Mass, radius and temperature Kepler-16b is a
gas giant, an exoplanet that is near the same mass and radius as the planets
Jupiter and
Saturn. It has a temperature of . The planet has a radius of 0.77 , slightly smaller than
Saturn, and has no solid surface.
Host stars The planet orbits in a
circumbinary orbit around a (
K-type) and (
M-type)
binary star system. The stars orbit each other about every 41 days. The stars have masses of 0.68 and 0.20 and radii of 0.64 and 0.22 , respectively. They have surface temperatures of 4450
K and 3311 K and luminosities about 14% and 0.5% that of the Sun, respectively. Based on the stellar characteristics and orbital dynamics, an estimated age of 2 billion years for the system is possible. In comparison, the Sun is about 4.6 billion years old and has a surface temperature of 5778 K.
Orbit Kepler-16b orbits its parent stars (more properly, their barycenter, or center of mass) every 228 days at a distance of 0.704
AU (nearly the same distance that
Venus orbits from the Sun, which is about 0.71 AU). It is unlikely to have formed in its current orbit, and likely migrated from elsewhere. The small eccentricity of Kepler-16b's orbit remains unexplained. ==Potential habitability==