Star in the constellation Hercules
32 Ophiuchi is a single[ 12] star located about 407[ 2] light years away from the Sun in the constellation Hercules . It is moving further away from the Sun with a heliocentric radial velocity of +43 km/s.[ 1] and is visible to the naked eye as a dim, red-hued star with an apparent visual magnitude of 4.97.[ 1]
This is an aging red giant star on the asymptotic giant branch [ 4] with a stellar classification of M3−III.[ 5] Having exhausted the supply of hydrogen at its core it has expanded to 63 times the radius of the Sun .[ 8] The star is radiating over a thounsand times the luminosity of the Sun [ 7] from its swollen photosphere at an effective temperature of around 3,728 K .[ 10]
32 Ophiuchi is a suspected variable star with a brightness range of about 0.1 magnitudes .[ 6]
References
^ a b c d e f g 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 .
XHIP record for this object at VizieR .
^ a b c d e f Vallenari, A.; et al. (Gaia collaboration) (2023), "Gaia Data Release 3. Summary of the content and survey properties" , Astronomy and Astrophysics , 674 : A1, arXiv :2208.00211 , Bibcode :2023A&A...674A...1G , doi :10.1051/0004-6361/202243940 , S2CID 244398875 .
Gaia DR3 record for this source at VizieR .
^ Lebzelter, Thomas; Hinkle, Kenneth H.; Straniero, Oscar; Lambert, David L.; Pilachowski, Catherine A.; Nault, Kristie A. (2019), "Carbon and Oxygen Isotopic Ratios. II. Semiregular Variable M Giants", The Astrophysical Journal , 886 (2): 117, arXiv :1912.04386 , Bibcode :2019ApJ...886..117L , doi :10.3847/1538-4357/ab4e9b .
^ a b Eggen, Olin J. (July 1992), "Asymptotic giant branch stars near the sun", Astronomical Journal , 104 (1): 275– 313, Bibcode :1992AJ....104..275E , doi :10.1086/116239 .
^ a b Keenan, P.; McNeil, R. (October 1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series , 71 : 245– 266, Bibcode :1989ApJS...71..245K , doi :10.1086/191373 .
^ a b Samus, N. N.; Durlevich, O. V.; et al. (2004), "VizieR Online Data Catalog: Combined General Catalogue of Variable Stars (Samus+ 2004)", Vizier Online Data Catalog , Bibcode :2004yCat.2250....0S .
^ a b c Charbonnel, C.; et al. (January 2020), "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era", Astronomy & Astrophysics , 633 : A34, arXiv :1910.12732 , Bibcode :2020A&A...633A..34C , doi :10.1051/0004-6361/201936360 , ISSN 0004-6361 .
^ a b Baines, Ellyn K.; Clark, James H.; Kingsley, Bradley I.; Schmitt, Henrique R.; Stone, Jordan M. (2025-05-07), "Vintage NPOI: New and Updated Angular Diameters for 145 Stars", The Astronomical Journal , 169 (6): 293, arXiv :2506.02912 , Bibcode :2025AJ....169..293B , doi :10.3847/1538-3881/adc930 , ISSN 1538-3881 .
^ a b Khalatyan, A.; Anders, F.; Chiappini, C.; Queiroz, A. B. A.; Nepal, S.; Dal Ponte, M.; Jordi, C.; Guiglion, G.; Valentini, M.; Torralba Elipe, G.; Steinmetz, M.; Pantaleoni-González, M.; Malhotra, S.; Jiménez-Arranz, Ó.; Enke, H.; Casamiquela, L.; Ardèvol, J. (2024), "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost", Astronomy and Astrophysics , 691 : A98, arXiv :2407.06963 , Bibcode :2024A&A...691A..98K , doi :10.1051/0004-6361/202451427 .
^ a b Deacon, N. R.; Henning, Th; Kossakowski, D. E. (2019), "Data-driven stellar parameters for southern TESS FGK targets", Monthly Notices of the Royal Astronomical Society , 486 (1): 251, arXiv :1903.03115 , Bibcode :2019MNRAS.486..251D , doi :10.1093/mnras/stz722 .
^ "HD 154143" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-06-19 .
^ 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 , S2CID 14878976 .