Alpha Centauri

alpha centauri star,alpha centauri ab

Alpha Centauri (α Cen) is a triple star system located in the constellation Centaurus. It is the nearest star system to the Sun and the third brightest point of light in the sky outside the solar system, after Sirius and Canopus. It outshines the northern luminaries Arcturus, Vega and Capella. With a combined apparent magnitude of -0.27, Alpha Centauri is also the brightest point of light in Centaurus, visibly outshining its neighbour Hadar (Beta Centauri) and the orange giant Menkent (Theta Centauri).

alpha centauri star,alpha centauri ab
Alpha Centauri, image: Wikisky

The Alpha Centauri star system consists of three components: Rigil Kentaurus (Alpha Centauri A), Toliman (Alpha Centauri B), and Proxima Centauri (Alpha Centauri C). Proxima Centauri, the faintest component, is the nearest individual star to the Sun, located only 4.244 light years from Earth. The brighter Rigil Kentaurus and Toliman lie at a distance of 4.37 light years. They form the Alpha Centauri AB binary system, which appears as a single star to the naked eye.

Proxima Centauri hosts the nearest planetary system to Earth. Two exoplanets have been confirmed to be orbiting the star. Proxima Centauri b, an Earth-sized planet discovered in 2016, orbits in the star’s habitable zone. Another planet, designated Proxima Centauri c, was confirmed in 2020.

Star system

The Alpha Centauri system consists of Alpha Centauri A, a yellow main sequence star of the spectral type G2V, Alpha Centauri B, an orange main sequence star with the stellar classification K1V, and Alpha Centauri C, a faint red dwarf of the spectral type M5.5Ve.

The components Alpha Centauri A and B, formally named Rigil Kentaurus and Toliman, form the binary star system Alpha Centauri AB. The two stars appear as a single star to the naked eye but can easily be resolved in smaller instruments. Their total mass is about 2 solar masses. With an absolute magnitude of +4.38, Alpha Centauri A is more luminous than Alpha Centauri B (+5.71).

alpha centauri a,alpha centauri b, toliman,rigil kentaurus
This NASA/ESA Hubble Space Telescope has given us this stunning view of the bright Alpha Centauri A (on the left) and Alpha Centauri B (on the right), shining like huge cosmic headlamps in the dark. The image was captured by the Wide-Field and Planetary Camera 2 (WFPC2). WFPC2 was Hubble’s most used instrument for the first 13 years of the space telescope’s life, being replaced in 2009 by Wide-Field Camera 3 (WFC3) during Servicing Mission 4. This portrait of Alpha Centauri was produced by observations carried out at optical and near-infrared wavelengths. Image: ESA/NASA (CC BY 2.0)

The two Sun-like stars are locked in a 79.91-year orbit with an eccentricity of 0.5179. Their orbit takes them within 11.2 astronomical units of each other and as far apart as 35.6 astronomical units. Their most recent closest approach (periastron) occurred in August 1955 and the next one will be in 2075. In 2019, the angular separation between the two stars was 4.92 arcseconds and it increased to 5.49 arcseconds in 2020. The observed apparent separation between the stars has been in the range from 1.7 arcseconds to 22 arcseconds. The maximum separation (apastron) was observed in 1976. The next apastron will be in January 2056.

Trajectory of Alpha Centauri B relative to A (fixed to the coordinate origin) as seen from the Earth (inclined ellipse) and face-on (horizontal ellipse). The orbit parameters are taken from Pourbaix et al. (2002). The graph has been created with gnuplot based on data generated by solving Kepler’s equation.
Note 1: The time stamps refer to the motion as seen from Earth, i.e. delayed with respect to the true motion by the travel of light by about 4.4 years. North is down, as usual in many astronomical charts.
Note 2: For simplicity, the points refer to steps of 1/80 of an orbit rather than to exact 1-year steps (which would be 1/79.91 of an orbit).
Note 3: The ascending node is the point where B (with respect to A) penetrates the celestial plane and becomes more distant to Earth than A. Image: Wikimedia Commons/SiriusB (CC BY-SA 3.0)

Since the naked eye can only resolve stars that are 60 or more arcseconds apart, the AB binary always appears as a single star. Most of the time, it can be resolved in binoculars and small telescopes.

This wide-field view of the sky around the bright star Alpha Centauri was created from photographic images forming part of the Digitized Sky Survey 2. The star appears so big just because of the scattering of light by the telescope’s optics as well as in the photographic emulsion. Image: ESO/DSS 2

Proxima Centauri orbits the main pair with a period of about 547,000 years (543,000 – 553,600 years) and an eccentricity of 0.50. While orbiting, it comes within 4,300 astronomical units (3,400 – 5,400 AU) of the main pair and gets as far away as 13,000 astronomical units (12,900 – 13,300 AU). Currently, the physical distance between the main pair and Proxima is about 0.21 light years, or 13,000 astronomical units. This is about 5% of the distance between the Sun and Alpha Centauri AB.

