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HD 117566

From Wikipedia, the free encyclopedia
High proper motion star; Camelopardalis
HD 117566
Location of HD 117566 on the map (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCamelopardalis
Right ascension13h 26m 56.80348s[1]
Declination+78° 38′ 37.9324″[1]
Apparent magnitude (V)5.74±0.01[2]
Characteristics
Evolutionary stageHertzsprung gap[3] orhorizontal branch[4]
Spectral typeG3 IIIb Fe−1 CH1[5]
U−Bcolor index+0.35[6]
B−Vcolor index+0.77[6]
Astrometry
Radial velocity (Rv)13.7±0.3[7] km/s
Proper motion (μ)RA: −140.497mas/yr[1]
Dec.: +30.403mas/yr[1]
Parallax (π)11.1974±0.0417 mas[1]
Distance291 ± 1 ly
(89.3 ± 0.3 pc)
Absolute magnitude (MV)+1.03[8]
Details
Mass2.29[9] M
Radius7.2±0.4[10] R
Luminosity38.2±0.3[1] L
Surface gravity (log g)3.69±0.18[11] cgs
Temperature5,420±26[12] K
Metallicity [Fe/H]+0.03[11] dex
Rotational velocity (v sin i)8.9±1[13] km/s
Age760±50[7] Myr
Other designations
AG+78°340,BD+79°422,FK5 3075,GC 18223,HD 117566,HIP 65595,HR 5091,SAO 7821[14]
Database references
SIMBADdata

HD 117566, also known asHR 5091, is a solitary yellow-huedstar[15] located in the northerncircumpolar constellationCamelopardalis. It has anapparent magnitude of 5.74,[2] making it faintly visible to thenaked eye. This object is relatively close at a distance of 291light years based onGaia DR3parallax measurements but is receding with a heliocentricradial velocity of14 km/s.[7] At its current distance, HD 117566's brightness is diminished by 0.12magnitudes due tointerstellar dust.[16]

HD 117566 has astellar classification of G3 IIIb Fe−1 CH1,[5] indicating that it is aG-type giant with an under-abundance ofiron and an overabundance of theCH radical in itsspectrum. Itsevolutionary stage is unclear. A 1994 paper places it in theHertzsprung gap,[3] indicating it has ceasedhydrogen core fusion and is now evolving toward thered giant branch (RGB). However, Mishenina et al. (2006) said that HD 117566 is already past the RGB and is on thehorizontal branch, fusinghelium at its core.[4] Nevertheless, it has 2.29 times themass of the Sun[9] and, at the age of 760million years,[7] it has expanded to 7.2 times theSun's radius.[10] It radiates 38.2 times theluminosity of the Sun[1] from itsphotosphere at aneffective temperature of5,420 K.[12] HD 117566 has a solarmetallicity[11] and spins modestly with aprojected rotational velocity ofkm/s.[13]

References

[edit]
  1. ^abcdefVallenari, 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.
  2. ^abHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.
  3. ^abWallerstein, George; Bohm-Vitense, Erika; Vanture, Andrew D.; Gonzalez, Guillermo (June 1994)."The lithium content and other properties of F2-G5 giants in the Hertzsprung Gap".The Astronomical Journal.107: 2211.Bibcode:1994AJ....107.2211W.doi:10.1086/117031.ISSN 0004-6256.
  4. ^abMishenina, T. V.; Bienaymé, O.; Gorbaneva, T. I.; Charbonnel, C.; Soubiran, C.; Korotin, S. A.; Kovtyukh, V. V. (September 2006)."Elemental abundances in the atmosphere of clump giants".Astronomy & Astrophysics.456 (3):1109–1120.arXiv:astro-ph/0605615.Bibcode:2006A&A...456.1109M.doi:10.1051/0004-6361:20065141.eISSN 1432-0746.ISSN 0004-6361.
  5. ^abKeenan, Philip C.; McNeil, Raymond C. (October 1989). "The Perkins catalog of revised MK types for the cooler stars".The Astrophysical Journal Supplement Series.71: 245.Bibcode:1989ApJS...71..245K.doi:10.1086/191373.eISSN 1538-4365.ISSN 0067-0049.
  6. ^abMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data. SIMBAD,Bibcode:1986EgUBV........0M
  7. ^abcdSoubiran, C.; Bienaymé, O.; Mishenina, T. V.; Kovtyukh, V. V. (9 January 2008)."Vertical distribution of Galactic disk stars".Astronomy & Astrophysics.480 (1):91–101.arXiv:0712.1370.Bibcode:2008A&A...480...91S.doi:10.1051/0004-6361:20078788.eISSN 1432-0746.ISSN 0004-6361.
  8. ^Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.eISSN 1562-6873.ISSN 1063-7737.S2CID 119257644.
  9. ^abLiu, Y. J.; Tan, K. F.; Wang, L.; Zhao, G.; Sato, Bun'ei; Takeda, Y.; Li, H. N. (31 March 2014)."The Lithium Abundances of a Large Sample of Red Giants".The Astrophysical Journal.785 (2): 94.arXiv:1404.1687.Bibcode:2014ApJ...785...94L.doi:10.1088/0004-637X/785/2/94.eISSN 1538-4357.ISSN 0004-637X.
  10. ^abKervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004)."The angular sizes of dwarf stars and subgiants".Astronomy & Astrophysics.426 (1):297–307.arXiv:astro-ph/0404180.Bibcode:2004A&A...426..297K.doi:10.1051/0004-6361:20035930.eISSN 1432-0746.ISSN 0004-6361.
  11. ^abcda Silva, Ronaldo; Milone, André de C.; Rocha-Pinto, Helio J. (August 2015)."Homogeneous abundance analysis of FGK dwarf, subgiant, and giant stars with and without giant planets".Astronomy and Astrophysics.580: A24.arXiv:1505.01726.Bibcode:2015A&A...580A..24D.doi:10.1051/0004-6361/201525770.ISSN 0004-6361.
  12. ^abStrassmeier, K.G.; Schordan, P. (December 2000). "A temperature calibration for MK-class III giants from high-resolution spectral line-depth ratios".Astronomische Nachrichten.321 (5–6):277–305.Bibcode:2000AN....321..277S.doi:10.1002/1521-3994(200012)321:5/6<277::AID-ASNA277>3.0.CO;2-H.eISSN 1521-3994.ISSN 0004-6337.
  13. ^abDe Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (January 2014)."A catalog of rotational and radial velocities for evolved stars".Astronomy & Astrophysics.561: A126.arXiv:1312.3474.Bibcode:2014A&A...561A.126D.doi:10.1051/0004-6361/201220762.eISSN 1432-0746.ISSN 0004-6361.
  14. ^"HD 117566".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedDecember 16, 2022.
  15. ^Eggleton, P. P.; Tokovinin, A. A. (11 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.eISSN 1365-2966.ISSN 0035-8711.
  16. ^Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017)."Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars".Monthly Notices of the Royal Astronomical Society.472 (4):3805–3820.arXiv:1709.01160.Bibcode:2017MNRAS.472.3805G.doi:10.1093/mnras/stx2219.eISSN 1365-2966.ISSN 0035-8711.
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