Kepler-35 is a binary star system in the constellation of Cygnus. These stars, called Kepler-35A and Kepler-35B have masses of 89% and 81% solar masses respectively, and both are assumed to be of spectral class G. They are separated by 0.176 AU, and complete an eccentric orbit around a common center of mass every 20.73 days. [5]

2024年10月24日 · Kepler-35 b is a gas giant exoplanet that orbits a G-type star. Its mass is 0.127 Jupiters, it takes 131.5 days to complete one orbit of its star, and is 0.60347 AU from its star. Its discovery was announced in 2011.

克卜勒35（Kepler-35）是一个联星系统。 该系统的成员星分别称为 克卜勒35A （Kepler-35A）和 克卜勒35B （Kepler-35B），两者的质量分别是太阳的89%和81%，并且都是 G型 恒星。

克卜勒35 （Kepler-35）是一個 聯星 系統。 該系統的成員星分別稱為 克卜勒35A （Kepler-35A）和 克卜勒35B （Kepler-35B），兩者的質量分別是太陽的89%和81%，並且都是 G型 恆星。 這兩顆恆星相距0.176天文單位，並以20.73日軌道週期在橢圓軌道互繞 [2]。 該系統有一顆 環聯星運轉行星 克卜勒35b（Kepler-35b），屬於 氣體巨行星。 該行星的質量稍微超過木星的八分之一，半徑大約是木星的0.728倍。 克卜勒35b以軌道週期131.458日在橢圓軌道上環繞克卜勒35聯 …

2012年1月13日 · An artist's rendition of the Kepler-35 planetary system, in which a Saturn-size planet orbits a pair of stars. Kepler-35b orbits its smaller and cooler host stars than our sun every 131 days, and the stellar pair orbits each other every 21 days.

开普勒35（Kepler-35）是一个联星系统。 该系统的成员星分别称为开普勒35A（Kepler-35A）和开普勒35B（Kepler-35B），两者的质量分别是太阳的89%和81%，并且都是G型恒星。

2012年1月11日 · Kepler-34 b orbits two Sun-like stars every 289 days, whereas Kepler-35 b orbits a pair of smaller stars (89% and 81% of the Sun’s mass) every 131 days. The planets experience large...

Kepler-35(AB) b is a planet orbiting two sub solar-mass stars which are in a binary (therefore the name with AB). The Kepler team estimates that approximately 1% of all close binary stars have planets.

2012年4月18日 · Here we present two additional transiting circumbinary planets, Kepler-34 and Kepler-35. Each is a low-density gas giant planet on an orbit closely aligned with that of its parent stars. Kepler-34 orbits two Sun-like stars every 289 days, while Kepler-35 orbits a pair of smaller stars (89% and 81% of the Sun's mass) every 131 days.

Here we report two additional transiting circumbinary planets: Kepler-34 (AB)b and Kepler-35 (AB)b, referred to here as Kepler-34 b and Kepler-35 b, respectively. Each is a low-density...