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NH-Charon-Day1-TenImages-20150714-20151120

Mosaic of best-resolution images of Charon from different angles

Charon, also called (134340) Pluto I,[1] is the largest of the five known moons of the dwarf planet Pluto. It was discovered in 1978 at the United States Naval Observatory in Washington, D.C., using photographic plates taken at the United States Naval Observatory Flagstaff Station (NOFS). With half the diameter and one eighth the mass of Pluto, it is a very large moon in comparison to its parent body. Its gravitational influence is such that the barycenter of the Pluto–Charon system lies outside Pluto.

The New Horizons spacecraft, to date the only probe to have visited the Pluto system, approached within 27,000 km (Template:Convert/round mi) of Charon.

HistoryEdit

DiscoveryEdit

Charon Discovery

Charon's discovery at the Naval Observatory Flagstaff Station as a time-varying bulge on the image of Pluto (seen near the top at left, but absent on the right). Negative image.

Charon was discovered by United States Naval Observatory astronomer James Christy, using the 1.55-meter telescope at NOFS,[2] and was formally announced to the world via the International Astronomical Union on July 7, 1978.[3] On June 22, 1978, he had been examining highly magnified images of Pluto on photographic plates taken at the 61-inch (Template:Convert/LoffAonSon) Flagstaff telescope two months prior. Christy noticed that a slight elongation appeared periodically. Later, the bulge was confirmed on plates dating back to April 29, 1965.

Subsequent observations of Pluto determined that the bulge was due to a smaller accompanying body. The periodicity of the bulge corresponded to Pluto's rotation period, which was previously known from Pluto's light curve. This indicated a synchronous orbit, which strongly suggested that the bulge effect was real and not spurious. This resulted in reassessments of Pluto's size, mass, and other physical characteristics, because the calculated mass and albedo of the Pluto–Charon system had previously been attributed to Pluto alone.

Doubts about Charon's existence were erased when it and Pluto entered a five-year period of mutual eclipses and transits between 1985 and 1990. This occurs when the Pluto–Charon orbital plane is edge-on as seen from Earth, which only happens at two intervals in Pluto's 248-year orbital period. It was fortuitous that one of these intervals happened to occur soon after Charon's discovery.

NameEdit

Charon was originally known by the temporary designation S/1978 P 1, according to the then recently instituted convention. On June 24, 1978, Christy first suggested the name Charon as a scientific-sounding version of his wife Charlene's nickname, "Char".[4][5] Although colleagues at the Naval Observatory proposed Persephone, Christy stuck with Charon after discovering it coincidentally refers to a Greek mythological figure:[4] Charon (Template:IPAc-en or Template:IPAc-en; Greek Χάρων) is the ferryman of the dead, closely associated in myth with the god Hades, whom the Romans identified with their god Pluto. The IAU officially adopted the name in late 1985 and it was announced on January 3, 1986.[6]

There is minor debate over the preferred pronunciation of the name. The practice of following the classical pronunciation established for the mythological ferryman Charon (IPA Template:IPA) is used by major English-language dictionaries, such as the Merriam-Webster and Oxford English Dictionary.[7][8] These indicate only one pronunciation of "Charon" when referring specifically to Pluto's moon: with an initial "k" sound. Speakers of many languages other than English, and many English-speaking astronomers as well, follow this pronunciation.[9]

However, Christy himself pronounced the ch as sh (IPA Template:IPA), after his wife Charlene. Because of this, as an acknowledgement of Christy and sometimes as an in-joke or shibboleth, the initial sh pronunciation is common among astronomers when speaking English,[10][9][11][12] and this is the prescribed pronunciation at NASA and of the New Horizons team.[13][14]

FormationEdit

Simulation work published in 2005 by Robin Canup suggested that Charon could have been formed by a collision around 4.5 billion years ago, much like Earth and the Moon. In this model, a large Kuiper belt object struck Pluto at high velocity, destroying itself and blasting off much of Pluto's outer mantle, and Charon coalesced from the debris.[15] However, such an impact should result in an icier Charon and rockier Pluto than scientists have found. It is now thought that Pluto and Charon might have been two bodies that collided before going into orbit about each other. The collision would have been violent enough to boil off volatile ices like methane (Template:Chem) but not violent enough to have destroyed either body. The very similar density of Pluto and Charon implies that the parent bodies were not fully differentiated when the impact occurred.[16]

OrbitEdit

Pluto-Charon System

An oblique view of the Pluto–Charon system showing that Pluto orbits a point outside itself. Also visible is the mutual tidal locking between the two bodies.