Orbital plot of Proxima Centauri showing its position with respect to Alpha Centauri over the coming millenia (graduations are in thousands of years). The large number of background stars is due to the fact that Proxima Cen is located very close to the plane of the Milky Way. Image: P. Kervella (CNRS/U. of Chile/Observatoire de Paris/LESIA), ESO/Digitized Sky Survey 2, D. De Martin/M. Zamani (CC BY 4.0)

With an apparent magnitude of 11.13, Proxima is invisible to the naked eye and does not appear in the immediate vicinity of Alpha Centauri AB. It lies 2.18 degrees southwest of the bright AB binary.

The two bright stars are (left) Alpha Centauri and (right) Beta Centauri, both binaries. The faint red star in the center of the red circle, at right angles to both and southwest of Alpha is Proxima Centauri, intensely red, smaller in size, weaker in brightness and a distant third element in a triple star system with the main close pair forming Alpha Centauri. Image: Wikimedia Commons/Skatebiker (CC BY-SA 3.0)

The Alpha Centauri star system is believed to be the same age or slightly older than the Sun (4.6 billion years). Estimates based on standard stellar models have yielded an age of 5.4 billion years for Alpha Centauri AB, while those based on asteroseismic observations and stellar parameters have yielded values of 4.85 ± 0.5, 5.0 ± 0.5, 5.2 ± 1.9, 6.4, and 6.52 ± 0.3 billion years. Gyrochronological methods have given an estimated age of 5.0 ± 0.3 billion years, and methods based on the stars’ chromospheric activity have yielded a value of 4.4 ± 2.1 billion years.

Alpha Centauri A

Rigil Kentaurus, the primary component in the system, is slightly larger and more massive than the Sun. Like the Sun, it is a main sequence star of the spectral type G2V and it exhibits coronal variability due to star spots coupled with the effect of rotation.

The star has a mass 1.1 times that of the Sun and a radius 1.2234 times solar. With an effective temperature of 5,790 K, it is 1.519 times more luminous than the Sun.

Rigil Kentaurus has an apparent magnitude of +0.01. Individually, it is the fourth brightest star in the sky, slightly outshining Vega (mag. +0.026), but fainter than Sirius (-1.46), Canopus (-0.74), and Arcturus (mag. -0.05). Various catalogues give slightly different values for the star. The Bright Star Catalogue and the Hipparchos and Tycho Catalogues (1997) list a visual magnitude of -0.01, while the Tycho-2 Catalogue gives a magnitude of +0.137, and the 2007 Hipparchos (the New Reduction) lists a value of +0.1373.

Alpha Centauri B

Toliman is smaller and less massive than Rigil Kentaurus. With the stellar classification of K1V, it appears more orange in colour. The star has a mass of 0.907 solar masses and a radius of 0.8632 solar radii. With a surface temperature of 5,260 K, it has only 50% of the Sun’s luminosity. It is about 5.3 billion years old, a little older than the Sun.

Even though it is not as luminous as Rigil Kentaurus, Toliman has a greater energy output in the X-ray band and dominates the system’s X-ray emission. A flare was discovered on the star in 2005.

Toliman has an apparent magnitude of +1.33. As a single star, it would be the third brightest star in Centaurus, fainter than Rigil Kentaurus and Hadar (mag. +0.61), but outshining Menkent (mag. +2.06). By itself, it would still be one of the brightest (first-magnitude) stars in the sky, slightly dimmer than Deneb (mag. +1.25) in Cygnus and Mimosa (mag. +1.25) in Crux, but brighter than Regulus (mag. +1.36) in Leo, Adhara (mag. +1.50) in Canis Major, and Castor (mag. +1.58) in Gemini.

Alpha Centauri C 

Proxima Centauri is the smallest of the three stars in the Alpha Centauri system. It is a red dwarf of the spectral type M5.5Ve. It has a mass of only 0.1221 solar masses and a radius of 0.1542 solar radii. With an effective temperature of 3,042 K, it shines with only 0.0017 solar luminosities. It is more than 20,000 times fainter than the Sun, with an absolute magnitude of +15.60.

This diagram illustrates, from left to right, the relative size of the Sun, α Centauri A, α Centauri B and Proxima Centauri. Image: Wikimedia Commons/RJHall (CC BY-SA 3.0)

With a visual magnitude of 11.13, Proxima is far too faint to be visible to the naked eye. Even from the Alpha Centauri AB system, it would only appear as a fifth magnitude star.

The star is classified as a UV Ceti variable, a flare star that shows sudden increases in brightness that last for only a few minutes. The increases in Proxima‘s brightness, up to magnitude 10.43, are caused by magnetic activity. The nearby red dwarf Wolf 359 also belongs to this group of variables. The prototype UV Ceti, also catalogued as Luyten 726-8B, is a red dwarf only 8.73 light years away. It is the most extreme example of this type of star. Its brightness has been observed to brighten by 75 times within only 20 seconds. The largest observed flares of Proxima occurred on August 13, 2015, when the star’s brightness increased 8.3 times in the B band.


The distance of Alpha Centauri AB is now believed to be 4.37 light years, or about 41.34 trillion kilometres, with a parallax of 754.81 ± 4.11 milliarcseconds. Proxima Centauri is slightly closer, at 4.244 light years.

