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Epoch J2000.0 Equinox J2000.0
|Alpha Centauri A|
|Right ascension||14h 39m 36.49400s|
|Declination||–60° 50′ 02.3737″|
|Apparent magnitude (V)||+0.01|
|Alpha Centauri B|
|Right ascension||14h 39m 35.06311s|
|Declination||–60° 50′ 15.0992″|
|Apparent magnitude (V)||+1.33|
|U−B colour index||+0.24|
|B−V colour index||+0.71|
|U−B colour index||+0.68|
|B−V colour index||+0.88|
|Radial velocity (Rv)||−21.4±0.76 km/s|
|Proper motion (μ)|| RA: −3679.25 mas/yr |
Dec.: 473.67 mas/yr
|Parallax (π)||754.81 ± 4.11 mas|
|Absolute magnitude (MV)||4.38|
|Radial velocity (Rv)||−18.6±1.64 km/s|
|Proper motion (μ)|| RA: −3614.39 mas/yr |
Dec.: 802.98 mas/yr
|Parallax (π)||754.81 ± 4.11 mas|
|Absolute magnitude (MV)||5.71|
|Alpha Centauri A|
|Surface gravity (log g)||4.30 cgs|
|Metallicity [Fe/H]||0.20 dex|
|Alpha Centauri B|
|Surface gravity (log g)||4.37 cgs|
|Period (P)||79.91±0.011 yr|
|Semi-major axis (a)||17.57±0.022″|
|Longitude of the node (Ω)||204.85±0.084°|
|Periastron epoch (T)||1875.66±0.012|
|Argument of periastron (ω)|
Toliman, Bungula, 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: α2 Centauri, HR 5460, HD 128621, LHS 51, HIP 71681|
Alpha Centauri (α Centauri, abbreviated Alf Cen or α Cen) is the star system closest to the Solar System, being 4.37 light-years (1.34 pc) from the Sun. It consists of three stars: Alpha Centauri A (also named Rigil Kentaurus) and Alpha Centauri B, which form the binary star Alpha Centauri AB, and a small and faint red dwarf, Alpha Centauri C (also named Proxima Centauri), which is loosely gravitationally bound and orbiting the other two at a current distance of about 13,000 astronomical units (0.21 ly). To the unaided eye, the two main components appear as a single point of light with an apparent magnitude of −0.27, forming the brightest star in the southern constellation of Centaurus and is the third-brightest star in the night sky, outshone only by Sirius and Canopus.
Alpha Centauri A (α Cen A) has 1.1 times the mass and 1.519 times the luminosity of the Sun, while Alpha Centauri B (α Cen B) is smaller and cooler, at 0.907 times the Sun's mass and 0.445 times its luminosity. During the pair's 79.91-year orbit about a common centre, the distance between them varies from nearly that between Pluto and the Sun (35.6 AU) to that between Saturn and the Sun (11.2 AU).
Proxima Centauri (α Cen C) is at the slightly smaller distance of 4.24 light-years (1.30 pc) from the Sun, making it the closest star to the Sun, even though it is not visible to the naked eye. The separation of Proxima from Alpha Centauri AB is about 13,000 astronomical units (0.21 ly), equivalent to about 430 times the size of Neptune's orbit. Proxima Centauri b, an Earth-sized exoplanet in the habitable zone of Proxima Centauri, was discovered in 2016.
- 1 Nomenclature
- 2 Nature and components
- 3 Observation
- 4 Observational history
- 5 Binary system
- 6 Kinematics
- 7 Planets
- 8 View from this system
- 9 Other names
- 10 Exploration
- 11 Distance
- 12 See also
- 13 Notes
- 14 References
- 15 External links
- 15.1 Hypothetical planets or exploration
- 15.2 Article(s) of the same category(ies)
- 15.3 Article(s) of the same category(ies)
- 15.4 Article(s) of the same category(ies)
- 15.5 Article(s) of the same category(ies)
- 15.6 Article(s) of the same category(ies)
- 15.7 Article(s) of the same category(ies)
- 15.8 Article(s) of the same category(ies)
- 15.9 Article(s) of the same category(ies)
- 15.10 Article(s) of the same category(ies)
- 15.11 Article(s) of the same category(ies)
α Centauri (Latinised to Alpha Centauri) is the system's Bayer designation. It bore the traditional name Rigil Kentaurus, which is a latinisation of the Arabic name رجل القنطورس Rijl al-Qanṭūris, meaning "Foot of the Centaur".