Charon and Pluto orbit each other every 6.387 days. The two objects are gravitationally locked to one another, so each keeps the same face towards the other. This is a case of mutual tidal locking, as compared to that of the Earth and the Moon, where the Moon always shows the same face to Earth, but not vice versa. The average distance between Charon and Pluto is 19,570 kilometres (Template:Convert/round mi). The discovery of Charon allowed astronomers to calculate accurately the mass of the Plutonian system, and mutual occultations revealed their sizes. However, neither indicated the two bodies' individual masses, which could only be estimated, until the discovery of Pluto's outer moons in late 2005. Details in the orbits of the outer moons reveal that Charon has approximately 12.18% of the mass of Pluto.[17] This shows it to have a density of 1.702 ± 0.021 g/cm3, suggesting a composition of 55 ± 5% rock to 45% ice, whereas Pluto is somewhat denser and about 70% rock.

Physical characteristicsEdit

Main article: Geology of Charon
Charonsinre

The two conflicting theories about Charon's internal structure

Charon, Earth & Moon size comparison

Size comparisons: Earth, the Moon, and Charon

Charon's diameter is 1,212 kilometres (Template:Convert/round mi), just over half that of Pluto,[17] and larger than the dwarf planet Ceres. Charon is sufficiently massive to have collapsed into a spheroid under its own gravity. Charon's slow rotation means that there is almost no flattening. Its equatorial and polar radii differ by less than 1%[18]

InteriorEdit

Charon's volume and mass allow calculation of its density, Template:Val,[17] from which it can be determined that Charon is slightly less dense than Pluto and thus contains a larger proportion of ice relative to rock in its interior. The difference is considerably lower than that of most suspected collisional satellites. Before New Horizons' flyby, there were two conflicting theories about Charon's internal structure: some scientists thought Charon to be a differentiated body like Pluto, with a rocky core and an icy mantle, whereas others thought it would be uniform throughout.[19] Evidence in support of the former position was found in 2007, when observations by the Gemini Observatory of patches of ammonia hydrates and water crystals on the surface of Charon suggested the presence of active cryogeysers. The fact that the ice was still in crystalline form suggested it had been deposited recently, because solar radiation would have degraded it to an amorphous state after roughly thirty thousand years.[20]

SurfaceEdit

Charon-Neutral-Bright-Release

Charon in enhanced color to bring out differences in surface composition

Unlike Pluto's surface, which is composed of nitrogen and methane ices, Charon's surface appears to be dominated by the less volatile water ice. 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 cryogeysers and cryovolcanoes.[20][21]

Photometric mapping of Charon's surface shows a latitudinal trend in albedo, with a bright equator band and darker poles. The north polar region is dominated by a very large dark area informally dubbed "Mordor" by the New Horizons team.[22][23][24] The favored explanation for this phenomenon is that they are formed by condensation of gases that escaped from Pluto's atmosphere. In winter, the temperature is −258 °C, and these gases, which include nitrogen, carbon monoxide, and methane, condense into their solid forms; when these ices are subjected to solar radiation, they chemically react to form various reddish tholins. Later, when the area is again heated by the Sun as Charon's seasons change, the temperature at the pole rises to −213 °C, resulting in the volatiles sublimating and escaping Charon, leaving only the tholins behind. Over millions of years, the residual tholin builds up thick layers, obscuring the icy crust.[25] In addition to Mordor, New Horizons found evidence of extensive past geology that suggests that Charon is probably differentiated;[23] in particular, the southern hemisphere has fewer craters than the northern and is considerably less rugged, suggesting that a massive resurfacing event—perhaps prompted by the partial or complete freezing of an internal ocean—occurred at some point in the past and removed many of the earlier craters.[26]

PIA20036-Charon-YoungestCrater-20150714

Charon – youngest crater

Mountain in a moatEdit

In a released photo by New Horizons, an unusual surface feature has captivated and baffled the scientist team of the mission. The image reveals a mountain rising out of a depression, in a zoomed in view. It's "a large mountain sitting in a moat", said Jeff Moore, of NASA’s Ames Research Center, in a statement. "This is a feature that has geologists stunned and stumped", he added. New Horizons captured the photo from a distance of 49,000 miles (Template:Convert/round km).[27][28]

Observation and explorationEdit

Since the first blurred images of the moon (1), images showing Pluto and Charon resolved into separate disks were taken for the first time by the Hubble Space Telescope in the 1990s (2). The telescope was responsible for the best, yet low quality images of the moon. In 1994, the clearest picture of the Pluto-Charon system showed two distinct and well defined circles (3). The image was taken by Hubble's Faint Object Camera (FOC) when the system was 2.6 billion miles (4.4 billion kilometers) away from Earth[29] Later, the development of adaptive optics made it possible to resolve Pluto and Charon into separate disks using ground-based telescopes.[5]

In June 2015, the New Horizons spacecraft captured consecutive images of the Pluto–Charon system as it approached it. The images were put together in an animation. It was the best image of Charon to that date (4). In July 2015, the New Horizons spacecraft made its closest approach to the Pluto system. It is the only spacecraft to date to have visited and studied Charon.