Distance estimates for Alpha Centauri AB have varied somewhat over the last two centuries. In 1839, the Scottish astronomer Thomas Henderson calculated a distance of 2.57 ± 0.53 light years from a parallax of 1160 ± 110 milliarcseconds (mas). In 1842, he corrected the estimate to 3.34 ± 0.5 light years based on a parallax of 912.8 ± 64 mas.

In 1851, South African astronomer Thomas Maclear gave similar numbers – a distance of 3.55 light years with a parallax of 918.7 ± 34 mas. In 1868, German astronomer Karl Wilhelm Moesta calculated a distance of 3.71 light years from a parallax of 880 ± 68 mas. The most accurate early estimate came from Scottish astronomer David Gill and his American colleague William Lewis Elkin, who found a distance of 4.35 light years and a parallax of 750 ± 10 mas in 1885. A decade later, Scottish-born South African amateur astronomer Alexander W. Roberts calculated a distance of 4.29 light years from a parallax of 710 ± 50 mas.

In more recent times, Woolley et al. derived a distance of 4.39 light years from a parallax of 743 ± 7 mas in 1970 and van Altena et al. found a distance of 4.349 light years with a parallax of 749.9 ± 5.4 mas. Perryman et al. gave values of 4.395 light years and 742.12 ± 1.40 mas in 1997 and, in 1999, Swedish astronomer Staffan Söderhjelm calculated a distance of 4.366 light years with a parallax of 747.1 ± 1.2 mas.

In 2007, Floor van Leeuwen found a distance of 4.321 light years with a parallax of 754.81 ± 4.11 mas for Alpha Centauri A and 4.09 light years with a parallax of 796.92 ± 25.90 mas for Alpha Centauri B.


There are two confirmed planets in the Alpha Centauri system, both orbiting Proxima Centauri. Designated Proxima Centauri b (or Alpha Centauri Cb) and Proxima Centauri c (Alpha Centauri Cc), these are the nearest known exoplanets to the Sun. Proxima b is a terrestrial planet, while Proxima c is believed to be a super-Earth or mini-Neptune.

The discovery of Proxima b was announced in August 2016. The planet was detected by a team at the European Southern Observatory (ESO) using the radial velocity method. The planet has a mass of at least 1.17 Earth masses and a radius of about 1.07 Earth radii. It orbits the host star from a distance of 0.049 astronomical units and takes 11.186 days to complete an orbit. With an equilibrium temperature of -39° C (234 K), it is a bit colder than Earth (-18° C/255 K).

The distance places Proxima b in the habitable zone of Proxima Centauri, where liquid water may exist on the surface, but the planet’s proximity to the host star makes it subject to flares and stellar winds more than 2,000 times stronger than those experienced by Earth, which would likely erode any atmosphere on the planet.

The discovery of Proxima Centauri c was confirmed in 2020. The planet has a mass of about 7 Earth masses and orbits Proxima from a distance of about 1.49 astronomical units. It takes 1,928 days (5.28 years) to complete an orbit around the star. The planet may have a large ring system around it, detected in June 2020.

In addition to the planets orbiting Proxima, two planets have been reported around Toliman, Alpha Centauri B. In 2012, the discovery of Alpha Centauri Bb was announced, but the planet’s existence was disputed in 2015, when a more recent analysis showed that it most likely did not exist.

In 2013, another candidate exoplanet was detected around Alpha Centauri B. A possible transit event was observed that may correspond to a planet with a radius of about 0.92 Earth radii orbiting the star with a period of 20.4 days or less. If it exists, Alpha Centauri Bc is too close to its host star to harbour life.

There may be additional planets orbiting Rigil Kentaurus and Toliman, either the individual stars or the Alpha Centauri AB binary, but none have been confirmed yet. Even though the system is a frequent target for observations and planet hunting, none of the studies have found evidence for the existence of gas giants or brown dwarfs in the system. The habitable zone around Alpha Centauri A is between 1 and 2 astronomical units from the star and, to be in Alpha Centauri B’s habitable zone, a planet would need to have an orbital radius between 0.7 and 1.2 astronomical units.

Current estimates give a probability of finding a terrestrial planet in the star system of about 75%. A study published in 2009 found that planetesimal growth was only marginally possible in the innermost part of Toliman’s habitable zone, around 0.5 astronomical units from the star, because beyond this point the gravitational pull of the companion star would make planetesimal accretion impossible. However, binarity itself is not an obstacle to planet formation. More than 12% of all discovered exoplanets have been found in binary or multiple star systems.

In 2008, a theoretical study simulated the formation of planetary systems around Toliman and all simulations led to the formation of multiple planets, with at least one with a mass of 1-2 Earth masses orbiting at a distance of 0.5 to 1.5 astronomical units. The study suggested that a planet with 1.8 Earth masses could be reliably detected in the star’s habitable zone through radial velocity analysis.

Radial velocity measurements with the High Accuracy Radial Velocity Planet Searcher (HARPS) did not detect any planets in the habitable zone of Alpha Centauri B, even though the HARPS spectrograph has the sensitivity and precision to detect a planet with 4 Earth masses.

A study published in 2014 found slight excesses of emissions at 24 μm (in the mid/far-infrared band) for both Alpha Centauri A and B. This may indicate the presence of thin circumstellar discs or dense interplanetary dust. Debris discs orbiting main sequence stars can indicate the presence of larger bodies.

