Alpha Centauri

Star system in the Centaurus constellation

This article is about α Centauri, the multi-star system in the constellation Centaurus and is not to be confused with a Centauri, A Centauri, or Centaurus A. For other uses, see Alpha Centauri (disambiguation).

Alpha Centauri AB[a]

Alpha Centauri AB (left) forms a triple star system with Proxima Centauri (below, south of, α Centauri AB), circled in red. The bright star to the right is Beta Centauri.

Observation data
Epoch J2000.0      Equinox J2000.0
Constellation | Centaurus
α Centauri A (Rigil Kentaurus)
Right ascension | 14h 39m 36.49400s[1]
Declination | −60° 50′ 02.3737″[1]
Apparent magnitude (V) | +0.01[2]
α Centauri B (Toliman)
Right ascension | 14h 39m 35.06311s[1]
Declination | −60° 50′ 15.0992″[1]
Apparent magnitude (V) | +1.33[2]
Characteristics

Spectral type | G2V[3]
B−V colour index | +0.71[2]

Spectral type | K1V[3]
B−V colour index | +0.88[2]
Astrometry

Radial velocity (Rv)| −21.4±0.76[4] km/s
Proper motion (μ)|  RA: −3679.25[1] mas/yr
Dec.: +473.67[1] mas/yr
Parallax (π)| 750.81±0.38 mas[5]
Distance| 4.344 ± 0.002 ly
(1.3319 ± 0.0007 pc)
Absolute magnitude (MV)| 4.38[6]

Radial velocity (Rv)| −18.6±1.64[4] km/s
Proper motion (μ)|  RA: −3614.39[1] mas/yr
Dec.: +802.98[1] mas/yr
Parallax (π)| 750.81±0.38 mas[5]
Distance| 4.344 ± 0.002 ly
(1.3319 ± 0.0007 pc)
Absolute magnitude (MV)| 5.71[6]
Orbit[5]
Primary| A
Companion| B
Period (P)| 79.762±0.019 yr
Semi-major axis (a)| 17.493±0.0096″
Eccentricity (e)| 0.51947±0.00015
Inclination (i)| 79.243±0.0089°
Longitude of the node (Ω)| 205.073±0.025°
Periastron epoch (T)| 1875.66±0.012
Argument of periastron (ω)
(secondary)| 231.519±0.027°
Details
α Centauri A
Mass| 1.0788±0.0029[5] M☉
Radius| 1.2175±0.0055[5] R☉
Luminosity| 1.5059±0.0019[5] L☉
Surface gravity (log g)| 4.30[7] cgs
Temperature| 5,804±13[8] K
Metallicity [Fe/H]| 0.20±0.01[8] dex
Rotation| 28.3±0.5 d[9]
Rotational velocity (v sin i)| 2.7±0.7[10] km/s
Age| 5.26±0.95[11] Gyr
α Centauri B
Mass| 0.9092±0.0025[5] M☉
Radius| 0.8591±0.0036[5] R☉
Luminosity| 0.4981±0.0007[5] L☉
Surface gravity (log g)| 4.37[7] cgs
Temperature| 5,207±12[8] K
Metallicity [Fe/H]| 0.24±0.01[8] dex
Rotation| 36.7±0.3 d[12]
Rotational velocity (v sin i)| 1.1±0.8[13] km/s
Age| 5.26±0.95[11] Gyr
Other designations
Gliese 559, FK5 538, CD−60°5483, CCDM J14396-6050, GC 19728
α Cen A: Rigil Kentaurus, Rigil Kent, α1 Centauri, HR 5459, HD 128620, GCTP 3309.00, LHS 50, SAO 252838, HIP 71683
α Cen B: Toliman, α2 Centauri, HR 5460, HD 128621, LHS 51, HIP 71681
Database references
SIMBAD| AB
| A
| B
Exoplanet Archive| data
ARICNS| data

Alpha Centauri (α Centauri, α Cen, or Alpha Cen) is a star system in the southern constellation of Centaurus. It consists of three stars: Rigil Kentaurus (α Centauri A), Toliman (α Centauri B), and Proxima Centauri (α Centauri C).[14] Proxima Centauri is the closest star to the Sun at 4.2465 light-years (ly), which is 1.3020 parsecs (pc).

Rigil Kentaurus and Toliman are Sun-like stars (class G and K, respectively) that together form the binary star system α Centauri AB. To the naked eye, these two main components appear to be a single star with an apparent magnitude of −0.27. It is the brightest star in the constellation and the third-brightest in the night sky, outshone by only Sirius and Canopus.

Rigil Kentaurus has 1.1 times the mass (M☉) and 1.5 times the luminosity of the Sun (L☉), while Toliman is smaller and cooler, at 0.9 M☉ and less than 0.5 L☉.[15] The pair orbit around a common centre with an orbital period of 79 years.[16] Their elliptical orbit is eccentric, so that the distance between A and B varies from 35.6 astronomical units (AU), or about the distance between Pluto and the Sun, to 11.2 AU, or about the distance between Saturn and the Sun. One astronomical unit is the distance from Earth to the Sun, 150 million kilometers.

Proxima Centauri is a small faint red dwarf (class M). Though not visible to the naked eye, Proxima Centauri is the closest star to the Sun at a distance of 4.24 ly (1.30 pc), slightly closer than α Centauri AB. The distance between Proxima Centauri and α Centauri AB is about 13,000 AU (0.21 ly),[17] equivalent to about 430 times the radius of Neptune's orbit.

Proxima Centauri has one confirmed planet — Proxima b, an Earth-sized planet in the habitable zone (though it is unlikely to be habitable); one candidate planet — Proxima d, a sub-Earth which orbits very closely to the star,[18] and the controversial Proxima c, a mini-Neptune 1.5 astronomical units away.[19] Rigil Kentaurus may have a Neptune-sized planet in the habitable zone, though it is not yet known with certainty to be planetary in nature and could be an artefact of the discovery mechanism.[20] Toliman has no known planets.[21]

## Etymology and nomenclature

[edit]

α Centauri (Latinised to Alpha Centauri) is the system's designation given by J. Bayer in 1603. It belongs to the constellation Centaurus, named after the part human, part horse creature in Greek mythology; Heracles accidentally wounded the centaur and placed him in the sky after his death. Alpha Centauri marks the right front hoof of the Centaur.[22] The common name Rigil Kentaurus is a Latinisation of the Arabic translation رجل القنطورس Rijl al-Qinṭūrus, meaning "the Foot of the Centaur".[23][24] Qinṭūrus is the Arabic transliteration of the Greek Κένταυρος (Kentaurus).[25] The name is frequently abbreviated to Rigil Kent (/ˈraɪdʒəl ˈkɛnt/) or even Rigil, though the latter name is better known for Rigel (β Orionis).[26][27][28][23][29][b]

An alternative name found in European sources, Toliman, is an approximation of the Arabic الظليمان aẓ-Ẓalīmān (in older transcription, aṭ-Ṭhalīmān), meaning 'the (two male) Ostriches', an appellation Zakariya al-Qazwini had applied to the pair of stars Lambda and Mu Sagittarii; it was often unclear on old star maps which name was intended to go with which star (or stars), and the referents changed over time.[33] The name Toliman originates with Jacob Golius' 1669 edition of Al-Farghani's Compendium. Tolimân is Golius' Latinisation of the Arabic name الظلمان al-Ẓulmān "the ostriches", the name of an asterism of which Alpha Centauri formed the main star.[34][35][36][37]

α Centauri C was discovered in 1915 by Robert T. A. Innes,[38] who suggested that it be named Proxima Centaurus,[39] from Latin 'the nearest [star] of Centaurus'.[40] The name Proxima Centauri later became more widely used and is now listed by the International Astronomical Union (IAU) as the approved proper name;[41][42] it is frequently abbreviated to Proxima.