Alpha Centauri C was discovered in 1915 by the Scottish astronomer Robert T. A. Innes, who suggested that it be named Proxima Centauri (actually Proxima Centaurus).[clarification needed] The name is from Latin, meaning 'nearest [star] of Centaurus'.
In 2016, the International Astronomical Union organised a Working Group on Star Names (WGSN) to catalog and standardise proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. The WGSN approved the name Proxima Centauri for Alpha Centauri C on 21 August 2016 and the name Rigil Kentaurus for Alpha Centauri A on 6 November 2016. They are now both so included in the List of IAU-approved Star Names.
Nature and components
Alpha Centauri is the designation given to what appears as a single star to the naked eye and the brightest star in the southern constellation of Centaurus. At −0.27 apparent magnitude (calculated from A and B magnitudes), it is fainter only than Sirius and Canopus. The next-brightest star in the night sky is Arcturus. Alpha Centauri is a multiple-star system, with its two main stars being Alpha Centauri A (α Cen A) and Alpha Centauri B (α Cen B), usually defined to identify them as the different components of the binary α Cen AB. A third companion—Proxima Centauri (or Proxima or α Cen C)—is much further away than the distance between stars A and B, but is still gravitationally associated with the AB system. As viewed from Earth, it has an angular separation of 2.2° from the two main stars. Proxima Centauri would appear to the naked eye as a separate star from α Cen AB if it were bright enough to be seen without a telescope. Alpha Centauri AB and Proxima Centauri form a visual double star. Together, the three components make a triple star system, referred to by double-star observers as the triple star (or multiple star), α Cen AB-C.
Together, the bright visible components of the binary star system are called Alpha Centauri AB (α Cen AB). This "AB" designation denotes the apparent gravitational centre of the main binary system relative to other companion star(s) in any multiple star system. "AB-C" refers to the orbit of Proxima around the central binary, being the distance between the centre of gravity and the outlying companion. Some older references use the confusing and now discontinued designation of A×B. Because the distance between the Sun and Alpha Centauri AB does not differ significantly from either star, gravitationally this binary system is considered as if it were one object.
Asteroseismic studies, chromospheric activity, and stellar rotation (gyrochronology) are all consistent with the α Cen system being similar in age to, or slightly older than, the Sun, with typical ages quoted between 4.5 and 7 billion years (Gyr). Asteroseismic analyses that incorporate the tight observational constraints on the stellar parameters for α Cen A and/or B have yielded age estimates of 4.85±0.5 Gyr, 5.0±0.5 Gyr, 5.2–7.1 Gyr, 6.4 Gyr, and 6.52±0.3 Gyr. Age estimates for stars A and B based on chromospheric activity (Calcium H & K emission) yield 4.4–6.5 Gyr, whereas gyrochronology yields 5.0±0.3 Gyr.
Alpha Centauri A
Alpha Centauri A is the principal member, or primary, of the binary system, being slightly larger and more luminous than the Sun. It is a solar-like main-sequence star with a similar yellowish colour, whose stellar classification is spectral type G2 V. From the determined mutual orbital parameters, Alpha Centauri A is about 10 percent more massive than the Sun, with a radius about 22 percent larger. The projected rotational velocity ( v·sin i ) of this star is 2.7±0.7 km/s, resulting in an estimated rotational period of 22 days, which gives it a slightly faster rotational period than the Sun's 25 days. When considered among the individual brightest stars in the sky (excluding the Sun), Alpha Centauri A is the fourth brightest at an apparent magnitude of +0.01, being fractionally fainter than Arcturus at an apparent magnitude of −0.04.