A 2018 study based on observations with NASA’s Chandra X-ray Observatory concluded that any planets orbiting Alpha Centauri A and B are probably not being bombarded with X-ray radiation to the point where life on the planets would be affected. In fact, any planets orbiting Alpha Centauri A would have better prospects of life than the planets orbiting the Sun. Those prospects would be slightly worse around Alpha Centauri B than around the Sun, but not bad enough to pose a threat to life on any planets orbiting the star. The Chandra observations have captured the X-ray activity in the system over more than a decade, including the period during the closest approach.


Rigil Kentaurus, Alpha Centauri A, is one of the 58 bright stars selected for use in navigation. It is one of three navigational stars in Centaurus constellation, along with Hadar (Beta Centauri) and Menkent (Theta Centauri). The three stars are among the 18 southern navigational stars with a declination between 30° S and 90° S. The group also includes Kaus Australis in Sagittarius, Shaula in Scorpius, Fomalhaut in Piscis Austrinus, Alnair in Grus, Peacock in Pavo, Acrux and Gacrux in Crux, Canopus, Miaplacidus and Avior in Carina, Atria in Triangulum Australe, Ankaa in Phoenix, Suhail in Vela, and Achernar and Acamar in Eridanus. Due to their location in the far southern sky, most of these stars are invisible to observers in mid-northern latitudes.

Alpha Centauri was mentioned in the Greek astronomer Ptolemy’s Almagest, a 2nd century star catalogue that also included the list of 48 Greek constellations. Ptolemy lived in Alexandria, Egypt (31° N), where the star was visible in his day. However, due to the Earth’s axial precession, Alpha Centauri now appears further south, at the declination -60° 51’, and it cannot be seen from locations north of the latitude 29° N.

Alpha and Beta Centauri from Paranal, image: John Colosimo/ESO (CC BY 4.0)

The southern luminaries Alpha Centauri, Canopus and Achernar were largely unknown to European observers until the English geographer, mathematician and explorer Robert Hues published his work Tractatus de globis et eorum usu (Treatise on Globes and Their Use) in 1594. Hues made observations of the Southern Cross and other bright southern stars from the South Atlantic, during a voyage with the English explorer Thomas Cavendish, and published his discoveries in Tractatus de globis. He described the positions of Canopus, Achernar and Alpha Centauri as “in the sterne of Argo” (Canopus), “in the end of Eridanus” (Achernar), and “in the right foote of the Centaure” (Alpha Centauri).

Alpha Centauri was one of the first binary star systems to be discovered. Father Jean Richaud, a Jesuit priest, resolved the two components from Pondicherry, India, in December 1689 while observing a comet. He noted, “On several occasions while looking at the comet through the 12-ft telescope I noticed at the feet of Centaur a most eastern and a more brilliant star, which was a double star, similar to the one at the feet of Crusade; the difference being that in the Crusade while looking through the telescope one star seemed particularly away from the other, whereas at the feet of Centaur, the two stars seemed to be practically touching each other, even though one could distinguish them easily.”

The high proper motion of the main pair was first reported by the British astronomer Manuel John Johnson, who observed the system from the island of Saint Helena in the South Atlantic Ocean. Johnson reported his findings to the Scottish astronomer Thomas Henderson at the Royal Observatory at the Cape of Good Hope in South Africa. Henderson made further observations of Alpha Centauri AB between April 1832 and May 1833 and determined the system’s parallax, concluding that the stars were relatively close. He used French astronomer Nicolas Louis de Lacaille’s observations made in 1751 and 1752 and compared the differences between the star system’s measured positions in the 1750s and 1830s. Even though the difference was considerable, Henderson withheld the results of his observations thinking that the values were too high to be accurate. He did not publish his findings until 1839, after the German astronomer and physicist Friedrich Wilhelm Bessel announced a parallax of 0.314 arcseconds for 61 Cygni, another nearby star (11.4 ly), in 1838. Even though Henderson measured the parallax of Alpha Centauri AB before Bessel, his work was not widely known at the time and it is 61 Cygni that is usually cited as the first star to have its parallax measured, as well as the first star to have its distance estimated.

Due to their proximity, the three stars in the Alpha Centauri system have a high proper motion (apparent motion across the background sky). The centre of mass of Alpha Centauri AB moves about 3620 milliarcseconds per year towards the west and 694 milliarcseconds per year towards the north. It moves about 6.1 arcminutes each century and 1.02 degrees each millennium. The system has a mean radial velocity of about 22.4 km/s in the direction of the Sun.

Even though it is the nearest star system to the Sun, Alpha Centauri does not have the highest proper motion measured of any star. The three stars with the largest proper motion are Barnard’s Star, the second nearest star (system) to Earth at 5.958 light years, Kapteyn’s Star, the nearest known galactic halo star at 12.76 light years, and Groombridge 1830 (Argelander’s Star), another halo star, located at a distance of 29.93 light years. 61 Cygni, Keid (Omicron2 Eridani) and Epsilon Indi are among other stars that have a higher proper motion than Alpha Centauri.

