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Pluto

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This article is about the dwarf planet. For other uses, see Pluto (disambiguation).
Pluto Astronomical symbol of Pluto
Pluto viewed by New Horizons 1 July 2015.jpg
Pluto photographed by the New Horizons spacecraft 1 July 2015.
Discovery
Discovered by Clyde W. Tombaugh
Discovery date 18 February 1930
Designations
MPC designation 134340 Pluto
Pronunciation Listeni/ˈplt/
Named after
Pluto
Adjectives Plutonian
Orbital characteristics[4][a]
Epoch J2000
Aphelion
  • 48.871 AU
  • (7311000000 km)
Perihelion
  • 29.657 AU
  • (4437000000 km)
  • (5 September 1989)[1]
  • 39.264 AU
  • (5874000000 km)
Eccentricity 0.244671664 (J2000)
0.248 807 66 (mean)[2]
366.73 days[2]
4.7 km/s[2]
14.85 deg
Inclination
  • 17.151394° 
  • (11.88° to Sun's equator)
110.28683° 
113.76349° 
Known satellites 5
Physical characteristics
Mean radius
  • 1184±10 km[5]
  • 0.18 Earths
  • 1161 km[6] (solid)
  • 1.665×107 km2[b]
  • 0.033 Earths
Volume
  • 6.39×109 km3[c]
  • 0.0059 Earths
Mass
  • (1.305±0.007)×1022 kg[7]
  • 0.00218 Earths
  • 0.178 Moons
Mean density
2.03±0.06 g/cm3[7]
1.229 km/s[e]
Equatorial rotation velocity
47.18 km/h
119.591°±0.014°  (to orbit)[7][f]
North pole right ascension
132.993°[8]
North pole declination
−6.163°[8]
Albedo 0.49 to 0.66 (geometric, varies by 35%)[2][9]
Surface temp. min mean max
Kelvin 33 K 44 K (−229 °C) 55 K
13.65[2] to 16.3[10]
(mean is 15.1)[2]
−0.7[11]
0.065″ to 0.115″[2][g]
Atmosphere
Surface pressure
0.30 Pa (summer maximum)
Composition by volume Nitrogen, methane, carbon monoxide[12]

Pluto (minor-planet designation: 134340 Pluto) is the second-most massive known dwarf planet, after Eris. It is the largest object in the Kuiper belt[h][i] and possibly the largest known trans-Neptunian object.[i] It is the tenth-most-massive known body directly orbiting the Sun. Like other Kuiper belt objects, Pluto is primarily made of rock and ice,[13] and is relatively small—about 16 the mass of the Moon and 13 its volume. It has a moderately eccentric and inclined orbit that takes it from 30 to 49 AU (4.4–7.4 billion km) from the Sun. This means that Pluto periodically comes closer to the Sun than Neptune. However, an orbital resonance with Neptune prevents them from colliding. In 2014, Pluto was 32.6 AU from the Sun. Light from the Sun takes about 5.5 hours to reach Pluto at its average distance (39.4 AU).[14]

Pluto was discovered in 1930 and was originally considered the ninth planet from the Sun. Its status as a planet fell into question following further study of it and the outer Solar System over the following 75 years. Starting in 1977 with the discovery of the minor planet Chiron, numerous icy objects with eccentric orbits were found.[15] The scattered disc object Eris, discovered in 2005, is 27% more massive than Pluto.[16] The knowledge that Pluto is only one of several large icy bodies in the outer Solar System prompted the International Astronomical Union (IAU) to formally define the term "planet" in 2006, which excluded Pluto and reclassified it as a member of the new "dwarf planet" category (and specifically as a plutoid).[17] Astronomers who oppose the exclusion state that Pluto should remain classified as a planet, and other dwarf planets and even moons should be added to the list of planets.[18][19][20]

Pluto has five known moons: Charon (the largest, with a diameter just over half that of Pluto), Styx, Nix, Kerberos, and Hydra.[21] Pluto and Charon are sometimes considered a binary system because the barycenter of their orbits does not lie within either body.[22] The IAU has not formalized a definition for binary dwarf planets, and Charon is officially classified as a moon of Pluto.[23]

On 14 July 2015, the New Horizons probe will fly by Pluto, the first spacecraft to do so,[24] when it will take detailed measurements and images of Pluto and its moons.[25] After this, there are plans for New Horizons to visit another object in the Kuiper belt.[26]

History

Further information: Planets beyond Neptune

Discovery

In the 1840s, Urbain Le Verrier used Newtonian mechanics to predict the position of the then-undiscovered planet Neptune after analysing perturbations in the orbit of Uranus.[27] Subsequent observations of Neptune in the late 19th century led astronomers to speculate that Uranus's orbit was being disturbed by another planet besides Neptune.

