| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 12h 26m 31.75955s [1] |
| Declination | −51° 27′ 02.2899″ [1] |
| Apparent magnitude (V) | 4.82 [2] |
| Characteristics | |
| Spectral type | B3V(n) [3] |
| B−V color index | −0.141±0.002 [2] |
| Astrometry | |
| Radial velocity (Rv) | +5.0±4.2 [2] km/s |
| Proper motion (μ) |
RA: −30.66
[1]
mas/
yr Dec.: −10.13 [1] mas/ yr |
| Parallax (π) | 7.28 ± 0.24 mas [1] |
| Distance | 450 ± 10
ly (137 ± 5 pc) |
| Absolute magnitude (MV) | −0.87 [2] |
| Details | |
| Mass | 6.2±0.1 [4] M☉ |
| Radius | 3.42 [5] R☉ |
| Luminosity | 483.06 [2] L☉ |
| Temperature | 13,732 [6] K |
| Metallicity [Fe/H] | −0.38±0.06 [7] dex |
| Rotational velocity (v sin i) | 298±12 [8] km/s |
| Age | 15.8±0.2 [4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
G Centauri is a single [10] star in the southern constellation of Centaurus. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of +4.82. This object is located approximately 450 light years from the Sun, based on parallax. [1] It is a member of the Lower Centaurus–Crux group of the Scorpius–Centaurus association, with the former having an age of about 17 million years. [11]
This object is a B-type main-sequence star with a stellar classification of B3V(n), [3] where the 'n' indicates "nebulous" (broad) lines due to rapid rotation. It is around 16 [4] million years old with a projected rotational velocity of up to 298 km/s. [8] The star has six [4] times the mass of the Sun and 3.4 [5] times the Sun's radius. It is radiating 483 [2] times the luminosity of the Sun from its photosphere at an effective temperature of 13,732 K. [6] An infrared excess indicates a circumstellar disk of dust with a mean temperature of 50 K is orbiting the star at a separation of 717.8 AU. [5]
- ^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv: 0708.1752, Bibcode: 2007A&A...474..653V, doi: 10.1051/0004-6361:20078357, S2CID 18759600.
- ^ a b c d e f Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ^ a b c d Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv: 1007.4883, Bibcode: 2011MNRAS.410..190T, doi: 10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
- ^ a b c Cotten, Tara H.; Song, Inseok (July 2016), "A Comprehensive Census of Nearby Infrared Excess Stars", The Astrophysical Journal Supplement Series, 225 (1): 24, arXiv: 1606.01134, Bibcode: 2016ApJS..225...15C, doi: 10.3847/0067-0049/225/1/15, S2CID 118438871, 15.
- ^ a b McDonald, I.; et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–357, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ Gáspár, András; et al. (2016), "The Correlation between Metallicity and Debris Disk Mass", The Astrophysical Journal, 826 (2): 171, arXiv: 1604.07403, Bibcode: 2016ApJ...826..171G, doi: 10.3847/0004-637X/826/2/171, S2CID 119241004.
- ^ a b Brown, A. G. A.; Verschueren, W. (1997), "High S/N Echelle spectroscopy in young stellar groups. II. Rotational velocities of early-type stars in SCO OB2", Astronomy and Astrophysics, 319: 811, arXiv: astro-ph/9608089, Bibcode: 1997A&A...319..811B. Note: "The He i λ4026 line in this star is broader than the models. The value of vsini may thus be overestimated."
- ^ "G Cen". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-15.
- ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ Jang-Condell, Hannah; et al. (August 2015), "Spitzer IRS Spectra of Debris Disks in the Scorpius–Centaurus OB Association", The Astrophysical Journal, 808 (2): 19, arXiv: 1506.05428, Bibcode: 2015ApJ...808..167J, doi: 10.1088/0004-637X/808/2/167, S2CID 118549483, 167.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Centaurus |
| Right ascension | 12h 26m 31.75955s [1] |
| Declination | −51° 27′ 02.2899″ [1] |
| Apparent magnitude (V) | 4.82 [2] |
| Characteristics | |
| Spectral type | B3V(n) [3] |
| B−V color index | −0.141±0.002 [2] |
| Astrometry | |
| Radial velocity (Rv) | +5.0±4.2 [2] km/s |
| Proper motion (μ) |
RA: −30.66
[1]
mas/
yr Dec.: −10.13 [1] mas/ yr |
| Parallax (π) | 7.28 ± 0.24 mas [1] |
| Distance | 450 ± 10
ly (137 ± 5 pc) |
| Absolute magnitude (MV) | −0.87 [2] |
| Details | |
| Mass | 6.2±0.1 [4] M☉ |
| Radius | 3.42 [5] R☉ |
| Luminosity | 483.06 [2] L☉ |
| Temperature | 13,732 [6] K |
| Metallicity [Fe/H] | −0.38±0.06 [7] dex |
| Rotational velocity (v sin i) | 298±12 [8] km/s |
| Age | 15.8±0.2 [4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
G Centauri is a single [10] star in the southern constellation of Centaurus. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of +4.82. This object is located approximately 450 light years from the Sun, based on parallax. [1] It is a member of the Lower Centaurus–Crux group of the Scorpius–Centaurus association, with the former having an age of about 17 million years. [11]
This object is a B-type main-sequence star with a stellar classification of B3V(n), [3] where the 'n' indicates "nebulous" (broad) lines due to rapid rotation. It is around 16 [4] million years old with a projected rotational velocity of up to 298 km/s. [8] The star has six [4] times the mass of the Sun and 3.4 [5] times the Sun's radius. It is radiating 483 [2] times the luminosity of the Sun from its photosphere at an effective temperature of 13,732 K. [6] An infrared excess indicates a circumstellar disk of dust with a mean temperature of 50 K is orbiting the star at a separation of 717.8 AU. [5]
- ^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv: 0708.1752, Bibcode: 2007A&A...474..653V, doi: 10.1051/0004-6361:20078357, S2CID 18759600.
- ^ a b c d e f Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ^ a b c d Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv: 1007.4883, Bibcode: 2011MNRAS.410..190T, doi: 10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
- ^ a b c Cotten, Tara H.; Song, Inseok (July 2016), "A Comprehensive Census of Nearby Infrared Excess Stars", The Astrophysical Journal Supplement Series, 225 (1): 24, arXiv: 1606.01134, Bibcode: 2016ApJS..225...15C, doi: 10.3847/0067-0049/225/1/15, S2CID 118438871, 15.
- ^ a b McDonald, I.; et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–357, arXiv: 1208.2037, Bibcode: 2012MNRAS.427..343M, doi: 10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ Gáspár, András; et al. (2016), "The Correlation between Metallicity and Debris Disk Mass", The Astrophysical Journal, 826 (2): 171, arXiv: 1604.07403, Bibcode: 2016ApJ...826..171G, doi: 10.3847/0004-637X/826/2/171, S2CID 119241004.
- ^ a b Brown, A. G. A.; Verschueren, W. (1997), "High S/N Echelle spectroscopy in young stellar groups. II. Rotational velocities of early-type stars in SCO OB2", Astronomy and Astrophysics, 319: 811, arXiv: astro-ph/9608089, Bibcode: 1997A&A...319..811B. Note: "The He i λ4026 line in this star is broader than the models. The value of vsini may thus be overestimated."
- ^ "G Cen". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-15.
- ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ Jang-Condell, Hannah; et al. (August 2015), "Spitzer IRS Spectra of Debris Disks in the Scorpius–Centaurus OB Association", The Astrophysical Journal, 808 (2): 19, arXiv: 1506.05428, Bibcode: 2015ApJ...808..167J, doi: 10.1088/0004-637X/808/2/167, S2CID 118549483, 167.
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