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HD 20781

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(Redirected fromHD 20781 c)
Star in a binary star system in the constellation Fornax
HD 20781
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationFornax[1]
Right ascension03h 20m 02.94286s[2]
Declination−28° 47′ 01.7905″[2]
Apparent magnitude (V)8.48[3]
Characteristics
Spectral typeK0V[3]
B−Vcolor index0.82[3]
Astrometry
Radial velocity (Rv)40.27±0.12[2] km/s
Proper motion (μ)RA: 348.869±0.015mas/yr[2]
Dec.: −66.614±0.019mas/yr[2]
Parallax (π)27.8123±0.0239 mas[2]
Distance117.3 ± 0.1 ly
(35.96 ± 0.03 pc)
Absolute magnitude (MV)5.70[3]
Details[3]
Mass0.7 M
Luminosity0.49±0.04 L
Surface gravity (log g)4.37±0.05 cgs
Temperature5256±29 K
Metallicity [Fe/H]−0.11±0.02 dex
Rotation46.8±4.4d
Rotational velocity (v sin i)1.1 km/s
Other designations
CD–29° 1229,HIP 15526,LTT 1581,SAO 168468, 2MASS J03200291-2847016, Gaia DR1 5060105892897388288[4]
Database references
SIMBADdata

HD 20781 is a star which is part of a widebinary system withHD 20782. The companion star has a very largeangular separation of 252 arcsec, corresponding to 9080 AU at the distance of HD 20782.[5] Both stars possess their ownplanetary systems inS type orbits, with a total of five known planets around both stars.[3][6] This is the first known example ofplanets being found orbiting both components of a wide binary system.[5][7] HD 20781 has no noticeablestarspot activity.[3]

Planetary system

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In 2011, a pair of Neptune-mass gas giants were detected with the radial velocity method.[7] In 2017, these planets were confirmed and an additional two innersuper-Earths were detected, with periods of 5.3 and 13.9 days respectively.[3]

The HD 20781 planetary system[3]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b≥1.93+0.39
−0.36
 M🜨
0.0529+0.0024
−0.0027
5.3135±0.00100.10+0.11
−0.07
c≥5.33+0.70
−0.67
 M🜨
0.1004+0.0046
−0.0051
13.8905+0.0033
−0.0034
0.09+0.09
−0.06
d≥10.61+1.20
−1.19
 M🜨
0.1647+0.0076
−0.0083
29.1580+0.0102
−0.0100
0.11+0.05
−0.06
e≥14.03±1.56 M🜨0.3374+0.0155
−0.0170
85.5073+0.0983
−0.0947
0.06+0.06
−0.04

See also

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References

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  1. ^Roman, Nancy G. (1987)."Identification of a Constellation From a Position".Publications of the Astronomical Society of the Pacific.99 (617):695–699.Bibcode:1987PASP...99..695R.doi:10.1086/132034.Vizier query form
  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. ^abcdefghiUdry, S.; Dumusque, X.; et al. (February 2019). "The HARPS search for southern extra-solar planets. XLIV. Eight HARPS multi-planet systems hosting 20 super-Earth and Neptune-mass companions".Astronomy & Astrophysics.622: A37.arXiv:1705.05153.Bibcode:2019A&A...622A..37U.doi:10.1051/0004-6361/201731173.S2CID 119095511.
  4. ^"HD 20781 -- High proper-motion Star".SIMBAD Astronomical Database.Centre de données astronomiques de Strasbourg. Retrieved2014-09-10.
  5. ^abDesidera, S.; Barbieri, M. (January 2007). "Properties of planets in binary systems. The role of binary separation".Astronomy and Astrophysics.462 (1):345–353.arXiv:astro-ph/0610623.Bibcode:2007A&A...462..345D.doi:10.1051/0004-6361:20066319.S2CID 13813761.
  6. ^"HD 20782".NASA Exoplanet Archive. Retrieved12 November 2022.
  7. ^abMayor, M.; Marmier, M.; et al. (2011). "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets".arXiv:1109.2497 [astro-ph].

External links

[edit]
TheHD 20781/HD 20782 system


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