In 2016, the Working Group on Star Names of the IAU,[14] having decided to attribute proper names to individual component stars rather than to multiple systems,[43] approved the name Rigil Kentaurus (/ˈraɪdʒəl kɛnˈtɔːrəs/) as being restricted to α Centauri A and the name Proxima Centauri (/ˈprɒksɪmə sɛnˈtɔːraɪ/) for α Centauri C.[44] On 10 August 2018, the IAU approved the name Toliman (/ˈtɒlɪmæn/) for α Centauri B.[45]

### Other names

[edit]

During the 19th century, the northern amateur popularist E.H. Burritt used the now-obscure name Bungula (/ˈbʌŋɡjuːlə/).[46] Its origin is not known, but it may have been coined from the Greek letter beta (β) and Latin ungula 'hoof', originally for Beta Centauri (the other hoof).[26][23]

In Chinese astronomy, 南門 Nán Mén, meaning Southern Gate, refers to an asterism consisting of Alpha Centauri and Epsilon Centauri. Consequently, the Chinese name for Alpha Centauri itself is 南門二 Nán Mén Èr, the Second Star of the Southern Gate.[47]

To the Indigenous Boorong people of northwestern Victoria in Australia, Alpha Centauri and Beta Centauri are Bermbermgle,[48] two brothers noted for their courage and destructiveness, who speared and killed Tchingal "The Emu" (the Coalsack Nebula).[49] The form in Wotjobaluk is Bram-bram-bult.[48]

## Observation

[edit]

class=notpageimage|

Location of α Cen in Centaurus

To the naked eye, α Centauri AB appear to be a single star, the brightest in the southern constellation of Centaurus.[50] Their apparent angular separation varies over about 80 years between 2 and 22 arcseconds (the naked eye has a resolution of 60 arcsec),[51] but through much of the orbit, both are easily resolved in binoculars or small telescopes.[52] At −0.27 apparent magnitude (combined for A and B magnitudes (see Apparent magnitude § Magnitude addition)), Alpha Centauri is a first-magnitude star and is fainter only than Sirius and Canopus.[50] It is the outer star of The Pointers or The Southern Pointers,[52] so called because the line through Beta Centauri (Hadar/Agena),[53] some 4.5° west,[52] points to the constellation Crux—the Southern Cross.[52][54] The Pointers easily distinguish the true Southern Cross from the fainter asterism known as the False Cross.[55]

South of about 29° South latitude, α Cen is circumpolar and never sets below the horizon.[c] North of about 29° N latitude, Alpha Centauri never rises. Alpha Centauri lies close to the southern horizon when viewed from latitude 29° N to the equator (close to Hermosillo and Chihuahua City in Mexico; Galveston, Texas; Ocala, Florida; and Lanzarote, the Canary Islands of Spain), but only for a short time around its culmination.[53] The star culminates each year at local midnight on 24 April and at local 9 p.m. on 8 June.[53][56]

As seen from Earth, Proxima Centauri is 2.2° southwest from α Centauri AB; this distance is about four times the angular diameter of the Moon.[57] Proxima Centauri appears as a deep-red star of a typical apparent magnitude of 11.1 in a sparsely populated star field, requiring moderately sized telescopes to be seen. Listed as V645 Cen in the General Catalogue of Variable Stars, version 4.2, this UV Ceti star or "flare star" can unexpectedly brighten rapidly by as much as 0.6 magnitude at visual wavelengths, then fade after only a few minutes.[58] Some amateur and professional astronomers regularly monitor for outbursts using either optical or radio telescopes.[59] In August 2015, the largest recorded flares of the star occurred, with the star becoming 8.3 times brighter than normal on 13 August, in the B band (blue light region).[60]

### Observational history

[edit]

The Very Large Telescope open to the night sky, with the Milky Way running diagonally across the sky above it and many southern stars and constellations labelled and connected by lines, including Alpha Centauri and the not visible Proxima Centauri.

Alpha Centauri is listed in the 2nd century star catalog appended to Ptolemy's Almagest. Ptolemy gave its ecliptic coordinates, but texts differ as to whether the ecliptic latitude reads 44° 10′ South or 41° 10′ South.[61] (Presently the ecliptic latitude is 43.5° South, but it has decreased by a fraction of a degree since Ptolemy's time due to proper motion.) In Ptolemy's time, Alpha Centauri was visible from Alexandria, Egypt, at 31° N, but, due to precession, its declination is now –60° 51′ South, and it can no longer be seen at that latitude. English explorer Robert Hues brought Alpha Centauri to the attention of European observers in his 1592 work Tractatus de Globis, along with Canopus and Achernar, noting:

> Now, therefore, there are but three Stars of the first magnitude that I could perceive in all those parts which are never seene here in England. The first of these is that bright Star in the sterne of Argo which they call Canobus [Canopus]. The second [Achernar] is in the end of Eridanus. The third [Alpha Centauri] is in the right foote of the Centaure.[62]

The binary nature of Alpha Centauri AB was recognized in December 1689 by Jean Richaud, while observing a passing comet from his station in Puducherry. Alpha Centauri was only the third binary star to be discovered, preceded by Mizar AB and Acrux.[63]

The large proper motion of Alpha Centauri AB was discovered by Manuel John Johnson, observing from Saint Helena, who informed Thomas Henderson at the Royal Observatory, Cape of Good Hope of it. The parallax of Alpha Centauri was subsequently determined by Henderson from many exacting positional observations of the AB system between April 1832 and May 1833\. He withheld his results, however, because he suspected they were too large to be true, but eventually published them in 1839 after Bessel released his own accurately determined parallax for 61 Cygni in 1838.[64] For this reason, Alpha Centauri is sometimes considered as the second star to have its distance measured because Henderson's work was not fully acknowledged at first.[64] (The distance of Alpha Centauri from the Earth is now reckoned at 4.396 light-years or 4.159×1013 km.)

Alpha Centauri (Rigel Kentaurus) around the South celestial pole

John Herschel made the first micrometrical observations in 1834.[65] Since the early 20th century, measures have been made with photographic plates.[66]

By 1926, William Stephen Finsen calculated the approximate orbit elements close to those now accepted for this system.[67] All future positions are now sufficiently accurate for visual observers to determine the relative places of the stars from a binary star ephemeris.[68] Others, like D. Pourbaix (2002), have regularly refined the precision of new published orbital elements.[16]

Robert T. A. Innes discovered Proxima Centauri in 1915 by blinking photographic plates taken at different times during a proper motion survey. These showed large proper motion and parallax similar in both size and direction to those of α Centauri AB, which suggested that Proxima Centauri is part of the α Centauri system and slightly closer to Earth than α Centauri AB. As a result, Innes concluded that Proxima Centauri was the closest star to Earth yet discovered.

## Location and motion

[edit]

Alpha Centauri may be inside the G-cloud of the Local Bubble,[69] and its nearest known system is the binary brown dwarf system Luhman 16, at 3.6 light-years (1.1 parsecs) distance.[70][failed verification]

### Historical distance estimates

[edit]

Alpha Centauri AB historical distance estimates  Source  | Year  | Subject | Parallax (mas) | Distance | References

|
|
|
|
|

parsecs | light-years | petametres
H. Henderson | 1839 | AB | 1160±110 | 0.86+0.09
−0.07 | 2.81 ± 0.53 | 26.6+2.8
−2.3 | [71]
T. Henderson  | 1842  | AB  | 912.8±64 | 1.10 ± 0.15  | 3.57 ± 0.5  | 33.8+2.5
−2.2 | [72]
Maclear  | 1851  | AB  | 918.7±34 | 1.09±0.04 | 3.55+0.14
−0.13 | 32.4 ± 2.5  | [73]
Moesta  | 1868  | AB  | 880±68 | 1.14+0.10
−0.08 | 3.71+0.31
−0.27 | 35.1+2.9
−2.5 | [74]
Gill & Elkin  | 1885  | AB  | 750±10 | 1.333±0.018 | 4.35±0.06 | 41.1+0.6
−0.5 | [75]
Roberts  | 1895  | AB  | 710±50 | 1.32 ± 0.2  | 4.29 ± 0.65  | 43.5+3.3
−2.9 | [76]
Woolley et al. | 1970  | AB  | 743±7 | 1.346±0.013 | 4.39±0.04 | 41.5±0.4 | [77]
Gliese & Jahreiß  | 1991  | AB  | 749.0±4.7 | 1.335±0.008 | 4.355±0.027 | 41.20±0.26 | [78]
van Altena et al. | 1995  | AB  | 749.9±5.4 | 1.334±0.010 | 4.349+0.032
−0.031 | 41.15+0.30
−0.29 | [79]
Perryman et al. | 1997  | AB  | 742.12±1.40 | 1.3475±0.0025 | 4.395±0.008 | 41.58±0.08[80][81]
Söderhjelm  | 1999  | AB  | 747.1±1.2 | 1.3385+0.0022
−0.0021 | 4.366±0.007 | 41.30±0.07 | [82]
van Leeuwen  | 2007  | A  | 754.81±4.11 | 1.325±0.007 | 4.321+0.024
−0.023 | 40.88±0.22 | [83]
B  | 796.92±25.90 | 1.25±0.04 | 4.09+0.14
−0.13 | 37.5 ± 2.5  | [84]
RECONS TOP100  | 2012  | AB  | 747.23±1.17[d] | 1.3383±0.0021 | 4.365±0.007 | 41.29±0.06 | [85]

### Kinematics

[edit]

Alpha Centauri (with unlabeled Proxima Centauri) on a radar map of all known stellar and substellar objects within 9 light years (ly), arranged clockwise in hours of right ascension, and marked by distance (▬) and position (◆). Distances are marked outward from the Sun (Sol), with concentric circles indicating the distance in one ly steps. Positions are marked inward from their distance markings, connected by lines according to their declinations (doted when positive), representing the arcs of the declinations viewed edge-on.

