Theta Eridani
Star in the constellation Eridanus
Theta Eridani , Latinized from θ Eridani , is a binary system in the constellation of Eridanus with a combined apparent magnitude of 2.88.[ 6] Its two components are designated θ1 Eridani , formally named Acamar (the traditional name of the system),[ 13] [ 14] and θ2 Eridani . The system's distance from the Sun based on parallax measurements is approximately 165 light-years .
Nomenclature
Theta Eridani is the system's Bayer designation ; θ1 and θ2 Eridani those of its two components.
The system bore the traditional name Acamar, derived from the Arabic آخِر النَّهْر [citation needed ] Ākhir an-nahr , which means "the end of the river", via a Roman-alphabet handwriting misread "rn" to "m". In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[ 15] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems .[ 16] It approved the name "Acamar" for θ1 Eridani on 20 July 2016 and it is now so entered in the IAU Catalog of Star Names.[ 14]
The term "Ākhir an-nahr", or "Achr al Nahr", appeared in the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket , which was translated into Latin as Postrema Fluminis .[ 17]
Historically, Acamar represented the end of the constellation Eridanus.[ 8] [ 18] Now that distinction is held by the star Achernar , which shares the same Arabic etymology . Achernar is not visible from the Greek isles (latitudes > 33° North),[ 19] hence the choice of Acamar as the river's end during the time of Hipparchus and, later, Ptolemy .
In Chinese , 天園 (Tiān Yuán ), meaning Celestial Orchard , refers to an asterism consisting of Theta Eridani, Chi Eridani , Phi Eridani , Kappa Eridani , HD 16754 , HD 23319 , HD 24072 , HD 24160 , Upsilon4 Eridani , Upsilon3 Eridani , Upsilon2 Eridani and Upsilon1 Eridani .[ 20] Consequently, the Chinese name for Theta Eridani itself is 天園六 (Tiān Yuán liù , English: the Sixth Star of Celestial Orchard ).[ 21]
Stellar system
Theta Eridani is a binary system with some evidence suggesting it is part of a multiple star system .[ 7] [ 22] The main star, θ1 Eridani, is of spectral class A4 with a +3.2 apparent magnitude . Its companion star, θ2 Eridani, is of spectral class A1 with an apparent magnitude of +4.1. The angular separation of the two stars is equal to 8.3 arcseconds .[ 8]
Notes
^ Retrieved from a luminosity of 96 L ☉ and a temperature of 8200 K [ 8]
References
^ a b c d e 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 .
^ a b Fabricius, C.; Høg, E.; Makarov, V. V.; Mason, B. D.; Wycoff, G. L.; Urban, S. E. (1 March 2002). "The Tycho double star catalogue" . Astronomy and Astrophysics . 384 : 180–189. Bibcode :2002A&A...384..180F . doi :10.1051/0004-6361:20011822 . ISSN 0004-6361 .
^ a b c d e 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 .
^ a b Gray, R. O.; et al. (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 .
^ a b Hoffleit; et al. (1991). "Bright Star Catalogue" . VizieR (5th Revised ed.). Centre de Données astronomiques de Strasbourg . Retrieved 2010-02-24 .
^ a b c d 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 .
^ a b NSV 01002, database entry, New Catalogue of Suspected Variable Stars, the improved version , Sternberg Astronomical Institute, Moscow, Russia. Accessed on line February 26, 2010.
^ a b c d e f Kaler, James B. "ACAMAR (Theta Eridani)" . Stars . University of Illinois. Retrieved 2010-02-24 .
^ Ammler-von Eiff, M.; Reiners, A. (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 . ISSN 0004-6361 .
^ a b c d Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; de Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18" . Astronomy & Astrophysics . 628 : A94. arXiv :1904.11302 . Bibcode :2019A&A...628A..94A . doi :10.1051/0004-6361/201935765 . ISSN 0004-6361 .
^ a b Stassun, Keivan G.; et al. (2019-10-01). "The Revised TESS Input Catalog and Candidate Target List" . The Astronomical Journal . 158 (4): 138. arXiv :1905.10694 . Bibcode :2019AJ....158..138S . doi :10.3847/1538-3881/ab3467 . hdl :1721.1/124721 . ISSN 0004-6256 . S2CID 166227927 .
^ Díaz, C. G.; et al. (July 2011). "Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum". Astronomy & Astrophysics . 531 : A143. arXiv :1012.4858 . Bibcode :2011A&A...531A.143D . doi :10.1051/0004-6361/201016386 . S2CID 119286673 .
^ Rumrill, H. B. (June 1936). "Star Name Pronunciation" . Publications of the Astronomical Society of the Pacific . 48 (283). San Francisco, California: 139. Bibcode :1936PASP...48..139R . doi :10.1086/124681 . S2CID 120743052 .
^ a b "IAU Catalog of Star Names" . Retrieved 28 July 2016 .
^ "IAU Working Group on Star Names (WGSN)" . Retrieved 22 May 2016 .
^ "WG Triennial Report (2015-2018) - Star Names" (PDF) . p. 5. Retrieved 2018-07-14 .
^ Knobel, E. B. (June 1895). "Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket" . Monthly Notices of the Royal Astronomical Society . 55 : 429. Bibcode :1895MNRAS..55..429K . doi :10.1093/mnras/55.8.429 .
^ Rogers, J. H. (1998). "Origins of the ancient constellations: II. The Mediterranean traditions". Journal of the British Astronomical Association . 108 (2): 79–89. Bibcode :1998JBAA..108...79R .
^ Larry Sessions. "Achernar: End of the River" . EarthSky Tonight Post 06-29-2009. Retrieved 2010-02-26 .
^ (in Chinese) 中國星座神話 , written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7 .
^ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 Archived 2010-09-03 at the Wayback Machine , Hong Kong Space Museum. Accessed on line November 23, 2010.
^ "Acamar" . Alcyone Bright Star Catalogue. Retrieved 2010-02-26 .