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HD 122430

Coordinates:Sky map14h 02m 22.7815s, −27° 25′ 47.183″
From Wikipedia, the free encyclopedia
Star in the constellation Hydra
HD 122430
Observation data
Epoch J2000      Equinox J2000
ConstellationHydra
Right ascension14h 02m 22.78173s[1]
Declination−27° 25′ 47.1992″[1]
Apparent magnitude (V)5.47[2]
Characteristics
Spectral typeK2–3III[3]
B−Vcolor index1.331±0.003[2]
Astrometry
Radial velocity (Rv)−0.61±0.24[1] km/s
Proper motion (μ)RA: −31.861±0.259[1]mas/yr
Dec.: −4.195±0.215[1]mas/yr
Parallax (π)7.3651±0.1407 mas[1]
Distance443 ± 8 ly
(136 ± 3 pc)
Absolute magnitude (MV)−0.17[2]
Details[4]
Mass1.62±0.19 M
Radius21.20±2.06 R
Luminosity189.6±4.2[1] L
Surface gravity (log g)1.96±0.07 cgs
Temperature4,383±19 K
Metallicity[Fe/H]−0.08±0.04 dex
Rotational velocity (v sin i)2.59±0.45 km/s
Age1.98±0.67 Gyr
Other designations
CD−26° 10060,GC 18954,HD 122430,HIP 68581,HR 5265,SAO 182182,GCRV 8247[5]
Database references
SIMBADdata

HD 122430 is singlestar[6] in theequatorialconstellation ofHydra. It has an orange hue and is faintly visible to the naked eye with anapparent visual magnitude of 5.47.[2] The star is located at a distance of 105.6 light years from theSun based onparallax. It has the Bayer designationh Hydrae.[7]

This is an aginggiant star with astellar classification of K2–3III.[3] It has completely run out of thehydrogenfuel that keeps it stable, although it is only two billion years old,[4] younger than the Sun's 4.6 billion years. HD 122430 has a mass of 1.6 times and radius of 22.9 times that of the Sun.[4] Despite its younger age, it has slightly lower metallicity, approximately 90%. It is radiating 190[1] times theluminosity of the Sun from itsphotosphere at aneffective temperature of 4300 K.[4]

A candidateexoplanet was reported orbiting the star via theradial velocity method at a conference in 2003, and designated HD 122430 b. It has anorbital period of 0.94 years and aneccentricity of 0.68.[8] However, a follow-up study by Soto et al. (2015) failed to detect a signal, so it remains unconfirmed.[9]

The HD 122430 planetary system[8]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b(unconfirmed)>3.71MJ1.02344.95±1.080.68±0.09

See also

[edit]

References

[edit]
  1. ^abcdefghBrown, A. G. A.; et al. (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 atVizieR.
  2. ^abcdAnderson, 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 119257644.
  3. ^abHouk, Nancy (1979).Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 3. Ann Arbor, Michigan: Department of Astronomy, University of Michigan.Bibcode:1982mcts.book.....H.
  4. ^abcdJofré, E.; et al. (2015). "Stellar parameters and chemical abundances of 223 evolved stars with and without planets".Astronomy & Astrophysics.574: A50.arXiv:1410.6422.Bibcode:2015A&A...574A..50J.doi:10.1051/0004-6361/201424474.S2CID 53666931.
  5. ^"HD 117207".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-07-23.
  6. ^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.
  7. ^Morton Wagman (2003).Lost Stars: Lost, Missing, and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas-Louis de Lacaille, John Flamsteed, and Sundry Others (2 ed.). McDonald & Woodward Publishing Company.ISBN 978-0-939923-78-6.OCLC 1131243914.
  8. ^abSetiawan, J. (October 2003).Planets around evolved stars. Proceedings of the Conference on Towards Other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets, 22–25 April 2003, Heidelberg, Germany. Vol. 539. Noordwijk, Netherlands: ESA Publications Division. pp. 595–598.Bibcode:2003ESASP.539..595S.ISBN 92-9092-849-2.
  9. ^Soto, M. G.; et al. (August 2015)."RAFT - I. Discovery of new planetary candidates and updated orbits from archival FEROS spectra".Monthly Notices of the Royal Astronomical Society.451 (3):3131–3144.arXiv:1505.04796.Bibcode:2015MNRAS.451.3131S.doi:10.1093/mnras/stv1144.


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