Star in the constellation Centaurus
HD 101930 , also known asGliese 3683 , is an orange huedstar with an orbitingexoplanet located in the southernconstellation Centaurus . It has anapparent magnitude of 8.21,[ 2] making it faintly visible inbinoculars but not to thenaked eye . The system is located relatively close at a distance of 98light years [ 1] but is receding with a heliocentricradial velocity of 18.4 km/s .[ 5] It has a relatively largeproper motion , traversing thecelestial sphere with anangular velocity of 0.320″ ·yr−1 .[ 13]
HD 101930 has astellar classification of K2 V+,[ 3] indicating that it is an ordinaryK-type main-sequence star . It has a current mass of 0.82 M ☉ [ 6] and is said to be 5.4billion years old,[ 8] which is slightly older than theSun . The object has 87% theradius of the Sun [ 7] and aneffective temperature of 5,079 K .[ 5] When combined, these parameters yield aluminosity 43% that of theSun from itsphotosphere .[ 8] As expected with planetary hosts, HD 101930 is metal enriched, having ametallicity 26% above solar levels.[ 10] The star'sprojected rotational velocity is similar to the Sun's, having a value of 2 km/s .[ 11]
A 2007 multicity survey found a co-moving companion located 73″ away,[ 14] making it abinary star . It has a class of M0-1[ 15] and amass of 0.7 M ☉ .[ 14]
In 2005, the discovery of an exoplanet orbiting the star was announced. This is another discovery using theradial velocity method with theHARPS spectrograph . As theinclination of theorbital plane is unknown, only a lower bound on the mass can be determined. It has at least 30% of themass of Jupiter .[ 5]
^a b c d e 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 atVizieR .^a b c Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters .38 (5):331– 346.arXiv :1108.4971 .Bibcode :2012AstL...38..331A .doi :10.1134/S1063773712050015 .eISSN 1562-6873 .ISSN 1063-7737 .S2CID 119257644 . ^a b Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (2 June 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 .eISSN 1538-3881 .ISSN 0004-6256 . ^ Cousins, A. W. J.; Stoy, R. H. (1963).Photoelectric magnitudes and colours of southern stars .Bibcode :1963pmcs.book.....C . ^a b c d e f Lovis, C.; Mayor, M.; Bouchy, F.; Pepe, F.; Queloz, D.; Santos, N. C.; Udry, S.; Benz, W.; Bertaux, J.-L.; Mordasini, C.; Sivan, J.-P. (30 June 2005)."The HARPS search for southern extra-solar planets" .Astronomy & Astrophysics .437 (3):1121– 1126.arXiv :astro-ph/0503660 .Bibcode :2005A&A...437.1121L .doi :10.1051/0004-6361:20052864 .eISSN 1432-0746 .ISSN 0004-6361 .S2CID 119492030 . ^a b Margaret C Turnbull (2015). "ExoCat-1: The Nearby Stellar Systems Catalog for Exoplanet Imaging Missions".arXiv :1510.01731 [astro-ph.SR ]. ^a b Stassun, Keivan G.; et al. (9 September 2019)."The RevisedTESS 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 .eISSN 1538-3881 . ^a b c d Bonfanti, A.; Ortolani, S.; Piotto, G.; Nascimbeni, V. (12 February 2015)."Revising the ages of planet-hosting stars" .Astronomy & Astrophysics .575 : A18.arXiv :1411.4302 .Bibcode :2015A&A...575A..18B .doi :10.1051/0004-6361/201424951 .eISSN 1432-0746 .ISSN 0004-6361 .S2CID 54555839 . ^ Sousa, S. G.; Santos, N. C.; Mayor, M.; Udry, S.; Casagrande, L.; Israelian, G.; Pepe, F.; Queloz, D.; Monteiro, M. J. P. F. G. (4 June 2008)."Spectroscopic parameters for 451 stars in the HARPS GTO planet search program" .Astronomy & Astrophysics .487 (1):373– 381.arXiv :0805.4826 .Bibcode :2008A&A...487..373S .doi :10.1051/0004-6361:200809698 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b Tsantaki, M.; Sousa, S. G.; Santos, N. C.; Montalto, M.; Delgado-Mena, E.; Mortier, A.; Adibekyan, V.; Israelian, G. (October 2014)."Spectroscopic parameters for solar-type stars with moderate-to-high rotation" .Astronomy & Astrophysics .570 : A80.arXiv :1407.6765 .Bibcode :2014A&A...570A..80T .doi :10.1051/0004-6361/201424257 .eISSN 1432-0746 .ISSN 0004-6361 . ^a b Llorente de Andrés, F.; Chavero, C.; de la Reza, R.; Roca-Fàbrega, S.; Cifuentes, C. (October 2021)."The evolution of lithium in FGK dwarf stars" .Astronomy & Astrophysics .654 : A137.arXiv :2108.05852 .Bibcode :2021A&A...654A.137L .doi :10.1051/0004-6361/202141339 .eISSN 1432-0746 .ISSN 0004-6361 . ^ "HD 101930" .SIMBAD .Centre de données astronomiques de Strasbourg . RetrievedMay 22, 2009 .^ Luyten, W. J. (June 1995). "NLTT Catalogue (Luyten, 1979)".VizieR On-line Data Catalog: I/98A. Originally Published in: 1979nltt.book.....L .Bibcode :1995yCat.1098....0L . ^a b Mugrauer, M.; Seifahrt, A.; Neuhauser, R. (11 July 2007)."The multiplicity of planet host stars - new low-mass companions to planet host stars" .Monthly Notices of the Royal Astronomical Society .378 (4):1328– 1334.arXiv :0704.1767 .Bibcode :2007MNRAS.378.1328M .doi :10.1111/j.1365-2966.2007.11858.x .eISSN 1365-2966 .ISSN 0035-8711 . ^ Lindgren, Sara; Heiter, Ulrike; Seifahrt, Andreas (February 2016)."Metallicity determination of M dwarfs" .Astronomy & Astrophysics .586 : A100.arXiv :1510.06642 .Bibcode :2016A&A...586A.100L .doi :10.1051/0004-6361/201526602 .eISSN 1432-0746 .ISSN 0004-6361 .