In 1906, Percival Lowell—a wealthy Bostonian who had founded the Lowell Observatory in Flagstaff, Arizona, in 1894—started an extensive project in search of a possible ninth planet, which he termed "Planet X".[28] By 1909, Lowell and William H. Pickering had suggested several possible celestial coordinates for such a planet.[29] Lowell and his observatory conducted his search until his death in 1916, but to no avail. Unknown to Lowell, on 19 March 1915, surveys had captured two faint images of Pluto, but they were not recognized for what they were.[29][30] There are fifteen other known prediscoveries, with the oldest made by the Yerkes Observatory on 20 August 1909.[31]

The same area of night sky with stars, shown twice, side by side. One of the bright points, located with an arrow, changes position between the two images.
Discovery photographs of Pluto

Because of a ten-year legal battle with Constance Lowell, Percival's widow, who attempted to wrest the observatory's million-dollar portion of his legacy for herself, the search for Planet X did not resume until 1929,[32] when its director, Vesto Melvin Slipher, summarily handed the job of locating Planet X to Clyde Tombaugh, a 23-year-old Kansan who had just arrived at the Lowell Observatory after Slipher had been impressed by a sample of his astronomical drawings.[32]

Tombaugh's task was to systematically image the night sky in pairs of photographs, then examine each pair and determine whether any objects had shifted position. Using a machine called a blink comparator, he rapidly shifted back and forth between views of each of the plates to create the illusion of movement of any objects that had changed position or appearance between photographs. On 18 February 1930, after nearly a year of searching, Tombaugh discovered a possible moving object on photographic plates taken on 23 and 29 January of that year. A lesser-quality photograph taken on 21 January helped confirm the movement.[33] After the observatory obtained further confirmatory photographs, news of the discovery was telegraphed to the Harvard College Observatory on 13 March 1930.[29]

Name

See also: Venetia Burney
A young man in his mid-twenties, wearing glasses, a white shirt, tie and long trousers, stands in an open field, next to a Newtonian telescope resting on the ground and tilted towards the sky. The telescope is taller than him, and is about eight inches in diameter. His right hand is resting up on the barrel, and he looks slightly past the telescope, out to the left.
Clyde Tombaugh, the discoverer of Pluto

The discovery made headlines across the globe. The Lowell Observatory, which had the right to name the new object, received over 1,000 suggestions from all over the world, ranging from Atlas to Zymal.[34] Tombaugh urged Slipher to suggest a name for the new object quickly before someone else did.[34] Constance Lowell proposed Zeus, then Percival and finally Constance. These suggestions were disregarded.[35]

The name Pluto, after the god of the underworld, was proposed by Venetia Burney (1918–2009), a then eleven-year-old schoolgirl in Oxford, England, who was interested in classical mythology.[36] She suggested it in a conversation with her grandfather Falconer Madan, a former librarian at the University of Oxford's Bodleian Library, who passed the name to astronomy professor Herbert Hall Turner, who cabled it to colleagues in the United States.[36]

The object was officially named on 24 March 1930.[37][38] Each member of the Lowell Observatory was allowed to vote on a short-list of three: Minerva (which was already the name for an asteroid), Cronus (which had lost reputation through being proposed by the unpopular astronomer Thomas Jefferson Jackson See), and Pluto. Pluto received every vote.[39] The name was announced on 1 May 1930.[36] Upon the announcement, Madan gave Venetia £5 (equivalent to £282, or $430 USD in 2015),[40] as a reward.[36]

The choice of name was partly inspired by the fact that the first two letters of Pluto are the initials of Percival Lowell, and Pluto's astronomical symbol (♇, unicode U+2647, ♇) is a monogram constructed from the letters 'PL'.[41] Pluto's astrological symbol resembles that of Neptune (Neptune symbol.svg), but has a circle in place of the middle prong of the trident (Pluto's astrological symbol.svg).

The name was soon embraced by wider culture. In 1930, Walt Disney was apparently inspired by it when he introduced for Mickey Mouse a canine companion named Pluto, although Disney animator Ben Sharpsteen could not confirm why the name was given.[42] In 1941, Glenn T. Seaborg named the newly created element plutonium after Pluto, in keeping with the tradition of naming elements after newly discovered planets, following uranium, which was named after Uranus, and neptunium, which was named after Neptune.[43]

Most languages use the name "Pluto" in various transliterations.[j] In Japanese, Houei Nojiri suggested the translation Meiōsei (冥王星?, "Star of the King (God) of the Underworld"), and this was borrowed into Chinese, Korean, and Vietnamese.[44][45][46] Some Indian languages use the name Pluto, but others, such as Hindi, use the name of Yama, the Guardian of Hell in Hindu and Buddhist mythology, as does Vietnamese.[45] Polynesian languages also tend to use the indigenous god of the underworld, as in Maori Whiro.[45]

Planet X disproved

Once found, Pluto's faintness and lack of a resolvable disc cast doubt on the idea that it was Lowell's Planet X.[28] Estimates of Pluto's mass were revised downward throughout the 20th century.[47]

Mass estimates for Pluto
Year Mass Estimate by
1931 1 Earth Nicholson & Mayall[48][49][50]
1948 0.1 (1/10) Earth Kuiper[51]
1976 0.01 (1/100) Earth Cruikshank, Pilcher, & Morrison[52]
1978 0.002 (1/500) Earth Christy & Harrington[53]
2006 0.00218 (1/459) Earth Buie et al.[7]

Astronomers initially calculated its mass based on its presumed effect on Neptune and Uranus. In 1931 Pluto was calculated to be roughly the mass of Earth, with further calculations in 1948 bringing the mass down to roughly that of Mars.[49][51] In 1976, Dale Cruikshank, Carl Pilcher and David Morrison of the University of Hawaii calculated Pluto's albedo for the first time, finding that it matched that for methane ice; this meant Pluto had to be exceptionally luminous for its size and therefore could not be more than 1 percent the mass of Earth.[52] (Pluto's albedo is 1.3–2.0 times greater than that of Earth.[2])

