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HD 126614

Coordinates:Sky map14h 26m 48.2804s, −05° 10′ 40.009″
From Wikipedia, the free encyclopedia
Multiple star system in the constellation Virgo
HD 126614
Observation data
Epoch J2000      Equinox J2000
ConstellationVirgo[1]
HD 126614 A
Right ascension14h 26m 48.27949s[2]
Declination−05° 10′ 40.0131″[2]
Apparent magnitude (V)8.81±0.03[3]
LP 680-57
Right ascension14h 26m 45.83640s[4]
Declination−05° 10′ 19.4279″[4]
Apparent magnitude (V)16.68±0.20[3]
Characteristics
Spectral typeG8IV[5] + M[6] + M5.5V[7]
Apparent magnitude (B)9.620[1]
Apparent magnitude (J)7.470±0.021[1]
Apparent magnitude (H)7.160±0.042[1]
Apparent magnitude (K)7.060±0.036[1]
B−Vcolor index0.810±0.004[1]
Astrometry
HD 126614 A
Radial velocity (Rv)−32.897±0.0042[8] km/s
Proper motion (μ)RA: −149.760±0.023mas/yr[2]
Dec.: −145.837±0.018mas/yr[2]
Parallax (π)13.6633±0.0166 mas[2]
Distance238.7 ± 0.3 ly
(73.19 ± 0.09 pc)
Absolute magnitude (MV)4.52[1]
LP 680-57
Radial velocity (Rv)−29.45±5.52[4] km/s
Proper motion (μ)RA: −147.861±0.038mas/yr[4]
Dec.: −149.118±0.034mas/yr[4]
Parallax (π)13.6050±0.0316 mas[4]
Distance239.7 ± 0.6 ly
(73.5 ± 0.2 pc)
Absolute magnitude (MV)12.02[6]
Orbit[9]
CompanionHD 126614 B
Period (P)59.979+4.696
−5.059
 yr
Semi-major axis (a)15.229+0.984
−1.094
 AU
Eccentricity (e)0.056+0.017
−0.018
Inclination (i)16.294+0.881
−0.771
°
Longitude of the node (Ω)284.664+2.600
−3.304
°
Periastronepoch (T)2450124.747+26.090
−28.486
Argument of periastron (ω)
(secondary)
240.567+30.578
−43.150
°
Semi-amplitude (K1)
(primary)
0.167573+0.012902
−0.011124
 km/s
Details
HD 126614 A
Mass1.145±0.03[6] M
Radius1.09±0.06[6] R
Luminosity1.21±0.19[6] L
Surface gravity (log g)4.39±0.08[6] cgs
Temperature5,585±44[6] K
Metallicity+0.56±0.04[6]
Rotation~99 days[6]
Rotational velocity (v sin i)2.0±0.5[6] km/s
Age7.2±2.0[6] Gyr
HD 126614 B
Mass81.128+7.778
−7.922
[9] MJup
LP 680-57
Mass0.32[10][11] M
Radius0.32[10][11] R
Luminosity0.0106[10] L
Surface gravity (log g)4.93[10] cgs
Temperature3,275[10][11] K
Metallicity[Fe/H]+0.46[7] dex
Age3.6  – 6.0[7] Gyr
Other designations
WDS J14268-0511[12]
HD 126614 AB:BD−04°3690,HD 126614,HIP 70623,SAO 139932,PPM 197558,G 124-40,LTT 5698,NLTT 37355[12]
LP 680-57:LP 680-57,NLTT 37349[13]
Database references
SIMBADA
C
Exoplanet Archivedata

HD 126614 is atrinary star[14] system in theequatorialconstellation ofVirgo. The primary member, designated component A, is host to anexoplanetary companion. With anapparent visual magnitude of 8.81,[1] it is too faint to be seen with the naked eye. The system is located at a distance of 239 light years from theSun based onparallax measurements,[2] but is drifting closer with aradial velocity of −33 km/s.[8]

Stellar system

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HD 126614 A

[edit]

The primary is alateG-type star with astellar classification of G8IV.[5] It is a supermetal-rich star; among the most metal-rich stars currently known.[15] This is most likely anevolvingsubgiant star, but the very high metallicity makes comparisons to standard spectral types difficult.[16]

HD 126614 C

[edit]

In 2010, a close stellar companion was resolved and designated component C. This object is a faintred dwarf at anangular separation of0.5, which corresponds to a projected physical separation of~ 36 AU.[16] More recent observations usingradial velocity andastrometry have refined the parameters of HD 126614 C. It has an orbital period of about 60 years, with a smallersemi-major axis of 15 AU and a very low mass of81.1 MJ.[9] This mass is very near the mass limit allowed forhydrogen fusion.