Alpha Centauri B
Alpha Centauri B is the companion star, or secondary, of the binary system, and is slightly smaller and less luminous than the Sun. It is a main-sequence star of spectral type K1 V, making it more an orange colour than the primary star. Alpha Centauri B is about 90 percent the mass of the Sun and 14 percent smaller in radius. The projected rotational velocity ( v·sin i ) is 1.1±0.8 km/s, resulting in an estimated rotational period of 41 days. (An earlier, 1995 estimate gave a similar rotation period of 36.8 days.) Although it has a lower luminosity than component A, star B emits more energy in the X-ray band. The light curve of B varies on a short time scale and there has been at least one observed flare. Alpha Centauri B at an apparent magnitude of 1.33 would be twenty-first in brightness if it could be seen independently of Alpha Centauri A.
Alpha Centauri C (Proxima Centauri)
Alpha Centauri C, also known as Proxima Centauri, is a red dwarf of spectral class M6 Ve, a small main-sequence star (Type V) with emission lines. Its B−V colour index is +1.82. It has an absolute magnitude of +15.60, which is only a small fraction of the Sun's luminosity. By mass, Proxima is calculated as 0.123±0.06 M☉ (rounded to 0.12 M☉) or about one-eighth that of the Sun.
Alpha Centauri C is about 13,000 astronomical units (AU) away from Alpha Centauri AB. This is equivalent to 0.21 ly or 1.9 trillion km—about 5% the distance between Alpha Centauri AB and the Sun. Due to the large distance between Proxima and Alpha, it was long unknown whether they were gravitationally bound. Estimating its small orbital speed required precise measurement of the speeds of Proxima and Alpha. Otherwise it was impossible to ascertain whether Proxima is bound to Alpha or a completely unrelated star that happens to be undergoing a close approach at a low relative speed.
It was only in 2017 that precision radial velocity measurements showed, with a high degree of confidence, that Proxima and Alpha Centauri are gravitationally bound. The orbital period of Proxima is approximately 550,000 years, with an eccentricity of 0.50+0.08
−0.09. Proxima comes within 4300+1100
−900 AU of Alpha Centauri AB at periastron, and the apastron occurs at 13000+300
The two stars of the binary Alpha Centauri AB are too close together to be resolved by the naked eye. Their apparent angular separation varies over about 80 years between 2 and 22 arcsec (the naked eye has a resolution of 60 arcsec), but through much of the orbit, both are easily resolved in binoculars or small telescopes.
Alpha Centauri forms the outer star of The Pointers or The Southern Pointers, so called because the line through Beta Centauri (Hadar/Agena), some 4.5° west, points directly to the constellation Crux—the Southern Cross. The Pointers easily distinguish the true Southern Cross from the fainter asterism known as the False Cross.
South of about 29° S latitude, Alpha Centauri is circumpolar and never sets below the horizon. Both stars and Crux are too far south to be visible for mid-latitude northern observers. Below about 29° N latitude to the equator (roughly Hermosillo, Chihuahua City in Mexico, Galveston, Texas, Ocala, Florida and Lanzarote, the Canary Islands of Spain) during the northern summer, Alpha Centauri lies close to the southern horizon. The star culminates each year at midnight on 24 April or 9 p.m. on 8 June.
As seen from Earth, Proxima Centauri is 2.2° southwest from Alpha Centauri AB. This is about four times the angular diameter of the Full Moon, and almost exactly half the distance between Alpha Centauri AB and Beta Centauri. Proxima appears as a deep-red star of an apparent magnitude of 11.1 in a sparsely populated star field, requiring moderately sized telescopes to see. Listed as V645 Cen in the General Catalogue of Variable Stars (G.C.V.S.) Version 4.2, this UV Ceti-type flare star can unexpectedly brighten rapidly by as much as 0.6 magnitudes at visual wavelengths, then fade after only a few minutes. Some amateur and professional astronomers regularly monitor for outbursts using either optical or radio telescopes. 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).
Alpha Centauri was listed in the 2nd-century star catalog of Ptolemy. He gave the ecliptic coordinates, but texts differ as to whether the ecliptic latitude reads 44° 10′ South or 41° 10′ South. (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 his city of 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. The second is in the end of Eridanus. The third [Alpha Centauri] is in the right foote of the Centaure."
