From Wikipedia, the free encyclopedia
Kappa1 Sculptoris
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Sculptor
Right ascension 00h 09m 21.06696s [1]
Declination −27° 59′ 16.5322″ [1]
Apparent magnitude (V) +5.51 (6.23 + 6.29) [2]
Characteristics
Spectral type F2V [3] (F4 III + F3 III) [2]
U−B color index +0.06 [4]
B−V color index +0.42 [4]
Astrometry
Radial velocity (Rv)7.7±1.6 [5] km/s
Proper motion (μ) RA: +70.11 [1]  mas/ yr
Dec.: −8.97 [1]  mas/ yr
Parallax (π)12.91 ± 0.72  mas [1]
Distance250 ± 10  ly
(77 ± 4  pc)
Absolute magnitude (MV)2.05 [6]
Orbit [7]
Period (P)616.04 yr
Semi-major axis (a)1.500″
Eccentricity (e)0.103
Inclination (i)98.98°
Longitude of the node (Ω)81.75°
Periastron epoch (T)2095.68
Argument of periastron (ω)
(secondary)
256.86°
Details
κ1 Scl A
Mass1.53 [8]  M
Luminosity31.3 [9]  L
Surface gravity (log g)3.94 [8]  cgs
Temperature6,697±228 [8]  K
Metallicity [Fe/H]+0.05 [10]  dex
Rotational velocity (v sin i)116.8±5.8 [6] km/s
Age2.0 [8]  Gyr
Other designations
κ1 Scl, CD−28° 16, HD 493, HIP 761, HR 24, SAO 166083, ADS 111, WDS J00094-2759AB [11]
Database references
SIMBAD data

Kappa1 Sculptoris is a binary star [2] system in the southern constellation of Sculptor. It is faintly visible to the naked eye, with a combined apparent visual magnitude of +5.51. [2] Based upon an annual parallax shift of 12.91  mas as measured from Earth, [1] it is located roughly 250  light years from the Sun.

The pair orbit each other with an estimated period of 616 years, a semimajor axis of 1.5  arc seconds, and an eccentricity of 0.1. [7] Both components are evolved, yellow-white hued, F-type giant stars. The primary, component A, has a visual magnitude of 6.23 [2] and a stellar classification of F4 III. [2] The companion, component B, is magnitude 6.29 [2] and of class F3 III. [2] Their composite spectrum is classified as F2V. [3] The mass ratio is 0.782, meaning the secondary is only 78.2% as massive as the primary. [12] An 18th magnitude companion star lies 73.4 arc seconds distant along a position angle of 243°, as of 1998. [13]