In 1978, the discovery of Pluto's moon Charon allowed the measurement of Pluto's mass for the first time. Its mass, roughly 0.2% that of Earth, was far too small to account for the discrepancies in the orbit of Uranus. Subsequent searches for an alternative Planet X, notably by Robert Sutton Harrington,[54] failed. In 1992, Myles Standish used data from Voyager 2's flyby of Neptune in 1989, which had revised the estimates of Neptune's mass downward by 0.5%—an amount comparable to the mass of Mars—to recalculate its gravitational effect on Uranus. With the new figures added in, the discrepancies, and with them the need for a Planet X, vanished.[55] Today, the majority of scientists agree that Planet X, as Lowell defined it, does not exist.[56] Lowell had made a prediction of Planet X's position in 1915 that was fairly close to Pluto's position at that time; Ernest W. Brown concluded soon after Pluto's discovery that this was a coincidence,[57] a view still held today.[55]

Classification

Further information: Definition of planet
Earth Dysnomia Eris Charon Nix Hydra S/2011 (134340) 1 Pluto Makemake Namaka Hi'iaka Haumea Sedna 2007 OR10 Weywot Quaoar Vanth Orcus File:EightTNOs.png
Artistic comparison of Eris, Pluto, Makemake, Haumea, Sedna, 2007 OR10, Quaoar, Orcus, and Earth.
( )

From 1992 onward, many bodies were discovered orbiting in the same area as Pluto, showing that Pluto is part of a population of objects (which is called the Kuiper belt). This made its official status as a planet controversial, with many questioning whether Pluto should be considered together with or separately from its surrounding population. Museum and planetarium directors occasionally created controversy by omitting Pluto from planetary models of the Solar System. The Hayden Planetarium reopened after renovation in 2000 with a model of only eight planets. The controversy made headlines at the time.[58]

As objects increasingly closer in size to Pluto were discovered in the region, it was argued that Pluto should be reclassified as one of the Kuiper belt objects, just as Ceres, Pallas, Juno and Vesta eventually lost their planet status after the discovery of many other asteroids. On 29 July 2005, the discovery of a new trans-Neptunian object, Eris, was announced, which was thought to be substantially larger than Pluto. This was the largest object discovered in the Solar System since Triton in 1846. Its discoverers and the press initially called it the tenth planet, although there was no official consensus at the time on whether to call it a planet.[59] Others in the astronomical community considered the discovery the strongest argument for reclassifying Pluto as a minor planet.[60]

IAU classification

The debate came to a head in 2006 with an IAU resolution that created an official definition for the term "planet". According to this resolution, there are three main conditions for an object to be considered a 'planet':

  1. The object must be in orbit around the Sun.
  2. The object must be massive enough to be rounded by its own gravity. More specifically, its own gravity should pull it into a shape of hydrostatic equilibrium.
  3. It must have cleared the neighborhood around its orbit.[61][62]

Pluto fails to meet the third condition, because its mass is only 0.07 times that of the mass of the other objects in its orbit (Earth's mass, by contrast, is 1.7 million times the remaining mass in its own orbit).[60][62] The IAU further decided that bodies that, like Pluto, do not meet criterion 3 would be called dwarf planets.

On 13 September 2006, the IAU included Pluto and Eris and its moon Dysnomia in their Minor Planet Catalogue, giving them the official minor-planet designations "(134340) Pluto", "(136199) Eris", and "(136199) Eris I Dysnomia".[63] If Pluto had been given one upon its discovery, the number would have been about 1,164 instead of 134,340.

There has been some resistance within the astronomical community toward the reclassification.[64][65][66] Alan Stern, principal investigator with NASA's New Horizons mission to Pluto, publicly derided the IAU resolution, stating that "the definition stinks, for technical reasons".[67] Stern's contention was that by the terms of the new definition Earth, Mars, Jupiter, and Neptune, all of which share their orbits with asteroids, would be excluded.[68] His other claim was that because less than five percent of astronomers voted for it, the decision was not representative of the entire astronomical community.[68] Marc W. Buie, then at Lowell Observatory, voiced his opinion on the new definition on his website and petitioned against the definition.[69] Others have supported the IAU. Mike Brown, the astronomer who discovered Eris, said "through this whole crazy circus-like procedure, somehow the right answer was stumbled on. It's been a long time coming. Science is self-correcting eventually, even when strong emotions are involved."[70]

A promotional event with a staged Pluto "protest". Members playing protesters of the reclassification of Pluto on the left, with those playing counter-protesters on the right

Public reception to the IAU decision was mixed. Although many accepted the reclassification, some sought to overturn the decision with online petitions urging the IAU to consider reinstatement. A resolution introduced by some members of the California State Assembly facetiously called the IAU decision a "scientific heresy".[71] New Mexico's House of Representatives passed a resolution in honor of Tombaugh, a longtime resident of that state, that declared that Pluto will always be considered a planet while in New Mexican skies and that 13 March 2007, was Pluto Planet Day.[72][73] The Illinois State Senate passed a similar resolution in 2009, on the basis that Clyde Tombaugh, the discoverer of Pluto, was born in Illinois. The resolution asserted that Pluto was "unfairly downgraded to a 'dwarf' planet" by the IAU.[74] Some members of the public have also rejected the change, citing the disagreement within the scientific community on the issue, or for sentimental reasons, maintaining that they have always known Pluto as a planet and will continue to do so regardless of the IAU decision.[75]

In 2006 in its 17th annual words of the year vote, the American Dialect Society voted plutoed as the word of the year. To "pluto" is to "demote or devalue someone or something".[76]

Researchers on both sides of the debate gathered on 14–16 August 2008, at the Johns Hopkins University Applied Physics Laboratory for a conference that included back-to-back talks on the current IAU definition of a planet.[77] Entitled "The Great Planet Debate",[78] the conference published a post-conference press release indicating that scientists could not come to a consensus about the definition of planet.[79] Just before the conference, on 11 June 2008, the IAU announced in a press release that the term "plutoid" would henceforth be used to refer to Pluto and other objects that have an orbital semimajor axis greater than that of Neptune and enough mass to be of near-spherical shape.[80][81][82]

Orbit and rotation

Orbit of Pluto—ecliptic view. This "side view" of Pluto's orbit (in red) shows its large inclination to the ecliptic.

