Planet Kepler-28 b
| Name | Kepler-28 b | |
| Discovered in | 2012 | |
| M × sin i | > 1.51 MJ | |
| Semi-major axis | 0.062 AU |  |
| Orbital period | 5.9123 days | |
| Eccentricity | — | |
| ω | — | |
| Tperi | — | |
| Radius | 0.32 RJ | |
| Inclination | — | |
| Update | Jan. 30, 2012 | |
| Detection method | detected by transit | |
| Molecules detected | — |
Remarks
28 Jan 2012: The upper mass limit is inferred from transit time variations and dynamical stability (Steffen et al. 2012).Star
| Name | Kepler-28 | |
| Distance | — | |
| Spectral type | None | |
| Apparent magnitude V | 15.5 | |
| Mass | 0.75 MSun | |
| Age | Gyr | |
| Effective temperature | 4590 K | |
| Radius | 0.7 RSun | |
| Metallicity [Fe/H] | 0.34 | |
| RA2000 | 19:28:33.0 | |
| Dec2000 | +42:25:46 | |
| Planetary system | 2 planets |
More data
- Simbad
- Most recent references (ADS)
Related publications
Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations
April 6, 2012
STEFFEN J., FABRYCKY D., FORD E., CARTER J., DESERT J.-M. & 30 additional authors
MNRAS, 421, 2342
paper arxiv
The Exoplanet Handbook
May 22, 2012
Michael Perryman
Content
Content and Chapter 5