References

  1. ^ 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.
  2. ^ a b c d e f g h 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.
  3. ^ a b Houk, 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. ^ a b Hurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles", Monthly Notes of the Astronomical Society of Southern Africa, 34: 7, Bibcode: 1975MNSSA..34....7H.
  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. ^ a b Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv: 1204.2459, Bibcode: 2012A&A...542A.116A, doi: 10.1051/0004-6361/201118724, S2CID  53666672.
  7. ^ a b Hartkopf, W. I.; et al., Sixth Catalog of Orbits of Visual Binary Stars, United States Naval Observatory, archived from the original on 2011-05-17, retrieved 2017-06-02
  8. ^ 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.
  9. ^ 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.
  10. ^ Casagrande, L.; et al. (2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics, 530 (A138): 21, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID  56118016.
  11. ^ "kap01 Scl -- Double or multiple star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2017-06-01.
  12. ^ Makarov, Valeri V.; Fabricius, Claus (2021). "Astrometric Mass Ratios of 248 Long-period Binary Stars Resolved in Hipparcos and Gaia EDR3". The Astronomical Journal. 162 (6): 260. arXiv: 2109.11951. Bibcode: 2021AJ....162..260M. doi: 10.3847/1538-3881/ac2ee0. S2CID  237635330.
  13. ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920, retrieved 2015-07-22
From Wikipedia, the free encyclopedia
Kappa1 Sculptoris
Observation data
Epoch J2000.0       Equinox J2000.0 ( ICRS)
Constellation Sculptor
Right ascension 00h 09m 21.06696s [1]
Declination −27° 59′ 16.5322″ [1]
Apparent magnitude (V) +5.51 (6.23 + 6.29) [2]
Characteristics
Spectral type F2V [3] (F4 III + F3 III) [2]
U−B color index +0.06 [4]
B−V color index +0.42 [4]
Astrometry
Radial velocity (Rv)7.7±1.6 [5] km/s
Proper motion (μ) RA: +70.11 [1]  mas/ yr
Dec.: −8.97 [1]  mas/ yr
Parallax (π)12.91 ± 0.72  mas [1]
Distance250 ± 10  ly
(77 ± 4  pc)
Absolute magnitude (MV)2.05 [6]
Orbit [7]
Period (P)616.04 yr
Semi-major axis (a)1.500″
Eccentricity (e)0.103
Inclination (i)98.98°
Longitude of the node (Ω)81.75°
Periastron epoch (T)2095.68
Argument of periastron (ω)
(secondary)
256.86°
Details
κ1 Scl A
Mass1.53 [8]  M
Luminosity31.3 [9]  L
Surface gravity (log g)3.94 [8]  cgs
Temperature6,697±228 [8]  K
Metallicity [Fe/H]+0.05 [10]  dex
Rotational velocity (v sin i)116.8±5.8 [6] km/s
Age2.0 [8]  Gyr
Other designations
κ1 Scl, CD−28° 16, HD 493, HIP 761, HR 24, SAO 166083, ADS 111, WDS J00094-2759AB [11]
Database references
SIMBAD data

Kappa1 Sculptoris is a binary star [2] system in the southern constellation of Sculptor. It is faintly visible to the naked eye, with a combined apparent visual magnitude of +5.51. [2] Based upon an annual parallax shift of 12.91  mas as measured from Earth, [1] it is located roughly 250  light years from the Sun.

The pair orbit each other with an estimated period of 616 years, a semimajor axis of 1.5  arc seconds, and an eccentricity of 0.1. [7] Both components are evolved, yellow-white hued, F-type giant stars. The primary, component A, has a visual magnitude of 6.23 [2] and a stellar classification of F4 III. [2] The companion, component B, is magnitude 6.29 [2] and of class F3 III. [2] Their composite spectrum is classified as F2V. [3] The mass ratio is 0.782, meaning the secondary is only 78.2% as massive as the primary. [12] An 18th magnitude companion star lies 73.4 arc seconds distant along a position angle of 243°, as of 1998. [13]

References

  1. ^ 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.
  2. ^ a b c d e f g h 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.
  3. ^ a b Houk, 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. ^ a b Hurly, P. R. (1975), "Combined-light UBV Photometry of 103 Bright Southern Visual Doubles", Monthly Notes of the Astronomical Society of Southern Africa, 34: 7, Bibcode: 1975MNSSA..34....7H.
  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. ^ a b Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics, 542: A116, arXiv: 1204.2459, Bibcode: 2012A&A...542A.116A, doi: 10.1051/0004-6361/201118724, S2CID  53666672.
  7. ^ a b Hartkopf, W. I.; et al., Sixth Catalog of Orbits of Visual Binary Stars, United States Naval Observatory, archived from the original on 2011-05-17, retrieved 2017-06-02
  8. ^ 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.
  9. ^ 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.
  10. ^ Casagrande, L.; et al. (2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics, 530 (A138): 21, arXiv: 1103.4651, Bibcode: 2011A&A...530A.138C, doi: 10.1051/0004-6361/201016276, S2CID  56118016.
  11. ^ "kap01 Scl -- Double or multiple star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2017-06-01.
  12. ^ Makarov, Valeri V.; Fabricius, Claus (2021). "Astrometric Mass Ratios of 248 Long-period Binary Stars Resolved in Hipparcos and Gaia EDR3". The Astronomical Journal. 162 (6): 260. arXiv: 2109.11951. Bibcode: 2021AJ....162..260M. doi: 10.3847/1538-3881/ac2ee0. S2CID  237635330.
  13. ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode: 2001AJ....122.3466M, doi: 10.1086/323920, retrieved 2015-07-22

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