Template:Multiple image

ClassificationEdit

Pluto charon 150709 color final

Pluto and Charon, to scale. Photo taken by New Horizons on approach

The center of mass (barycenter) of the Pluto–Charon system lies outside either body. Because neither object truly orbits the other, and Charon has 12.2% the mass of Pluto, it has been argued that Charon should be considered to be part of a binary system with Pluto. The International Astronomical Union (IAU) states that Charon is considered to be just a satellite of Pluto, but the idea that Charon might be classified a dwarf planet in its own right may be considered at a later date.[30]

In a draft proposal for the 2006 redefinition of the term, the IAU proposed that a planet be defined as a body that orbits the Sun that is large enough for gravitational forces to render the object (nearly) spherical. Under this proposal, Charon would have been classified as a planet, because the draft explicitly defined a planetary satellite as one in which the barycenter lies within the major body. In the final definition, Pluto was reclassified as a dwarf planet, but the formal definition of a planetary satellite was not decided upon. Charon is not in the list of dwarf planets currently recognized by the IAU.[31] Had the draft proposal been accepted, even the Moon would be classified as a planet in billions of years when the tidal acceleration that is gradually moving the Moon away from Earth takes it far enough away that the center of mass of the system no longer lies within Earth.[32]

The other moons of Pluto, Nix, Hydra, Kerberos and Styx, orbit the same barycenter, but they are not large enough to be spherical, and they are simply considered to be satellites of Pluto (or of Pluto–Charon).[33]

In popular cultureEdit

Charon is the final mission (level 27, excluding the secret levels) in the first Descent video game.

The Mass Effect video game franchise is built around the premise of a series of relays that allow faster-than-light travel around the Milky Way without time dilation. In the series, Charon is discovered in 2149 not to be a moon or a dwarf planet, but to be a chunk of ice containing an intricate piece of technology built by an ancient civilization that allows this travel to occur, leading to the discovery of other planetary systems and enabling their colonization. Operating the Charon Relay gradually circularized Pluto's orbit.

The Jonathan Coulton song "I'm Your Moon" from the Thing a Week Four album is a love song sung to Pluto by Charon.[34]

