72 Leonis is a single[9]variable star in the zodiac constellation of Leo, located roughly 1,000light years away from the Sun.[1] It has the variable star designationFN Leonis; 72 Leonis is the Flamsteed designation. In Chinese astronomy, 72 Leonis is called 虎賁, Pinyin: Hǔbēn, meaning Emperor’s Bodyguard, because this star is marking itself and stands alone in the Emperor’s Bodyguard asterism, Supreme Palace enclosure mansion (see: Chinese constellation).[10] It is dedicated to the memory of Julio Cubillas, who died in December 2020, by the White Dwarf Research Corporation.[11]
Single, variable M-type giant star in the constellation Leo
This object is visible to the naked eye as a red-hued star with an apparent visual magnitude of 4.56.[4] It is an evolved bright giant with a stellar classification of M3IIb and was listed as a spectral standard star for that class.[3] The star is classified as an irregular variable of type LC, ranging from Hipparcos magnitude 4.56 down to 4.64.[5] It has a radius 162 to 179[12] times that of the Sun and radiates 5,407[13] times the Sun's luminosity at an effective temperature of around 3,734K.[14] The star is moving away from the Earth with a heliocentric radial velocity of 15km/s.[4]
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.
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.
Baines, Ellyn K.; Armstrong, J. Thomas; Schmitt, Henrique R.; Zavala, R. T.; Benson, James A.; Hutter, Donald J.; Tycner, Christopher; Van Belle, Gerard T. (2018), "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer", The Astronomical Journal, 155 (1): 30, arXiv:1712.08109, Bibcode:2018AJ....155...30B, doi:10.3847/1538-3881/aa9d8b, S2CID119427037.
McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017), "Fundamental parameters and infrared excesses of Tycho-Gaia stars", Monthly Notices of the Royal Astronomical Society, 471 (1): 770, arXiv:1706.02208, Bibcode:2017MNRAS.471..770M, doi:10.1093/mnras/stx1433, S2CID73594365.
"72 Leo". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-02-09.
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): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID14878976.
Leo the Lion, Ian Ridpath's Startales, retrieved 2019-02-10.
Dyck, H. M.; etal. (1998), "Radii and Effective Temperatures for K and M Giants and Supergiants. II", The Astronomical Journal, 116 (2): 981, Bibcode:1998AJ....116..981D, CiteSeerX10.1.1.24.1889, doi:10.1086/300453.
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