All components of α Centauri display significant proper motion against the background sky. Over centuries, this causes their apparent positions to slowly change.[86] Proper motion was unknown to ancient astronomers. Most assumed that the stars were permanently fixed on the celestial sphere, as stated in the works of the philosopher Aristotle.[87] In 1718, Edmond Halley found that some stars had significantly moved from their ancient astrometric positions.[88]

In the 1830s, Thomas Henderson discovered the true distance to α Centauri by analysing his many astrometric mural circle observations.[71][89] He then realised this system also likely had a high proper motion.[90][91][67] In this case, the apparent stellar motion was found using Nicolas Louis de Lacaille's astrometric observations of 1751–1752,[92] by the observed differences between the two measured positions in different epochs.

Calculated proper motion of the centre of mass for α Centauri AB is about 3620 mas/y (milliarcseconds per year) toward the west and 694 mas/y toward the north, giving an overall motion of 3686 mas/y in a direction 11° north of west.[93][e] The motion of the centre of mass is about 6.1 arcmin each century, or 1.02° each millennium. The speed in the western direction is 23.0 km/s (14.3 mi/s) and in the northerly direction 4.4 km/s (2.7 mi/s). Using spectroscopy the mean radial velocity has been determined to be around 22.4 km/s (13.9 mi/s) towards the Solar System.[93] This gives a speed with respect to the Sun of 32.4 km/s (20.1 mi/s), very close to the peak in the distribution of speeds of nearby stars.[94]

Since α Centauri AB is almost exactly in the plane of the Milky Way as viewed from Earth, many stars appear behind it. In early May 2028, α Centauri A will pass between the Earth and a distant red star, when there is a 45% probability that an Einstein ring will be observed. Other conjunctions will also occur in the coming decades, allowing accurate measurement of proper motions and possibly giving information on planets.[93]

#### Predicted future changes

[edit]

Distances of the nearest stars from 20,000 years ago until 80,000 years in the future[citation needed] Animation showing motion of α Centauri through the sky. (The other stars are held fixed for didactic reasons.) "Oggi" means today; "anni" means years.

Based on the system's common proper motion and radial velocities, α Centauri will continue to change its position in the sky significantly and will gradually brighten. For example, in about 6,200 CE, α Centauri's true motion will cause an extremely rare first-magnitude stellar conjunction with Beta Centauri, forming a brilliant optical double star in the southern sky.[54] It will then pass just north of the Southern Cross or Crux, before moving northwest and up towards the present celestial equator and away from the galactic plane. By about 26,700 CE, in the present-day constellation of Hydra, α Centauri will reach perihelion at 0.90 pc or 2.9 ly away,[95] though later calculations suggest that this will occur in 27,000 AD.[96] At its nearest approach, α Centauri will attain a maximum apparent magnitude of −0.86, comparable to present-day magnitude of Canopus, but it will still not surpass that of Sirius, which will brighten incrementally over the next 60,000 years, and will continue to be the brightest star as seen from Earth (other than the Sun) for the next 210,000 years.[97]

## Stellar system

[edit]

Alpha Centauri is a triple star system, with its two main stars, A and B, together comprising a binary component. The AB designation, or older A×B, denotes the mass centre of a main binary system relative to companion star(s) in a multiple star system.[98] AB-C refers to the component of Proxima Centauri in relation to the central binary, being the distance between the centre of mass and the outlying companion. Because the distance between Proxima (C) and either of Alpha Centauri A or B is similar, the AB binary system is sometimes treated as a single gravitational object.[99]

### Orbital properties

[edit]

Apparent and true orbits of Alpha Centauri. The A component is held stationary, and the relative orbital motion of the B component is shown. The apparent orbit (thin ellipse) is the shape of the orbit as seen by an observer on Earth. The true orbit is the shape of the orbit viewed perpendicular to the plane of the orbital motion. According to the radial velocity versus time,[100] the radial separation of A and B along the line of sight had reached a maximum in 2007, with B being further from Earth than A. The orbit is divided here into 80 points: each step refers to a timestep of approx. 0.99888 years or 364.84 days. Orbital plot of Proxima Centauri around the bright apparent star Alpha Centauri AB, with position change marked (in thousands of years).

The A and B components of Alpha Centauri have an orbital period of 79.762 years. Their orbit is moderately eccentric, as it has an eccentricity of almost 0.52;[5] their closest approach or periastron is 11.2 AU (1.68×10 ~~^~~ 9 km), or about the distance between the Sun and Saturn; and their furthest separation or apastron is 35.6 AU (5.33×10 ~~^~~ 9 km), about the distance between the Sun and Pluto.[16] The most recent periastron was in August 1955 and the next will occur in May 2035; the most recent apastron was in May 1995 and will next occur in 2075.

Viewed from Earth, the apparent orbit of A and B means that their separation and position angle (PA) are in continuous change throughout their projected orbit. Observed stellar positions in 2019 are separated by 4.92 arcsec through the PA of 337.1°, increasing to 5.49 arcsec through 345.3° in 2020.[16] The closest recent approach was in February 2016, at 4.0 arcsec through the PA of 300°.[16][101] The observed maximum separation of these stars is about 22 arcsec, while the minimum distance is 1.7 arcsec.[67] The widest separation occurred during February 1976, and the next will be in January 2056.[16]

Alpha Centauri C is about 13,000 AU (0.21 ly; 1.9×10 ~~^~~ 12 km) from Alpha Centauri AB, equivalent to about 5% of the distance between Alpha Centauri AB and the Sun.[17][57][66] Until 2017, measurements of its small speed and its trajectory were of too little accuracy and duration in years to determine whether it is bound to Alpha Centauri AB or unrelated.

Radial velocity measurements made in 2017 were precise enough to show that Proxima Centauri and Alpha Centauri AB are gravitationally bound.[17] The orbital period of Proxima Centauri is approximately 511000+41000
−30000 years, with an eccentricity of 0.5, much more eccentric than Mercury's. Proxima Centauri comes within 4100+700
−600 AU of AB at periastron, and its apastron occurs at 12300+200
−100 AU.[5]

### Physical properties

[edit]

ESO - Alpha Centauri in the HR-System (by) Relative sizes and colour of the Alpha Centauri A, B and C (Proxima) and other local stars, incl. the Sun and Jupiter (artist's impression)

Asteroseismic studies, chromospheric activity, and stellar rotation (gyrochronology) are all consistent with the Alpha Centauri system being similar in age to, or slightly older than, the Sun.[102] Asteroseismic analyses that incorporate tight observational constraints on the stellar parameters for the Alpha Centauri stars have yielded age estimates of 4.85±0.5 Gyr,[103] 5.0±0.5 Gyr,[104] 5.2 ± 1.9 Gyr,[105] 6.4 Gyr,[106] and 6.52±0.3 Gyr.[107] Age estimates for the stars based on chromospheric activity (Calcium H & K emission) yield 4.4 ± 2.1 Gyr, whereas gyrochronology yields 5.0±0.3 Gyr.[102] Stellar evolution theory implies both stars are slightly older than the Sun at 5 to 6 billion years, as derived by their mass and spectral characteristics.[57][108]

From the orbital elements, the total mass of Alpha Centauri AB is about 2.0 M☉[f] – or twice that of the Sun.[67] The average individual stellar masses are about 1.08 M☉ and 0.91 M☉, respectively,[5] though slightly different masses have also been quoted in recent years, such as 1.14 M☉ and 0.92 M☉,[85] totaling 2.06 M☉. Alpha Centauri A and B have absolute magnitudes of +4.38 and +5.71, respectively.

