Planet KOI-730 b
| Name | KOI-730 b | |
| Discovered in | 2011 | |
| M × sin i | — | |
| Semi-major axis | 0.12 AU |  |
| Orbital period | 14.7903 ± 0.0002 days | |
| Eccentricity | — | |
| ω | — | |
| Tperi | — | |
| Radius | 0.31 RJ | |
| Inclination | — | |
| Update | Sept. 7, 2011 | |
| Detection method | detected by transit | |
| Molecules detected | — |
Remarks
6 Sep 2011: In spite of the absence of confirmation by radial velocity measurements, this planetary system is likely to be real, given the 3:4:6:8 resonance nature of the orbital periods (Fabrycky et al. 2011, Lissauer et al. 2011)6 Sep 2011: Object KOI-730b designated as KOI 730.01 by Borucki et al. 2011
Star
| Name | KOI-730 | |
| Distance | — | |
| Spectral type | None | |
| Apparent magnitude V | 15.0 | |
| Mass | 1.07 MSun | |
| Age | Gyr | |
| Effective temperature | 5590 K | |
| Radius | 1.1 RSun | |
| Metallicity [Fe/H] | ||
| RA2000 | 19:53:16.0 | |
| Dec2000 | +47:16:46 | |
| Planetary system | 4 planets |
More data
- Simbad
- Most recent references (ADS)
Related publications
The Exoplanet Handbook
May 22, 2012
Michael Perryman
Content
Content and Chapter 5
Architecture and Dynamics of Kepler's Candidate Multiple Transiting Planet Systems
Sept. 7, 2011
LISSAUER J., RAGOZZINE D., FABRYCKY D., BATALHA N., BORUCKI J. & 17 additional authors
ApJ.
arxiv
Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data
Sept. 7, 2011
BORUCKI W., KOCH D., BASRI G., BATALHA N., BROWN T. & 61 additional authors
ApJ., 736, 19
paper arxiv
KOI-730 As A System OF Four Planets in A Chain of Resonances
Sept. 6, 2011
FABRYCKY D., HOLMAN M., CARTER J., ROWE J., RAGOZZINE D. & 2 additional authors & Kepler Team
abstract