HD 214810

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HD 214810
Observation data
Epoch J2000      Equinox J2000
Constellation Aquarius
Right ascension 22h 40m 47.95600s[1]
Declination −03° 33′ 15.2789″[1]
Apparent magnitude (V) 6.32 (6.52 + 8.63)[2]
Characteristics
Spectral type G9 V Fe-0.7[3]
U−B color index −0.02[4]
B−V color index +0.52[4]
Astrometry
Radial velocity (Rv) 13.73 km/s
Proper motion (μ) RA: -7.52[1] mas/yr
Dec.: -45.25[1] mas/yr
Parallax (π) 28.93 ± 0.77[1] mas
Distance 113 ± 3 ly
(34.6 ± 0.9 pc)
Orbit[2]
Period (P) 54.20 yr
Semi-major axis (a) 0.360"
Details
HD 214810 A
Mass 1.26[5] M
Surface gravity (log g) 4.19[3] cgs
Temperature 6,151[3] K
Metallicity [Fe/H] −0.22[3] dex
Age 3.7[6] Gyr
HD 214810 B
Mass 0.87[5] M
Other designations
BD-04° 5728, HD 214810, HIP 111965, HR 8629, SAO 146239.
Database references
SIMBAD data

HD 214810 is a visual binary star in the equatorial constellation of Aquarius. The pair orbit each other with a period of about 54.2 years.[2]

References[edit]

  1. ^ a b c d e 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 
  2. ^ a b c Cvetkovic, Z.; Ninkovic, S. (2010), "On the Component Masses of Visual Binaries", Serbian Astronomical Journal 180: 71–80, Bibcode:2010SerAJ.180...71C, doi:10.2298/SAJ1080071C 
  3. ^ a b c d Gray, R. O. et al. (July 2006), "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample", The Astronomical Journal 132 (1): 161–170, arXiv:astro-ph/0603770, Bibcode:2006AJ....132..161G, doi:10.1086/504637 
  4. ^ a b Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV data. SIMBAD, Bibcode:1986EgUBV........0M 
  5. ^ a b Tokovinin, Andrei (April 2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal 147 (4): 14, Bibcode:2014AJ....147...87T, doi:10.1088/0004-6256/147/4/87, 87 
  6. ^ Holmberg, J.; Nordström, B.; Andersen, J. (July 2009), "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics", Astronomy and Astrophysics 501 (3): 941–947, arXiv:0811.3982, Bibcode:2009A&A...501..941H, doi:10.1051/0004-6361/200811191 

External links[edit]