Pluto's orbital period is 248 Earth years. Its orbital characteristics are substantially different from those of the planets, which follow nearly circular orbits around the Sun close to a flat reference plane called the ecliptic. In contrast, Pluto's orbit is highly inclined relative to the ecliptic (over 17°) and highly eccentric (elliptical). This high eccentricity means a small region of Pluto's orbit lies nearer the Sun than Neptune's. The Pluto–Charon barycenter came to perihelion on 5 September 1989,[1][k] and was last closer to the Sun than Neptune between 7 February 1979, and 11 February 1999.[83]

In the long term, Pluto's orbit is chaotic. Although computer simulations can be used to predict its position for several million years (both forward and backward in time), after intervals longer than the Lyapunov time of 10–20 million years, calculations become speculative: Pluto is sensitive to unmeasurably small details of the Solar System, hard-to-predict factors that will gradually disrupt its orbit.[84][85]

Relationship with Neptune

Orbit of Pluto—polar view. This "view from above" shows how Pluto's orbit (in red) is less circular than Neptune's (in blue), and how Pluto is sometimes closer to the Sun than Neptune. The darker halves of both orbits show where they pass below the plane of the ecliptic.

Despite Pluto's orbit appearing to cross that of Neptune when viewed from directly above, the two objects' orbits are aligned so that they can never collide or even approach closely. There are several reasons why.

At the simplest level, one can examine the two orbits and see that they do not intersect. When Pluto is closest to the Sun, and hence closest to Neptune's orbit as viewed from above, it is also the farthest above Neptune's path. Pluto's orbit passes about 8 AU above that of Neptune, preventing a collision.[86][87][88] Pluto's ascending and descending nodes, the points at which its orbit crosses the ecliptic, are currently separated from Neptune's by over 21°.[89]

This alone is not enough to protect Pluto; perturbations from the planets (especially Neptune) could alter aspects of Pluto's orbit (such as its orbital precession) over millions of years so that a collision could be possible. Some other mechanism or mechanisms must therefore be at work. The most significant of these is that Pluto lies in the 2:3 mean-motion resonance with Neptune: for every two orbits that Pluto makes around the Sun, Neptune makes three. The two objects then return to their initial positions and the cycle repeats, each cycle lasting about 500 years. This pattern is such that, in each 500-year cycle, the first time Pluto is near perihelion, Neptune is over 50° behind Pluto. By Pluto's second perihelion, Neptune will have completed a further one and a half of its own orbits, and so will be a similar distance ahead of Pluto. Pluto and Neptune's minimum separation is over 17 AU. Pluto comes closer to Uranus (11 AU) than it does to Neptune.[88]

The 2:3 resonance between the two bodies is highly stable, and is preserved over millions of years.[90] This prevents their orbits from changing relative to one another; the cycle always repeats in the same way, and so the two bodies can never pass near each other. Thus, even if Pluto's orbit were not highly inclined, the two bodies could never collide.[88]

Other factors

Numerical studies have shown that over periods of millions of years, the general nature of the alignment between the orbits of Pluto and Neptune does not change.[86][91] There are several other resonances and interactions that govern the details of their relative motion, and enhance Pluto's stability. These arise principally from two additional mechanisms (besides the 2:3 mean-motion resonance).

First, Pluto's argument of perihelion, the angle between the point where it crosses the ecliptic and the point where it is closest to the Sun, librates around 90°.[91] This means that when Pluto is closest to the Sun, it is at its farthest above the plane of the Solar System, preventing encounters with Neptune. This is a direct consequence of the Kozai mechanism,[86] which relates the eccentricity of an orbit to its inclination to a larger perturbing body—in this case Neptune. Relative to Neptune, the amplitude of libration is 38°, and so the angular separation of Pluto's perihelion to the orbit of Neptune is always greater than 52° (90°–38°). The closest such angular separation occurs every 10,000 years.[90]

Second, the longitudes of ascending nodes of the two bodies—the points where they cross the ecliptic—are in near-resonance with the above libration. When the two longitudes are the same—that is, when one could draw a straight line through both nodes and the Sun—Pluto's perihelion lies exactly at 90°, and hence it comes closest to the Sun when it is highest above Neptune's orbit. This is known as the 1:1 superresonance. All the Jovian planets, particularly Jupiter, play a role in the creation of the superresonance.[86]

To understand the nature of the libration, imagine a polar point of view, looking down on the ecliptic from a distant vantage point where the planets orbit counterclockwise. After passing the ascending node, Pluto is interior to Neptune's orbit and moving faster, approaching Neptune from behind. The strong gravitational pull between the two causes angular momentum to be transferred to Pluto, at Neptune's expense. This moves Pluto into a slightly larger orbit, where it travels slightly more slowly, according to Kepler's third law. As its orbit changes, this has the gradual effect of changing the perihelion and longitude of Pluto's orbit (and, to a lesser degree, of Neptune). After many such repetitions, Pluto is sufficiently slowed, and Neptune sufficiently speeded up, that Neptune begins to catch up with Pluto at the opposite side of its orbit (near the opposing node to where we began). The process is then reversed, and Pluto loses angular momentum to Neptune, until Pluto is sufficiently speeded up that it begins to catch Neptune again at the original node. The whole process takes about 20,000 years to complete.[88][90]

Rotation

Images of nearly one orbit of Charon around Pluto, taken by New Horizons along the ecliptic on 19–24 July 2014, showing its sideways rotation.