The binary nature of Alpha Centauri AB was first recognised in December 1689 by astronomer and Jesuit priest Jean Richaud. The finding was made incidentally while observing a passing comet from his station in Puducherry. Alpha Centauri was only the second binary star system to be discovered, preceded by Alpha Crucis.
By 1752, French astronomer Nicolas Louis de Lacaille made astrometric positional measurements using state-of-the-art instruments of that time. Its large proper motion 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 Friedrich Wilhelm Bessel released his own accurately determined parallax for 61 Cygni in 1838. 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. (The distance of Alpha is now reckoned at 4.396 ly or 41.59 trillion km.)
By 1926, South African astronomer William Stephen Finsen calculated the approximate orbit elements close to those now accepted for this system. All future positions are now sufficiently accurate for visual observers to determine the relative places of the stars from a binary star ephemeris. Others, like the Belgian astronomer D. Pourbaix (2002), have regularly refined the precision of new published orbital elements.
Alpha Centauri is inside the G-cloud, and the nearest known system to it is the binary brown dwarf system Luhman 16 at 3.6 ly (1.1 pc).
Robert T. A. Innes discovered Proxima Centauri in 1915 by blinking photographic plates taken at different times during a dedicated proper motion survey. This showed the large proper motion and parallax of the star was similar in both size and direction to those of Alpha Centauri AB, suggesting immediately it was part of the system and slightly closer to Earth than Alpha Centauri AB. Lying 4.24 ly (1.30 pc) away, Proxima Centauri is the nearest star to the Sun. All current derived distances for the three stars are from the parallaxes obtained from the Hipparcos star catalogue (HIP) and the Hubble Space Telescope.
With the orbital period of 79.91 years, the A and B components of Alpha Centauri can approach each other to 11.2 AU (1.68 billion km), or about the mean distance between the Sun and Saturn; and may recede as far as 35.6 AU (5.33 billion km), approximately the distance from the Sun to Pluto. This is a consequence of the binary's moderate orbital eccentricity e = 0.5179. From the orbital elements, the total mass of both stars is about 2.0 M☉—or twice that of the Sun. The average individual stellar masses are 1.09 M☉ and 0.90 M☉, respectively, though slightly higher masses have been quoted in recent years, such as 1.14 M☉ and 0.92 M☉, or totalling 2.06 M☉. Alpha Centauri A and B have absolute magnitudes of +4.38 and +5.71, respectively. Stellar evolution theory implies both stars are slightly older than the Sun at 5 to 6 billion years, as derived by both mass and their spectral characteristics.
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 2010 are separated by 6.74 arcsec through the PA of 245.7°, reducing to 6.04 arcsec through 251.8° in 2011. The closest recent approach was in February 2016, at 4.0 arcsec through 300°. The observed maximum separation of these stars is about 22 arcsec, while the minimum distance is 1.7 arcsec. The widest separation occurred during February 1976 and the next will be in January 2056.
In the true orbit, closest approach or periastron was in August 1955, and next in May 2035. Furthest orbital separation at apastron last occurred in May 1995 and the next will be in 2075. The apparent distance between the two stars is rapidly decreasing, at least until 2019.
All components of Alpha Centauri display significant proper motions against the background sky, similar to the first-magnitude stars Sirius and Arcturus. Over the centuries, this causes the apparent stellar positions to slowly change. Such motions define the high-proper-motion stars. These stellar motions were unknown to ancient astronomers. Most assumed that all stars were immortal and permanently fixed on the celestial sphere, as stated in the works of the philosopher Aristotle.
Edmond Halley in 1718 found that some stars had significantly moved from their ancient astrometric positions. For example, the bright star Arcturus (α Boo) in the constellation of Boötes showed an almost 0.5° difference in 1800 years, as did the brightest star, Sirius, in Canis Major (α CMa). Halley's positional comparison was Ptolemy's catalogue of stars contained in the Almagest whose original data included portions from an earlier catalogue by Hipparchos during the 1st century BCE. Halley's proper motions were mostly for northern stars, so the southern star Alpha Centauri was not determined until the early 19th century.
