Kepler-296 b is an s-type exoplanet located in the binary star system Kepler-296. All 5 planets in this system orbit around the primary star.
Discovery[1] | |
---|---|
Discovery date | 2014 |
Detection method | Transit[2] |
Orbital characteristics[1] | |
Semi-major axis | 0.079±0.013 AU |
Eccentricity | < 0.33[2] |
Orbital period (sidereal) | 10.8644+0.0001 −0.0000 |
Physical characteristics[1] | |
Mean radius | 1.6±0.3 REarth (0.14+0.03 −0.02 RJ) |
Mass | 3.22 MEarth[2] |
It has been classed as a hot superterran.
It was discovered by the Kepler space telescope in 2014 using the transit method and was originally classed as a planet candidate, but during a study[4] by members of the NASA Ames Research Center on two other planets in the Kepler-296 system, Kepler-296f and Kepler-296e, they were able to confirm that Kepler-296 b is an exoplanet with "more than 99% confidence".
As with most other exoplanets, not many parameters are known about Kepler-296b. The few that are, are listed in the infobox to the right.
{{cite web}}
: External link in |last=
(help)