Kepler-296

Kepler-296 is a binary star system in the constellation Draco. The primary star appears to be a late K-type main-sequence star, while the secondary is a red dwarf.

Kepler-296d is an exoplanet orbiting the M-dwarf star Kepler-296, located in the constellation Draco. It was discovered in 2014 by the Kepler space telescope using the transit method.

Kepler-296c is a confirmed exoplanet located in the binary star system Kepler-296. It was discovered in 2014 by the Kepler space telescope using the transit method. 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 confirmed that Kepler-296c was an exoplanet with "more than 99% confidence".

thumb|The following plot shows the approximate sizes of the planets in this system compared to planets in the Solar System. 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.