HD 213429
Binary star system in the constellation Aquarius
HD 213429
Observation dataEpoch J2000 Equinox ICRS
Constellation
Aquarius
Right ascension
22h 31m 18.31271s
Declination
−06° 33′ 18.5437″
Apparent magnitude (V)
6.160
Characteristics
Spectral type
F8V
U−B color index
+0.03
B−V color index
+0.55
Astrometry Radial velocity (Rv ) −9.9± 6.3 km/s Proper motion (μ) RA: +161.61 mas /yr Dec.: −108.40 mas /yr Parallax (π)39.35± 0.70 mas Distance 83 ± 1 ly (25.4 ± 0.5 pc ) Absolute magnitude (MV )4.13
Details HD 213429 A Mass 1.18 M ☉ Surface gravity (log g )4.10 cgs Temperature 6,001 K Metallicity [Fe/H] −0.23 dex Rotational velocity (v sin i )6 km/s Age 3.7 Gyr HD 213429 B Mass 0.78 M ☉
Other designations BD −07°5797, HD 213429, HIP 111170, HR 8581, GJ 862.1, GJ 9786, LTT 9053, SAO 146135
Database references SIMBAD data Data sources:
Hipparcos Catalogue ,CCDM (2002),Bright Star Catalogue (5th rev. ed.)
HD 213429 is a spectroscopic binary system in the equatorial constellation of Aquarius . It has a combined apparent magnitude of 6.16 and is located around 83 light years away. The pair orbit each other with a period of 631 days, at an average separation of 1.74 AU and an eccentricity of 0.38.
References
↑ Roman, Nancy G. (1987). "Identification of a constellation from a position" . Publications of the Astronomical Society of the Pacific . 99 (617): 695. Bibcode :1987PASP...99..695R . doi :10.1086/132034 .
Constellation record for this object at VizieR .
1 2 3 4 5 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
1 2 3 4 Nordström, B.; et al. (May 2014), "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ~14000 F and G dwarfs", Astronomy and Astrophysics , 418 : 989– 1019, arXiv :astro-ph/0405198 , Bibcode :2004A& A...418..989N , doi :10.1051/0004-6361:20035959 , S2CID 11027621
1 2 3 4 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 , S2CID 119476992
1 2 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data. SIMBAD , Bibcode :1986EgUBV........0M
1 2 3 4 Tokovinin, Andrei (April 2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal , 147 (4): 14, arXiv :1401.6827 , Bibcode :2014AJ....147...87T , doi :10.1088/0004-6256/147/4/87 , S2CID 56066740 , 87
↑ Uesugi, Akira; Fukuda, Ichiro (1970), "Catalogue of rotational velocities of the stars", Contributions from the Institute of Astrophysics and Kwasan Observatory , University of Kyoto, Bibcode :1970crvs.book.....U
↑ Jaime, Luisa G.; et al. (September 2014), "Habitable zones with stable orbits for planets around binary systems", Monthly Notices of the Royal Astronomical Society , 443 (1): 260– 274, arXiv :1401.1006 , Bibcode :2014MNRAS.443..260J , doi :10.1093/mnras/stu1052