HD 126614 B

[edit]

The outer companion, designated LP 680-57, was first reported in 1960 with theW. J. Luyten proper motion catalog.[17] It is a magnitude 17.0 red dwarf with a class of M5.5,[7] located at anangular separation of41.90″ from the primary along aposition angle of 299°, as of 2015.[17] They have a physicalprojected separation of3,040 AU.[7] Thecommon proper motion of the system has been confirmed, indicating that they are gravitationally bound.[16] Many multiple star catalogues still refer to this companion as component B, as it was known prior to the discovery of the closer companion.[17]

Planetary system

[edit]

A Doppler search for giant planets begun in 1997 at theKeck Observatory provided an 11 year baseline for detecting periodicity in the primary star's radial velocity data. In 2010, a Jovian companion was announced with anorbital period of 3.41 years.[6] In 2022, the inclination and true mass of HD 126614 Ab were measured viaastrometry.[9]

The HD 126614 A planetary system[9]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(years)
EccentricityInclinationRadius
b0.339+0.204
−0.019
 MJ
2.249+0.088
−0.096
3.442+0.016
−0.017
0.548+0.063
−0.062
97.477+35.340
−37.849
°

See also

[edit]

References

[edit]
  1. ^abcdefghAnderson, 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.
  2. ^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.
  3. ^ab"HD 126614".NASA Exoplanet Archive. Retrieved30 August 2022.
  4. ^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.
  5. ^abHouk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  6. ^abcdefghijklHoward, Andrew W.; et al. (2010). "The California Planet Survey. I. Four New Giant Exoplanets".The Astrophysical Journal.721 (2):1467–1481.arXiv:1003.3488.Bibcode:2010ApJ...721.1467H.doi:10.1088/0004-637X/721/2/1467.S2CID 14147776.
  7. ^abcdeDeacon, Niall R.; et al. (2014). "Wide Cool and Ultracool Companions to Nearby Stars from Pan-STARRS 1".The Astrophysical Journal.792 (2). 119.arXiv:1407.2938.Bibcode:2014ApJ...792..119D.doi:10.1088/0004-637X/792/2/119.S2CID 38354181.
  8. ^abSoubiran, C.; et al. (2018). "Gaia Data Release 2. The catalogue of radial velocity standard stars".Astronomy and Astrophysics.616: A7.arXiv:1804.09370.Bibcode:2018A&A...616A...7S.doi:10.1051/0004-6361/201832795.S2CID 52952408.
  9. ^abcdeFeng, Fabo; Butler, R. Paul; et al. (August 2022)."3D Selection of 167 Substellar Companions to Nearby Stars".The Astrophysical Journal Supplement Series.262 (21): 21.arXiv:2208.12720.Bibcode:2022ApJS..262...21F.doi:10.3847/1538-4365/ac7e57.S2CID 251864022.
  10. ^abcdeStassun, Keivan G.; Oelkers, Ryan J.; Pepper, Joshua; Paegert, Martin; De Lee, Nathan; Torres, Guillermo; Latham, David W.; Charpinet, Stéphane; Dressing, Courtney D.; Huber, Daniel; Kane, Stephen R.; Lépine, Sébastien; Mann, Andrew; Muirhead, Philip S.; Rojas-Ayala, Bárbara; Silvotti, Roberto; Fleming, Scott W.; Levine, Al; Plavchan, Peter; the TESS Target Selection Working Group (2018)."The TESS Input Catalog and Candidate Target List".The Astronomical Journal.156 (3): 102.arXiv:1706.00495.Bibcode:2018AJ....156..102S.doi:10.3847/1538-3881/aad050.S2CID 73582386.
  11. ^abcMuirhead, Philip S.; Dressing, Courtney D.; Mann, Andrew W.; Rojas-Ayala, Bárbara; Lépine, Sébastien; Paegert, Martin; De Lee, Nathan; Oelkers, Ryan (2018)."A Catalog of Cool Dwarf Targets for the Transiting Exoplanet Survey Satellite".The Astronomical Journal.155 (4): 180.arXiv:1710.00193.Bibcode:2018AJ....155..180M.doi:10.3847/1538-3881/aab710.S2CID 119184794.
  12. ^ab"HD 126614".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2021-10-10.
  13. ^"LP 680-57".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2022-08-30.
  14. ^Busetti, F.; et al. (November 2018). "Stability of planets in triple star systems".Astronomy & Astrophysics.619: 12.arXiv:1811.08221.Bibcode:2018A&A...619A..91B.doi:10.1051/0004-6361/201833097.S2CID 119477324. A91.
  15. ^Castro, Sandra; et al. (July 1997). "High-Resolution Abundance Analysis of Very Metal-rich Stars in the Solar Neighborhood".Astronomical Journal.114:376–387.arXiv:astro-ph/9704220.Bibcode:1997AJ....114..376C.doi:10.1086/118481.S2CID 119368399.
  16. ^abcLodieu, N.; et al. (September 2014). "Binary frequency of planet-host stars at wide separations. A new brown dwarf companion to a planet-host star".Astronomy & Astrophysics.569: 14.arXiv:1408.1208.Bibcode:2014A&A...569A.120L.doi:10.1051/0004-6361/201424210.S2CID 118516214. A120.
  17. ^abcMason, B. D.; et al. (2014)."The Washington Visual Double Star Catalog".The Astronomical Journal.122 (6):3466–3471.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.


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