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Centaurus

Coordinates:Sky map13h 00m 00s, −50° 00′ 00″
From Wikipedia, the free encyclopedia
Constellation in the southern celestial hemisphere
For other uses, seeCentaurus (disambiguation).
Centaurus
Constellation
Centaurus
AbbreviationCen
GenitiveCentauri
Pronunciation/sɛnˈtɔːrəs,-ˈtɑːr-/, genitive/sɛnˈtɔːr,-ˈtɔːri,-ˈtɑːri/
SymbolismtheCentaur
Right ascension11h 05m 20.9415s15h 03m 11.1071s[1]
Declination−29.9948788°–−64.6957885°[1]
Area1060 sq. deg. (9th)
Main stars11
Bayer/Flamsteed
stars
69
Stars withplanets15
Stars brighter than 3.00m10
Stars within 10.00 pc (32.62 ly)8
Brightest starα Cen (−0.27m)
Nearest starProxima Centauri (α Cen C)
Messier objects0
Meteor showersAlpha Centaurids
Omicron Centaurids
Theta Centaurids
Bordering
constellations
Antlia
Carina
Circinus
Crux
Hydra
Libra (corner)
Lupus
Musca
Vela
Visible at latitudes between +25° and −90°.
Best visible at 21:00 (9 p.m.) during the month ofMay.

Centaurus (/sɛnˈtɔːrəs,-ˈtɑːr-/) is a bright constellation in thesouthern sky. One of thelargest constellations, Centaurus was included among the 48constellations listed by the 2nd-century astronomerPtolemy, and it remains one of the88 modern constellations. InGreek mythology, Centaurus represents acentaur; a creature that is half human, half horse (another constellation named after a centaur is one from thezodiac:Sagittarius). Notable stars includeAlpha Centauri, the nearest star system to theSolar System, its neighbour in the skyBeta Centauri, andHR 5171, one of the largest stars yet discovered. The constellation also containsOmega Centauri, the brightestglobular cluster as visible from Earth and the largest identified in the Milky Way, possibly a remnant of a dwarf galaxy.

Notable features

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Centaurus is a large constellation with many bright stars, two stars brighter than magnitude 1, and a number of the best-known deep-sky objects, although theMilky Way does not lie within its borders.

Stars

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See also:List of stars in Centaurus
The two bright stars are (left)Alpha Centauri and (right)Beta Centauri. The faint red star in the center of the red circle isProxima Centauri.
Centaurus in the southwestern sky, shortly after sunset. South is to the left.
Centaurus in theFirmamentum Sobiescianum ofJohannes Hevelius.N.B. This image is reversed from what one sees looking at the sky — it is as though one is looking at the "celestial sphere" from the outside.

Centaurus contains several very bright stars. Its alpha and beta stars are used as "pointer stars" to help observers find the constellationCrux. Centaurus has 281 stars above magnitude 6.5, meaning that they are visible to the unaided eye, the most of any constellation.Alpha Centauri, the closest star system to the Sun, has a highproper motion; it will be a mere half-degree from Beta Centauri in approximately 4000 years.[2]

Alpha Centauri is atriple star system composed of a binary system orbited by Proxima Centauri, currently the nearest star to the Sun. Traditionally called Rigil Kentaurus (from Arabic رجل قنطورس, meaning "foot of the centaur") or Toliman (from Arabic الظليمين meaning "two male ostriches"), the system has an overall magnitude of −0.28 and is 4.4light-years from Earth. The primary and secondary are both yellow-hued stars; the first is of magnitude −0.01 and the second: 1.35. Proxima, the tertiary star, is ared dwarf of magnitude 11.0; it appears almost 2 degrees away from the close pairing of Alpha and has a period of approximately one million years. Also aflare star, Proxima has minutes-long outbursts where it brightens by over a magnitude. The Alpha couple revolve in 80-year periodicity and will next appear closest as seen from Earth's telescopes in 2037 and 2038, together as they appear to the naked eye they present thethird-brightest "star" in the night sky.[2]

One otherfirst magnitude star Beta Centauri is in the constellation in a position beyond Proxima and toward the narrow axis of Crux, thus with Alpha forming a far-south limb of the constellation. Also called Hadar and Agena, it is a double star; the primary is a blue-hued giant star of magnitude 0.6, 525 light-years from Earth. The secondary is of magnitude 4.0 and has a modest separation, appearing only under intense magnification due to its distance.

