PIA14725: Three Eclipsing Bodies (Artist Concept)
 Mission:  Kepler
 Product Size:  3000 x 2400 pixels (w x h)
 Produced By:  IPAC-Caltech
 Full-Res TIFF:  PIA14725.tif (21.6 MB)
 Full-Res JPEG:  PIA14725.jpg (935.9 kB)

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This artist's movie illustrates Kepler-16b, the first directly detected circumbinary planet, which is a planet that orbits two stars. The movie begins by showing the gaseous surface of the rotating planet then pans out to show the stars it orbits.

The two orbiting stars regularly eclipse each other, as seen from our point of view on Earth. The planet also eclipses, or transits, each star, and Kepler data from these planetary transits allowed the size, density and mass of the planet to be extremely well determined. The fact that the orbits of the stars and the planet align within a degree of each other indicate that the planet formed within the same circumbinary disk that the stars formed within, rather than being captured later by the two stars.

NASA's Kepler telescope discovered the planet by observing it cross in front of, or transit, the pair of stars from our point of view on Earth. The stars can also be detected eclipsing each other. Stellar eclipses are shown here, as well as the transits of the planet across both stars.

Such events allow astronomers to measure the sizes of the stars and the planet with extreme accuracy. Kepler-16b is one of the most accurately measured planets outside our solar system, with a size (radius) of 0.7538 that of Jupiter; a mass of 0.333 that of Jupiter (about the mass of Saturn), and a density of 0.964 grams per cubic centimeter. The planet is cold, lying just beyond the "habitable zone" of its star, and is made up of about half gaseous material with a rocky core.

The largest star in the Kepler-16b system is a bit smaller than our sun (about 69 percent of its mass), and the smaller star, called a red dwarf, is even lower in mass (about 20 percent of the sun's mass).

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