Scottish-born observer Thomas Henderson in the 1830s at the Royal Observatory at the Cape of Good Hope discovered the true distance to Alpha Centauri by analysing his many astrometric mural circle observations. He then realised this system also likely had a high proper motion. In this case, the apparent stellar motion was found using Nicolas Louis de Lacaille's astrometric observations of 1751–1752, by the observed differences between the two measured positions in different epochs.
The proper motion of the centre of mass of Alpha Centauri is about 3620 mas (milli-arcseconds 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. The motion of the center of mass is about 6.1 arcmin each century, or 1.02° each millennium. These motions are about one-fifth and twice, respectively, the diameter of the full Moon. The velocity in the western direction is 23.0 km/s and in the northerly direction 4.4 km/s. Using spectroscopy the mean radial velocity has been determined to be around 22.4 km/s towards the Solar System.
Since α Centauri A and B are almost exactly in the plane of the Milky Way as viewed from here, there are many stars behind them. In early May, 2028, α Centauri A will pass between us and a distant red star. There is a 45% probability that an Einstein ring may be observed. Other near conjunctions will also happen in the coming decades. These will allow accurate measurements of the proper motions of the components and may give information on planets.
Predicted future changes
As the stars of Alpha Centauri approach the Solar System, measured common proper motions and trigonometric parallaxes slowly increase. These small effects will change until the star system becomes closest to Earth, and begin reversing as the distance increases again. Furthermore, other small changes also occur with the binary star's orbital elements. For example, in the size of the semi-major axis of the orbital ellipse will increasing by 0.03 arcsec per century. Also the observed position angles of the stars are also subject to small cumulative changes (additional to position angle changes caused by the Precession of the Equinoxes), as first determined by W. H. van den Bos in 1926.
Based on knowing these common proper motions and radial velocities, Alpha Centauri will continue to gradually brighten, passing 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 29,700 AD, in the present-day constellation of Hydra, Alpha Centauri will be 1.00 pc or 3.3 ly away., though later calculations suggest 0.90 pc or 2.9 ly in 29,000 AD. Then it will reach the stationary radial velocity (RVel) of 0.0 km/s and the maximum apparent magnitude of −0.86v (which is comparable to present-day magnitude of Canopus). Even during the time of this nearest approach, however, the apparent magnitude of Alpha Centauri 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 for the next 210,000 years.
About 28,000 years from now, the Alpha Centauri system will then begin to move away from the Solar System, showing a positive radial velocity. Because of visual perspective, these stars will reach a final vanishing point and slowly disappear among the countless stars of the Milky Way.
Viewed from the Earth in about AD 6200 Alpha Centauri will appear only about 43 arcmin (or one and a half diameters of the Moon) north of Beta Centauri. This will form a brilliant feature in the southern sky. Such a close approach of two first-magnitude stars will not occur again for a long time. Beta Centauri is in reality far more distant than Alpha Centauri.
Proxima Centauri b
In August 2016, the European Southern Observatory announced the discovery of a planet slightly larger than the Earth orbiting Proxima Centauri. Proxima Centauri b was found using the radial velocity method, where periodic Doppler shifts of spectral lines of the host star suggest an orbiting object. From these readings, the radial velocity of the parent star relative to the Earth is varying with an amplitude of about 2 metres (6.6 ft) per second. The planet lies in the habitable zone of Proxima Centauri, but it is possible that the planet is tidally locked to the star, resulting in temperature extremes that would be difficult for life to overcome.
Alpha Centauri Bb & Bc
In 2012, a planet around Alpha Centauri B was announced, but in 2015 a new analysis concluded that it almost certainly does not exist and was just a spurious artefact of the data analysis.
The existence of Alpha Centauri Bc was announced in 2013. It has an estimated orbital period of approximately 12 Earth days – smaller than that of Mercury – with a semimajor axis of 0.10 AU and an eccentricity smaller than 0.24.
