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HD 131040

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Star in the constellation Boötes
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HD 131040
Observation data
Epoch J2000Equinox ICRS
Constellation Boötes [1]
Right ascension 14h 49m 32.38200s[2]
Declination +51°22′28.2117′′[2]
Apparentmagnitude(V) 6.51[3]
Characteristics
Evolutionarystage main sequence [2]
Spectraltype F3V[4]
U−B color index +0.00[3]
B−V color index +0.40[3]
Astrometry
Radial velocity (Rv)−6.90[5] km/s
Proper motion (μ) RA:+15.592[2] mas/yr
Dec.:+1.961[2] mas/yr
Parallax (π)19.1763±0.0147mas [2]
Distance 170.1 ± 0.1ly
(52.15 ± 0.04pc)
Absolutemagnitude(MV)+2.93[1]
Details
Mass 1.4[6] M☉
Radius 1.7[6] R☉
Luminosity 5.6[6] L☉
Surface gravity (logg)4.12[6] cgs
Temperature 6,743[6] K
Metallicity [Fe/H]+0.04[7] dex
Age 1.80[7] Myr
Other designations
BD+51°1957, HD 131040, HIP 72508, HR 5537, SAO 29296[8]
Database references
SIMBAD data

HD 131040 is an F-type main-sequence star in the northern constellation of Boötes. It has an apparent magnitude of 6.51 and is 170 light years away.

The brightness of HD 131040 has been reported to vary slightly by 0.04 magnitudes.[9] Radial velocity variations and an apparent over-luminosity have led to the theory that D 131040 is a spectroscopic binary.[10]

Multiple star catalogues list a 10th-magnitude companion at an angular separation of 15.1′′ along a position angle of 93°, and a 14th-magnitude companion at a separation of 62".[11] Neither is thought to be physically associated with HD 131040, but there is a possible white dwarf 9.4" away, which is at a similar distance and has a similar proper motion.[10]

References

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  1. 1 2 Anderson, 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. 1 2 3 4 5 6 Vallenari, 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 at VizieR .
  3. 1 2 3 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data. SIMBAD, Bibcode:1986EgUBV........0M.
  4. ↑ Abt, H. A. (1981). "Visual multiples. VII. MK classifications". The Astrophysical Journal Supplement Series. 45: 437. Bibcode:1981ApJS...45..437A. doi:10.1086/190719.
  5. ↑ Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system", Astronomy Letters, 32 (11): 759–771, arXiv:1606.08053 , Bibcode:2006AstL...32..759G, doi:10.1134/S1063773706110065, S2CID 119231169.
  6. 1 2 3 4 5 Stassun, 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 .
  7. 1 2 Casagrande, L.; Schönrich, R.; Asplund, M.; Cassisi, S.; Ramírez, I.; Meléndez, J.; Bensby, T.; Feltzing, S. (2011). "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey". Astronomy and Astrophysics. 530. arXiv:1103.4651 . Bibcode:2011A&A...530A.138C. doi:10.1051/0004-6361/201016276.
  8. ↑ "HD 131040". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2025年04月18日.
  9. ↑ Adelman, S. J.; Coursey, B. C.; Harris, E. A. (December 2000), "On the Variability of F1-F9 Luminosity Class III-V Stars", Information Bulletin on Variable Stars, 5003 (5003): 1, Bibcode:2000IBVS.5003....1A
  10. 1 2 Tokovinin, Andrei (2018). "The Updated Multiple Star Catalog". The Astrophysical Journal Supplement Series. 235 (1): 6. arXiv:1712.04750 . Bibcode:2018ApJS..235....6T. doi:10.3847/1538-4365/aaa1a5 .
  11. ↑ 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年07月22日
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