Top Results for Long Period
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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...
Why this score
Long-period eclipsing mystery with disk companion, strong variable-star reputation but specialist appeal.
Scoring methodology
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...
Why this score
K-dwarf super-Jupiter host, useful long-period system but limited standout status.
Scoring methodology
Discovered in 2010 by the CoRoT satellite, CoRoT-9b is a gas giant notable for being the first transiting temperate exoplanet with a large orbit similar to the planet Mercury.
GJ 849 b is a gas-giant exoplanet detected by radial-velocity measurements around the nearby M dwarf GJ 849, about 29 light-years from the Sun. It has a minimum mass close to that of Jupiter, an orbital period of about 1,925 days, and a semimajor axis near 2.3 astronomical units. Its long orbit and...
HD 190360 b is a gas-giant exoplanet orbiting the nearby star HD 190360, a G-type subgiant in the constellation Lyra. Its orbit has a period of roughly eight years, placing it much farther from its star than the short-period giants found in many early exoplanet surveys. The planet was detected throu...
HD 34445 b is a giant exoplanet orbiting HD 34445, a Sun-like star about 152 light-years from Earth. It was discovered through radial-velocity observations made with the Keck Observatory and reported in 2009. The planet has a long orbital period compared with hot Jupiters, so it is commonly grouped...
HD 219134 h is a confirmed exoplanet orbiting the nearby K3V star HD 219134 in the constellation Cassiopeia. It was identified through radial-velocity measurements as part of a compact multi-planet system whose host star lies about 21 light-years from the Sun. The planet has a minimum mass greater t...
HD 72659 b is a gas-giant exoplanet orbiting the solar-type star HD 72659. It was detected through radial-velocity measurements and completes one orbit in roughly 3.6 years. The planet has a minimum mass several times that of Jupiter, so the term Jupiter analog refers mainly to its broad orbital sca...
HD 217107 c is a long-period giant exoplanet orbiting the star HD 217107 in the constellation Pisces. It was inferred from extended radial-velocity monitoring of a system that also contains the short-period planet HD 217107 b. The outer planet has a minimum mass of roughly two to three Jupiter masse...
HD 50499 b is a giant exoplanet orbiting the G-type star HD 50499. It was detected by radial-velocity measurements and has an orbital period of several years, placing it among the long-period planets found through extended stellar monitoring. Its wide orbit distinguishes it from close-in gas giants...
HD 95338 b is a giant exoplanet detected through radial-velocity observations of the star HD 95338. The host is a metal-rich star generally classified near the boundary between the G and K spectral types, and the planet has a long orbital period. It is an example of a massive planetary companion ide...
HD 183263 c is a confirmed gas-giant exoplanet in the HD 183263 system. It orbits a G-type star and is the outer member of a system that also contains the inner planet HD 183263 b. Its existence was established through radial-velocity observations, and its orbital period is substantially longer than...
Frequently Asked Questions
What leads the Long Period ranking?
Epsilon Aurigae currently leads the Long Period results with a displayed score of 8.00/10. This is an editorial ranking result for the items included on this page, not a universal verdict for every use case.
How should I read the score and confidence label?
The 0 to 10 score is Lunoo's ranking judgment. Strong confidence means 10 or more recorded comparison checks, some means 2 to 9, and provisional means fewer than 2.
What supports this ranking?
Lunoo combines category fit, feature coverage, pricing and value signals, public reception, recency, and peer comparisons. Public source links support factual item details when available, but they are not required for membership in this 12-item ranking.
Can I compare the leading results for Long Period?
Yes. The comparison links put adjacent leaders side by side so you can inspect differences that one ranking score cannot capture.