GalleryEdit

Template:Gallery

VideosEdit

File:NH-PlutoMoon-Charon-FlyOverAnimation-20151001.webm

See alsoEdit

NotesEdit

  1. Cite error: Invalid <ref> tag; no text was provided for refs named Nomenclature
  2. "Solar System Exploration: Multimedia: Gallery: Charon Discovery Image". Solarsystem.nasa.gov. http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=572. Retrieved 2013-07-10. 
  3. "IAUC 3241: 1978 P 1; 1978 (532) 1; 1977n". http://www.cbat.eps.harvard.edu/iauc/03200/03241.html. Retrieved 2011-07-05. 
  4. 4.0 4.1 Govert Shilling, "A Bump in the Night" in Sky & Telescope (June 2008), pp. 26–27. Prior to this, Christy had considered naming the moon Oz.
  5. 5.0 5.1 "Pluto's Moon Charon". http://www.universetoday.com/41619/charon/. Retrieved 2015-10-08. 
  6. "IAU Circular No. 4157". January 3, 1986. http://www.cbat.eps.harvard.edu/iauc/04100/04157.html. Retrieved 2011-07-05. 
  7. Charon – 5 dictionary results
  8. Charon at Oxford English Dictionary
  9. 9.0 9.1 Pronounced "KAIR en" or "SHAHR en" per "Charon". http://www.nineplanets.org/pluto.html#charon. Retrieved 2008-10-03. 
  10. Astronomer Mike Brown can be heard pronouncing it Template:IPA in ordinary conversation on the KCET interview "Julia Sweeney and Michael E. Brown". Hammer Conversations: KCET podcast. 2007. Archived from the original on 2008-10-06. https://web.archive.org/web/20081006182705/http://www.pluggd.tv/audio/channels/kcet_podcast__hammer_conversations/episodes/2h10l. Retrieved 2008-10-01.  at 42min 48sec. Being a long-time resident of California, he does not distinguish the Template:IPA vowel of the name Sharon and the Template:IPA vowel of the classical pronunciation of Charon.
  11. Pronounced 'with a soft "sh" ' per "Welcome to the solar system, Nix and Hydra!". The Planetary Society Weblog. http://www.planetary.org/blog/article/00000613/. Retrieved 2008-10-03. 
  12. US Naval Observatory spokesman Jeff Chester, when interviewed on the NPR commentary "Letters: Radiology Dangers, AIDS, Charon". Morning Edition. 2006-01-19. http://www.npr.org/templates/story/story.php?storyId=5162958. Retrieved 2008-10-03.  (at 2min 49sec), says Christy pronounced it Template:IPA rather than classical Template:IPA. In normal conversation, the second vowel is reduced to a schwa: Template:IPA in RP (ref: OED).
  13. Pronounced "Sharon" Template:IPA per "NASA New Horizons: The PI's Perspective—Two for the Price of One". http://www.spaceref.com/news/viewsr.html?pid=17180. Retrieved 2008-10-03.  and per "New Horizons Team Names Science Ops Center After Charon's Discoverer". http://www.spaceref.com/news/viewpr.html?pid=9477. Retrieved 2008-10-03. 
  14. Hal Weaver, who led the team that discovered Nix and Hydra, also pronounces it Template:IPA (Template:IPA with a General American accent) on the Discovery Science Channel documentary Passport to Pluto, premiered 2006-01-15.
  15. Template:Cite journal
  16. http://www.sciencemag.org/content/350/6258/aad1815.full
  17. Cite error: Invalid <ref> tag; no text was provided for refs named Sci_2015.28a.29
  18. Template:Cite journal
  19. "Charon Moon | PlanetsEdu.com". http://www.planetsedu.com/moon/charon/. Retrieved 2015-10-08. 
  20. 20.0 20.1 "Charon: An ice machine in the ultimate deep freeze". Gemini Observatory. 2007. http://www.spaceflightnow.com/news/n0707/17charon/. Retrieved 2007-07-18. 
  21. Template:Cite journal
  22. "The New Horizons team refers to a dark patch on Pluto's moon as 'Mordor'". The Week. https://theweek.com/speedreads/566694/new-horizons-team-refers-dark-patch-plutos-moon-mordor. Retrieved 15 July 2015. 
  23. 23.0 23.1 "New Horizons Photos Show Pluto's Ice Mountains and Charon's Huge Crater". NBC News. http://www.nbcnews.com/science/space/pluto-photo-n392691. Retrieved 15 July 2015. 
  24. Corum, Jonathan (15 July 2015). "New Horizons Reveals Ice Mountains on Pluto". New York Times. http://www.nytimes.com/interactive/2015/07/15/science/space/new-horizons-pluto-flyby-photos.html. Retrieved 15 July 2015. 
  25. Howett, Carley (11 September 2015). "New Horizons probes the mystery of Charon's red pole". http://phys.org/news/2015-09-horizons-probes-mystery-charon-red.html. Retrieved 16 September 2015. 
  26. Template:Cite news
  27. "Pluto's Big Moon Charon Has a Bizarre Mountain in a Moat (Photo)". http://www.space.com/29970-pluto-moon-charon-mountain-photo.html. Retrieved 2015-10-08. 
  28. "Mysterious Mountain Revealed in First Close-up of Pluto’s Moon Charon". http://www.universetoday.com/121425/mysterious-mountain-revealed-in-first-close-up-of-plutos-moon-charon/. Retrieved 2015-10-08. 
  29. "Pluto and Charon". http://www.spacetelescope.org/images/opo9417a/. Retrieved 2015-10-08. 
  30. "Pluto and the Solar System". IAU. http://www.iau.org/public/themes/pluto/. Retrieved 2013-07-10. 
  31. Template:Cite news
  32. Robert Roy Britt (2006-08-18). "Earth's moon could become a planet". CNN Science & Space. http://edition.cnn.com/2006/TECH/space/08/18/moon.planet. Retrieved 2009-11-25. 
  33. Stern, Alan (2005-05-15). "Background Information Regarding Our Two Newly Discovered Satellites of Pluto". Planetary Science Directorate (Boulder Office). http://www.boulder.swri.edu/plutomoons/. Retrieved 2006-08-30. 
  34. "Thing a Week 47 – I’m Your Moon". August 25, 2006. http://www.jonathancoulton.com/2006/08/25/thing-a-week-47-im-your-moon/. Retrieved 2014-06-18. 

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ReferencesEdit

External linksEdit

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