The northerly starTheta Centauri, officially named Menkent, is an orange giant star of magnitude 2.06. It is the only bright star of Centaurus that is easily visible from mid-northern latitudes.

The next bright object isGamma Centauri, abinary star which appears to the naked eye at magnitude 2.2. The primary and secondary are both blue-white hued stars of magnitude 2.9; their period is 84 years.[2]

Centaurus also has many dimmer double stars and binary stars.3 Centauri is a double star with a blue-white hued primary of magnitude 4.5 and a secondary of magnitude 6.0. The primary is 344 light-years away.[2]

Centaurus is home to manyvariable stars.R Centauri is aMira variable star with a minimum magnitude of 11.8 and a maximum magnitude of 5.3; it is about 1,250 light-years from Earth and has a period of 18 months.[2]V810 Centauri is asemiregular variable.

BPM 37093 is awhite dwarf star whosecarbon atoms are thought to have formed a crystalline structure. Sincediamond also consists of carbon arranged in a crystalline lattice (though of a different configuration), scientists have nicknamed this star "Lucy" after the Beatles song "Lucy in the Sky with Diamonds."[3]

PDS 70, (V1032 Centauri) a low mass T Tauri star is found in the constellation Centaurus. In July 2018 astronomers captured the first conclusive image of aprotoplanetary disk containing a nascentexoplanet, namedPDS 70b.[4][5][6]

Deep-sky objects

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ω Centauri (NGC 5139), despite being listed as the constellation's "omega" star, is in fact a naked-eyeglobular cluster, 17,000 light-years away with a diameter of 150 light-years. It is the largest and brightest globular cluster in theMilky Way; at ten times the size of the next-largest cluster,[7] it has a magnitude of 3.7. It is also the mostluminous globular cluster in the Milky Way, at over one millionsolar luminosities.[2] Omega Centauri is classified as a Shapley class VIII cluster, which means that its center is loosely concentrated. It is also one of only two globular clusters to be given astellar designation; in its case aBayer letter. The other is47 Tucanae (Xi Tucanae), which has aFlamsteed number.[8] Omega Centauri contains several million stars, most of which areyellow dwarf stars, but also possessesred giants andblue-white stars; the stars have an average age of 12 billion years. This has prompted suspicion that Omega Centauri was thecore of adwarf galaxy that had beenabsorbed by the Milky Way. Omega Centauri was determined to be nonstellar in 1677 by the English astronomerEdmond Halley,[7] though it was visible as a star to the ancients. Its status as a globular cluster was determined byJames Dunlop in 1827.[9] To the unaided eye, Omega Centauri appears fuzzy and is obviously non-circular; it is approximately half a degree in diameter, the same size as the full Moon.[2]

Centaurus is also home to open clusters.NGC 3766 is an open cluster 6,300 light-years from Earth that is visible to the unaided eye. It contains approximately 100 stars, the brightest of which are 7th magnitude.NGC 5460 is another naked-eye open cluster, 2,300 light-years from Earth, that has an overall magnitude of 6 and contains approximately 40 stars.[2]

There is one brightplanetary nebula in Centaurus,NGC 3918, also known as the Blue Planetary. It has an overall magnitude of 8.0 and a central star of magnitude 11.0; it is 2600 light-years from Earth. The Blue Planetary was discovered byJohn Herschel and named for its color's similarity toUranus, though the nebula is apparently three times larger than the planet.[2]

Centaurus is rich in galaxies as well.NGC 4622 is a face-onspiral galaxy located 200 million light-years from Earth (redshift 0.0146). Itsspiral arms wind in both directions, which makes it nearly impossible for astronomers to determine the rotation of the galaxy. Astronomers theorize that acollision with a smaller companion galaxy near the core of the main galaxy could have led to the unusual spiral structure.[7]NGC 5253, a peculiarirregular galaxy, is located near the border with Hydra andM83, with which it likely had a close gravitational interaction 1–2 billion years ago. This may have sparked the galaxy's high rate of star formation, which continues today and contributes to its high surface brightness. NGC 5253 includes a large nebula and at least 12 large star clusters. In the eyepiece, it is a small galaxy of magnitude 10 with dimensions of 5 arcminutes by 2 arcminutes and a bright nucleus.[10] NGC 4945 is a spiral galaxy seen edge-on from Earth, 13 million light-years away. It is visible with any amateur telescope, as well asbinoculars under good conditions; it has been described as "shaped like a candle flame", being long and thin (16' by 3'). In the eyepiece of a large telescope, its southeastern dust lane becomes visible. Another galaxy isNGC 5102, found by star-hopping fromIota Centauri. In the eyepiece, it appears as an elliptical object 9 arcminutes by 2.5 arcminutes tilted on a southwest–northeast axis.[11]

