Best Long Period
Epsilon Aurigae is an eclipsing binary star system situated in the northern constellation of Auriga. The system is composed of an F-type supergiant primary star and a secondary component that consists of a large, opaque disk of dust and gas surrounding a smaller, hotter star. Astronomers have studie...
14 Herculis is a K-type main-sequence star located approximately 59 light-years from Earth in the constellation Hercules. It is notable for hosting a confirmed gas giant exoplanet, designated 14 Herculis b, which was discovered in 2002. This exoplanet is categorized as a super-Jupiter and completes...
Jupiter analog orbiting the nearby G-type star HD 190360 with an approximately 8-year period, one of the longer-period planets confirmed by radial velocity surveys.
HD 34445 b is a gas giant exoplanet orbiting the Sun-like star HD 34445 about 152 light-years away, discovered in 2009 via radial-velocity measurements from the Keck Observatory in Hawaii.
HD 219134 h is a distant exoplanet orbiting HD 219134, a nearby K-dwarf star mapped using radial velocity, located roughly 21 light-years away in the constellation Cassiopeia.
Jupiter analog orbiting the solar-type star HD 72659 with a period of roughly 3.6 years, discovered via radial velocity and notable for its long orbital period.
HD 217107 c is a long-period giant planet sharing the HD 217107 system with a hot Jupiter, detected through extended radial velocity monitoring over several years.
Long-period Jupiter-mass planet orbiting the G-type star HD 50499, discovered via radial velocity with an orbital period spanning several years.
HD 95338 b is a giant planet detected via radial velocity around HD 95338, a metal-rich sun-like star hosting a long-period planetary companion.
Outer gas giant companion in the HD 183263 system, detected via radial velocity with a longer orbital period than the inner planet HD 183263 b.
