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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Kepler-16b is an extrasolar planet. It is a Saturn-mass planet consisting of half rock and half gas, and it orbits a binary star, Kepler-16, with a period of 229 days. This is the first observationally confirmed example of a circumbinary planet. The planet was discovered using the space observatory aboard NASA's Kepler spacecraft. Scientists were able to detect the planet using the transit method, when they noticed the dimming of one of the system's stars even when the other was not eclipsing it.