[{"@context":"http:\/\/schema.org\/","@type":"BlogPosting","@id":"https:\/\/wiki.edu.vn\/en\/wiki24\/37-tauri-wikipedia\/#BlogPosting","mainEntityOfPage":"https:\/\/wiki.edu.vn\/en\/wiki24\/37-tauri-wikipedia\/","headline":"37 Tauri – Wikipedia","name":"37 Tauri – Wikipedia","description":"From Wikipedia, the free encyclopedia Star in the constellation Taurus 37 Tauri is a single,[9] orange-hued star in the zodiac","datePublished":"2017-08-08","dateModified":"2017-08-08","author":{"@type":"Person","@id":"https:\/\/wiki.edu.vn\/en\/wiki24\/author\/lordneo\/#Person","name":"lordneo","url":"https:\/\/wiki.edu.vn\/en\/wiki24\/author\/lordneo\/","image":{"@type":"ImageObject","@id":"https:\/\/secure.gravatar.com\/avatar\/c9645c498c9701c88b89b8537773dd7c?s=96&d=mm&r=g","url":"https:\/\/secure.gravatar.com\/avatar\/c9645c498c9701c88b89b8537773dd7c?s=96&d=mm&r=g","height":96,"width":96}},"publisher":{"@type":"Organization","name":"Enzyklop\u00e4die","logo":{"@type":"ImageObject","@id":"https:\/\/wiki.edu.vn\/wiki4\/wp-content\/uploads\/2023\/08\/download.jpg","url":"https:\/\/wiki.edu.vn\/wiki4\/wp-content\/uploads\/2023\/08\/download.jpg","width":600,"height":60}},"image":{"@type":"ImageObject","@id":"https:\/\/en.wikipedia.org\/wiki\/Special:CentralAutoLogin\/start?type=1x1","url":"https:\/\/en.wikipedia.org\/wiki\/Special:CentralAutoLogin\/start?type=1x1","height":"1","width":"1"},"url":"https:\/\/wiki.edu.vn\/en\/wiki24\/37-tauri-wikipedia\/","wordCount":3004,"articleBody":"From Wikipedia, the free encyclopediaStar in the constellation Taurus37 Tauri is a single,[9] orange-hued star in the zodiac constellation of Taurus. It can be seen with the naked eye, having an apparent visual magnitude of 4.36.[2] A magnitude 10.01 visual companion has an angular separation of 134.30\u2033 on a position angle of 138.6\u00b0, as of 2003.[10] Based on an annual parallax shift of 17.43\u00b10.21\u00a0mas,[1] 37 Tauri is about 187\u00a0light years away. It is moving further from the Sun with a heliocentric radial velocity of 9.5\u00a0km\/s.[6]This is an evolved K-type giant star with a stellar classification of K0\u00a0III-IIIb.[3] At the age of 1.39[5] billion years, it has become a red clump giant, indicating that it is generating energy through helium fusion at its core.[11] The star has around double the mass of the Sun and has expanded to 10[7] times the Sun’s radius. It is radiating roughly 60[7] times the Sun’s luminosity from its enlarged photosphere at an effective temperature of 4,732\u00a0K.[5]Chinese astronomy[edit]In Chinese astronomy, 37 Tauri is called \u6708, Pinyin: Yu\u00e8, meaning Moon, because this star is marking itself and stand alone in Moon asterism, Hairy Head mansion (see\u00a0: Chinese constellation).[12]References[edit]^ a b c d e f van Leeuwen, F. (2007), “Validation of the new Hipparcos reduction”, Astronomy and Astrophysics, 474 (2): 653\u2013664, arXiv:0708.1752, Bibcode:2007A&A…474..653V, doi:10.1051\/0004-6361:20078357, S2CID\u00a018759600.^ a b c 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\u00a0119257644.^ a b Keenan, Philip C.; McNeil, Raymond C. (1989), “The Perkins catalog of revised MK types for the cooler stars”, Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS…71..245K, doi:10.1086\/191373.^ a b Ducati, J. R. (2002), “VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson’s 11-color system”, CDS\/ADC Collection of Electronic Catalogues, 2237, Bibcode:2002yCat.2237….0D.^ a b c d e f Luck, R. Earle (2015), “Abundances in the Local Region. I. G and K Giants”, Astronomical Journal, 150 (3), 88, arXiv:1507.01466, Bibcode:2015AJ….150…88L, doi:10.1088\/0004-6256\/150\/3\/88, S2CID\u00a0118505114.^ a b c Massarotti, Alessandro;  et\u00a0al. (January 2008), “Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity”, The Astronomical Journal, 135 (1): 209\u2013231, Bibcode:2008AJ….135..209M, doi:10.1088\/0004-6256\/135\/1\/209, S2CID\u00a0121883397.^ a b c d e f Piau, L.;  et\u00a0al. (2010), “Surface convection and red-giants radii measurements”, Astronomy and Astrophysics, 526: 12, arXiv:1010.3649, Bibcode:2011A&A…526A.100P, doi:10.1051\/0004-6361\/201014442, S2CID\u00a0118533297, A100.^ “37 Tau”. SIMBAD. Centre de donn\u00e9es astronomiques de Strasbourg. Retrieved 2018-03-22.^ 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\u2013879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111\/j.1365-2966.2008.13596.x, S2CID\u00a014878976.^ Mason, B. D.;  et\u00a0al. (2014), “The Washington Visual Double Star Catalog”, The Astronomical Journal, 122 (6): 3466, Bibcode:2001AJ….122.3466M, doi:10.1086\/323920^ Puzeras, E.;  et\u00a0al. (October 2010), “High-resolution spectroscopic study of red clump stars in the Galaxy: iron-group elements”, Monthly Notices of the Royal Astronomical Society, 408 (2): 1225\u20131232, arXiv:1006.3857, Bibcode:2010MNRAS.408.1225P, doi:10.1111\/j.1365-2966.2010.17195.x, S2CID\u00a044228180.^ Ian Ridpath’s Star Tales – Taurus the Bull  "},{"@context":"http:\/\/schema.org\/","@type":"BreadcrumbList","itemListElement":[{"@type":"ListItem","position":1,"item":{"@id":"https:\/\/wiki.edu.vn\/en\/wiki24\/#breadcrumbitem","name":"Enzyklop\u00e4die"}},{"@type":"ListItem","position":2,"item":{"@id":"https:\/\/wiki.edu.vn\/en\/wiki24\/37-tauri-wikipedia\/#breadcrumbitem","name":"37 Tauri – Wikipedia"}}]}]