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Xi1 Centauri

From Wikipedia, the free encyclopedia
Star in the constellation Centaurus
For other stars with this Bayer designation, seeXi Centauri.
ξ1 Centauri
Location of ξ1 Centauri (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCentaurus[1]
Right ascension13h 03m 33.305s[2]
Declination−49° 31′ 38.15″[2]
Apparent magnitude (V)+4.83[3]
Characteristics
Evolutionary stageMain sequence
Spectral typeA0 V[4]
U−Bcolor index+0.014[3]
B−Vcolor index+0.030[3]
Astrometry
Radial velocity (Rv)0.00±3.70[5] km/s
Proper motion (μ)RA: −47.858mas/yr[2]
Dec.: −11.496mas/yr[2]
Parallax (π)14.8276±0.1073 mas[2]
Distance220 ± 2 ly
(67.4 ± 0.5 pc)
Absolute magnitude (MV)+0.68[1]
Details[6]
Mass2.39 M
Radius2.7[7] R
Luminosity43.2[8] L
Surface gravity (log g)4.11±0.14 cgs
Temperature10,462±356 K
Rotational velocity (v sin i)185[9] km/s
Age125 Myr
Other designations
ξ1 Cen,CD−48° 7887,HD 113314,HIP 63724,HR 4933,SAO 223870[10]
Database references
SIMBADdata
ξ1 Cen is the brightest star in the picture, at the right of the galaxyNGC 4945.

Xi1 Centauri is a solitary[11]star in the southernconstellation ofCentaurus. Its name is aBayer designation that isLatinized from ξ1 Centauri, and abbreviated Xi1 Cen or ξ1 Cen. This star is visible to thenaked eye with anapparent visual magnitude of +4.83.[3] With an annualparallax shift of14.83 mas,[2] it is located around 220 light years from theSun. At that distance, the apparent visual magnitude of the star is diminished by an interstellarextinction factor of 0.10[12] due to intervening dust. Just 17 arc minutes to the east of Xi1 Centauri lies the galaxyNGC 4945.[13]

This is anA-type main sequence star with astellar classification of A0 V.[4] It is about 125 million years old[6] with a relatively high rate of spin, having aprojected rotational velocity of 185 km/s.[9] The star has an estimated 2.4 times themass of the Sun[6] and about 2.7 times theSun's radius.[7] It is radiating 43 times thesolar luminosity[8] from itsouter atmosphere at aneffective temperature of 10,462 K.[6]

References

[edit]
  1. ^abAnderson, 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 atVizieR.
  2. ^abcdeVallenari, 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 atVizieR.
  3. ^abcdGutierrez-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.
  4. ^abBauwens, 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, retrieved2016-01-10.
  5. ^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.
  6. ^abcdDavid, 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.
  7. ^abPasinetti 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.
  8. ^abMcDonald, 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.
  9. ^abUesugi, 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.
  10. ^"ksi01 Cen",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2017-01-09.
  11. ^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.
  12. ^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.
  13. ^O'Meara, Stephen James (2016),Deep-Sky Companions: The Caldwell Objects (2nd ed.),Cambridge University Press, p. 392,ISBN 978-1316033531.
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