Summary
Kepler-16 is an eclipsing binary star system in the constellation of Cygnus 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.
 An artist's rendering of the Kepler-16 system, showing the binary star being orbited by Kepler-16b. Credit: NASA/JPL-Caltech | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 16m 18.1759s[1] |
| Declination | +51° 45′ 26.778″[1] |
| Characteristics | |
| Spectral type | K / M[2] |
| Astrometry | |
| Proper motion (μ) | RA: 14.041±0.054[1] mas/yr Dec.: −48.601±0.051[1] mas/yr |
| Parallax (π) | 13.2893 ± 0.0271 mas[1] |
| Distance | 245.4 ± 0.5 ly (75.2 ± 0.2 pc) |
| Orbit[3] | |
| 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[4] L☉ |
| Surface gravity (log g) | 4.6527±0.0017 cgs |
| Temperature | 4,450±150) K |
| Metallicity [Fe/H] | −0.3±0.2 dex |
| Rotation | 35.1±1.0 days[5] |
| Kepler-16B | |
| Mass | 0.20255±0.00065 M☉ |
| Radius | 0.22623±0.00059 R☉ |
| Luminosity | ~0.0057[4] L☉ |
| Surface gravity (log g) | 5.0358±0.0017 cgs |
| Temperature | ~3,311[4] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
| KIC | data |
Eclipses edit
The Kepler-16 system is almost edge-on to Earth and the two stars eclipse each other as they orbit. The larger and brighter primary star is partially eclipsed by the secondary for about six hours and the brightness drops by about 0.15 magnitudes. The secondary star is completely occulted by the primary star for about two hours, but the overall brightness only drops by about 0.02 magnitudes.
There are also shallow eclipses caused by a large exoplanet. When this transits across the primary star, the brightness drops by slightly more than the secondary eclipse. When it transits the secondary star, the brightness drops by 0.001 magnitudes.[3]
Planetary system edit
Kepler-16b is a gas giant that orbits the two stars in the Kepler-16 system.[3] 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 edit
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia Data Release 2 catalog entry
- ^ Jean Schneider (2011). "Notes for star Kepler-16 (AB)". Extrasolar Planets Encyclopaedia. Archived from the original on October 5, 2011. Retrieved 23 September 2011.
- ^ a b c d Doyle, Laurance R.; Carter, Joshua A.; Fabrycky, Daniel C.; Slawson, Robert W.; Howell, Steve B.; Winn, Joshua N.; Orosz, Jerome A.; Prša, Andrej; Welsh, William F.; et al. (2011). "Kepler-16: A Transiting Circumbinary Planet". Science. 333 (6049): 1602–6. arXiv:1109.3432. Bibcode:2011Sci...333.1602D. doi:10.1126/science.1210923. PMID 21921192. S2CID 206536332.
- ^ a b c Haghighipour, Nader; Kaltenegger, Lisa (24 October 2013). "Calculating the Habitable Zone of Binary Star Systems. II. P-type Binaries". The Astrophysical Journal. 777 (2): 13. arXiv:1306.2890. Bibcode:2013ApJ...777..166H. doi:10.1088/0004-637X/777/2/166. S2CID 118494204.
- ^ Winn, Joshua N.; et al. (2011). "Spin-Orbit Alignment for the Circumbinary Planet Host Kepler-16 A". The Astrophysical Journal Letters. 741 (1). L1. arXiv:1109.3198. Bibcode:2011ApJ...741L...1W. doi:10.1088/2041-8205/741/1/L1.
- ^ "Kepler-16". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-08-09.
- ^ Jean Schneider (2011). "Notes for Planet Kepler-16 (AB) b". Extrasolar Planets Encyclopaedia. Archived from the original on 11 October 2011. Retrieved 23 September 2011.