Kepler-167
Kepler-167 is a K-type main-sequence star located about  away from the Solar System in the constellation of Cygnus. The star has about 78% the mass and 75% the radius of the Sun, and a temperature of . It hosts a system of four known exoplanets. There is also a companion red dwarf star at a separation of about , with an estimated orbital period of over 15,000 years. Planetary system 

Kepler-167 is orbited by four known transiting exoplanets, discovered using the Kepler space telescope. The inner three planets are all super-Earths of unknown composition orbiting closer to their star than Mercury is to the Sun. The outermost planet, Kepler-167e, is a Jupiter analog, with , , and an equilibrium temperature of . It is the first transiting Jupiter analog discovered. The inner two planets were confirmed in 2014, as part of a study validating hundreds of Kepler planets, and the outer two planets were confirmed in 2016. Observations of Kepler-167e using the Spitzer Space Telescope, published in 2019, ruled out significant transit timing variations, making it easier to predict future transits and plan follow-up observations. As a rare example of a long-period transiting gas giant, Kepler-167e is a target of interest for further observations, for example to characterize its atmosphere. , four transits of planet e have been detected, with both space-based and ground-based observations. References 

Cygnus (constellation)
Binary stars
K-type main-sequence stars
M-type main-sequence stars
Planetary systems with four confirmed planets
0490
J19303802+3820434