Kepler-296b is an s-type exoplanet located in the binary star system Kepler-296. All 5 planets in this system orbit around the primary star. 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 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-296b is an exoplanet with "more than 99% confidence".
Data 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.
References

![Kepler-296b: The following plot shows the approximate sizes of the planets in this system compared to planets in the Solar System.[3]](https://upload.wikimedia.org/wikipedia/commons/thumb/2/21/Kepler296scale.png/500px-Kepler296scale.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
