Planet KOI-204 b
| Name | KOI-204 b | |
| Discovered in | 2011 | |
| M × sin i | 1.02 ± 0.07 MJ |  |
| Semi-major axis | 0.0455 ± 0.0013 AU | |
| Orbital period | 3.24674 ± 1.8e-05 days | |
| Eccentricity | > 0.021 | |
| ω | — | |
| Tperi | — | |
| Radius | 1.24 ± 0.07 RJ | |
| Inclination | 83.78 +0.55-0.55° | |
| Update | Oct. 26, 2011 | |
| Detection method | detected by transit | |
| Molecules detected | — |
Star
| Name | KOI-204 | |
| Distance | 2250 ± 300 pc | |
| Spectral type | G2IV | |
| Apparent magnitude V | 15.0 | |
| Mass | 1.19 ± 0.1 MSun | |
| Age | 6.95 +1.7-1.7 Gyr | |
| Effective temperature | 5757 ± 134 K | |
| Radius | 1.52 ± 0.09 RSun | |
| Metallicity [Fe/H] | 0.26 ± 0.1 | |
| RA2000 | 20:00:25.0 | |
| Dec2000 | +45:45:44 | |
| Planetary system | 1 planet |
More data
- Simbad
- Most recent references (ADS)
Related publications
SOPHIE velocimetry of Kepler transit candidates VI. A false positive rate of 35% for Kepler close-in giant candidates
July 20, 2012
SANTERNE A., DIAZ ., MOUTOU C., BOUCHY F., HEBRARD G. & 4 additional authors
Astron. & Astrophys., 545, A76
paper arxiv
A Correlation Between the Eclipse Depths of Kepler Gas Giant Candidates and the Metallicities of their Parent Stars
April 12, 2012
DODSON-ROBINSON S.
ApJ.
arxiv
SOPHIE velocimetry of Kepler transit candidates. V. The three hot Jupiters KOI-135b, KOI-204b and KOI-203b (alias Kepler-17b)
Feb. 11, 2012
BONOMO A., HEBRARD G., SANTERNE A., SANTOS N., DELEUIL M. & 5 additional authors
Astron. & Astrophys., 538, A96
paper arxiv
The Exoplanet Handbook
May 22, 2012
Michael Perryman
Content
Content and Chapter 5