Binary star system in the constellation Andromeda
Pi Andromedae
Location of π Andromedae (circled)
Observation dataEpoch J2000 Equinox J2000
Constellation
Andromeda
Right ascension
00 36 52.85132
Declination
+33° 43′ 09.6363″
Apparent magnitude (V)
4.36 (4.9/5.3)
Characteristics
Spectral type
B5 V (B5 V + B5 V)
U−B color index
–0.55
B−V color index
–0.16
Astrometry Radial velocity (Rv )+8.7 km/s Proper motion (μ) RA: 14.669(118) mas /yr Dec.: −3.385(93) mas /yr Parallax (π)5.6563 ± 0.1474 mas Distance 580 ± 20 ly (177 ± 5 pc )
Orbit Period (P)143.6 days Eccentricity (e)0.56
Details Luminosity 1,136 L ☉ Surface gravity (log g )4.10 cgs Temperature 15,276 K Metallicity –0.20 dex Rotational velocity (v sin i )25 km/s
Other designations π Andromedae, 29 Andromedae, ADS 513, BD +32°101, FK5 18, HD 3369, HIP 2912, HR 154, SAO 54033, PPM 65480
Database references SIMBAD data
π Andromedae in optical light
Pi Andromedae (Pi And , π Andromedae , π And ) is the Bayer designation for a binary star system in the northern constellation of Andromeda . With an apparent visual magnitude of 4.4, it is visible to the naked eye . It is located approximately 580 light-years (180 parsecs ) from Earth .
The pair is classified as a blue-white B-type main sequence dwarf , with an apparent magnitude of +4.34. It is a spectroscopic binary with an orbital period of 143.6 days and an eccentricity of 0.56.
The spectroscopic binary forms a triple system with BD+32 102 , a magnitude 8.6 star located 35.9 arcseconds away. At 55 arcseconds separation is an 11th magnitude companion that is just located on the same line of sight, but at a very different distance from us.
Naming
In Chinese , 奎宿 (Kuí Sù ), meaning Legs (asterism) , refers to an asterism consisting of π Andromedae, η Andromedae , 65 Piscium , ζ Andromedae , ε Andromedae , δ Andromedae , ν Andromedae , μ Andromedae , β Andromedae , σ Piscium , τ Piscium , 91 Piscium , υ Piscium , φ Piscium , χ Piscium and ψ¹ Piscium . Consequently, the Chinese name for π Andromedae itself is 奎宿六 (Kuí Sù liù , English: the Sixth Star of Legs.)
References
^ Brown, A. G. A. ; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties" . Astronomy & Astrophysics . 649 : A1. arXiv :2012.01533 . Bibcode :2021A&A...649A...1G . doi :10.1051/0004-6361/202039657 . S2CID 227254300 . (Erratum: doi :10.1051/0004-6361/202039657e ). Gaia EDR3 record for this source at VizieR .
^ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory , 4 (99): 99, Bibcode :1966CoLPL...4...99J .
^ Eggleton, P. P.; Tokovinin, A. A. (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 . S2CID 14878976 .
^ Cenarro, A. J.; et al. (January 2007), "Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters", Monthly Notices of the Royal Astronomical Society , 374 (2): 664–690, arXiv :astro-ph/0611618 , Bibcode :2007MNRAS.374..664C , doi :10.1111/j.1365-2966.2006.11196.x , S2CID 119428437 .
Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication , Washington: Carnegie Institution of Washington, Bibcode :1953GCRV..C......0W .
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 , S2CID 119257644 .
Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal , 573 (1): 359–365, Bibcode :2002ApJ...573..359A , doi :10.1086/340590 .
(in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 19 日 Archived 2016-03-03 at the Wayback Machine
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