Kepler-429

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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[4]
Spectral type sdB[4]
Apparent magnitude (J) 16.36±0.10[5]
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[6] M
Radius0.24[6] R
Luminosity3.54[7] L
Surface gravity (log g)5.35[7] cgs
Temperature27,500[6] K
Metallicity [Fe/H]0.0[6] dex
Other designations
Gaia DR2 2130473176626619136, Kepler-429, KIC 10001893, 2MASS J19093340+4659041[5]
Database references
SIMBADdata
Exoplanet Archivedata

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

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.[8]

Planetary system

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Kepler-429 has been reported to have three possible exoplanets,[9] though their existence is questioned.[10] They were detected by orbital brightness modulation.[11]

The KIC 10001893 planetary system[12]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (unconfirmed) 0.005541 0.21970 0[13]
c (unconfirmed) 0.007197 0.32528 0[14]
d (unconfirmed) 0.01324 0.81161 0[15]

See also

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References

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  2. ^ a b c d e Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). Gaia DR3 record for this source at VizieR.
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