#### Alpha Centauri AB System

[edit]

α Centauri A (left) is of the same stellar type G2 as the Sun, while α Centauri B (right) is a K1-type star.[109]

##### Alpha Centauri A

[edit]

Alpha Centauri A, also known as Rigil Kentaurus, is the principal member, or primary, of the binary system. It is a solar-like main-sequence star with a similar yellowish colour,[110] whose stellar classification is spectral type G2-V;[3] it is about 10% more massive than the Sun,[103] with a radius about 22% larger.[111] When considered among the individual brightest stars in the night sky, it is the fourth-brightest at an apparent magnitude of +0.01,[2] being slightly fainter than Arcturus at an apparent magnitude of −0.05.

The type of magnetic activity on Alpha Centauri A is comparable to that of the Sun, showing coronal variability due to star spots, as modulated by the rotation of the star. However, since 2005 the activity level has fallen into a deep minimum that might be similar to the Sun's historical Maunder Minimum. Alternatively, it may have a very long stellar activity cycle and is slowly recovering from a minimum phase.[112]

##### Alpha Centauri B

[edit]

This section is about α Centauri B, also known as Toliman and is not to be confused with β Centauri, B Centauri, or b Centauri. For other uses, see Toliman (disambiguation).

Alpha Centauri B, also known as Toliman, is the secondary star of the binary system. It is a main-sequence star of spectral type K1-V, making it more an orange colour than Alpha Centauri A;[110] it has around 90% of the mass of the Sun and a 14% smaller diameter. Although it has a lower luminosity than A, Alpha Centauri B emits more energy in the X-ray band.[113] Its light curve varies on a short time scale, and there has been at least one observed flare.[113] It is more magnetically active than Alpha Centauri A, showing a cycle of 8.2±0.2 yr compared to 11 years for the Sun, and has about half the minimum-to-peak variation in coronal luminosity of the Sun.[112] This cycle was recently re-estimated based on more than 20 years of high-resolution spectroscopic observations of the CaIIH&K lines showing a cycle of 7.8±0.2 yr.[114] Alpha Centauri B has an apparent magnitude of +1.35, slightly dimmer than Mimosa.[44]

#### Alpha Centauri C

[edit]

Main article: Proxima Centauri

Alpha Centauri C, better known as Proxima Centauri, is a small main-sequence red dwarf of spectral class M6-Ve. It has an absolute magnitude of +15.60, over 20,000 times fainter than the Sun. Its mass is calculated to be 0.1221 M☉.[115] It is the closest star to the Sun but is too faint to be visible to the naked eye.[116]

Relative positions of Sun, Alpha Centauri AB and Proxima Centauri. Grey dot is projection of Proxima Centauri, located at the same distance as Alpha Centauri AB.

## Planetary system

[edit]

The Alpha Centauri system as a whole has two confirmed planets, both of them around Proxima Centauri. While other planets have been claimed to exist around all of the stars, none of the discoveries have been confirmed.

### Planets of Proxima Centauri

[edit]

Main articles: Proxima Centauri b, c, and d

See also: Proxima Centauri § Planetary system

Proxima Centauri b is a terrestrial planet discovered in 2016 by astronomers at the European Southern Observatory (ESO). It has an estimated minimum mass of 1.17 M🜨 (Earth masses) and orbits approximately 0.049 AU from Proxima Centauri, placing it in the star's habitable zone.[117][118]

The discovery of Proxima Centauri c was formally published in 2020 and could be a super-Earth or mini-Neptune.[119][120] It has a mass of roughly 7 M🜨 and orbits about 1.49 AU from Proxima Centauri with a period of 1,928 days (5.28 yr).[121] In June 2020, a possible direct imaging detection of the planet hinted at the presence of a large ring system.[122] However, a 2022 study disputed the existence of this planet.[19]

A 2020 paper refining Proxima b's mass excludes the presence of extra companions with masses above 0.6 M🜨 at periods shorter than 50 days, but the authors detected a radial-velocity curve with a periodicity of 5.15 days, suggesting the presence of a planet with a mass of about 0.29 M🜨.[118] This planet, Proxima Centauri d, was detected in 2022.[18][19]

### Planets of Alpha Centauri A

[edit]

Main article: Alpha Centauri Ab

The discovery image of Alpha Centauri's candidate Neptunian planet, marked here as "C1" The Alpha Centauri A planetary system  Companion
(in order from star) | Mass | Semimajor axis
(AU) | Orbital period
(days) | Eccentricity | Inclination | Radius

|
|
|
|
|
|

b (unconfirmed) | 9~35[g] M🜨 | 1.1  | ~360  | —  | ~65 ± 25° | 3.3~7 R🜨

In 2021, a candidate planet named Candidate 1 (or C1) was detected around Alpha Centauri A, thought to orbit at approximately 1.1 AU with a period of about one year, and to have a mass between that of Neptune and one-half that of Saturn, though it may be a dust disk or an artefact. The possibility of C1 being a background star has been ruled out.[123][20] If this candidate is confirmed, the temporary name C1 will most likely be replaced with the scientific designation Alpha Centauri Ab in accordance with current naming conventions.[124]

GO Cycle 1 observations are planned for the James Webb Space Telescope (JWST) to search for planets around Alpha Centauri A, as well as observations of Epsilon Muscae.[125] The coronographic observations, which occurred on July 26 and 27, 2023, were failures, though there are follow-up observations in March 2024.[126] Pre-launch estimates predicted that JWST will be able to find planets with a radius of 5 R🜨 at 1–3 AU. Multiple observations every 3–6 months could push the limit down to 3 R🜨.[127] Post-launch estimates based on observations of HIP 65426 b find that JWST will be able to find planets even closer to Alpha Centauri A and could find a 5 R🜨 planet at 0.5–2.5 AU.[128] Candidate 1 has an estimated radius between 3.3–11 R🜨[20] and orbits at 1.1 AU. It is therefore likely within the reach of JWST observations.

### Planets of Alpha Centauri B

[edit]

Main article: Alpha Centauri Bb

The first claim of a planet around Alpha Centauri B was that of Alpha Centauri Bb in 2012, which was proposed to be an Earth-mass planet in a 3.2-day orbit.[129] This was refuted in 2015 when the apparent planet was shown to be an artefact of the way the radial velocity data was processed.[130][131][21]

A search for transits of planet Bb was conducted with the Hubble Space Telescope from 2013 to 2014. This search detected one potential transit-like event, which could be associated with a different planet with a radius around 0.92 R🜨. This planet would most likely orbit Alpha Centauri B with an orbital period of 20.4 days or less, with only a 5% chance of it having a longer orbit. The median of the likely orbits is 12.4 days. Its orbit would likely have an eccentricity of 0.24 or less.[132] It could have lakes of molten lava and would be far too close to Alpha Centauri B to harbour life.[133] If confirmed, this planet might be called Alpha Centauri Bc. However, the name has not been used in the literature, as it is not a claimed discovery.

### Hypothetical planets

[edit]

Additional planets may exist in the Alpha Centauri system, either orbiting Alpha Centauri A or Alpha Centauri B individually, or in large orbits around Alpha Centauri AB. Because both stars are fairly similar to the Sun (for example, in age and metallicity), astronomers have been especially interested in making detailed searches for planets in the Alpha Centauri system. Several established planet-hunting teams have used various radial velocity or star transit methods in their searches around these two bright stars.[134] All the observational studies have so far failed to find evidence for brown dwarfs or gas giants.[134][135]

In 2009, computer simulations showed that a planet might have been able to form near the inner edge of Alpha Centauri B's habitable zone, which extends from 0.5–0.9 AU from the star. Certain special assumptions, such as considering that the Alpha Centauri pair may have initially formed with a wider separation and later moved closer to each other (as might be possible if they formed in a dense star cluster), would permit an accretion-friendly environment farther from the star.[136] Bodies around Alpha Centauri A would be able to orbit at slightly farther distances due to its stronger gravity. In addition, the lack of any brown dwarfs or gas giants in close orbits around Alpha Centauri make the likelihood of terrestrial planets greater than otherwise.[137] A theoretical study indicates that a radial velocity analysis might detect a hypothetical planet of 1.8 M🜨 in Alpha Centauri B's habitable zone.[138]

Radial velocity measurements of Alpha Centauri B made with the High Accuracy Radial Velocity Planet Searcher spectrograph were sufficiently sensitive to detect a 4 M🜨 planet within the habitable zone of the star (i.e. with an orbital period P = 200 days), but no planets were detected.[129]

Current estimates place the probability of finding an Earth-like planet around Alpha Centauri at roughly 75%.[139] The observational thresholds for planet detection in the habitable zones by the radial velocity method are currently (2017) estimated to be about 53 M🜨 for Alpha Centauri A, 8.4 M🜨 for Alpha Centauri B, and 0.47 M🜨 for Proxima Centauri.[140]

