Zeta Andromedae
Zeta Andromedae (Zeta And, ζ Andromedae, ζ And) is a star system in the constellation Andromeda. It is approximately 189 light years from Earth.
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Andromeda |
Right ascension | 00h 47m 20.32547s[1] |
Declination | +24° 16′ 01.8408″[1] |
Apparent magnitude (V) | 3.92 to 4.14[2] |
Characteristics | |
Spectral type | K1III + KV[3] |
U−B color index | +0.90[4] |
B−V color index | +1.12[4] |
R−I color index | +0.59[4] |
Variable type | ELL/RS[2] |
Astrometry | |
Radial velocity (Rv) | −24.43 ± 0.1[5] km/s |
Proper motion (μ) | RA: −101.17[1] mas/yr Dec.: −81.77[1] mas/yr |
Parallax (π) | 17.24 ± 0.26[1] mas |
Distance | 189 ± 3 ly (58.0 ± 0.9 pc) |
Absolute magnitude (MV) | +0.14[3] |
Orbit[3] | |
Period (P) | 17.769426 |
Semi-major axis (a) | 2.7 R* |
Eccentricity (e) | 0.0 |
Inclination (i) | 65 ± 5° |
Details | |
Aa | |
Mass | 2.6 ± 0.4[3] M☉ |
Radius | 15.9 ± 0.8[6] R☉ |
Luminosity | 95.5[3] L☉ |
Surface gravity (log g) | 2.8[3] cgs |
Temperature | 4,665 ± 140[6] K |
Metallicity [Fe/H] | −0.30[3] dex |
Rotation | 17.77 days[7] |
Rotational velocity (v sin i) | 41.4 ± 0.2[3] km/s |
Ab | |
Mass | 0.75[3] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Zeta Andromedae is a spectroscopic binary whose primary is classified as an orange K-type giant with a mean apparent magnitude of +4.08. In addition to brightness variation due to the ellipsoidal shape of the giant primary star, the system is also an RS Canum Venaticorum type variable star. Its brightness varies from magnitude +3.92 to +4.14 with a period of 17.77 days, and its spectrum shows strong and variable Ca II H and K lines.[3] The orbital period of the binary is 17.77 days.
Location
This star's location in the constellation Andromeda can be seen in the following diagram:
Direct imaging
The primary component of this binary system, Zeta Andromedae Aa, is one of the few stars who has been imaged directly using Doppler imaging and long-baseline infrared interferometry. With direct imaging we can recover additional information about this star.
Parameter | Value |
---|---|
Oblateness | 1.060 ± 0.011 |
Polar radius | 15.0 ± 0.8 R☉ |
Axis Inclination[lower-alpha 1] | 70.0 ± 2.8 ° |
Pole angle[lower-alpha 2] | 126 ± 1.9 ° |
Direct imaging also allowed observation of starspots, (the analogue to sunspots), on this star, and their asymmetric distribution showed that the magnetic field of the star is generated by a mechanism different from the solar dynamo.[8] A Sun-like differential rotation of the star was observed instead.[3]
Visual companions
The WDS lists more than one visual companion to the eclipsing binary.[4] B has common proper motion with A. C is probably only a line-of-sight companion that has no physical association. The parallax of the D component has been measured by Gaia and the distance of this star is much different.[9]
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Naming
In Chinese, 奎宿 (Kuí Sù), meaning Legs (asterism), refers to an asterism consisting of ζ Andromedae, η Andromedae, 65 Piscium, ε Andromedae, δ Andromedae, π 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 ζ Andromedae itself is 奎宿二 (Kuí Sù èr, English: the Second Star of Legs.)[11]
Notes
- Azimuthal angle between the rotational axis and our line of sight
- Longitudinal angle between the north pole and the East direction
References
- 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.
- zet And, database entry, The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars, Sternberg Astronomical Institute, Moscow, Russia. Accessed on line August 29, 2008.
- Kővári, Zs.; Bartus, J.; Strassmeier, K. G.; Oláh, K.; Weber, M.; Rice, J. B.; Washuettl, A. (2007). "Doppler imaging of stellar surface structure. XXIII. The ellipsoidal K giant binary ζ Andromedae". Astronomy and Astrophysics. 463 (3): 1071. arXiv:1301.0445. Bibcode:2007A&A...463.1071K. doi:10.1051/0004-6361:20065982.
- HR 215, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line August 29, 2008.
- Karataş, Y.; Bilir, S.; Eker, Z.; Demircan, O. (2004). "Kinematics of chromospherically active binaries and evidence of an orbital period decrease in binary evolution". Monthly Notices of the Royal Astronomical Society. 349 (3): 1069. arXiv:astro-ph/0404219. Bibcode:2004MNRAS.349.1069K. doi:10.1111/j.1365-2966.2004.07588.x. S2CID 15290475.
- Korhonen, H.; Wittkowski, M.; Kovári, Zs.; Granzer, Th.; Hackman, T.; Strassmeier, K. G. (2010). "Ellipsoidal primary of the RS CVn binary ζ Andromedae . Investigation using high-resolution spectroscopy and optical interferometry". Astronomy and Astrophysics. 515: A14. arXiv:1002.4201. Bibcode:2010A&A...515A..14K. doi:10.1051/0004-6361/200913736. S2CID 118683792.
- Strassmeier, Klaus G. (September 2009), "Starspots", The Astronomy and Astrophysics Review, 17 (3): 251–308, Bibcode:2009A&ARv..17..251S, doi:10.1007/s00159-009-0020-6
- Roettenbacher, R.M.; Monnier, J.D.; Korhonen, H.; Aarnio, A.N.; Baron, F.; Che, X.; Harmon, R.O.; Kővári, Zs.; Kraus, S.; Schaefer, G.H.; Torres, G.; Zhao, M.; Ten Brummelaar, T.A.; Sturmann, J.; Sturmann, L. (2016). "No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry". Nature. 533 (7602): 217–220. arXiv:1709.10107. Bibcode:2016Natur.533..217R. doi:10.1038/nature17444. PMID 27144357. S2CID 4466687.
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- Entry 00473+2416, The Washington Double Star Catalog Archived April 12, 2008, at the Wayback Machine, United States Naval Observatory. Accessed on line August 29, 2008.
- (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 19 日
External links
- Zeta Andromedae at Alcyone Software's Star Data Pages
- Image ζ Andromedae
- Rachael Roettenbacher, "How the face of a distant star reveals our place in the cosmos," Aeon Magazine [retrieved July 27, 2016]