Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lyra |
Right ascension | 19h 24m 35.54310s[1] |
Declination | +40° 40′ 09.8099″[1] |
Apparent magnitude (V) | 13.257[2] |
Characteristics | |
Spectral type | G6V[3] |
Astrometry | |
Radial velocity (Rv) | −19.51±1.63[1] km/s |
Proper motion (μ) | RA: 1.150(11) mas/yr[1] Dec.: 4.956(15) mas/yr[1] |
Parallax (π) | 2.6495 ± 0.0109 mas[1] |
Distance | 1,231 ± 5 ly (377 ± 2 pc) |
Absolute magnitude (MV) | 5.46±0.16[4] |
Details | |
Mass | 0.990±0.023[5] M☉ |
Radius | 0.897±0.016[5] R☉ |
Luminosity | 0.598+0.079 −0.070[4] L☉ |
Surface gravity (log g) | 4.528+0.025 −0.019[4] cgs |
Temperature | 5466±60[5] K |
Metallicity [Fe/H] | +0.27±0.06[5] dex |
Rotation | 30.689±0.383 days[6] |
Age | 1.9±1.6[5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
KIC | data |
Kepler-88 is a G-type star 1,230 light-years (380 parsecs) away in the constellation of Lyra, with three confirmed exoplanets.[5] SIMBAD lists a subgiant spectral type of G8IV,[2] while other sources give it a main sequence spectral type of G6V.[3] The latter is more consistent with its properties (it is less luminous than the Sun).
GaiaDR3
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Barros2013
was invoked but never defined (see the help page).Nesvorny
was invoked but never defined (see the help page).Weiss2019
was invoked but never defined (see the help page).McQuillan2013
was invoked but never defined (see the help page).