Possible detection of another planet
On 25 March 2015, transit results for Alpha Centauri B obtained using the Hubble Space Telescope were published. They evidenced a transit event possibly corresponding to a planetary body 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 percent chance of it having a longer orbit. The median average of the likely orbits is 12.4 days with an impact parameter of around 0–0.3. Its orbit would likely have an eccentricity of 0.24 or less. Like the probably spurious Alpha Centauri Bb, it likely has lakes of molten lava and would be far too close to Alpha Centauri B to harbour life.
Possibility of additional planets
The discovery of planets orbiting other star systems, including similar binary systems (Gamma Cephei), raises the possibility that additional planets may exist in the Alpha Centauri system. Such planets could orbit Alpha Centauri A or Alpha Centauri B individually, or be on large orbits around the Alpha Centauri AB. Because both the principal 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. All the observational studies have so far failed to find evidence for brown dwarfs or gas giants.
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 to 0.9 AU from the star. Certain special assumptions, such as considering that Alpha Centauri A and B 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. Bodies around A would be able to orbit at slightly farther distances due to A's stronger gravity. In addition, the lack of any brown dwarfs or gas giants in close orbits around A or B make the likelihood of terrestrial planets greater than otherwise. Theoretical studies on the detectability via radial velocity analysis have shown that a campaign of high-cadence observations with a 1-meter class telescope could detect a hypothetical planet of 1.8 M⊕ in the habitable zone of B within three years.
Radial velocity measurements of Alpha Centauri B with High Accuracy Radial Velocity Planet Searcher spectrograph ruled out planets of more than 4 M⊕ to the distance of the habitable zone of the star (orbital period P = 200 days).
Current estimates place the probability of finding an earth-like planet around Alpha Centauri A or B at roughly 85%. The observational thresholds for planet detection in the habitable zones via the radial velocity method are currently (2017) estimated to be about 50 M⊕ for Alpha Centauri A, 8 M⊕ for B, and 0.5 M⊕ for Proxima.
Early computer-generated models of planetary formation predicted the existence of terrestrial planets around both Alpha Centauri A and B, but most recent numerical investigations have shown that the gravitational pull of the companion star renders the accretion of planets difficult. 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.
In the Solar System both Jupiter and Saturn were probably crucial in perturbing comets into the inner Solar System. Here, the comets provided the inner planets with their own source of water and various other ices. In the Alpha Centauri system, Proxima Centauri may have influenced the planetary disk as the Alpha Centauri system was forming, enriching the area around Alpha Centauri A and B with volatile materials. This would be discounted if, for example, Alpha Centauri B happened to have gas giants orbiting Alpha Centauri A (or conversely, Alpha Centauri A for Alpha Centauri B), or if the stars B and A themselves were able to perturb comets into each other's inner system as Jupiter and Saturn presumably have done in the Solar System. 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 starwards. Such ideas also apply to the close approach of Alpha Centauri or other stars to the Solar System, when in the distant future of our Oort Cloud may be disrupted enough to see increased numbers of active comets.
To be in the habitable zone, a planet around Alpha Centauri A would have an orbital radius of about 1.25 AU away  so as to have similar planetary temperatures and conditions for liquid water to exist. For the slightly less luminous and cooler Alpha Centauri B, the habitable zone is closer at about 0.7 AU (100 million km).
With the goal of finding evidence of such planets, both Proxima Centauri and Alpha Centauri AB were among the listed "Tier 1" target stars for NASA's Space Interferometry Mission (SIM). Detecting planets as small as three Earth-masses or smaller within two astronomical units of a "Tier 1" target would have been possible with this new instrument. The SIM mission, however, was cancelled due to financial issues in 2010.
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. 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. 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. This would put A's disc entirely within the frost line, and a small part of B's outer disc just outside.
