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HD 127334

From Wikipedia, the free encyclopedia

Star in the constellation Boötes
HD 127334
Location of HD 127334 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationBoötes[1]
Right ascension14h 29m 36.80877s[2]
Declination+41° 47′ 45.2854″[2]
Apparent magnitude (V)6.36[3]
Characteristics
Spectral typeG5V CH0.3[4]
B−Vcolor index1.010[3][5]
J−Hcolor index0.258[6]
J−Kcolor index0.369[6]
Astrometry
Radial velocity (Rv)−0.401±0.0007[7] km/s
Proper motion (μ)RA: 161.373[2]mas/yr
Dec.: −220.361[2]mas/yr
Parallax (π)42.7526±0.0174 mas[2]
Distance76.29 ± 0.03 ly
(23.390 ± 0.010 pc)
Absolute magnitude (MV)+4.48[1]
Details
Mass1.02±0.02,[8] 1.07[9] M
Radius1.2[10] R
Luminosity1.4[10] L
Surface gravity (log g)4.37±0.13[11] cgs
Temperature5758±76,[11]5635±50[8] K
Metallicity[Fe/H]0.24±0.06,[11]0.19±0.04[8] dex
Rotational velocity (v sin i)7.1[12] km/s
Age8.6±1.3,[8] 10.5–10.7,[13] ~7.1[12] Gyr
Other designations
AG+42°1283,BD+42°2508,Gaia DR2 1491593733326694912,GC 19550,GJ 3852,HD 127334,HIP 70873,HR 5423,SAO 45075,PPM 54166,TIC 27525457,TYC 3039-237-1,2MASS J14293678+4147456[6]
Database references
SIMBADdata

HD 127334 is a solitary[9]Sun-like star in the northernconstellation ofBoötes. With anapparent magnitude of 6.36, it can be faintly seen by the naked eye fromEarth as a yellow-hued dot of light. As such, it is listed in theBright Star Catalogue asHR 5423. It is located at a distance of 76.29 light-years (23.39 parsecs) according toGaia EDR3parallax measurements.

Stellar properties

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This is aG-type main-sequence star much like the Sun, with aspectral type of G5V CH0.3,[4] where the suffix notation indicates an anomalous overabundance of themethylidyne radical. It is slightly more massive than the Sun but marginally cooler at 5,758 K (5,485 °C; 9,905 °F) or 5,635 K (5,362 °C; 9,683 °F). The Sun'seffective temperature, for comparison, is 5,772 K (5,499 °C; 9,930 °F).[14]

The star belongs to thethin disk population of theMilky Way[13] and is thought to be ancient: its age estimate varies between publications, but generally lies between 7–11Gyr, much older than theSolar System (aged 4.568 Gyr[15]). Despite its old age, it is enriched in heavy elements, possessing a super-solarmetallicity of0.24±0.06 or0.19±0.04 dex.

It has a low or very low level ofsurface activity, unlike some other similar stars such asToliman (Alpha Centauri B).[3]

HD 127334 has been a long-term target of theCalifornia Planet Search,[16] but noexoplanets have been discovered to orbit the star.[11]

See also

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References

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  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.
  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. ^abcRajpaul, V M; et al. (1 March 2020)."A robust, template-free approach to precise radial velocity extraction".Monthly Notices of the Royal Astronomical Society.492 (3):3960–3983.arXiv:1912.09563.doi:10.1093/mnras/stz3599.ISSN 0035-8711.
  4. ^abGray, R. O.; et al. (2003)."Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I."The Astronomical Journal.126 (4):2048–2059.arXiv:astro-ph/0308182.Bibcode:2003AJ....126.2048G.doi:10.1086/378365.ISSN 0004-6256.
  5. ^Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI".Astronomy & Astrophysics Supplement Series.89: 415.Bibcode:1991A&AS...89..415O.
  6. ^abc"HD 127334".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved15 November 2024.
  7. ^Soubiran, C.; et al. (2018)."Gaia Data Release 2: The catalogue of radial velocity standard stars".Astronomy & Astrophysics.616: A7.arXiv:1804.09370.Bibcode:2018A&A...616A...7S.doi:10.1051/0004-6361/201832795.ISSN 0004-6361.
  8. ^abcdGonzalez, G. (1 January 2015)."Parent stars of extrasolar planets – XIV. Strong evidence of Li abundance deficit".Monthly Notices of the Royal Astronomical Society.446 (1):1020–1025.arXiv:1410.4108.doi:10.1093/mnras/stu2156.ISSN 1365-2966.
  9. ^abFuhrmann, K.; et al. (10 February 2017)."Multiplicity among Solar-type Stars".The Astrophysical Journal.836 (1): 139.Bibcode:2017ApJ...836..139F.doi:10.3847/1538-4357/836/1/139.ISSN 0004-637X.
  10. ^abStassun, Keivan G.; et al. (2019)."The Revised TESS Input Catalog and Candidate Target List".The Astronomical Journal.158 (4): 138.arXiv:1905.10694.Bibcode:2019AJ....158..138S.doi:10.3847/1538-3881/ab3467.
  11. ^abcdLienhard, F; Mortier, A; Buchhave, L; Collier Cameron, A; López-Morales, M; Sozzetti, A; Watson, C A; Cosentino, R (26 May 2022)."Multi-mask least-squares deconvolution: extracting RVs using tailored masks".Monthly Notices of the Royal Astronomical Society.513 (4):5328–5343.arXiv:2204.13556.doi:10.1093/mnras/stac1098.ISSN 0035-8711.
  12. ^abde Andrés, F. Llorente; de la Reza, R.; Cruz, P.; Cuenda-Muñoz, D.; Alfaro, E. J.; Chavero, C.; Cifuentes, C. (2024)."The evolution of lithium in FGK dwarf stars: Influence of planets and Galactic migration".Astronomy & Astrophysics.684: A28.arXiv:2402.01315.Bibcode:2024A&A...684A..28L.doi:10.1051/0004-6361/202346744.ISSN 0004-6361.
  13. ^abŽenovienė, R.; Tautvaišienė, G.; Nordström, B.; Stonkutė, E.; Barisevičius, G. (2015)."Stellar substructures in the solar neighbourhood: IV. Kinematic Group 1 in the Geneva-Copenhagen survey".Astronomy & Astrophysics.576: A113.arXiv:1501.06401.Bibcode:2015A&A...576A.113Z.doi:10.1051/0004-6361/201425088.ISSN 0004-6361.
  14. ^Prša, Andrej; Harmanec, Petr; Torres, Guillermo; et al. (1 August 2016)."NOMINAL VALUES FOR SELECTED SOLAR AND PLANETARY QUANTITIES: IAU 2015 RESOLUTION B3 * †".The Astronomical Journal.152 (2): 41.arXiv:1510.07674.doi:10.3847/0004-6256/152/2/41.ISSN 0004-6256.
  15. ^Bouvier, A.;Wadhwa, M. (2010). "The age of the Solar System redefined by the oldest Pb–Pb age of a meteoritic inclusion".Nature Geoscience.3 (9):637–641.Bibcode:2010NatGe...3..637B.doi:10.1038/NGEO941.S2CID 56092512.
  16. ^Johnson, John Asher; Winn, Joshua N.; Albrecht, Simon; Howard, Andrew W.; Marcy, Geoffrey W.; Gazak, J. Zachary (2009)."A Third Exoplanetary System with Misaligned Orbital and Stellar Spin Axes".Publications of the Astronomical Society of the Pacific.121 (884):1104–1111.arXiv:0907.5204.Bibcode:2009PASP..121.1104J.doi:10.1086/644604.ISSN 0004-6280.
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