This diagram illustrates the locations of the star systems closest to the sun. The year when the distance to each system was determined is listed after the system’s name. Image: NASA/Penn State University

The high proper motion of Alpha Centauri will gradually take it to Hadar’s position, and around the year 6200 CE, the two stars will form a conjunction and shine as a visual double. Even though it lies at a much greater distance (390 light years), Hadar (Beta Centauri) is a first-magnitude star, the 11th brightest star in the sky, and the conjunction of the two exceptionally bright stars will be an extremely rare event. Alpha Centauri will then move north of the Southern Cross and the constellation Vela toward the celestial equator and across Hydra, where it will be found around the year 26,700 CE. In the year 27,000 CE, the star will make its closest approach to the Sun, coming within 2.9 light years. At perihelion, it will shine at magnitude -0.86, which is a little brighter than Canopus is today (-0.74). It will not, however, outshine Sirius, which will keep getting brighter and stay the brightest star in the Earth’s sky for the next 210,000 years.

Proxima Centauri was discovered in 1915 by the Scottish astronomer Robert T. A. Innes from the Union Observatory in South Africa. Innes used a 9-inch refractor and a 10-inch astrographic camera and found a star that had the same high proper motion as Alpha Centauri AB. He believed that the star was closer to the Sun than Alpha Centauri, which was already considered the nearest star system, and gave it the name Proxima. However, he could not measure the star’s distance accurately with his equipment. The distance of Proxima was definitively measured by the American astronomer Harold Lee Alden from the Yale observatory station in Johannesburg. Alden’s work confirmed that Proxima was indeed the nearest star to the Sun.

The orbital elements of Alpha Centauri AB were first calculated with some accuracy in 1926 by the South African astronomer William Stephen Finsen, who made his observations from the Union Observatory in South Africa, where Robert Innes had discovered Proxima Centauri over a decade earlier. Finsen gave an orbital period of 80.089 years with a major axis of 35.33 arcseconds. The currently accepted orbital period of 79.91 years is credited to Belgian astronomer Dimitri Pourbaix and his team, who derived the value from their observations at Université libre de Bruxelles in Belgium in 2002.

Alpha Centauri lies within the G-Cloud complex, a neighbouring interstellar cloud to the Local Interstellar Cloud. The Sun is believed to be either in the Local Interstellar Cloud or in the area between the two clouds, but it is moving towards the G-Cloud. The G-Cloud also contains Altair, the brightest star in the constellation Aquila and the 12th brightest star in the sky, located at a distance of 16.73 light years from the Sun.

The nearest star or star system to Alpha Centauri is not the Sun, but Luhman 16, a binary system composed of two brown dwarfs. Luhman 16 is located only 3.577 light years from Alpha Centauri AB, 3.520 light years from Proxima Centauri, and 6.516 light years from the Sun. The system does not appear very close to Alpha Centauri on the sky as it lies in the constellation Vela, south of Mu Velorum and north of the Carina Nebula in Carina. It is the third nearest star system to the Sun, after Alpha Centauri and Barnard’s Star, and its two components are the nearest known brown dwarfs.

An observer on a hypothetical planet in the Alpha Centauri system would see pretty much the same sky that observers on Earth see. However, they would see Centaurus without its brightest star. Alpha Centauri AB would appear as a close visual double that could be resolved by the naked eye most of the time. The two stars would have apparent magnitudes of -6.5 (Rigil Kentaurus) and -5.2 (Toliman). The Sun would appear as a first-magnitude star in the constellation Cassiopeia. At magnitude +0.47, it would be as bright from Alpha Centauri as Achernar is from Earth. It would appear in the same line of sight as the Heart Nebula, east of Segin (Epsilon Cassiopeiae), the leftmost star of Cassiopeia’s W, and it would give Cassiopeia’s W a /W shape.

The sky from Alpha Centauri, image: Wikimedia Commons/Skatebiker (CC BY-SA 3.0)

As the nearest star system to the Sun, Alpha Centauri is a target for several interstellar exploration missions that are still in concept stage and will likely remain so for the foreseeable future because the technology that would reduce travel time to the star system does not yet exist. The existing spacecraft would take several millennia to get there. In 2017, NASA introduced a project aiming to launch an interstellar probe by the year 2069 – on the 100th anniversary of the Moon landing – to search for biosignatures on planets in the system. Even though the mission concept is in the preliminary stage, the use of solar sails propelled by high energy lasers to reduce travel time has been suggested.

Solar sails are also the method of choice for the well-funded Breakthrough Starshot project, announced on April 12, 2016. The project was developed by the physicist and entrepreneur Yuri Milner, physicist Stephen Hawking, and internet entrepreneur Mark Zuckerberg, with the goal to develop a fleet of solar sail spacecraft that could be sent to the Alpha Centauri system. A flyby mission to Proxima Centauri b was proposed after the planet’s existence was confirmed in August 2016. In January 2017, Breakthrough Initiatives also started collaborating with the European Southern Observatory to search for planets in the habitable zones of the Alpha Centauri system. The Breakthrough Starshot concept would entail launching a mothership with about a thousand small, centimetre-sized spacecraft to high-altitude Earth orbit, then using ground-based (or space-based) lasers to focus a light beam on the crafts’ sails to accelerate them. The journey would take 20-30 years and a return message to Earth would take only about four years. The first craft may launch by the year 2036.

