| |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Capricornus |
| Right ascension | 20h18m 03.25595s[1] |
| Declination | −12° 32′ 41.4684″[1] |
| Apparent magnitude (V) | +3.57[2] |
| Characteristics | |
| Spectral type | G8.5III-IV[3] |
| U−B color index | +0.69[2] |
| B−V color index | +0.94[2] |
| Astrometry | |
| Radial velocity (Rv) | −0.47±0.47[4] km/s |
| Proper motion (μ) | RA: +62.63[1] mas/yr Dec.: +2.66[1] mas/yr |
| Parallax (π) | 31.9795 ± 0.3485 mas[5] |
| Distance | 102 ± 1 ly (31.3 ± 0.3 pc) |
| Absolute magnitude (MV) | +0.98+0.07 −0.06[6] |
| Details[7] | |
| α2 Cap A | |
| Mass | 2.05±0.29 M☉ |
| Radius | 8.38±0.58 R☉ |
| Luminosity | 40.4±2.2 L☉ |
| Surface gravity (log g) | 3.0[4] cgs |
| Temperature | 5,030±160 K |
| Metallicity [Fe/H] | −0.15±0.10 dex |
| Rotational velocity (v sin i) | 2.7[4] km/s |
| Age | 1.30±1.04 Gyr |
| Other designations | |
Gredi, Algedi, Secunda Giedi, Algiedi Secunda, α2 Cap, 6 Cap, ADS 13645, BD−12° 5685, FK5 761, HD 192947, HIP 100064, HR 7754, SAO 163427, WDS J20181-1233A,BC[8] | |
| Database references | |
| SIMBAD | data |
Alpha2 Capricorni (α2 Capricorni), or Algedi /ælˈdʒiːdi/,[9][10] is a triple star system[11] in the southern constellationofCapricornus. It is visible to the naked eye with an apparent visual magnitude of +3.57.[2] It is separated from the fainter α¹ Capricorni by 0.11° of the sky, a gap just resolvable with the naked eye, similar to Mizar and Alcor. Based on parallax shift as refined from orbits around the Sun of the Gaia spacecraft at Earth's Lagrange point 2, the star is 101 to 103 light years from the Solar System.
The primary, component A, is an evolved G-type star with a stellar classification of G8.5III-IV,[3] indicating that the spectrum displays mixed traits of a giant and subgiant star. At the age of 1.3 billion years, is currently on the red giant branch[7] and is generating energy through hydrogen fusion along a shell surrounding an inert helium core. The star has around double the mass of the Sun and has expanded to more than eight times the Sun's radius. The star is radiating 40 times the solar luminosity from its photosphere at an effective temperature of 5,030 K.[7]
The secondary components B and C form a binary system that orbit each other with a period of about 244 years. Both stars have masses about half that of the Sun. They orbit the primary with an estimated period of around 1,500 years.[12] As of 2010, the pair lies at an angular separation of 6.6 arc seconds from the primary along a position angle of 196°.[13]
α² Capricorni (LatinisedtoAlpha² Capricorni) is the star's Bayer designation. It bore the traditional names Secunda GiediorAlgiedi Secunda and shared the name Algedi (from the Arabic الجدي al-jadii 'the goat') with α¹ Capricorni. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[14] to catalogue and standardize proper names for stars. The WGSN approved the name Algedi for α² Capricorni on 21 August 2016 and it is now so entered in the IAU Catalog of Star Names.[10]
In Chinese, 牛宿 (Niú Xiù), meaning Ox (asterism), refers to an asterism consisting of α² Capricorni, Beta Capricorni, ξ² Capricorni, Pi Capricorni, Omicron Capricorni and Rho Capricorni.[15] Consequently, α² Capricorni itself is known as 牛宿二 (Niú Xiù èr, the Second Star of Ox.)[16]
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