Kepler-87

Kepler-87
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cygnus
Right ascension 19h 51m 40.0490s[1]
Declination +46° 57′ 54.425″[1]
Apparent magnitude (V) 15
Characteristics
Spectral type G4IV
Variable type planetary transit
Astrometry
Proper motion (μ) RA: −4.382(19) mas/yr[1]
Dec.: −0.821(20) mas/yr[1]
Parallax (π)0.7803 ± 0.0154 mas[1]
Distance4,180 ± 80 ly
(1,280 ± 30 pc)
Details
Mass1.01 M
Radius1.49669 R
Luminosity0.3260445 L
Temperature5692 ± 60.7121 K
Metallicity [Fe/H]0.0562149±0.0587866 dex
Age7.24+1.50
−1.56
 years
Other designations
KOI-1574, 2MASS J19514005+4657544, KIC 10028792, WISE J195140.04+465754.4

Kepler-87 is a star slightly more massive than the Sun and it is nearing the end of its main-sequence period.[2]

  1. ^ a b c d Cite error: The named reference Gaia DR3 was invoked but never defined (see the help page).
  2. ^ "Kepler-87 | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 10 September 2023.