy; Rodrίguez-López, Cristina; Sarmiento, Luis F.; Strachan, John P.; Tsapras, Yiannis; Tuomi, Mikko; Zechmeister, Mathias (25 August 2016). “A terrestrial planet candidate in a temperate orbit round Proxima Centauri”. Nature. 536 (7617): 437–440. arXiv:1609.03449. Bibcode:2016Natur.536..437A. doi:10.1038/nature19106. ISSN 0028-0836. PMID 27558064. S2CID 4451513.

^ “Stars inside 10 mild years”. SolStation. Retrieved 2 April 2007.

^ “Tau Ceti”. SolStation. Retrieved 2 April 2007.

^ Luhman, K. L. (2014). “DISCOVERY OF A ∼250 K BROWN DWARF AT 2 pc FROM THE SUN”. The Astrophysical Journal. 786 (2): L18. arXiv:1404.6501. Bibcode:2014ApJ…786L..18L. doi:10.1088/2041-8205/786/2/L18. S2CID 119102654.

^ a b c d e Martin, Rebecca G.; Livio, Mario (2015). “The Solar System as an Exoplanetary System”. The Astrophysical Journal. 810 (2): one zero five. arXiv:1508.00931. Bibcode:2015ApJ…810..105M. doi:10.1088/0004-637X/810/2/one zero five. S2CID 119119390.

^ How Normal is Our Solar System?, By Susanna Kohler on 25 September 2015

^ Volk, Kathryn; Gladman, Brett (2015). “Consolidating and Crushing Exoplanets: Did it show up here?”. arXiv:1502.06558v2 [astro-ph.EP].

^ Mercury Sole Survivor of Close Orbiting Planets, Nola Taylor Redd. 8 June 2015

^ Goldreich, Peter; Lithwick, Yoram; Sari, Re’em (2004). “Final Stages of Planet Formation”. The Astrophysical Journal. 614 (1): 497–507. arXiv:astro-ph/0404240. Bibcode:2004ApJ…614..497G. doi:10.1086/423612. S2CID 16419857.

External hyperlinks

This audio report became constructed from a revision of this article dated 31 May 2021, and does not mirror next edits.

“Solar System” . Encyclopædia Britannica. 25 (11th ed.). 1911. pp. 157–158.

A Cosmic History of the Solar System

A Tediously Accurate Map of the Solar System (net based scroll map scaled to the Moon being 1 pixel)

NASA’s Solar System Exploration (Archive)

NASA’s Solar System Profile

NASA’s Solar System Simulator

NASA Eyes-on-the-Solar-System

NASA/JPL Solar System essential page

Leave a Reply

Your email address will not be published.