Pluto's rotation period, its day, is equal to 6.39 Earth days.[92] Like Uranus, Pluto rotates on its "side" on its orbital plane, with an axial tilt of 120°, and so its seasonal variation is extreme; at its solstices, one-fourth of its surface is in continuous daylight, whereas another fourth is in continuous darkness.[93]

Quasi-satellite

At least one minor body, (15810) 1994 JR1, is a quasi-satellite of Pluto, a specific type of co-orbital configuration.[94] It has been a quasi-satellite of Pluto for about 100,000 years and it will remain so for perhaps another 250,000 years. Its quasi-satellite behavior is recurrent with a periodicity of 2 million years.[94][95] There may be additional Pluto co-orbitals.

Physical characteristics

Map of Pluto's surface by NASA, ESA and Marc W. Buie
Hubble map of Pluto's surface, showing great variations in color and albedo
Three views of Pluto from different orientations

Because of Pluto's distance from Earth, in-depth study from Earth is difficult. Therefore, many details about Pluto will remain unknown until 14 July 2015 and onwards, when New Horizons will fly through the Pluto system, sending data back to Earth for analysis.[24]

Surface

Pluto's surface is composed of more than 98 percent nitrogen ice, with traces of methane and carbon monoxide.[96] The face of Pluto oriented toward Charon contains more methane ice, whereas the opposite face contains more nitrogen and carbon monoxide ice.[97]

Maps produced from images taken by the Hubble Space Telescope (HST), together with Pluto's lightcurve and the periodic variations in its infrared spectra, indicate that Pluto's surface is very varied, with large changes in both brightness and color.[98] Pluto is one of the most contrastive bodies in the Solar System, with as much contrast as Saturn's moon Iapetus.[99] The color varies between charcoal black, dark orange and white:[100] Buie et al. term it "significantly less red than Mars and much more similar to the hues seen on Io with a slightly more orange cast".[101]

Pluto's surface has changed between 1994 and 2002–3: the northern polar region has brightened and the southern hemisphere has darkened.[100] Pluto's overall redness has also increased substantially between 2000 and 2002.[100] These rapid changes are probably related to seasonal condensation and sublimation of portions of Pluto's atmosphere, amplified by Pluto's extreme axial tilt and high orbital eccentricity.[100]

Surface feature nomenclature

In anticipation of the forthcoming mapping of Pluto's surface by New Horizons, the International Astronomical Union has decided that its surface features will be given names deriving from the following themes: historic explorers, space missions, spacecraft, scientists and engineers; fictional explorers, travellers, vessels, destinations and origins; authors and artists who have envisioned exploration; and underworlds, underworld beings, and travellers to the underworld. In collaboration with the New Horizons science team, the IAU has invited members of the public to propose names and vote on them before the spacecraft's arrival.[102]

Internal structure

Theoretical structure of Pluto[103]
1. Frozen nitrogen[96]
2. Water ice
3. Rock

Pluto's density is 2.03±0.06 g/cm3.[7] Because the decay of radioactive elements would eventually heat the ices enough for the rock to separate from them, scientists expect that Pluto's internal structure is differentiated, with the rocky material having settled into a dense core surrounded by a mantle of ice. The diameter of the core is hypothesized to be approximately 1700 km, 70% of Pluto's diameter.[103] It is possible that such heating continues today, creating a subsurface ocean layer of liquid water some 100 to 180 km thick at the core–mantle boundary.[103][104] The DLR Institute of Planetary Research calculated that Pluto's density-to-radius ratio lies in a transition zone, along with Neptune's moon Triton, between icy satellites like the mid-sized moons of Uranus and Saturn, and rocky satellites such as Jupiter's Io.[105]

Mass and size

Size comparison of Earth, the Moon, and Pluto (bottom left). Pluto's volume is about 0.6% that of Earth.
Pluto and Charon compared to the United States

Pluto's mass is 1.31×1022 kg, less than 0.24 percent that of Earth,[106] and its diameter is 2306±20 km, or roughly 66% that of the Moon.[7] Its surface area is 1.665×107 km2, approximately 10% less than that of South America. Pluto's atmosphere complicates determining its true solid size within a certain margin.[6] Pluto's albedo varies from 0.49–0.66.[9]

The discovery of Pluto's satellite Charon in 1978 enabled a determination of the mass of the Pluto–Charon system by application of Newton's formulation of Kepler's third law. Once Charon's gravitational effect was measured, the mass of the Pluto–Charon system could be determined. Observations of Pluto in occultation with Charon allowed scientists to establish Pluto's diameter more accurately, whereas the invention of adaptive optics allowed them to determine its shape more accurately.[107]

Selected size estimates for Pluto
Year Radius (diameter) Notes
1993 1195 (2390) km Millis, et al.[108] (if no haze)[109]
1993 1180 (2360) km Millis, et al. (surface & haze)[109]
1994 1164 (2328) km Young & Binzel[110]
2006 1153 (2306) km Buie, et al.[7]
2007 1161 (2322) km Young, Young, & Buie[6]
2011 1180 (2360) km Zalucha, et al.[111]
2014 1184 (2368) km Lellouch, et al.[5]

With less than 0.2 lunar masses, Pluto is much less massive than the terrestrial planets, and also less massive than seven moons, Ganymede, Titan, Callisto, Io, the Moon, Europa, and Triton.

