Planet KELT-6 b
| Name | KELT-6 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2013 | ||
| Mass | 0.442 ( -0.019 +0.019 ) MJ | ||
| Mass*sin(i) | 0.442 ( -0.019 +0.019 ) MJ |  |
+ |
| Semi-Major Axis | 0.08 (± 0.001) AU | |
+ |
| Orbital Period | 7.845582 (± 7e-07) day | |
+ |
| Eccentricity | 0.029 (± 0.016) | |
+ |
| ω | 308.0 ( -272.0 +30.0 ) deg | |
|
| Tperi | — | ||
| Radius | 1.18 ( -0.11 +0.11 ) RJ | |
+ |
| Inclination | 88.81 ( -0.91 +0.79 ) deg | |
|
| Update | 2015-08-27 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2457124.50954 (± 0.00057) JD | |
|
| Secondary transit | — | ||
| λ | 324.0 (± 11.0) deg | |
|
| Impact Parameter b | 0.2 (± 0.14) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 41.8 (± 1.1) m/s | |
|
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
KELT-6| Name | KELT-6 | ||
| Distance | — | ||
| Spectral type | F | ||
| Apparent magnitude V | 10.38 | ||
| Mass | 1.126 (± 0.058) MSun | |
+ |
| Age | 4.9 ( -0.46 +0.66 ) Gyr | |
|
| Effective temperature | 6272.0 (± 61.0) K | |
+ |
| Radius | 1.529 ( -0.137 +0.143 ) RSun | |
+ |
| Metallicity [Fe/H] | -0.27 (± 0.06) | |
+ |
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 13:03:56.0 | ||
| Dec2000 | +30:38:24 | ||
| Alternate Names | |||
| Planetary system | 2 planets |
Related publications
KELT: The Kilodegree Extremely Little Telescope, a Survey for Exoplanets Transiting Bright, Hot Stars
2018
PEPPER J., STASSUN K. & GAUDI S.
in the 'Handbook of Exoplanets,' Springer
arxiv
High-precision time-series photometry for the
discovery and characterization of transiting
exoplanets.
2015
COLLINS K.
Electronic Theses and Dissertations., 2104
Full Text
The GAPS Programme with HARPS-N@TNG X. The multi-planet system KELT-6: detection of the planet KELT-6 c and measurement of the Rossiter-McLaughlin effect for KELT-6 b
2015
DAMASSO M., ESPOSITO M., NACIMBENI V., DESIDERA S., BONOMO A. et al.
Astron. & Astrophys., 581, L6
paper arxiv
KELT-6b: A P~7.9 d Hot Saturn Transiting a Metal-Poor Star with a Long-Period Companion
2014
COLLINS K., EASTMAN J., BEATTY T., SIVERD R. GAUDI B. & 37 additional authors
Astron. J., 147, 39
paper arxiv
KELT-6b: A Transiting Mildly-Inflated Saturn with a Metal-Poor Host
2013
COLLINS K., SIVERD R., BEATTY Th., EASTMAN J., GAUDI B. & 34 additional authors
in 222nd AAS Meeting (Indianapolis), 302.03
abstract
The Frequency of Binary Companions Around KELT Planet
Host Stars
1917
COKER C.
Ohio State Univ. PhD Tesis
Full Text
