Kepler-1658

Kepler-1658
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 18h 46m 22.24188s
Declination +75° 26′ 02.2400″
Apparent magnitude (V) 11.556±0.100
Characteristics
A
Evolutionary stage Subgiant
Spectral type F5
BC
Evolutionary stage main sequence
Spectral type KV + MV
Variable type eclipsing binary
Astrometry
Radial velocity (Rv)−21.815±0.053 km/s
Proper motion (μ) RA: +0.100 mas/yr
Dec.: −5.542 mas/yr
Parallax (π)1.2260±0.0173 mas
Distance2,660 ± 40 ly
(820 ± 10 pc)
Orbit
PrimaryA
NameBC
Semi-major axis (a)50 AU
Orbit
PrimaryB
NameC
Period (P)3.849363145 days
Details
Kepler-1658 A
Mass1.45±0.03 M
Radius3.26±0.14 R
Surface gravity (log g)4.13±0.05 cgs
Temperature5,948±100 K
Metallicity [Fe/H]−0.27±0.06 dex
Rotational velocity (v sin i)38 km/s
Age2.0±0.1 Gyr
Kepler-1658 B
Mass0.75 M
Kepler-1658 C
Mass0.19 M
Radius0.23 R
Other designations
KOI-4, KIC 3861595, TIC 377873569, TYC 3135-652-1
Database references
SIMBADdata

Kepler-1658 is a triple star system located in the constellation Cygnus. Based on parallax measurements by the Gaia spacecraft, it is located at a distance of 2,660 light-years (820 parsecs).

This is an hierarchical triple system whose primary is an F-type subgiant star with 1.45 times the Sun's mass and 3.26 times the Sun's radius. The outer system, 50 astronomical units away from the primary, is an eclipsing binary whose components have an orbital period of 3.8 days: star B is probably a K-type dwarf with 0.8 times the Sun's mass, and star C a red dwarf with 0.19 times the mass of the Sun and 0.23 times the radius.