Alpha Centauri has played a prominent role in many cultures in the southern hemisphere. The Bushmen in South Africa called Alpha and Beta Centauri Two Men That Once Were Lions. In Australia, the Boorong people of northwest Victoria called the stars Bermbermgle, after two brothers known for their courage. In local lore, the brothers helped kill Tchingal, the Emu, represented by the nearby dark Coalsack Nebula. The Wotjobaluk people of Victoria had a similar legend and called the brothers Bram-bram-bult.

Alpha and Beta Centauri, the Coalsack Nebula and the Southern Cross, image: ESA/A. Fujii (CC BY 4.0)

Like many other bright and nearby stars, Alpha Centauri has been used in countless works of fiction, including literature, film and television, comic books, and video games. Notable uses in literature include a poem by Jan Neruda in the collection “Cosmic Songs” (1878), the short story “Proxima Centauri” (1935) by Murray Leinster, Isaac Asimov’s short story “Homo Sol” (1940), Larry Niven’s “Like Banquo’s Ghost” (1968), Frederick Pohl’s “The Gold at the Starbow’s End” (1972), and “Far Centaurus” (1944) by A. E. van Vogt, the novels Revolt on Alpha C (1955) by Robert Silverberg, Stanislaw Lem’s The Magellanic Cloud (1955), Gordon R. Dickson’s Childe Cycle (1959) series, Edmund Cooper’s Seed of Light (1959), Leigh Brackett’s Alpha Centauri or Die! (1963), Philip K. Dick’s Clans of the Alphane Moon (1964), Larry Niven’s The Man-Kzin Wars (1966), M. John Harrison’s The Centauri Device (1975), James P. Hogan’s Voyage from Yesteryear (1982), William Gibson’s Neuromancer (1984), Isaac Asimov’s Foundation and Earth (1986), Arthur C. Clarke’s The Songs of Distant Earth (1986), Poul Anderson’s Harvest of Stars (1994), Charles R. Pellegrino and George Zebrowski’s The Killing Star (1995), S. M. Stirling’s Drakon (1996), John Barnes and Buzz Aldrin’s Encounter with Tiber (1996), Mary Doria Russell’s The Sparrow (1996), Robert J. Sawyer’s Factoring Humanity (1998), Michael Ely’s Centauri Dawn (2000), Paul Levinson’s Borrowed Tides (2001), Liu Cixin’s Three Body (2008), Alastair Mayer’s Alpha Centauri trilogy (2016-17), and Kevin Emerson’s The Oceans Between Stars (2018).

Memorable uses and mentions in television include the series Lost in Space (1965-68), the episodes “Tomorrow is Yesterday” and “Metamorphosis” (1967) of Star Trek: The Original Series, the episode “Past Tense, Part 1” of Star Trek: Deep Space Nine, the serials “The Curse of Peladon” (1972) and “The Monster of Peladon” (1974) of Doctor Who, the episode “The Golden Man” (1981) of Buck Rogers in the 25th Century, and the episode “No Surrender, No Retreat” of Babylon 5.  In film, the star system was used in Event Horizon (1997), Lost in Space (1998), Impostor (2002), Hitchhiker’s Guide to the Galaxy (2005), Avatar (2009), and Princess of Mars (2012).


All three components of the Alpha Centauri system have formal names. The primary component, Alpha Centauri A, is called Rigil Kentaurus, Alpha Centauri B is also known as Toliman, and Alpha Centauri C has the formal name Proxima Centauri.

The name Rigil Kentaurus (pronunciation: /ˈraɪdʒəl kɛnˈtɔːrəs/) comes from the Arabic phrase Rijl al-Qinṭūrus, meaning “the foot of the Centaur.” It is the star’s traditional name and it refers to its position in the constellation. The name was approved by the International Astronomical Union’s (IAU) Working Group on Star Names (WGSN) on November 6, 2016. It has also been abbreviated to Rigil Kent or just Rigil. It shares the same etymology as Rigel (Beta Orionis), the name of the bright star that marks the foot of Orion.

The name Toliman (pronunciation: /ˈtɒlɪmæn/) comes from the Arabic aẓ-Ẓalīmān or aṭ-Ṭhalīmān, meaning “the (two male) ostriches.” It refers to an asterism, “the ostriches,” in which Alpha Centauri was the brightest star. The name was once colloquially used for the entire star system. The IAU approved it for Alpha Centauri B on August 10, 2018.

The name Proxima Centauri (pronunciation: /ˈprɒksɪmə sɛnˈtɔːraɪ/) comes from a suggestion made by the Scottish astronomer Robert T. A. Innes, who discovered the star in 1915 and proposed the name Proxima Centaurus, believing that the star was closer to us than Alpha Centauri AB. The name means “the nearest (star) of Centaurus.” The version with the genitive Centauri became widely used later and was approved by the IAU on August 21, 2016.

Alpha Centauri was known by many other names across different cultures throughout history. It was called Bungula (pronunciation: /ˈbʌŋɡjuːlə/), possibly derived from the letter β (beta) and the Latin ungula, meaning “hoof.”

