Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 38m 32.612s[1] |
Declination | +46h 03m 59.14s[1] |
Apparent magnitude (V) | 12.69[2] |
Characteristics | |
Spectral type | sdBV+dM[3] |
Astrometry | |
Proper motion (μ) | RA: 5.225(37) mas/yr[1] Dec.: −4.405(42) mas/yr[1] |
Parallax (π) | 2.4410 ± 0.0316 mas[1] |
Distance | 1,340 ± 20 ly (410 ± 5 pc) |
Orbit[4] | |
Period (P) | 0.125765282(5) d |
Inclination (i) | 69.45±0.20° |
Semi-amplitude (K1) (primary) | 65.7±0.6 km/s |
Details | |
Kepler-451 A | |
Mass | 0.48±0.03[5] M☉ |
Radius | 0.203±0.001[6] R☉ |
Temperature | 29564±106[5] K |
Age | 6±2[citation needed] Gyr |
Kepler-451 B | |
Mass | 0.12±0.01[5] M☉ |
Radius | 0.168±0.001[6] R☉ |
Other designations | |
Database references | |
SIMBAD | data |
Kepler-451 (also known as 2MASS J19383260+4603591 and abbreviated to 2M1938+4603) is an eclipsing post-common envelope binary star system that comprises two stars, a pulsating subdwarf B star and a small red dwarf star.[5] It is located about 1,340 light-years (410 parsecs) away in the constellation Cygnus.[1] It has been hypothesized to host one or more exoplanets.[6]
GaiaDR3
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Krzesinski2020
was invoked but never defined (see the help page).Baran2015
was invoked but never defined (see the help page).Østensen2010
was invoked but never defined (see the help page).Esmer2022
was invoked but never defined (see the help page).