gamma Cephei b is the first planet discovered in a close binary star system. At their closest, the two stars are only 12 AU from each other, proving that such close systems can support planets. This discovery also ups the likely number of planets in the galaxy as most stars are in double or triple star systems.
View a VRML model of the system. Please be patient while the file downloads.
For a VRML tour of our galaxy's exoplanets, check out Extrasolar VR.
 | gamma Cephei Ab Photochemically generated sulfurous compounds stain the water clouds of gamma Cephei Ab yellow. In the foreground, a dense rocky moon with the mass of Mercury bears the scars of tectonic fractures and basaltic lava plains caused by the intense gravitational tides of its parent jovian. |  | In the Shadow of g Cep Ab The night side of gamma Cephei Ab flickers with titanic lightning storms. Only a thin sliver of the planet and its moon remain in sunlight from this vantage point. In the distance, the planet's two stars glow. The nearby K1 subgiant shines brightly, but the light of the M1 red dwarf, 13 AU away, is feeble and distant.
|
|