| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Centaurus[1] |
| Right ascension | 13h 03m 33.305s[2] |
| Declination | −49° 31′ 38.15″[2] |
| Apparent magnitude (V) | +4.83[3] |
| Characteristics | |
| Evolutionary stage | Main sequence |
| Spectral type | A0 V[4] |
| U−B color index | +0.014[3] |
| B−V color index | +0.030[3] |
| Astrometry | |
| Radial velocity (Rv) | 0.00±3.70[5] km/s |
| Proper motion (μ) | RA: −47.858 mas/yr[2] Dec.: −11.496 mas/yr[2] |
| Parallax (π) | 14.8276±0.1073 mas[2] |
| Distance | 220 ± 2 ly (67.4 ± 0.5 pc) |
| Absolute magnitude (MV) | +0.68[1] |
| Details[6] | |
| Mass | 2.39 M☉ |
| Radius | 2.7[7] R☉ |
| Luminosity | 43.2[8] L☉ |
| Surface gravity (log g) | 4.11±0.14 cgs |
| Temperature | 10,462±356 K |
| Rotational velocity (v sin i) | 185[9] km/s |
| Age | 125 Myr |
| Other designations | |
| ξ1 Cen, CD−48° 7887, HD 113314, HIP 63724, HR 4933, SAO 223870[10] | |
| Database references | |
| SIMBAD | data |
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Xi1 Centauri is a solitary[11] star in the southern constellation of Centaurus. Its name is a Bayer designation that is Latinized from ξ1 Centauri, and abbreviated Xi1 Cen or ξ1 Cen. This star is visible to the naked eye with an apparent visual magnitude of +4.83.[3] With an annual parallax shift of 14.83 mas,[2] it is located around 220 light years from the Sun. At that distance, the apparent visual magnitude of the star is diminished by an interstellar extinction factor of 0.10[12] due to intervening dust. Just 17 arc minutes to the east of Xi1 Centauri lies the galaxy NGC 4945.[13]
This is an A-type main sequence star with a stellar classification of A0 V.[4] It is about 125 million years old[6] with a relatively high rate of spin, having a projected rotational velocity of 185 km/s.[9] The star has an estimated 2.4 times the mass of the Sun[6] and about 2.7 times the Sun's radius.[7] It is radiating 43 times the solar luminosity[8] from its outer atmosphere at an effective temperature of 10,462 K.[6]
References
- ^ a b 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. XHIP record for this object at VizieR.
- ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023), "Gaia Data Release 3. Summary of the content and survey properties", Astronomy and Astrophysics, 674: A1, arXiv:2208.00211, Bibcode:2023A&A...674A...1G, doi:10.1051/0004-6361/202243940, S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b c d Gutierrez-Moreno, Adelina; Moreno, Hugo (June 1968), "A photometric investigation of the Scorpio-Centaurus association", Astrophysical Journal Supplement, 15: 459, Bibcode:1968ApJS...15..459G, doi:10.1086/190168.
- ^ a b Bauwens, E. K. J.; et al. (2010), "Candidate Calibrators for the In-Orbit Spectrophotometric Calibration of the MIRI Medium Resolution Spectrograph Onboard the James Webb Space Telescope", in Deustua, Susana; Oliveira, Cristina (eds.), The 2010 STScI Calibration Workshop (PDF), Space Telescope Science Institute, retrieved 2016-01-10.
- ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
- ^ a b c d David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv:1501.03154, Bibcode:2015ApJ...804..146D, doi:10.1088/0004-637X/804/2/146, S2CID 33401607.
- ^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (3rd ed.): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
- ^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
- ^ a b Uesugi, Akira; Fukuda, Ichiro (1970), "Catalogue of rotational velocities of the stars", Contributions from the Institute of Astrophysics and Kwasan Observatory, University of Kyoto, Bibcode:1970crvs.book.....U.
- ^ "ksi01 Cen", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2017-01-09.
- ^ 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.
- ^ Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters, 38 (11): 694–706, arXiv:1606.09028, Bibcode:2012AstL...38..694G, doi:10.1134/S1063773712110035, S2CID 119108982.
- ^ O'Meara, Stephen James (2016), Deep-Sky Companions: The Caldwell Objects (2nd ed.), Cambridge University Press, p. 392, ISBN 978-1316033531.
