Planet Kepler-67 b
| Name | Kepler-67 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2013 | ||
| Mass | 0.047 MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.1171 (± 0.0015) AU | |
|
| Orbital Period | 15.7259 (± 0.00011) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.26 ( -0.014 +0.014 ) RJ | |
|
| Inclination | — | ||
| Update | 2018-11-28 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Theoretical | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2454966.9855 (± 0.0048) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
Kepler-67| Name | Kepler-67 | ||
| Distance | 1107.0 (± 90.0) pc | |
|
| Spectral type | G9V | ||
| Apparent magnitude V | 16.4 | ||
| Mass | 0.865 (± 0.034) MSun | |
|
| Age | 1.0 (± 0.17) Gyr | |
|
| Effective temperature | 5331.0 (± 63.0) K | |
|
| Radius | 0.778 (± 0.031) RSun | |
|
| Metallicity [Fe/H] | 0.012 (± 0.003) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 19:36:37.0 | ||
| Dec2000 | +46:09:59 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
How do disks and planetary systems in high-mass open clusters differ from those around field stars?
2018
VINCKE K. & PFALZNER S.
ApJ, 868, 1
paperarxiv
The same frequency of planets inside and outside open clusters of stars
2013
MEIBOM S., TORRES G., FRESSIN F., LATHAM D., ROWE J. & 14 additional authors
Nature, 499, 55
paper arxiv
