Kepler-16
Characteristics | |
---|---|
Spectral type | K / M[1] |
Astrometry | |
Distance | 196 ly (60 pc) |
Orbit[2] | |
Primary | Kepler-16A |
Companion | Kepler-16B |
Period (P) | 41.079220 (± 0.000078) d |
Semi-major axis (a) | 0.22431 (± 0.00035) AU |
Eccentricity (e) | 0.15944 (± 0.00062) |
Inclination (i) | 90.30401 (± 0.0019)° |
Longitude of the node (Ω) | 0° |
Periastron epoch (T) | BJD 2455212.12316 |
Argument of periastron (ω) (secondary) |
263.464 (± 0.027)° |
Details | |
Kepler-16A | |
Mass | 0.6897 (± 0.0035) M☉ |
Radius | 0.6489 (± 0.0013) R☉ |
Luminosity | 0.148[3] L☉ |
Surface gravity (log g) | 4.6527 (± 0.0017) cgs |
Temperature | 4450 (± 150) K |
Metallicity [Fe/H] | -0.3 (± 0.2) dex |
Rotation | 35.1 ± 1.0 days[4] |
Kepler-16B | |
Mass | 0.20255 (± 0.00065) M☉ |
Radius | 0.22623 (± 0.00059) R☉ |
Luminosity | ~0.0057[3] L☉ |
Surface gravity (log g) | 5.0358 (± 0.0017) cgs |
Temperature | ~3311[3] K |
Other designations | |
Kepler-16 is a binary star system in the constellation of Cygnus[5] that was targeted by the Kepler spacecraft. Both stars are smaller than the Sun; the primary, Kepler-16A, is a K-type main-sequence star and the secondary, Kepler-16B, is an M-type red dwarf. They are separated by 0.22 AU, and complete an orbit around a common center of mass every 41 days.
The system is host to one known extrasolar planet in circumbinary orbit: the Saturn-sized Kepler-16b.
Planetary system
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Kepler-16b is a gas giant that orbits the two stars in the Kepler-16 system.[2] The planet is a third of Jupiter's mass and slightly smaller than Saturn at 0.7538 Jupiter radii, but is more dense. Kepler-16b completes a nearly circular orbit every 228.776 days.
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.333 MJ | 0.7048 | 228.776 | 0.0069 | 90.032° | 0.7538 RJ |
References
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Coordinates: 19h 16m 18.17s, +51° 45′ 26.78″
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