Early computer-generated models of planetary formation predicted the existence of terrestrial planets around both Alpha Centauri A and B,[138][141] but most recent numerical investigations have shown that the gravitational pull of the companion star renders the accretion of planets difficult.[136][142] Despite these difficulties, given the similarities to the Sun in spectral types, star type, age and probable stability of the orbits, it has been suggested that this stellar system could hold one of the best possibilities for harbouring extraterrestrial life on a potential planet.[6][137][143][141]

In the Solar System, it was once thought that Jupiter and Saturn were probably crucial in perturbing comets into the inner Solar System, providing the inner planets with a source of water and various other ices.[144] However, since isotope measurements of the deuterium to hydrogen (D/H) ratio in comets Halley, Hyakutake, Hale–Bopp, 2002T7, and Tuttle yield values approximately twice that of Earth's oceanic water, more recent models and research predict that less than 10% of Earth's water was supplied from comets. In the α Centauri system, Proxima Centauri may have influenced the planetary disk as the α Centauri system was forming, enriching the area around Alpha Centauri with volatile materials.[145] This would be discounted if, for example, α Centauri B happened to have gas giants orbiting α Centauri A (or vice versa), or if α Centauri A and B themselves were able to perturb comets into each other's inner systems, as Jupiter and Saturn presumably have done in the Solar System.[144] Such icy bodies probably also reside in Oort clouds of other planetary systems. When they are influenced gravitationally by either the gas giants or disruptions by passing nearby stars, many of these icy bodies then travel star-wards.[144] Such ideas also apply to the close approach of Alpha Centauri or other stars to the Solar system, when, in the distant future, the Oort Cloud might be disrupted enough to increase the number of active comets.[95]

To be in the habitable zone, a planet around Alpha Centauri A would have an orbital radius of between about 1.2 and 2.1 AU so as to have similar planetary temperatures and conditions for liquid water to exist.[146] For the slightly less luminous and cooler α Centauri B, the habitable zone is between about 0.7 and 1.2 AU.[146]

With the goal of finding evidence of such planets, both Proxima Centauri and α Centauri AB were among the listed "Tier-1" target stars for NASA's Space Interferometry Mission (S.I.M.). Detecting planets as small as three Earth-masses or smaller within two AU of a "Tier-1" target would have been possible with this new instrument.[147] The S.I.M. mission, however, was cancelled due to financial issues in 2010.[148]

### Circumstellar discs

[edit]

Based on observations between 2007 and 2012, a study found a slight excess of emissions in the 24 μm (mid/far-infrared) band surrounding α Centauri AB, which may be interpreted as evidence for a sparse circumstellar disc or dense interplanetary dust.[149] The total mass was estimated to be between 10−7 to 10−6 the mass of the Moon, or 10–100 times the mass of the Solar System's zodiacal cloud.[149] If such a disc existed around both stars, α Centauri A's disc would likely be stable to 2.8 AU, and α Centauri B's would likely be stable to 2.5 AU [149] This would put A's disc entirely within the frost line, and a small part of B's outer disc just outside.[149]

## Interaction with surrounding

[edit]

There have been studies that there is a considerable amount of material exchanged with the far regions of the Solar System,[150] resulting in possibly material coming from Alpha Centauri going also deeper into the Solar System. If proven the galaxy could form an interconnected network of larger material.[151]

## View from this system

[edit]

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|

Looking towards the sky around Orion from Alpha Centauri with Sirius near Betelgeuse, Procyon in Gemini, and the Sun in Cassiopeia generated by Celestia Simulated night-sky image with a "W" of stars from Cassiopeia connected by lines, and the Sun, labeled "Sol", as it would appear to the left of the "W"

The sky from α Centauri AB would appear much as it does from the Earth, except that Centaurus's brightest star, being α Centauri AB itself, would be absent from the constellation. The Sun would appear as a white star of apparent magnitude +0.5,[152] roughly the same as the average brightness of Betelgeuse from Earth. It would be at the antipodal point of α Centauri AB's current right ascension and declination, at 02h 39m 36s +60° 50′ 02.308″ (2000), in eastern Cassiopeia, easily outshining all the rest of the stars in the constellation. With the placement of the Sun east of the magnitude 3.4 star Epsilon Cassiopeiae, nearly in front of the Heart Nebula, the "W" line of stars of Cassiopeia would have a "/W" shape.[153]

Other nearby stars' placements may be affected somewhat drastically. Sirius, at 9.2 light years away from the system, would still be the brightest star in the night sky, with a magnitude of -1.2, but would be located in Orion less than a degree away from Betelgeuse. Procyon, which would also be at a slightly further distance than from the Sun, would move to outshine Pollux in the middle of Gemini.

A planet around either α Centauri A or B would see the other star as a very bright secondary. For example, an Earth-like planet at 1.25 AU  from α Cen A (with a revolution period of 1.34 years) would get Sun-like illumination from its primary, and α Cen B would appear 5.7–8.6 magnitudes dimmer (−21.0 to −18.2), 190–2,700 times dimmer than α Cen A but still 150–2,100 times brighter than the full Moon. Conversely, an Earth-like planet at 0.71 AU  from α Cen B (with a revolution period of 0.63 years) would get nearly Sun-like illumination from its primary, and α Cen A would appear 4.6–7.3 magnitudes dimmer (−22.1 to −19.4), 70 to 840 times dimmer than α Cen B but still 470–5,700 times brighter than the full Moon.

Proxima Centauri would appear dim as one of many stars, being magnitude 4.5 at its current distance, and magnitude 2.6 at periastron.[154]

## Future exploration

[edit]

See also: 2069 Alpha Centauri mission

Diagram of the closest stars to the Sun, within 7.5 light years

Alpha Centauri is a first target for crewed or robotic interstellar exploration. Using current spacecraft technologies, crossing the distance between the Sun and Alpha Centauri would take several millennia, though the possibility of nuclear pulse propulsion or laser light sail technology, as considered in the Breakthrough Starshot program, could make the journey to Alpha Centauri in 20 years.[155][156][157] An objective of such a mission would be to make a fly-by of, and possibly photograph, planets that might exist in the system.[158][159] The existence of Proxima Centauri b, announced by the European Southern Observatory (ESO) in August 2016, would be a target for the Starshot program.[158][160]

NASA released a mission concept in 2017 that would send a spacecraft to Alpha Centauri in 2069, scheduled to coincide with the 100th anniversary of the first crewed lunar landing in 1969, Apollo 11. Even at 10% of the speed of light (about 108 million km/h), which NASA experts say may be possible, it would take a spacecraft 44 years to reach the system, by the year 2113, and would take another 4 years for a signal, by the year 2117 to reach Earth. The concept received no further funding or development.[161][162]

## In culture

[edit]

Alpha Centauri has been recognized and associated throughout history, particularly in the Southern Hemisphere. Polynesians have been using Alpha Centauri for their star navigation and have called it Kamailehope. In the Ngarrindjeri culture of Australia, Alpha Centauri represents with Beta Centauri two sharks chasing a stingray, the Southern Cross, and in Incan culture it with Beta Centauri form the eyes of a llama-shaped dark constellation embedded in the band of stars that the visible Milky Way forms in the sky. In ancient Egypt it was also revered and in China it is known as part of the South Gate asterism.[163]

The Sagan Planet Walk in Ithaca, New York, is a walkable scale model of the solar system. An obelisk representing the scaled position of Alpha Centauri has been added at ʻImiloa Astronomy Center in Hawaii.[164]

This section is an excerpt from Stars in fiction § Real stars.[edit]

The Alpha Centauri system is the closest star system to Earth—with Proxima Centauri being the closest of the system's stars—which has given it a special position in science fiction literature. Several stories of the first interstellar journeys have featured it as the intended destination. Among the earliest examples are the 1931 short story "Across the Void" by Leslie F. Stone and the 1935 short story "Proxima Centauri" by Murray Leinster.[165][166] The spacecraft in the latter reaches its destination in less than a decade but has the capacity to function as a generation starship if needed; the use of an actual generation starship headed for the system was later depicted in the 1944 novel Far Centaurus by A. E. van Vogt,[167][168] and the 1997 novel Alpha Centauri by William Barton and Michael Capobianco portrays such a mission being endangered by terrorists.[165][169] Conversely, Liu Cixin's 2006 novel The Three-Body Problem depicts aliens from Alpha Centauri coming to Earth.[166]

## See also

[edit]

* Project Longshot
* List of nearest K-type stars
* List of nearest G-type stars

## Notes

[edit]

