Kepler-429 (KIC 10001893) is a variable subdwarf B star in the constellation Lyra, about 5,900 light years away.

Quick Facts Constellation, Right ascension ...
Kepler-429
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Lyra[1]
Right ascension 19h 09m 33.4137s[2]
Declination +46° 59 04.108[2]
Apparent magnitude (V) 14.69 (var.)[3]
Characteristics
Evolutionary stage Subdwarf B star
Spectral type sdB[4]
Apparent magnitude (J) 16.36±0.10[4]
Variable type V361 Hya[3]
Astrometry
Proper motion (μ) RA: 1.133[2] mas/yr
Dec.: −5.907[2] mas/yr
Parallax (π)0.5573 ± 0.0372 mas[2]
Distance5,900 ± 400 ly
(1,800 ± 100 pc)
Details
Mass0.47[5] M
Radius0.24[5] R
Luminosity3.54[6] L
Surface gravity (log g)5.35[6] cgs
Temperature27,500[5] K
Metallicity [Fe/H]0.0[5] dex
Other designations
Gaia DR2 2130473176626619136, Kepler-429, KIC 10001893, 2MASS J19093340+4659041[4]
Database references
SIMBADdata
Exoplanet Archivedata
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The brightness of Kepler-429 changes unpredictably by up to 0.13 magnitudes.[3] It has been classified as a V361 Hydrae variable, but also as a V1093 Herculis variable, which typically has slower variations and a cooler temperature. Over 100 pulsation modes were identified with periods from 256 seconds to over three hours.[7]

Planetary system

Kepler-429 has been reported to have three possible exoplanets,[8] though their existence is questioned.[9] They were detected by orbital brightness modulation.[10]

More information Companion (in order from star), Mass ...
The KIC 10001893 planetary system[11]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (unconfirmed) 0.005541 0.21970 0[12]
c (unconfirmed) 0.007197 0.32528 0[13]
d (unconfirmed) 0.01324 0.81161 0[14]
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See also

References

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