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Xi Sculptoris

From Wikipedia, the free encyclopedia
Star in the constellation Sculptor
Xi Sculptoris
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationSculptor[1]
Right ascension01h 01m 18.27548s[2]
Declination−38° 54′ 59.5033″[2]
Apparent magnitude (V)5.59[1]
Characteristics
Spectral typeK1 III[3]
B−Vcolor index+1.185±0.008[1]
Astrometry
Radial velocity (Rv)−31.1±2.9[4] km/s
Proper motion (μ)RA: +66.892[2]mas/yr
Dec.: +49.891[2]mas/yr
Parallax (π)6.6662±0.0829 mas[2]
Distance489 ± 6 ly
(150 ± 2 pc)
Absolute magnitude (MV)−0.39[1]
Details
Mass2.9[5] M
Radius22.29+1.18
−1.74
[2] R
Luminosity198[5] L
Surface gravity (log g)2.12[5] cgs
Temperature4,403[5] K
Metallicity[Fe/H]−0.48[6] dex
Rotational velocity (v sin i)<1.0[7] km/s
Other designations
ξ Scl,CD−39°260,HD 6055,HIP 4770,HR 288,SAO 192870[8]
Database references
SIMBADdata

Xi Sculptoris,Latinized from ξ Sculptoris, is a solitary[9] orange-huedstar in the southernconstellation ofSculptor, near the southern constellation boundary withPhoenix. It is just visible to the naked eye as a dim point of light with anapparent visual magnitude of 5.59.[1] The distance to Xi Sculptoris is approximately 489 light years based onparallax, while it is drifting closer with aradial velocity of −31 km/s.[4] It has an absolute magnitude of −0.39.[1]

This object is an aginggiant star with astellar classification of K1 III,[3] which indicates it has exhausted the supply of hydrogen at itscore then expanded and cooled off themain sequence. At present it has 22[2] times the girth of the Sun. It is radiating 182 times theluminosity of the Sun from its swollenphotosphere at aneffective temperature of 4,489 K.[2]

References

[edit]
  1. ^abcdefAnderson, 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. ^abcdefghBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  3. ^abHouk, Nancy (1979),Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,Bibcode:1982mcts.book.....H.
  4. ^abde 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.
  5. ^abcdFouesneau, M.; Andrae, R.; Dharmawardena, T.; Rybizki, J.; Bailer-Jones, C. A. L.; Demleitner, M. (2022). "Astrophysical parameters from Gaia DR2, 2MASS, and AllWISE".Astronomy and Astrophysics.662: A125.arXiv:2201.03252.Bibcode:2022A&A...662A.125F.doi:10.1051/0004-6361/202141828.
  6. ^Ye, Xianhao; Wu, Wenbo; Allende Prieto, Carlos; Aguado, David S.; Zhao, Jingkun; González Hernández, Jonay I.; Rebolo, Rafael; Zhao, Gang; Li, Zhuohan; Del Burgo, Carlos; Chen, Yuqin (2025). "Mapping the Milky Way with Gaia Bp/Rp spectra: I. Systematic flux corrections and atmospheric parameters for 68 million stars".Astronomy and Astrophysics.695.arXiv:2411.19105.Bibcode:2025A&A...695A..75Y.doi:10.1051/0004-6361/202452871.
  7. ^De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014). "A catalog of rotational and radial velocities for evolved stars. V. Southern stars".Astronomy and Astrophysics.561: A126.arXiv:1312.3474.Bibcode:2014A&A...561A.126D.doi:10.1051/0004-6361/201220762.
  8. ^"ksi Scl".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-10-08.
  9. ^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.
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