1. ^ Proxima Centauri is gravitationally bound to the α Centauri system, but for practical and historical reasons it is described in detail in its own article.
2. ^ Spellings include Rigjl Kentaurus,[30] Portuguese Riguel Kentaurus,[31][32]
3. ^ This is calculated for a fixed latitude by knowing the star's declination (δ) using the formulae (90°+ δ). α Centauri's declination is −60° 50′, so the observed latitude where the star is circumpolar will be south of −29° 10′ South or 29°. Similarly, the place where Alpha Centauri never rises for northern observers is north of the latitude (90°+ δ) N or +29° North.
4. ^ Weighted parallax based on parallaxes from van Altena et al. (1995) and Söderhjelm (1999).
5. ^ Proper motions are expressed in smaller angular units than arcsec, being measured in milliarcsec (mas.) (thousandths of an arcsec). Negative values for proper motion in RA indicate the sky motion is from east to west, and in declination north to south.
6. ^ (   11.2 + 35.6   2 ) 3 1   79.91 2   ≈ 2.0 {\displaystyle {\begin{smallmatrix}\left({\frac {\ 11.2+35.6\ }{2}}\right)^{3}{\frac {1}{~79.91^{2}\ }}\approx 2.0\end{smallmatrix}}\qquad } – see formula in standard gravitational parameter article.
7. ^ These mass limits are calculated from the observed radius of  3.3~7 R🜨 applied to the equation quoted, and presumably used, to calculate the planet mass from the planet radius in the Wagner et al 2021 paper:[20] R ∝ M 0.55 (although this radius-mass relationship is for low-mass planets and not for larger gas giants). Therefore  3.31.82 = 8.77  M🜨 and  71.82 = 34.52 M🜨. The  Msin i ≥ 53 M🜨 is for a planet at the outer edge of the conservative habitable zone, 2.1 AU, and so the upper mass limit is lower than that for the C1 planet at just 1.1 AU.

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[edit]

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119. ^ Billings, Lee (12 April 2019). "A Second Planet May Orbit Earth's Nearest Neighboring Star". Scientific American. Retrieved 2 August 2020.
120. ^ Damasso, Mario; Del Sordo, Fabio; et al. (January 2020). "A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU". Science Advances. 6 (3): eaax7467. Bibcode:2020SciA....6.7467D. doi:10.1126/sciadv.aax7467. PMC 6962037. PMID 31998838.
121. ^ Benedict, G. Fritz; McArthur, Barbara E. (June 2020). "A Moving Target — Revising the Mass of Proxima Centauri c". Research Notes of the AAS. 4 (6): 86. Bibcode:2020RNAAS...4...86B. doi:10.3847/2515-5172/ab9ca9. S2CID 225798015.
122. ^ Gratton, Raffaele; Zurlo, Alice; Le Coroller, Hervé; et al. (June 2020). "Searching for the near-infrared counterpart of Proxima c using multi-epoch high-contrast SPHERE data at VLT". Astronomy & Astrophysics. 638: A120. arXiv:2004.06685. Bibcode:2020A&A...638A.120G. doi:10.1051/0004-6361/202037594. S2CID 215754278.
123. ^ Sample, Ian (10 February 2021). "Astronomers' hopes raised by glimpse of possible new planet?". The Guardian. Retrieved 16 January 2022.
124. ^ "Naming of Exoplanets". International Astronomical Union. Archived from the original on 10 January 2020. Retrieved 24 July 2021.
125. ^ "1618 Program Information". www.stsci.edu. Archived from the original on 1 September 2022. Retrieved 1 September 2022.
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127. ^ Beichman, Charles; Ygouf, Marie; Llop Sayson, Jorge; Mawet, Dimitri; Yung, Yuk; Choquet, Elodie; Kervella, Pierre; Boccaletti, Anthony; Belikov, Ruslan; Lissauer, Jack J.; Quarles, Billy; Lagage, Pierre-Olivier; Dicken, Daniel; Hu, Renyu; Mennesson, Bertrand (1 January 2020). "Searching for Planets Orbiting α Cen A with the James Webb Space Telescope". Publications of the Astronomical Society of the Pacific. 132 (1007): 015002. arXiv:1910.09709. Bibcode:2020PASP..132a5002B. doi:10.1088/1538-3873/ab5066. ISSN 0004-6280. S2CID 204823856.
128. ^ Carter, Aarynn L.; Hinkley, Sasha; Kammerer, Jens; Skemer, Andrew; Biller, Beth A.; Leisenring, Jarron M.; Millar-Blanchaer, Maxwell A.; Petrus, Simon; Stone, Jordan M.; Ward-Duong, Kimberly; Wang, Jason J.; Girard, Julien H.; Hines, Dean C.; Perrin, Marshall D.; Pueyo, Laurent (2023). "The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 μm". The Astrophysical Journal Letters. 951 (1): L20. arXiv:2208.14990. Bibcode:2023ApJ...951L..20C. doi:10.3847/2041-8213/acd93e.
129. ^ a b Dumusque, X.; Pepe, F.; Lovis, C.; Ségransan, D.; Sahlmann, J.; Benz, W.; Bouchy, F.; Mayor, M.; Queloz, D.; Santos, N.; Udry, S. (17 October 2012). "An Earth mass planet orbiting Alpha Centauri B" (PDF). Nature. 490 (7423): 207–211\. Bibcode:2012Natur.491..207D. doi:10.1038/nature11572. PMID 23075844. S2CID 1110271. Archived (PDF) from the original on 9 October 2022. Retrieved 17 October 2012.
130. ^ Wenz, John (29 October 2015). "It turns out the closest exoplanet to us doesn't actually exist". Popular Mechanics. Retrieved 8 December 2018.
131. ^ "Poof! The planet closest to our Solar system just vanished". National Geographic News. 29 October 2015. Archived from the original on 30 October 2015. Retrieved 8 December 2018.
132. ^ Demory, Brice-Olivier; Ehrenreich, David; Queloz, Didier; Seager, Sara; Gilliland, Ronald; Chaplin, William J.; et al. (June 2015). "Hubble Space Telescope search for the transit of the Earth-mass exoplanet Alpha Centauri Bb". Monthly Notices of the Royal Astronomical Society. 450 (2): 2043–2051\. arXiv:1503.07528. Bibcode:2015MNRAS.450.2043D. doi:10.1093/mnras/stv673. S2CID 119162954.
133. ^ Aron, Jacob. "Twin Earths may lurk in our nearest star system". New Scientist. Retrieved 8 December 2018.
134. ^ a b "Why haven't planets been detected around Alpha Centauri?". Universe Today. 19 April 2008. Archived from the original on 21 April 2008. Retrieved 19 April 2008.
135. ^ Stephens, Tim (7 March 2008). "Nearby star should harbor detectable, Earth-like planets". News & Events. UC Santa Cruz. Archived from the original on 17 April 2008. Retrieved 19 April 2008.
136. ^ a b Thebault, P.; Marzazi, F.; Scholl, H. (2009). "Planet formation in the habitable zone of alpha centauri B". Monthly Notices of the Royal Astronomical Society. 393 (1): L21 – L25. arXiv:0811.0673. Bibcode:2009MNRAS.393L..21T. doi:10.1111/j.1745-3933.2008.00590.x. S2CID 18141997.
137. ^ a b Quintana, E. V.; Lissauer, J. J.; Chambers, J. E.; Duncan, M. J. (2002). "Terrestrial Planet Formation in the Alpha Centauri System". Astrophysical Journal. 576 (2): 982–996\. Bibcode:2002ApJ...576..982Q. CiteSeerX 10.1.1.528.4268. doi:10.1086/341808. S2CID 53469170.
138. ^ a b Guedes, Javiera M.; Rivera, Eugenio J.; Davis, Erica; Laughlin, Gregory; Quintana, Elisa V.; Fischer, Debra A. (2008). "Formation and Detectability of Terrestrial Planets Around Alpha Centauri B". Astrophysical Journal. 679 (2): 1582–1587\. arXiv:0802.3482. Bibcode:2008ApJ...679.1582G. doi:10.1086/587799. S2CID 12152444.
139. ^ Billings, Lee. Miniature Space Telescope Could Boost the Hunt for "Earth Proxima". Scientific American (scientificamerican.com) (video).
140. ^ Zhao, L.; Fischer, D.; Brewer, J.; Giguere, M.; Rojas-Ayala, B. (January 2018). "Planet detectability in the Alpha Centauri system". Astronomical Journal. 155 (1): 12. arXiv:1711.06320. Bibcode:2018AJ....155...24Z. doi:10.3847/1538-3881/aa9bea. S2CID 118994786. Retrieved 29 December 2017.
141. ^ a b Quintana, Elisa V.; Lissauer, Jack J. (2007). "Terrestrial planet formation in binary star systems". In Haghighipour, Nader (ed.). Planets in Binary Star Systems. Springer. pp. 265–284\. ISBN 978-90-481-8687-7.
142. ^ Barbieri, M.; Marzari, F.; Scholl, H. (2002). "Formation of terrestrial planets in close binary systems: The case of α Centauri A". Astronomy & Astrophysics. 396 (1): 219–224\. arXiv:astro-ph/0209118. Bibcode:2002A&A...396..219B. doi:10.1051/0004-6361:20021357. S2CID 119476010.α+Centauri+A&rft.volume=396&rft.issue=1&rft.pages=219-224&rft.date=2002&rft_id=info:arxiv/astro-ph/0209118&rft_id=https://api.semanticscholar.org/CorpusID:119476010#id-name=S2CID&rft_id=info:doi/10.1051/0004-6361:20021357&rft_id=info:bibcode/2002A&A...396..219B;&rft.aulast=Barbieri&rft.aufirst=M.&rft.au=Marzari,+F.&rft.au=Scholl,+H.&rfr_id=info:sid/en.wikipedia.org:Alpha+Centauri" class="Z3988">
143. ^ Lissauer, J.J.; Quintana, E.V.; Chambers, J.E.; Duncan, M.J.; Adams, F.C. (2004). "Terrestrial planet formation in binary star systems". Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. 22: 99–103\. arXiv:0705.3444. Bibcode:2004RMxAC..22...99L.
144. ^ a b c Croswell, Ken (April 1991). "Does Alpha Centauri have intelligent life?". Astronomy Magazine. Vol. 19, no. 4\. pp. 28–37\. Bibcode:1991Ast....19d..28C.
145. ^ Gilster, Paul (5 July 2006). "Proxima Centauri and habitability". Centauri Dreams. Retrieved 12 August 2010.
146. ^ a b Kaltenegger, Lisa; Haghighipour, Nader (2013). "Calculating the habitable zone of binary star systems. I. S-type binaries". The Astrophysical Journal. 777 (2): 165. arXiv:1306.2889. Bibcode:2013ApJ...777..165K. doi:10.1088/0004-637X/777/2/165. S2CID 118414142.
147. ^ This article incorporates text from this source, which is in the public domain: "Planet hunting by numbers" (Press release). Jet Propulsion Laboratory. 18 October 2006. Archived from the original on 4 August 2010. Retrieved 24 April 2007.
148. ^ Mullen, Leslie (2 June 2011). "Rage Against the Dying of the Light". Astrobiology Magazine. Archived from the original on 4 June 2011. Retrieved 7 June 2011.
149. ^ a b c d Wiegert, J.; Liseau, R.; Thébault, P.; Olofsson, G.; Mora, A.; Bryden, G.; et al. (March 2014). "How dusty is α Centauri? Excess or non-excess over the infrared photospheres of main-sequence stars". Astronomy & Astrophysics. 563: A102. arXiv:1401.6896. Bibcode:2014A&A...563A.102W. doi:10.1051/0004-6361/201321887. S2CID 119198201.α+Centauri?+Excess+or+non-excess+over+the+infrared+photospheres+of+main-sequence+stars&rft.volume=563&rft.pages=A102&rft.date=2014-03&rft_id=info:arxiv/1401.6896&rft_id=https://api.semanticscholar.org/CorpusID:119198201#id-name=S2CID&rft_id=info:doi/10.1051/0004-6361/201321887&rft_id=info:bibcode/2014A&A...563A.102W;&rft.aulast=Wiegert&rft.aufirst=J.&rft.au=Liseau,+R.&rft.au=Thébault,+P.&rft.au=Olofsson,+G.&rft.au=Mora,+A.&rft.au=Bryden,+G.&rft.au=Marshall,+J.P.&rft.au=Eiroa,+C.&rft.au=Montesinos,+B.&rft.au=Ardila,+D.&rft.au=Augereau,+J.C.&rft.au=Bayo+Aran,+A.&rft.au=Danchi,+W.C.&rft.au=del+Burgo,+C.&rft.au=Ertel,+S.&rft.au=Fridlund,+M.C.W.&rft.au=Hajigholi,+M.&rft.au=Krivov,+A.V.&rft.au=Pilbratt,+G.L.&rft.au=Roberge,+A.&rft.au=White,+G.J.&rft.au=Wolf,+S.&rfr_id=info:sid/en.wikipedia.org:Alpha+Centauri" class="Z3988">
150. ^ López, Gustavo V.; Nieto, Juan A. (2018). "Alpha Centauri System and Meteorites Origin". Journal of Applied Mathematics and Physics. 06 (11): 2370–2381\. Bibcode:2018JApMP...6.2370L. doi:10.4236/jamp.2018.611199. ISSN 2327-4352.
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156. ^ O'Neill, Ian (8 July 2008). "How long would it take to travel to the nearest star?". Universe Today.
157. ^ Domonoske, Camila (12 April 2016). "Forget Starships: New Proposal Would Use 'Starchips' To Visit Alpha Centauri". NPR. Retrieved 14 April 2016.
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162. ^ "Do aliens live at Alpha Centauri? NASA wants to send a mission in 2069 to find Out". Newsweek.
163. ^ "Alpha Centauri, the star system closest to our sun". Earth & Sky. 16 April 2023. Retrieved 13 March 2024.
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169. ^ Stableford, Brian (2004). "Barton, William R.". Historical Dictionary of Science Fiction Literature. Scarecrow Press. p. 23\. ISBN 978-0-8108-4938-9. "Alpha Centauri (1997), in which terrorists plague the colony ship which is humankind's last hope"

