J1407b Also known as Super Saturn, is an Exoplanet located 433.8 light-years from Earth in the constellation of Centaurus. The planet was discovered in 2012 by the University of Rochester, located in New York.
J1407b is widely known for the massive size of its rings, which are approximately 640 times the extent of the rings found on Saturn. The planet itself is regarded as the first possible exoplanet, or brown dwarf with a ring system. J1407b orbits its parent star, 1SWASP J140747.93β394542.6 (known simply as V1400 Centauri) in an eccentric (oval) orbit, which could disrupt J1407b's own ring system. If we replaced Saturn with J1407b, the rings are 10x visible by both day and night. J1407b has more than 30 rings!