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HD 22781

Coordinates:Sky map03h 40m 49.5246s, +31° 49′ 34.6489″
From Wikipedia, the free encyclopedia
Star in the constellation Perseus
HD 22781
Observation data
Epoch J2000      Equinox J2000
ConstellationPerseus
Right ascension03h 40m 49.5246s[1]
Declination+31° 49′ 34.6489″[1]
Apparent magnitude (V)8.78[2]
Characteristics
Evolutionary stagemain-sequence star[3]
Spectral typeK0[2]
Astrometry
Radial velocity (Rv)8.26[1] km/s
Proper motion (μ)RA: 40.576[1]mas/yr
Dec.: −94.254[1]mas/yr
Parallax (π)30.6433±0.1071 mas[4]
Distance106.4 ± 0.4 ly
(32.6 ± 0.1 pc)
Details[5]
Mass0.75±0.02 M
Radius0.70±0.02 R
Surface gravity (log g)4.57±0.04 cgs
Temperature5175±15 K
Metallicity [Fe/H]−0.35±0.02 dex
Rotational velocity (v sin i)1.73[3] km/s
Age4.14±3.63 Gyr
Other designations
BD+31 630,Gaia DR2 217334764042444288,HD 22781,HIP 17187,TYC 2355-246-1,GSC 02355-00246,2MASS J03404953+3149345[1]
Database references
SIMBADdata

HD 22781, is a single star about106 light-years away. It is aK-type main-sequence star. The star’s age is poorly constrained at4.14±3.63 billion years, but is likely similar to that of theSun.[5] HD 22781 is heavily depleted inheavy elements, having just 45% of Sun's concentration of iron,[2] yet is comparatively rich in carbon, having 90% of Sun`s abundance.[5]

An imaging survey in 2012 has failed to find any stellar companions, suggesting HD 22781 is a single star.[6]

Planetary system

[edit]

In 2011 atransitingsuperjovian planet orbrown dwarfb was detected on an extremelyeccentric orbit.[3] It is located just outside of the conservativehabitable zone of the parent star.[7] Planets around such metal-poor stars are rare; the only three known similar cases areHD 111232 andHD 181720.[8]

In 2012, a radial velocity data review indicated there are no additional giant planets in the system.[9]

The HD 22781 planetary system[3]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b≥13.65±0.97 MJ1.167±0.039528.07±0.140.8191±0.0023

References

[edit]
  1. ^abcdef"HD 22781".SIMBAD.Centre de données astronomiques de Strasbourg.
  2. ^abcMaldonado, J.; Villaver, E.; Eiroa, C.; Micela, G. (2019), "Connecting substellar and stellar formation. The role of the host star's metallicity",Astronomy & Astrophysics,624: A94,arXiv:1903.01141,Bibcode:2019A&A...624A..94M,doi:10.1051/0004-6361/201833827,S2CID 118934484
  3. ^abcdDíaz, Rodrigo F.; Santerne, Alexandre; Sahlmann, Johannes; Hébrard, Guillaume; Eggenberger, Anne; Santos, Nuno C.; Moutou, Claire; Arnold, Luc; Boisse, Isabelle; Bonfils, Xavier; Bouchy, François; Delfosse, Xavier; Desort, Morgan; Ehrenreich, David; Forveille, Thierry; Lagrange, Anne-Marie; Lovis, Christophe; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Ségransan, Damien; Udry, Stéphane; Vidal-Madjar, Alfred (2012), "The SOPHIE search for northern extrasolar planets IV. Massive companions in the planet-brown dwarf boundary",Astronomy & Astrophysics,A113: 538,arXiv:1111.1168,Bibcode:2012A&A...538A.113D,doi:10.1051/0004-6361/201117935,S2CID 55322205
  4. ^Brown, 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.
  5. ^abcMaldonado, J.; Villaver, E. (2017), "Searching for chemical signatures of brown dwarf formation",Astronomy & Astrophysics,602: A38,arXiv:1702.02904,Bibcode:2017A&A...602A..38M,doi:10.1051/0004-6361/201630120,S2CID 56225222
  6. ^Ginski, C.; Mugrauer, M.; Seeliger, M.; Eisenbeiss, T. (2012), "A lucky imaging multiplicity study of exoplanet host stars",Monthly Notices of the Royal Astronomical Society,421 (3):2498–2509,arXiv:1202.4586,Bibcode:2012MNRAS.421.2498G,doi:10.1111/j.1365-2966.2012.20485.x,S2CID 118573795
  7. ^Agnew, Matthew T.; Maddison, Sarah T.; Thilliez, Elodie; Horner, Jonathan (2017), "Stable habitable zones of single Jovian planet systems",Monthly Notices of the Royal Astronomical Society,471 (4):4494–4507,arXiv:1706.05805,Bibcode:2017MNRAS.471.4494A,doi:10.1093/mnras/stx1449,S2CID 119227856
  8. ^Adibekyan, Vardan (2019), "Heavy Metal Rules. I. Exoplanet Incidence and Metallicity",Geosciences,9 (3): 105,arXiv:1902.04493,Bibcode:2019Geosc...9..105A,doi:10.3390/geosciences9030105,S2CID 119089419
  9. ^Wittenmyer, Robert A.; Wang, Songhu; Horner, Jonathan; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; O'Toole, S. J.; Bailey, J.; Carter, B. D.; Salter, G. S.; Wright, D.; Zhou, Ji-Lin (2013), "Forever alone? Testing single eccentric planetary systems for multiple companions",The Astrophysical Journal Supplement Series,208 (1): 2,arXiv:1307.0894,Bibcode:2013ApJS..208....2W,doi:10.1088/0067-0049/208/1/2,S2CID 14109907


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