## External links

[edit]

Wikimedia Commons has media related to Alpha Centauri.

* "SIMBAD observational data". simbad.u-strasbg.fr.
* "Sixth Catalogue of Orbits of Visual Binary Stars". usno.navy.mil. US Naval Observatory. Archived from the original on 12 April 2009.
* "The Imperial Star". Alpha Centauri. southastrodel.com.
* "A voyage to Alpha Centauri". Alpha Centauri. southastrodel.com.
* "Immediate history of Alpha Centauri". Alpha Centauri. southastrodel.com.
* "Alpha Centauri". Stars. glyphweb.com. eSky.

### Hypothetical planets or exploration

[edit]

* "Alpha Centauri system". Nearby stars. jumk.de. Astronomy.
* "O sistema Alpha Centauri". uranometrianova.pro.br (in Portuguese). Archived from the original on 3 March 2016.
* "Alpha Centauri". alpha-centauri.pt (in Portuguese). Associação de Astronomia.
* Thompson, Andrea (7 March 2008). "Nearest star system might harbor Earth twin". Science / Astronomy. Space.com. Archived from the original on 2 June 2008. Retrieved 18 November 2021.

* v
* t
* e

The Alpha Centauri system

Stars|

* Rigil Kentaurus (A)
* Toliman (B)
* Proxima Centauri (C)

Planets|

* Ab?
* Bb†
* Bc?
* Cd
* Cb
* Cc?

Proposed mission concepts|

* 2069 Alpha Centauri mission
* AIMStar
* Breakthrough Starshot
* Project Longshot
* Starlight

* † \- Disproven
* Category

* v
* t
* e

Celestial objects within 10 light-years →

| Primary member type|

Celestial objects by systems.

| Main-sequence
stars|

| A-type|

* Sirius (Alpha Canis Majoris) (8.7094±0.0054 ly)
* white dwarf B

|

G-type|

* Sun (0 ly)
* rest of Solar System
* Alpha Centauri
* α Cen (Rigil Kentaurus) (4.3441±0.0022 ly)
* K-type main-sequence star B (Toliman)
* red dwarf C (Proxima Centauri) (4.2465 ± 0.0003 ly)
* 2 (5?) planets: Ab?; Bc?; Cb, Cc?, Cd