Pluto is more than twice the diameter and a dozen times the mass of the dwarf planet Ceres, the largest object in the asteroid belt. It is less massive than the dwarf planet Eris, a trans-Neptunian object discovered in 2005. Given the error bars in the different size estimates, it is currently unknown whether Eris or Pluto has the larger diameter.[109] Both Pluto and Eris are estimated to have solid-body diameters of about 2330 km.[109]

Determinations of Pluto's size are complicated by its atmosphere, and possible hydrocarbon haze.[109] In March 2014, Lellouch, de Bergh et al. published findings regarding methane mixing ratios in Pluto's atmosphere consistent with a Plutonian diameter greater than 2360 km, with a "best guess" of 2368 km, which would make it slightly larger than Eris.[5]

Atmosphere

Main article: Atmosphere of Pluto

Pluto has a thin atmosphere consisting of nitrogen (N2), methane (CH4), and carbon monoxide (CO), which are in equilibrium with their ices on Pluto's surface.[112] The surface pressure ranges from 6.5 to 24 μbar (0.65 to 2.4 Pa),[113] roughly one million to 100,000 times less than Earth's atmospheric pressure. Pluto's elliptical orbit is predicted to have a major effect on its atmosphere: as Pluto moves away from the Sun, its atmosphere should gradually freeze out. When Pluto is closer to the Sun, the temperature of Pluto's solid surface increases, causing the ices to sublimate. Just like sweat cools the body as it evaporates from the skin, this sublimation cools the surface of Pluto.[114]

The presence of methane, a powerful greenhouse gas, in Pluto's atmosphere creates a temperature inversion, with average temperatures 36 K warmer 10 km above the surface.[115] The lower atmosphere contains a higher concentration of methane than its upper atmosphere.[115]

Even though Pluto is receding from the Sun, in 2002, the atmospheric pressure (0.3 Pa) was higher than in 1988, because in 1987, the north pole of Pluto came out of the shadow for the first time in 120 years, causing extra nitrogen to start sublimating from the polar cap. It will take decades for this nitrogen to condense out of the atmosphere as it freezes onto Pluto's now continuously dark south pole's ice cap.[116]

On 29 June 2015, Pluto passed between a distant star and Earth, producing a shadow on Earth near New Zealand that allowed SOFIA, an airborne observatory, to study the atmosphere of Pluto.[117]

Satellites

Main article: Moons of Pluto
The Pluto system: Pluto, Charon, Styx, Nix, Kerberos, and Hydra, taken by the Hubble Space Telescope in July 2012[118]
Comparison of the scale and brightness of the moons of Pluto (artist's concept).[119]

Pluto has five known natural satellites: Charon, first identified in 1978 by astronomer James Christy; Nix and Hydra, both discovered in 2005,[120] Kerberos, discovered in 2011,[121] and Styx, discovered in 2012.[122] The satellites' orbits are circular (eccentricity < 0.006) and coplanar with Pluto's equator (inclination < 1°),[123][124] and therefore tilted approximately 120° relative to Pluto's orbit. The Plutonian system is highly compact: the five known satellites orbit within the inner 3% of the region where prograde orbits would be stable.[125] Closest to Pluto orbits Charon, which is large enough to be in hydrostatic equilibrium and for the system's barycenter to be outside Pluto. Beyond Charon orbit Pluto's smaller circumbinary moons, Styx, Nix, Kerberos, and Hydra, respectively.

The orbital periods of all of Pluto's moons are linked in a system of orbital resonances and near resonances.[126][124] When precession is accounted for, the orbital periods of Styx, Nix, and Hydra are in an exact 18:22:33 ratio.[124] There is also a 3:4:5:6 sequence of approximate ratios between the periods of Styx, Nix, Kerberos and Hydra with that of Charon, which becomes closer to exact going outward.[124][127]

The Pluto–Charon system is one of the few systems in the Solar System whose barycenter lies above the primary's surface (617 Patroclus is a smaller example, the Sun and Jupiter the only larger one).[128] This and the large size of Charon relative to Pluto have led some astronomers to call it a double dwarf planet.[129] The system is also unusual among planetary systems in that each is tidally locked to the other: Charon always presents the same face to Pluto, and Pluto always presents the same face to Charon: from any position on either body, the other is always at the same position in the sky, or always obscured.[130] This also means that the rotation period of each is equal to the time it takes the entire system to rotate around its common center of gravity.[92] In 2007, observations by the Gemini Observatory of patches of ammonia hydrates and water crystals on the surface of Charon suggested the presence of active cryo-geysers.[131]

Pluto's moons are believed to have been formed by a collision between Pluto and a similar-sized body early in the history of the Solar System. The collision released material that consolidated into the moons around Pluto.[132] However, Kerberos has a much lower albedo than the other moons of Pluto,[133] which is difficult to explain with a giant collision.[134]

Origins

Further information: Kuiper belt and Nice model
Plot of the known Kuiper belt objects, set against the four giant planets

