[{"@context":"http:\/\/schema.org\/","@type":"BlogPosting","@id":"https:\/\/wiki.edu.vn\/en\/wiki24\/hd-44131-wikipedia\/#BlogPosting","mainEntityOfPage":"https:\/\/wiki.edu.vn\/en\/wiki24\/hd-44131-wikipedia\/","headline":"HD 44131 – Wikipedia","name":"HD 44131 – Wikipedia","description":"From Wikipedia, the free encyclopedia Star in the constellation Orion HD 44131 is a star in the equatorial constellation of","datePublished":"2019-08-01","dateModified":"2019-08-01","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:\/\/upload.wikimedia.org\/wikipedia\/commons\/thumb\/a\/a8\/HD44131LightCurve.png\/220px-HD44131LightCurve.png","url":"https:\/\/upload.wikimedia.org\/wikipedia\/commons\/thumb\/a\/a8\/HD44131LightCurve.png\/220px-HD44131LightCurve.png","height":"143","width":"220"},"url":"https:\/\/wiki.edu.vn\/en\/wiki24\/hd-44131-wikipedia\/","wordCount":2850,"articleBody":"From Wikipedia, the free encyclopediaStar in the constellation OrionHD 44131 is a star in the equatorial constellation of Orion, positioned near the eastern constellation border with Monoceros. It has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.91.[2] The star is located at a distance of approximately 465\u00a0light years from the Sun based on parallax,[1] and it is drifting further away with a radial velocity of +48.6\u00a0km\/s.[6] Based on radial velocity variations, it is a candidate spectroscopic binary system and a preliminary orbital solution was published in 1991 with a period of 9.29\u00a0yr. However, these velocity variations may be due to other causes.[9]  This is an aging red giant star currently on the asymptotic giant branch[3] with a stellar classification of M1III.[4] With the supply of core hydrogen exhausted, this star has cooled and expanded off the main sequence. It is now estimated to have 56 times the radius of the Sun and is radiating 673 times the Sun’s luminosity from its swollen photosphere at an effective temperature of 3,932\u00a0K.[7] This is a periodic variable of unknown type with a frequency of 0.11212 cycles per day (period of 8.9\u00a0days) and an amplitude of 0.0106 in magnitude.[11]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. Vizier catalog entry^ 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. Vizier catalog entry^ a b Eggen, Olin J. (July 1992), “Asymptotic giant branch stars near the sun”, Astronomical Journal, 104 (1): 275\u2013313, Bibcode:1992AJ….104..275E, doi:10.1086\/116239.^ a b Houk, N.; Swift, C. (1999). “Michigan catalogue of two-dimensional spectral types for the HD Stars”. Michigan Spectral Survey. 5. Bibcode:1999MSS…C05….0H.^ a b Mallama, A. (2014). “Sloan Magnitudes for the Brightest Stars”. The Journal of the American Association of Variable Star Observers. 42 (2): 443. Bibcode:2014JAVSO..42..443M.Vizier catalog entry^ a b Gontcharov, G. A. (2006). “Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system”. Astronomy Letters. 32 (11): 759\u2013771. arXiv:1606.08053. Bibcode:2006AstL…32..759G. doi:10.1134\/S1063773706110065. S2CID\u00a0119231169.^ a b c d Brown, A. G. A.;  et\u00a0al. (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.^ “HD 44131”. SIMBAD. Centre de donn\u00e9es astronomiques de Strasbourg. Retrieved 2020-11-21.^ Mazeh, Tsevi;  et\u00a0al. (July 1996). “Spectroscopic Orbits for Three Binaries with Low-Mass Companions and the Distribution of Secondary Masses near the Substellar Limit”. Astrophysical Journal. 466: 415. Bibcode:1996ApJ…466..415M. doi:10.1086\/177521.^ “Light Curve”. Hipparcos ESA. ESA. Retrieved 11 October 2022.^ Koen, Chris; Eyer, Laurent (March 2002). “New periodic variables from the Hipparcos epoch photometry”. Monthly Notices of the Royal Astronomical Society. 331 (1): 45\u201359. arXiv:astro-ph\/0112194. Bibcode:2002MNRAS.331…45K. doi:10.1046\/j.1365-8711.2002.05150.x. S2CID\u00a010505995.Wikimedia ErrorOur servers are currently under maintenance or experiencing a technical problem.Please try again in a few\u00a0minutes.See the error message at the bottom of this page for more\u00a0information. "},{"@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\/hd-44131-wikipedia\/#breadcrumbitem","name":"HD 44131 – Wikipedia"}}]}]