Alpha and Beta Centauri (Hadar) are known as the Southern Pointers, or simply the Pointers in the southern hemisphere. The two stars point in the direction of the Southern Cross, a conspicuous southern asterism commonly used to find true south.

The Chinese know Alpha Centauri as 南門二 (Nán Mén Èr), the Second Star of the Southern Gate. The Chinese Southern Gate asterism is formed by Alpha Centauri with Epsilon Centauri. It is part of the Horn mansion, which represents the horns of the Azure Dragon.


Alpha Centauri is very easy to find. It lies near Hadar, the 11th brightest star in the sky, and the Southern Cross, a prominent southern asterism formed by the bright stars Acrux, Mimosa, Gacrux, Imai and Ginan in the constellation Crux.

how to find alpha centauri,where is alpha centauri in the sky
Alpha Centauri location, image: Wikisky

However, due to its location in the far southern sky, Alpha Centauri stays invisible to observers in mid-northern latitudes. Observers south of the latitude 29° S can see Alpha Centauri throughout the year because the star is circumpolar, i.e. it never sinks below the horizon. Observers north of the latitude 29° N, however, never see the star because it never rises above the horizon. Alpha Centauri can be seen from locations between the latitude 29° N and the equator, but only at certain times of the year and it always stays close to the southern horizon.

Alpha Centauri culminates, i.e. it reaches the highest point in the sky, at midnight on April 24 and around 9 pm on June 8.

Unlike the bright Alpha Centauri AB, Proxima Centauri is not very easy to find. The faint red dwarf lies 2.2 degrees – about four full Moons away – from the main pair. With an apparent magnitude of 11.1, it requires medium-sized telescopes to be seen.

This picture combines a view of the southern skies over the ESO 3.6-metre telescope at the La Silla Observatory in Chile with images of the stars Proxima Centauri (lower-right) and the double star Alpha Centauri AB (lower-left) from the NASA/ESA Hubble Space Telescope. Proxima Centauri is the closest star to the Solar System and is orbited by the planet Proxima b, which was discovered using the HARPS instrument on the ESO 3.6-metre telescope. Image: ESO, August 24, 2016. (CC BY 4.0)

Alpha and Beta Centauri are known as the Southern Pointers. They point the way to the Southern Cross, which is used to find the south celestial pole. A line drawn from Alpha through Beta Centauri leads to Gacrux, the top star of the Cross, which lies about 4.5 degrees to the west. Formed by two first-magnitude and one second-magnitude star, the Southern Cross is easy to find even without the Pointers, but the Centaurus stars help distinguish it from the False Cross, a similar asterism formed by Alsephina (Delta Velorum), Markeb (Kappa Velorum), Avior (Epsilon Carinae), and Aspidiske (Iota Carinae). The south celestial pole lies about halfway between the Southern Cross and Achernar, the ninth brightest star in the sky.

Alpha and Beta Centauri, the Southern Cross and the south celestial pole, image: Wikisky

Another way to locate the pole is to extend a line from Gacrux through Acrux and draw another line at a right angle to the line connecting the Pointers. The pole is near the point where the two lines cross.

Alpha Centauri can be used to find several deep sky objects that appear in the vicinity. The open clusters NGC 5617 and Trumpler 22 appear about a degree west-northwest of the star, in the direction of Hadar. The open cluster NGC 5606 lies north of NGC 5617, on the imaginary line connecting Alpha and Epsilon Centauri.

Alpha Centauri. Hadar, NGC 5617 and Trumpler 22, image: Wikisky


Alpha Centauri is located in the constellation Centaurus. The celestial Centaur has been known since ancient times and is one of the 48 Greek constellations, first listed by Claudius Ptolemy of Alexandria in his Almagest in the 2nd century CE. It is the ninth largest of all 88 constellations, occupying 1,060 square degrees of the southern sky. Centaurus is also one of the brightest constellations, containing 10 stars brighter than magnitude 3.00, including Alpha Centauri and Hadar (Beta Centauri), the third and 11th brightest stars in the sky. The constellation is also home to HR 5171 (V766 Centauri), one of the largest stars known.

centaurus stars
Centaurus constellation, image: Roberto Mura

Centaurus contains many interesting deep sky objects. These include Omega Centauri, the largest (36′.3), brightest (mag. 3.9) and most massive globular cluster known in the Milky Way, the starburst galaxy Centaurus A, one of the brightest galaxies in the sky (mag. 6.84), the spiral galaxies NGC 4945 and NGC 4622 (the Backward Galaxy), the irregular galaxy NGC 5253, a member of the Centaurus A/M83 Group, the elliptical galaxy NGC 4696, the brightest galaxy in the Centaurus Cluster, the polar-ring lenticular galaxy NGC 4650A, the open clusters NGC 3766 and NGC 5460, the protoplanetary nebula ESO 172-7, also known as the Boomerang Nebula, and the bright planetary nebula NGC 3918, also known as the Blue Planetary or the Southerner.

While it stays mostly invisible to northern observers, Centaurus is circumpolar in the southern hemisphere, i.e. it never falls below the horizon and can be seen throughout the year.

The best time of year to see the stars and deep sky objects in the constellation is during the month of May, when it rises high in the evening sky. The entire constellation is visible from locations between the latitudes 25° N and 90° S.