Pluto's origin and identity had long puzzled astronomers. One early hypothesis was that Pluto was an escaped moon of Neptune, knocked out of orbit by its largest current moon, Triton. This idea was eventually rejected after dynamical studies of the two planets' orbits showed it to be impossible.[135][136]

Pluto's true place in the Solar System began to reveal itself only in 1992, when astronomers began to find small icy objects beyond Neptune that were similar to Pluto not only in orbit but also in size and composition. This trans-Neptunian population is believed to be the source of many short-period comets. Astronomers now believe Pluto to be the largest[i] member of the Kuiper belt, a stable belt of objects located between 30 and 50 AU from the Sun. As of 2011, surveys of the Kuiper belt to magnitude 21 were nearly complete and any remaining Pluto-sized objects are expected to be beyond 100 AU from the Sun.[137] Like other Kuiper-belt objects (KBOs), Pluto shares features with comets; for example, the solar wind is gradually blowing Pluto's surface into space, in the manner of a comet.[138] It has been claimed that if Pluto were placed as near to the Sun as Earth, it would develop a tail, as comets do.[139] This claim has been disputed with the argument that Pluto's escape velocity is too high for this to happen.[140]

Though Pluto is the largest Kuiper belt object discovered,[109][i] Neptune's moon Triton, which is slightly larger than Pluto, is similar to it both geologically and atmospherically, and is believed to be a captured Kuiper belt object.[141] Eris (see below) is about the same size as Pluto (though more massive) but is not strictly considered a member of the Kuiper belt population. Rather, it is considered a member of a linked population called the scattered disc.

A large number of Kuiper belt objects, like Pluto, are in a 2:3 orbital resonance with Neptune. KBOs with this orbital resonance are called "plutinos", after Pluto.[142]

Like other members of the Kuiper belt, Pluto is thought to be a residual planetesimal; a component of the original protoplanetary disc around the Sun that failed to fully coalesce into a full-fledged planet. Most astronomers agree that Pluto owes its current position to a sudden migration undergone by Neptune early in the Solar System's formation. As Neptune migrated outward, it approached the objects in the proto-Kuiper belt, setting one in orbit around itself (Triton), locking others into resonances, and knocking others into chaotic orbits. The objects in the scattered disc, a dynamically unstable region overlapping the Kuiper belt, are believed to have been placed in their current positions by interactions with Neptune's migrating resonances.[143] A computer model created in 2004 by Alessandro Morbidelli of the Observatoire de la Côte d'Azur in Nice suggested that the migration of Neptune into the Kuiper belt may have been triggered by the formation of a 1:2 resonance between Jupiter and Saturn, which created a gravitational push that propelled both Uranus and Neptune into higher orbits and caused them to switch places, ultimately doubling Neptune's distance from the Sun. The resultant expulsion of objects from the proto-Kuiper belt could also explain the Late Heavy Bombardment 600 million years after the Solar System's formation and the origin of the Jupiter trojans.[144] It is possible that Pluto had a near-circular orbit about 33 AU from the Sun before Neptune's migration perturbed it into a resonant capture.[145] The Nice model requires that there were about a thousand Pluto-sized bodies in the original planetesimal disk, which included Triton and Eris.[144]

Observation and exploration

Pluto's distance from Earth makes in-depth study from Earth difficult. Many details about Pluto will remain unknown until 14 July 2015 and onwards, when New Horizons will fly through the Pluto system, sending data back to Earth for analysis.[24]

Observations

Pluto's visual apparent magnitude averages 15.1, brightening to 13.65 at perihelion.[2] To see it, a telescope is required; around 30 cm (12 in) aperture being desirable.[146] It looks star-like and without a visible disk even in large telescopes, because its angular diameter is only 0.11".

The earliest maps of Pluto, made in the late 1980s, were brightness maps created from close observations of eclipses by its largest moon, Charon. Observations were made of the change in the total average brightness of the Pluto–Charon system during the eclipses. For example, eclipsing a bright spot on Pluto makes a bigger total brightness change than eclipsing a dark spot. Computer processing of many such observations can be used to create a brightness map. This method can also track changes in brightness over time.[147][148]

Current maps have been produced from images taken by the Hubble Space Telescope (HST), which offers the highest resolution currently available, and show considerably more detail,[99] resolving variations several hundred kilometres across, including polar regions and large bright spots.[101] The maps are produced by complex computer processing, which find the best-fit projected maps for the few pixels of the Hubble images.[149] The two cameras on the HST used for these maps are no longer in service, so these will likely remain the most detailed maps of Pluto until the flyby of New Horizons in July 2015.[149]

Exploration

Further information: New Horizons
New Horizons, launched on 19 January 2006
First Pluto sighting from New Horizons
The first released color animation of Pluto and Charon by New Horizons

Pluto presents significant challenges for spacecraft because of its small mass and large distance from Earth. Voyager 1 could have visited Pluto, but controllers opted instead for a close flyby of Saturn's moon Titan, resulting in a trajectory incompatible with a Pluto flyby. Voyager 2 never had a plausible trajectory for reaching Pluto.[150] No serious attempt to explore Pluto by spacecraft occurred until the last decade of the 20th century. In August 1992, JPL scientist Robert Staehle telephoned Pluto's discoverer, Clyde Tombaugh, requesting permission to visit his planet. "I told him he was welcome to it", Tombaugh later remembered, "though he's got to go one long, cold trip".[151] Despite this early momentum, in 2000, NASA cancelled the Pluto Kuiper Express mission, citing increasing costs and launch vehicle delays.[152]

