Star in the constellation Fornax
ζ Fornacis (often Latinised as Zeta Fornacis ) is the Bayer designation for a star in the southern constellation of Fornax . It is faintly visible to the naked eye with an apparent visual magnitude of 5.67. Based upon a measured annual parallax shift of 29.9 mas , it is located at a distance of about 109 light-years from the Sun . The star is drifting further away with a radial velocity of +29 km/s. Positioned about 1.3° to the southeast of Zeta Fornacis is the galaxy NGC 1232 .
This is an F-type main-sequence star with a stellar classification of F4 V. With an estimated age of 1.5 billion years, it has 1.8 times the mass of the Sun and 1.6 times the Sun's radius . The star is radiating 4.77 times the luminosity of the Sun from its photosphere at an effective temperature of 6,699 K . It is spinning with a projected rotational velocity of 84.9 km/s, and has a near-solar metallicity —what astronomers term the abundance of elements other than hydrogen and helium. This star is a probable member of the Hyades Stream —a group of stars that share a common motion through space with the Hyades cluster.
Zeta Fornacis has a common proper motion companion, NLTT 9563, a magnitude 13.50 star with a classification of M 2.5. As of 2004, this companion was positioned at an angular separation of 176.1 arcseconds along a position angle of 288.1°.
References
^ 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 .
^ Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data , SIMBAD , Bibcode :1986EgUBV........0M .
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^ Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics , 542 : A116, arXiv :1204.2459 , Bibcode :2012A&A...542A.116A , doi :10.1051/0004-6361/201118724 , S2CID 53666672 .
^ David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal , 804 (2): 146, arXiv :1501.03154 , Bibcode :2015ApJ...804..146D , doi :10.1088/0004-637X/804/2/146 , S2CID 33401607 .
"zet For" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-01-22.
Bakich, Michael E. (2010), 1,001 Celestial Wonders to See Before You Die: The Best Sky Objects for Star Gazers , The Patrick Moore Practical Astronomy Series, Springer Science & Business Media, p. 400, ISBN 978-1441917775 .
Eggen, O. J. (June 1985), "A systematic search for members of the Hyades Supercluster. IV - The metallic-line stars and ultrashort-period Cepheids", Astronomical Journal , 90 : 1046−1059, Bibcode :1985AJ.....90.1046E , doi :10.1086/113812 .
^ Gould, Andrew; Chanamé, Julio (February 2004), "New Hipparcos-based Parallaxes for 424 Faint Stars", The Astrophysical Journal Supplement Series , 150 (2): 455−464, arXiv :astro-ph/0309001 , Bibcode :2004ApJS..150..455G , doi :10.1086/381147 , S2CID 8494577 .
Scholz, R.-D.; et al. (October 2005), "Search for nearby stars among proper motion stars selected by optical-to-infrared photometry. III. Spectroscopic distances of 322 NLTT stars", Astronomy and Astrophysics , 442 (1): 211−227, arXiv :astro-ph/0507284 , Bibcode :2005A&A...442..211S , doi :10.1051/0004-6361:20053004 , S2CID 7013323 .
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