One of the closestactive galaxies to Earth is theCentaurus A galaxy, NGC 5128, at 11 million light-years away (redshift 0.00183). It has asupermassive black hole at its core, which expels massive jets of matter that emitradio waves due tosynchrotron radiation. Astronomers posit that its dust lanes, not common inelliptical galaxies, are due to a previousmerger with another galaxy,[2] probably aspiral galaxy. NGC 5128 appears in theoptical spectrum as a fairly large elliptical galaxy with a prominentdust lane. Its overall magnitude is 7.0 and it has been seen under perfect conditions with the naked eye, making it one of the most distant objects visible to the unaided observer. In equatorial and southern latitudes, it is easily found bystar hopping from Omega Centauri. In small telescopes, the dust lane is not visible; it begins to appear with about 4 inches of aperture under good conditions. In large amateur instruments, above about 12 inches in aperture, the dust lane's west-northwest to east-southeast direction is easily discerned. Another dim dust lane on the east side of the 12-arcminute-by-15-arcminute galaxy is also visible.[10]ESO 270-17, also called the Fourcade-Figueroa Object, is a low-surface brightness object believed to be the remnants of a galaxy; it does not have a core and is very difficult to observe with an amateur telescope. It measures 7 arcminutes by 1 arcminute.[11] It likely originated as a spiral galaxy and underwent a catastrophic gravitational interaction with Centaurus A around 500 million years ago, stopping its rotation and destroying its structure.[12]

NGC 4650A is apolar-ring galaxy 136 million light-years from Earth (redshift 0.01). It has a central core made of older stars that resembles anelliptical galaxy, and an outer ring of young stars that orbits around the core. The plane of the outer ring is distorted, which suggests that NGC 4650A is the result of agalaxy collision about a billion years ago. This galaxy has also been cited in studies ofdark matter, because the stars in the outer ring orbit too quickly for their collective mass. This suggests that the galaxy is surrounded by adark matter halo, which provides the necessary mass.[7]

One of the closestgalaxy clusters to Earth is theCentaurus Cluster atc. 160 million light-years away, havingredshift 0.0114. It has a cooler, denser central region of gas and a hotter, more diffuse outer region. Theintracluster medium in the Centaurus Cluster has a high concentration of metals (elements heavier than helium) due to a large number ofsupernovae. This cluster also possesses a plume of gas whose origin is unknown.[7]

History

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Centaurus, 1602

While Centaurus now has a high southern latitude, at the dawn of civilization it was an equatorial constellation.Precession has been slowly shifting it southward for millennia, and it is now close to its maximal southerndeclination. In a little over 7000 years it will be at maximum visibility for those in the northern hemisphere, visible at times in the year up to quite a high northern latitude.The figure of Centaurus can be traced back to a Babylonian constellation known as the Bison-man (MUL.GUD.ALIM). This being was depicted in two major forms: firstly, as a 4-legged bison with a human head, and secondly, as a being with a man's head and torso attached to the rear legs and tail of a bull or bison. It has been closely associated with the Sun god Utu-Shamash from very early times. By the late 3rd millennium the Bison-man had been replaced by a new constellation, the Wild Boar.[13]

The Greeks depicted the constellation as a centaur and gave it its current name. It was mentioned byEudoxus in the 4th century BC andAratus in the 3rd century BC. In the 2nd century AD,Claudius Ptolemy catalogued 37 stars in Centaurus, including Alpha Centauri. Large as it is now, in earlier times it was even larger, as the constellationLupus was treated as anasterism within Centaurus, portrayed in illustrations as an unspecified animal either in the centaur's grasp or impaled on its spear.[14] TheSouthern Cross, which is now regarded as a separate constellation, was treated by the ancients as a mere asterism formed of the stars composing the centaur's legs. Additionally, what is now the minor constellationCircinus was treated as undefined stars under the centaur's front hooves.