View from this system
Viewed from near the Alpha Centauri system, the sky would appear much as it does for an observer on Earth, except that Centaurus would be missing its brightest star. The Sun would be a yellow star of an apparent magnitude of +0.5 in eastern Cassiopeia, at the antipodal point of Alpha Centauri's current right ascension and declination, at 02h 39m 35s +60° 50′ (2000). This place is close to the 3.4-magnitude star ε Cassiopeiae. Because of the placement of the Sun, an interstellar or alien observer would find the \/\/ of Cassiopeia had become a /\/\/ shape[note 1] nearly in front of the Heart Nebula in Cassiopeia. Sirius lies less than a degree from Betelgeuse in the otherwise unmodified Orion and with a magnitude of −1.2 is a little fainter than from Earth but still the brightest star in the Alpha Centauri sky. Procyon is also displaced into the middle of Gemini, outshining Pollux, whereas both Vega and Altair are shifted northwestward relative to Deneb (which barely moves, due to its great distance), giving the Summer Triangle a more equilateral appearance.
From Proxima Centauri b
From Proxima Centauri b, Alpha Centauri AB would appear like two close bright stars with the combined apparent magnitude of −6.8. Depending on the binary's orbital position, the bright stars would appear noticeably divisible to the naked eye, or occasionally, but briefly, as a single unresolved star. Based on the calculated absolute magnitudes, the apparent magnitudes of Alpha Centauri A and B would be −6.5 and −5.2, respectively.
Rigil Kent is short for Rigil Kentaurus, which is sometimes further abbreviated to Rigil or Rigel, though that is ambiguous with Beta Orionis, which is also called Rigel. Although the short form Rigel Kent is often cited as an alternative name, the star system is most widely referred to by its Bayer designation Alpha Centauri.
The name Toliman originates with Jacobus Golius' edition of Al-Farghani's Compendium (published posthumously in 1669). 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.
Together, Alpha and Beta Centauri form the "Southern Pointers" or "The Pointers", as they point towards the Southern Cross, the asterism of the constellation of Crux.
In Standard Mandarin Chinese, 南門 Nán Mén, meaning Southern Gate, refers to an asterism consisting of α Centauri and ε Centauri. Consequently, α Centauri itself is known as 南門二 Nán Mén Èr, the Second Star of the Southern Gate.
To the Australian aboriginal Boorong people of northwestern Victoria, Alpha and Beta Centauri are Bermbermgle, two brothers noted for their courage and destructiveness, who speared and killed Tchingal "The Emu" (the Coalsack Nebula). The form in Wotjobaluk is Bram-bram-bult.
Alpha Centauri is a likely first target for manned or unmanned 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 reduce the journey time to decades.
Breakthrough Starshot is a proof-of-concept initiative to send a fleet of ultra-fast light-driven nanocraft to explore the Alpha Centauri system, which could pave the way for a first launch within the next generation. An objective of the mission would be to make a fly-by of, and possibly photograph, planets that might exist in the system. Proxima Centauri b, announced by the European Southern Observatory (ESO) in August 2016, would be a target for the Starshot program.
In January 2017, Breakthrough Initiatives and the ESO entered a collaboration to search for habitable planets in the Alpha Centauri system. The agreement involves Breakthrough Initiatives providing funding for an upgrade to the VISIR (VLT Imager and Spectrometer for mid-Infrared) instrument on ESO's Very Large Telescope (VLT) in Chile. This upgrade will greatly increase the likelihood of planet detection in the system.
|Source||Parallax, mas||Distance, pc||Distance, ly||Distance, Pm||Ref.|
|Gill & Elkin (1885)||750±10||1.333±0.018||4.35±0.06||41.1+0.6
|Woolley et al. (1970)||743±7||1.346±0.013||4.39±0.04||41.5±0.4|||
|Gliese & Jahreiß (1991)||749.0±4.7||1.335±0.008||4.355±0.027||41.20±0.26|||
|van Altena et al. (1995)||749.9±5.4||1.334±0.010||4.349+0.032
|Perryman et al. (1997) (A and B)||742.12±1.40||1.3475±0.0025||4.395±0.008||41.58±0.08|||
|van Leeuwen (2007) (A)||754.81±4.11||1.325±0.007||4.321+0.024
|van Leeuwen (2007) (B)||796.92±25.90||1.25±0.04||4.09+0.14
|RECONS TOP100 (2012)||747.23±1.17[note 3]||1.3383±0.0021||4.365±0.007||41.29±0.06|||
- Alpha Centauri in fiction
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