M-type
(red dwarfs)|

* Barnard's Star (5.9629±0.0004 ly)
* 4 planets: b, c, d, e
* Wolf 359 (7.8558±0.0013 ly)
* 1? planets: b?
* Lalande 21185 (8.3044±0.0007 ly)
* 2 (3?) planets: b, d?, c
* Gliese 65 A (BL Ceti) (8.724±0.012 ly)
* red dwarf B (UV Ceti)
* 1? planets: b?
* Ross 154 (9.7063±0.0009 ly)

| Brown dwarfs|

| L-type|

* Luhman 16 (6.5029±0.0011 ly)
* T-type brown dwarf B

|

| Sub-brown dwarfs
and rogue planets|

| Y-type|

* WISE 0855−0714 (7.430±0.041 ly)

|

* v
* t
* e

Constellation of Centaurus

* List of stars in Centaurus
* Centaurus in Chinese astronomy

Stars|

| Bayer|

* α
* A (Rigil Kentaurus)
* B (Toliman)
* C (Proxima Centauri)
* β (Hadar)
* γ (Muhlifain)
* δ
* ε
* ζ (Leepwal)
* η
* θ (Menkent)
* ι (Kulou)
* κ
* λ
* μ
* ν (Heng)
* ξ1
* ξ2
* ο1
* ο2
* π
* ρ
* σ
* τ
* υ1
* υ2
* φ
* χ
* ψ

|

Flamsteed|

* 1 (i)
* 2 (g)
* 3 (k)
* 4 (h)

Variable|

* R
* T
* U
* V
* Y
* RR
* SV
* SX
* BV
* DY
* UY
* V346
* V553
* V744
* V752
* V761 (a)
* V763 (C1)
* V766
* V779
* V803
* V810
* V816 (Przybylski's Star)
* V831
* V842
* V885
* V886
* V863
* V945 (H)
* V1032
* V1369
* V1400

HR|

* 4460 (A)
* 4466 (C2)
* 4476 (C3)
* 4499
* 4522
* 4523
* 4537 (j)
* 4546 (B)
* 4620 (E)
* 4652 (D)
* 4682 (F)
* 4712 (x1)
* 4721
* 4724 (x2)
* 4732 (G)
* 4748 (u)
* 4796
* 4817 (l)
* 4831 (w)
* 4874 (p)
* 4888 (e)
* 4889 (n)
* 4940 (f)
* 4979
* 4989
* 5006 (r)
* 5035 (J)
* 5041 (m)
* 5071 (K)
* 5089 (d)
* 5141 (Q)
* 5172 (M)
* 5174 (z)
* 5207 (N)
* 5222 (y)
* 5224
* 5241
* 5297
* 5358 (v)
* 5371
* 5471 (b)
* 5485 (c1)
* 5489 (c2)

HD|

* 97413
* 98176
* 100453
* 101581
* 101930
* 102117 (Uklun)
* 103197
* 107914
* 108236
* 109749
* 110113
* 113538
* 113766
* 114386
* 114729
* 115600
* 116434 (Matza)
* 117207
* 117618 (Dofida)
* 120411
* 121228
* 121504
* 124448
* 125072
* 125595
* 131399

Other|

* 2MASS J1126−5003
* 2M1207
* Gaia BH2
* J1407b
* PSR B1259−63
* PSR J1311–3430
* TOI-763
* WASP-15 (Nyamien)
* WASP-41
* WASP-42
* WASP-167/KELT-13

| Exoplanets|

* 2M1207b
* b Centauri b
* HD 102117 b
* HD 103197 b
* HD 109749 b
* HD 101930 b
* HD 113538 b
* c
* HD 114386 b
* HD 114729 b
* HD 117207 b
* HD 117618 b
* HD 121504 b
* HIP 65426 b
* HIP 67522 b
* Proxima Centauri b
* c
* d
* WASP-15b

|

| Star clusters|

* IC 2944
* NGC 3766
* NGC 4230
* NGC 5286
* NGC 5281
* NGC 5316
* NGC 5460
* NGC 5617
* NGC 5662
* ω Centauri
* Scorpius–Centaurus association
* Stock 16

|

| Nebulae|

* Boomerang Nebula
* Fleming 1
* G292.0+1.8
* IC 2944
* NGC 3918
* NGC 5307
* RCW 79
* Southern Crab Nebula
* SN 185 (RCW 86)
* SuWt 2

|

Galaxies|

| NGC|

* 3783
* 4444
* 4603
* 4622
* 4650A
* 4683
* 4696
* 4706
* 4709
* 4729
* 4730
* 4743
* 4744
* 4930
* 4945
* 4976
* 5011
* A
* 5026
* 5090
* 5091
* 5102
* 5114
* 5121
* 5128 (Centaurus A)
* 5161
* 5253
* 5291
* 5398
* 5408
* 5419
* 5483

|

Other|

* ESO 269-57
* ESO 325-G004
* ESO 383-76
* ESO 444-46
* Fourcade-Figueroa Object
* IC 3370
* IRAS 13224-3809
* LEDA 677373
* PKS 1144-379
* PKS 1353−341
* PKS 1424-418

| Galaxy clusters|

* Abell S740
* Shapley Supercluster

|

| Astronomical events|

* SN 185
* SN 1895B
* SN 1986G

|

Category

* v
* t
* e

2021 in space

* « 2020

2022 »

Space probe and
telescope launches |

* Tiangong space station Tianhe (April 2021)
* Lucy (Oct 2021)
* DART / LICIACube (Nov 2021)
* James Webb Space Telescope (Dec 2021)

Impact events|

* Winchcombe meteorite

Selected NEOs|

* Asteroid close approaches
* 2021 AV7
* 2020 XR
* 2016 DV1
* 2021 DW1
* 99942 Apophis
* (231937) 2001 FO32
* 2021 GW4
* 2021 PH27
* (620094) 2016 AJ193
* 2021 SG
* 2021 TP21
* 2021 UA1
* (679648) 2019 XS
* 3361 Orpheus
* 1994 WR12
* 4660 Nereus
* (163899) 2003 SD220
* 2018 AH

Exoplanets |

* Alpha Centauri Ab (unconfirmed)
* COCONUTS-2b
* Gliese 486
* HD 108236 f
* HD 110082 b
* Kepler-1704b
* KOI-5Ab
* L 98-59
* e
* f?
* Lalande 21185 c
* Lambda Serpentis b
* LHS 1678
* b
* c
* NGTS-13b
* NGTS-14Ab
* OGLE-2019-BLG-0960Lb
* PDS 70c circumplanetary disk
* TIC 172900988 b
* TOI-178
* b
* c
* d
* e
* f
* g
* TOI-755
* b
* c
* Vega b (unconfirmed)
* YSES 2 b

Discoveries|

* QSO J0313−1806 (distant quasar)
* ID2299 (elliptical galaxy)
* TIC 168789840 sextuple system
* V723 Mon black hole candidate
* 2018 AG37 (TNO)
* 2021 DR15 (TNO)
* ALESS 073.1 (spiral galaxy)
* PJ352–15 astrophysical jet
* 2MASS J0348−6022 (rapidly-rotating brown dwarf)
* ZTF J1901+1458 (massive white dwarf)
* WISE 1534–1043 (brown dwarf)
* 1 moon of Jupiter
* 1 moon of Saturn
* Andy's object (radio source)

Comets |

* C/2021 A1 (Leonard)
* C/2021 J1 (Maury–Attard)
* (248370) 2005 QN173
* 8P/Tuttle
* C/2014 OG392 (PanSTARRS)
* C/2014 UN271 (Bernardinelli-Bernstein)
* C/2021 T4 (Lemmon)
* P/2021 U3 (Attard–Maury)

Space
exploration|

* Hope Mars mission (Mars orbit insertion: Feb 2021)
* Mars 2020 (Mars orbit insertion: Feb 2021; Perseverance Mars landing: Feb 2021)
* Tianwen-1 (Mars orbit insertion: Feb 2021; Zhurong rover Mars landing: May 2021)

* Outer space portal
* Category:2020 in outer space — Category:2021 in outer space — Category:2022 in outer space

Authority control databases

International|

* VIAF
* FAST

National|

* Germany
* Israel

Other|

* Yale LUX

Portals:

* Astronomy
* Stars
* Spaceflight

*[RA:]: Right Ascension
*[Dec.:]: Declination
*[v]: View this template
*[t]: Discuss this template
*[e]: Edit this template
*[Primary]: Primary member of a system is the brightest one (and, in most cases, also the most massive one).
*[rest]: 8 planets; over 1,100,000 minor planets (including 5 dwarf planets); over 5000 comets; 206 moons of planets; over 200 moons of minor planets (including 9 moons of dwarf planets); bodies of planetary rings (mostly were observed rings, not separate bodies, but over 150 moonlets were observed); numerous small bodies, observed as meteors and meteorites, but not catalogued as minor planets or comets; spacecraft; space debris; cosmonauts. Some known comets and spacecrafts, currently located within Solar System boundaries, are not gravitationally bound with the Sun, and therefore formally are separate (interstellar) objects.