According to the Roman poetOvid (Fasti v.379), the constellation honors the centaurChiron, who was tutor to many of the earlier Greek heroes includingHeracles (Hercules),Theseus, andJason, the leader of the Argonauts. It is not to be confused with the more warlike centaur represented by the zodiacal constellationSagittarius. The legend associated with Chiron says that he was accidentally poisoned with an arrow shot by Hercules, and was subsequently placed in the heavens.[2]

Equivalents

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InChinese astronomy, the stars of Centaurus are found in three areas: theAzure Dragon of the East (東方青龍,Dōng Fāng Qīng Lóng), theVermillion Bird of the South (南方朱雀,Nán Fāng Zhū Què), and theSouthern Asterisms (近南極星區,Jìnnánjíxīngōu). Not all of the stars of Centaurus can be seen from China, and the unseen stars were classified among the Southern Asterisms byXu Guangqi, based on his study of western star charts. However, most of the brightest stars of Centaurus, including α Centauri,θ Centauri (or Menkent[15]),ε Centauri andη Centauri, can be seen in the Chinese sky.

SomePolynesian peoples considered the stars of Centaurus to be a constellation as well. OnPukapuka, Centaurus had two names:Na Mata-o-te-tokolua andNa Lua-mata-o-Wua-ma-Velo. InTonga, the constellation was called by four names:O-nga-tangata,Tautanga-ufi,Mamangi-Halahu, andMau-kuo-mau. Alpha and Beta Centauri were not named specifically by the people of Pukapuka or Tonga, but they were named by the people ofHawaii and theTuamotus. In Hawaii, the name for Alpha Centauri was eitherMelemele orKa Maile-hope and the name for Beta Centauri was eitherPolapola orKa Maile-mua. In the Tuamotu islands, Alpha was calledNa Kuhi and Beta was calledTere.[16]

The Pointer (α Centauri and β Centauri) is one of the asterisms used byBugis sailors for navigation, calledbintoéng balué, meaning "the widowed-before-marriage". It is also calledbintoéng sallatang meaning "southern star".[17]

Namesakes

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TwoUnited States Navy ships,USS Centaurus (AKA-17) andUSS Centaurus (AK-264), were named after Centaurus, the constellation.

See also

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References

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Citations
  1. ^ab"Centaurus, constellation boundary".The Constellations. Retrieved15 February 2014.
  2. ^abcdefghijkRidpath & Tirion 2017, pp. 110–113.
  3. ^"Discovery of largest known diamond".AZoM. February 15, 2004. Retrieved2008-12-04.
  4. ^Staff (2 July 2018)."First confirmed image of newborn planet caught with ESO's VLT – Spectrum reveals cloudy atmosphere".EurekAlert!. Retrieved2 July 2018.
  5. ^Müller, a.; et al."Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk"(PDF).ESO.Archived(PDF) from the original on 2018-07-02. Retrieved2 July 2018.
  6. ^Keppler, M.; et al."Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70"(PDF).ESO.Archived(PDF) from the original on 2018-07-02. Retrieved2 July 2018.
  7. ^abcdeWilkins, Jamie; Dunn, Robert (2006).300 Astronomical Objects: A Visual Reference to the Universe (1st ed.). Buffalo, New York: Firefly Books.ISBN 978-1-55407-175-3.
  8. ^Levy 2005, p. 161.
  9. ^Levy 2005, p. 163.
  10. ^abDalrymple 2013, p. 40.
  11. ^abDalrymple 2013, p. 41.
  12. ^Steinicke 2007, p. 182.
  13. ^Babylonian Star-lore by Gavin White, Solaria Pubs, 2008, page 57ff
  14. ^Allen, Richard Hinckley (1963).Star Names: Their Lore and Meaning. Dover. p. 279.ISBN 978-0-486-21079-7.{{cite book}}: CS1 maint: ignored ISBN errors (link)
  15. ^"Naming Stars". IAU.org. Retrieved30 July 2018.
  16. ^Makemson 1941, p. 281.
  17. ^Kelley, David H.; Milone, Eugene F.; Aveni, A.F. (2011).Exploring Ancient Skies: A Survey of Ancient and Cultural Astronomy. New York, New York: Springer. p. 344.ISBN 978-1-4419-7623-9.
References

External links

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