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Kepler-39

From Wikipedia, the free encyclopedia
Star in the constellation Cygnus
Kepler-39
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus[1]
Right ascension19h 47m 50.4746s[2]
Declination+46° 02′ 03.500″[2]
Apparent magnitude (V)14.3[3]
Characteristics
Spectral typeF7V[4]
Astrometry
Proper motion (μ)RA: 3.894(18)mas/yr[2]
Dec.: −2.345(17)mas/yr[2]
Parallax (π)0.9316±0.0139 mas[2]
Distance3,500 ± 50 ly
(1,070 ± 20 pc)
Details[4]
Mass1.29+0.06
−0.07
 M
Radius1.40±0.10 R
Surface gravity (log g)4.25±0.06 cgs
Temperature6350±100 K
Metallicity[Fe/H]0.10±0.14 dex
Rotation4.464±0.013 days[5]
Rotational velocity (v sin i)16±2.5 km/s
Age2.1+0.8
−0.9
 Gyr
Other designations
KOI-423,KIC 9478990,2MASS J19475046+4602034,Gaia DR2 2080168561154800384
Database references
SIMBADdata
KICdata

Kepler-39 (2MASS J19475046+4602034) is anF-typemain sequence star located in the constellationCygnus. It is located about 3,500 light-years (1,070 parsecs) away.[2] One knownsubstellar companion orbits it,Kepler-39b.[6]

Planetary system

[edit]

Kepler-39b is generally considered abrown dwarf rather than a planet since it does not meet the standarddefinition of planet. Some authorities such as theExtrasolar Planets Encyclopaedia and theNASA Exoplanet Archive include it among their list of confirmed planets.[3][7]

The Kepler-39 planetary system[4]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b20.1+1.3
−1.2
 MJ
0.164±0.00321.087210±0.0000370.112±0.05789.07±0.22°1.24+0.09
−0.10
 RJ

References

[edit]
  1. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  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"Kepler-39 b".Extrasolar Planets Encyclopaedia. Retrieved2018-06-09.
  4. ^abcBonomo, A. S.; et al. (2015)."Improved parameters of seven Kepler giant companions characterized with SOPHIE and HARPS-N".Astronomy and Astrophysics.575. A85.arXiv:1501.02653.Bibcode:2015A&A...575A..85B.doi:10.1051/0004-6361/201323042.S2CID 119230291.
  5. ^McQuillan, A.; Mazeh, T.; Aigrain, S. (2013). "Stellar Rotation Periods of The Kepler objects of Interest: A Dearth of Close-In Planets Around Fast Rotators".The Astrophysical Journal Letters.775 (1). L11.arXiv:1308.1845.Bibcode:2013ApJ...775L..11M.doi:10.1088/2041-8205/775/1/L11.S2CID 118557681.
  6. ^Bouchy, F.; et al. (2011)."SOPHIE velocimetry of Kepler transit candidates. III. KOI-423b: an 18 MJup transiting companion around an F7IV star".Astronomy and Astrophysics.533. A83.arXiv:1106.3225.Bibcode:2011A&A...533A..83B.doi:10.1051/0004-6361/201117095.S2CID 62836749.
  7. ^"Kepler-39 b".NASA Exoplanet Archive. Retrieved2018-06-09.
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