After an intense political battle, a revised mission to Pluto, dubbed New Horizons, was granted funding from the US government in 2003.[153] New Horizons was launched successfully on 19 January 2006. The mission leader, S. Alan Stern, confirmed that some of the ashes of Clyde Tombaugh, who died in 1997, had been placed aboard the spacecraft.[154]

In early 2007 the craft made use of a gravity assist from Jupiter. Its closest approach to Pluto will be on 14 July 2015; scientific observations of Pluto have begun five months before the closest approach and will continue for at least a month after the encounter. New Horizons captured its first (distant) images of Pluto in late September 2006, during a test of the Long Range Reconnaissance Imager (LORRI).[155] The images, taken from a distance of approximately 4.2 billion kilometres, confirm the spacecraft's ability to track distant targets, critical for maneuvering toward Pluto and other Kuiper belt objects.

New Horizons will use a remote sensing package that includes imaging instruments and a radio science investigation tool, as well as spectroscopic and other experiments, to characterize the global geology and morphology of Pluto and its moon Charon, map their surface composition and analyse Pluto's neutral atmosphere and its escape rate. New Horizons will also photograph the surfaces of Pluto and Charon.

Pluto's small moons, discovered shortly before and after the probe's launch, may present it with unforeseen challenges. Debris from collisions between Kuiper belt objects and the smaller moons, with their relatively low escape velocities, may produce a tenuous dusty ring. If New Horizons flies through such a ring system, there would be an increased potential for micrometeoroid damage that could disable the probe.[156]

On 4 February 2015, NASA released new images of Pluto (taken on 25 and 27 January) from the approaching probe.[157] New Horizons was more than 203,000,000 km (126,000,000 mi) away from Pluto when it began taking the photos, which showed Pluto and its largest moon, Charon.

On 20 March 2015, NASA invited the general public to suggest names for surface features that will be discovered on Pluto and Charon.[158]

On 15 April 2015, Pluto was imaged showing a possible polar cap.[159]

Concepts

A Pluto orbiter/lander/sample return mission was proposed in 2003. The plan included a twelve-year trip from Earth to Pluto, mapping from orbit, multiple landings, a warm water probe, and possible in situ propellant production for another twelve-year trip back to Earth with samples. Power and propulsion would come from the bimodal MITEE nuclear reactor system.[160]

Gallery

January 2015: New Horizons takes images of Pluto and its largest moon, Charon. 
April 2015: Pluto and its moon Charon. Possible polar cap on Pluto detected.[159] 
May 2015: Pluto as seen by LORRI during AP2 on May 12 from distance of 46,6 million miles, 2015[161] 
May 2015: Pluto as seen by LORRI during AP2 on May 29 to June 2[162] 
June 2015: Pluto system, taken by the New Horizons space probe. 
June 2015: Pluto (left) and its moon Charon, taken by the New Horizons space probe. 
June 2015: Pluto - two faces - away from Charon (left); toward Charon (right). 
June 2015: Pluto - two different sides - in color. 

See also

Notes

  1. ^ Orbital elements refer to the barycenter of the Pluto system, and are the instantaneous osculating values at the precise J2000 epoch. Barycenter quantities are given because, in contrast to the planetary center, they do not experience appreciable changes on a day-to-day basis from the motion of the moons. The orbital period of Pluto is listed as 248 years because most references use the more stable barycenter of the Solar System (Sun+Jupiter) to list the orbital period of the Pluto-Charon system. A J2000 heliocentric solution would give a value of 246 years.
  2. ^ Surface area derived from the radius r: 4\pi r^2.
  3. ^ Volume v derived from the radius r: 4\pi r^3/3.
  4. ^ Surface gravity derived from the mass M, the gravitational constant G and the radius r: GM/r^2.
  5. ^ Escape velocity derived from the mass M, the gravitational constant G and the radius r: \sqrt{2GM/r}.
  6. ^ Based on the orientation of Charon's orbit, which is assumed the same as Pluto's spin axis due to the mutual tidal locking.
  7. ^ Based on geometry of minimum and maximum distance from Earth and Pluto radius in the factsheet
  8. ^ Astronomers do not expect to find an object larger than Pluto closer than 100 AU from the Sun. Of the 1547 TNOs known, 1347 of them have perihelion further out than Neptune (30.1 AU).
  9. ^ a b c d The dwarf planet Eris is roughly the same size as Pluto, about 2330 km; estimates of Pluto's size are currently uncertain due to Pluto's atmosphere, which may be increasing its apparent diameter. Eris is, however, 28% more massive than Pluto. Eris is a scattered-disc object, often considered a distinct population from Kuiper-belt objects like Pluto; Pluto is the largest body in the Kuiper belt proper, which excludes the scattered objects.
  10. ^ The equivalence is less close in languages whose phonology differs widely from Greek's, such as Somali Buluuto and Navajo Tłóotoo.
  11. ^ The discovery of Charon in 1978 allowed astronomers to accurately calculate the mass of the Plutonian system. But it did not indicate the two bodies' individual masses, which could only be estimated after other moons of Pluto's were discovered in late 2005. As a result, because Pluto came to perihelion in 1989, most Pluto perihelion date estimates are based on the Pluto–Charon barycenter. Charon came to perihelion 1989-Sep-04. The Pluto–Charon barycenter came to perihelion 1989-Sep-05. Pluto came to perihelion 1989-Sep-08.

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