Kepler-56

Kepler-56 [1][2][3]

Graphical sketch of the Kepler-56 system. The line of sight from Earth is illustrated by the dashed line, and dotted lines show the orbits of three detected companions in the system. The solid arrow marks the rotation axis of the host star, and the thin solid line marks the host star equator.
Credit: NASA GSFC/Ames/D Huber
Observation data
Epoch J2000.0[1]      Equinox J2000.0[1]
Constellation Cygnus
Right ascension 19h 35m 02.0012s[4]
Declination +41° 52′ 18.692″[4]
Apparent magnitude (V) 13
Characteristics
Evolutionary stage red giant[5]
Spectral type K3III
Astrometry
Radial velocity (Rv)-53.740601[1] km/s
Proper motion (μ) RA: −6.596(12) mas/yr[4]
Dec.: −12.081(13) mas/yr[4]
Parallax (π)1.0755 ± 0.0118 mas[4]
Distance3,030 ± 30 ly
(930 ± 10 pc)
Details[5]
Mass1.286±0.011 M
Radius4.179±0.132 R
Luminosity (bolometric)9.589±0.129 L
Temperature4973±14 K
Metallicity [Fe/H]0.0251±0.013 dex
Age3.917±0.157 Gyr
Other designations
Kepler-56, KOI-1241, KIC 6448890, 2MASS 19350200+4152187
Database references
SIMBADdata

Kepler-56 is a red giant[6] in constellation Cygnus roughly 3,030 light-years (930 pc) away[4] with slightly more mass than the Sun.

  1. ^ a b c "Kepler-56". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ Cite error: The named reference EPE-Kepler56b was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference EPE-Kepler56c was invoked but never defined (see the help page).
  4. ^ a b c d e Cite error: The named reference Gaia DR3 was invoked but never defined (see the help page).
  5. ^ a b Fellay, L.; Buldgen, G.; et al. (October 22, 2021). "Asteroseismology of evolved stars to constrain the internal transport of angular momentum". Astronomy & Astrophysics. 654. 12. arXiv:2108.02670. doi:10.1051/0004-6361/202140518. S2CID 239652877. Retrieved March 30, 2022.
  6. ^ Cite error: The named reference 2013Sci...342..331H was invoked but never defined (see the help page).