The 10 brightest stars in Centaurus are Alpha Centauri (mag. -0.27), Hadar (Beta Cen, mag. 0.61), Menkent (Theta Cen, mag. 2.06), Gamma Centauri (mag. 2.17), Epsilon Centauri (mag. 2.30), Eta Centauri (mag. 2.35), Zeta Centauri (mag. 2.55), Delta Centauri (mag. 2.57), Iota Centauri (mag. 2.73), and Lambda Centauri (mag. 3.13).

Alpha Centauri

Apparent magnitude-0.27
Parallax742 mas
Radial velocity-22.3 km/s
Proper motionRA: -3608 mas/yr
Dec.: 686 mas/yr
Right ascension14h 39m 29.71993s
Declination-60° 49’ 55.9990’’
Names and designationsAlpha Centauri, α Cen, FK5 538, GC 19728, GCRV 8519, CD−60°5483, GJ 559, SAO 252838, CCDM J14396-6050, RHD 1, LDS 494AB, IDS 14328-6025 AB, IRAS 14359-6037, LPM 534, WDS J14396-6050AB, WDS J14403-6051AB

Rigil Kentaurus – Alpha Centauri A

Spectral classG2V
U-B colour index+0.24
B-V colour index+0.71
Apparent magnitude0.01
Absolute magnitude4.38
Distance4.7 light years
Parallax743 ± 1.3 mas
Radial velocity−21.40 ± 0.76 km/s
Proper motionRA: −3679.25 mas/yr
Dec.: 473.67 mas/yr
Mass1.100 M
Luminosity1.519 L
Radius1.2234 ± 0.0053 R
Temperature5,790 K
Metallicity0.20 dex
Rotational velocity2.7 ± 0.7 km/s
Rotation22 ± 5.9 days
Surface gravity4.30 cgs
Right ascension14h 39m 36.49400s
Declination−60° 50′ 02.3737″
Names and designationsRigil Kentaurus, Rigil Kent, Alpha Centauri A, α Cen A, Alpha1 Centauri, HR 5459, HD 128620, HIP 71683, LHS 50, PLX 3309.00, GCRV 8517, LFT 1127, LTT 5806, NLTT 37984, PPM 360911, TYC 9007-5849-1

Toliman – Alpha Centauri B

Spectral classK1V
U-B colour index+0.68
B-V colour index+0.88
Apparent magnitude1.33
Absolute magnitude5.71
Distance4.37 light years
Parallax743 ± 1.3 mas
Radial velocity-22.586 ± 0.0001 km/s
Proper motionRA: −3614.39 mas/yr
Dec.: 802.98 mas/yr
Mass0.907 M
Luminosity0.5002 L
Radius0.8632 ± 0.0037 R
Temperature5,260 K
Metallicity0.23 dex
Age5.3 ± 0.3 billion years
Rotational velocity1.1 ± 0.8 km/s
Rotation36 days
Surface gravity4.37 cgs
Right ascension14h 39m 35.06311
Declination−60° 50′ 15.0992″
Names and designationsToliman, Alpha Centauri B, α Cen B, Alpha2 Centauri, HD 128621, HR 5460, HIP 71681, LHS 51, GCRV 8518, LFT 1128, LTT 5807, NLTT 37985, TYC 9007-5848-1

Proxima Centauri – Alpha Centauri C

Spectral classM5.5Ve
Variable typeUV Ceti
U-B colour index1.26
B-V colour index1.82
V-R colour index1.68
R-I colour index2.04
J-H colour index0.522
J-K colour index0.973
Apparent magnitude (V)10.43 – 11.11
Apparent magnitude (U)14.21
Apparent magnitude (B)12.95
Apparent magnitude (V)11.13
Apparent magnitude (R)9.45
Apparent magnitude (I)7.41
Apparent magnitude (J)5.357 ± 0.023
Apparent magnitude (H)4.835 ± 0.057
Apparent magnitude (K)4.384 ± 0.033
Absolute magnitude15.60
Distance4.244 ± 0.001 light years (1.3012 ± 0.0003 parsecs)
Parallax768.5004 ± 0.2030 mas
Radial velocity−22.204 ± 0.032 km/s
Proper motionRA: −3781.306 mas/yr
Dec.: 769.766 mas/yr
Mass0.1221 ± 0.0022 M
Luminosity (bolometric)0.0017 L
Luminosity (visual, LV)0.00005 L
Radius0.1542 ± 0.0045 R
Temperature3,042 ± 117 K
Metallicity0.21 dex
Age4.85 billion years
Rotational velocity< 0.1 km/s
Rotation82.6 ± 0.1 days
Surface gravity5.20 ± 0.23 cgs
Right ascension14h 29m 42.9451234609s
Declination−62° 40′ 46.170818907″
Names and designationsProxima Centauri, Alpha Centauri C, α Cen C, V645 Centauri, HIP 70890, GJ 551, LTT 5721, NLTT 37460, PLX 3278.00, CCDM J14396-6050C, LPM 526, LHS 49, LFT 1110, IRAS 14260-6227, 2MASS J14294291-6240465, Gaia DR2 5853498713160606720