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HD 101930

Coordinates:Sky map11h 43m 30.11s, −58° 00′ 24.793″
From Wikipedia, the free encyclopedia
Star in the constellation Centaurus
HD 101930
Observation data
Epoch J2000      Equinox J2000
ConstellationCentaurus
Right ascension11h 43m 30.11338s[1]
Declination–58° 00′ 24.7787″[1]
Apparent magnitude (V)8.21[2]
Characteristics
Spectral typeK2 V+[3]
B−Vcolor index+0.91[4]
Astrometry
Radial velocity (Rv)+18.36[5] km/s
Proper motion (μ)RA: +16.680mas/yr[1]
Dec.: +349.125mas/yr[1]
Parallax (π)33.3814±0.0180 mas[1]
Distance97.71 ± 0.05 ly
(29.96 ± 0.02 pc)
Absolute magnitude (MV)+5.88[2]
Details
Mass0.82[6] M
Radius0.87+0.05
−0.04
[7] R
Luminosity0.43±0.01[8] L
Surface gravity (log g)4.40±0.11[9] cgs
Temperature5,079±62[5] K
Metallicity [Fe/H]+0.1±0.03[10] dex
Rotational velocity (v sin i)2[11] km/s
Age5.4±4.4[8] Gyr
Other designations
CD-57°4096,GJ 3683,HIP 57172,LTT 4350,NLTT 28356,SAO 239322[12]
Database references
SIMBADdata
ARICNSdata

HD 101930, also known asGliese 3683, is an orange huedstar with an orbitingexoplanet located in the southernconstellationCentaurus. 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 of18.4 km/s.[5] It has a relatively largeproper motion, traversing thecelestial sphere with anangular velocity of0.320·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 of5,079 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 ofkm/s.[11]

A 2007 multicity survey found a co-moving companion located73 away,[14] making it abinary star. It has a class of M0-1[15] and amass of 0.7 M.[14]

Planetary system

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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]

The HD 101930 planetary system[5]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b≥ 0.30 MJ0.30270.46 ± 0.180.11 ± 0.02

See also

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References

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  1. ^abcdeVallenari, 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.
  2. ^abcAnderson, 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.
  3. ^abGray, 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.
  4. ^Cousins, A. W. J.; Stoy, R. H. (1963).Photoelectric magnitudes and colours of southern stars.Bibcode:1963pmcs.book.....C.
  5. ^abcdefLovis, 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.
  6. ^abMargaret C Turnbull (2015). "ExoCat-1: The Nearby Stellar Systems Catalog for Exoplanet Imaging Missions".arXiv:1510.01731 [astro-ph.SR].
  7. ^abStassun, 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.
  8. ^abcdBonfanti, 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.
  9. ^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.
  10. ^abTsantaki, 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.
  11. ^abLlorente 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.
  12. ^"HD 101930".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedMay 22, 2009.
  13. ^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.
  14. ^abMugrauer, 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.
  15. ^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.

External links

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