2024年10月24日 · Kepler-39 b is a gas giant exoplanet that orbits a F-type star. Its mass is 20.1 Jupiters, it takes 21.1 days to complete one orbit of its star, and is 0.164 AU from its star. Its discovery was announced in 2011.

Kepler-39b (formerly known as KOI-423b), is a confirmed extrasolar object (either a Jovian planet or brown dwarf because of its mass) discovered orbiting the F-type star Kepler-39. It is eighteen times more massive than Jupiter, and is about five fourths its size.

开普勒39b （英语：Kepler-39b，先前称为 KOI-423b）是一个已确认的 太阳系外 天体。 由于其质量而它被认为可能是类木行星或 棕矮星。 该行星被发现绕F型恒星 开普勒39 运行。 它的质量是木星的十八倍，大小约为木星的四分之五。 这颗行星围绕其主恒星运行的轨道距离约为地球与太阳平均距离的15%。 欧洲天文学家使用法国 上普罗旺斯天文台 的设备，对开普勒39b的主星以及其他三颗恒星（包括 开普勒40b 的主星）进行了研究。 2010年底的数据收集和分析确认了开普 …

開普勒39b （英語：Kepler-39b，先前稱為 KOI-423b ）是一個已確認的 太陽系外 天體。 由於其質量而它被認為可能是類木行星或 棕矮星 。 該行星被發現繞F型恆星 開普勒39 運行。 它的質量是木星的十八倍，大小約為木星的四分之五。 這顆行星圍繞其主恆星運行的軌道距離約為地球與太陽平均距離的15%。 歐洲天文學家使用法國 上普羅旺斯天文台 的設備，對開普勒39b的主星以及其他三顆恆星（包括 開普勒40b 的主星）進行了研究。 2010年底的數據收集和分析確認了開普 …

Kepler-39 (2MASS J19475046+4602034) is an F-type main sequence star located in the constellation Cygnus. It is located about 3,500 light-years (1,070 parsecs) away. [ 1 ] One known substellar companion orbits it, Kepler-39b .

Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. Transit Timing Observations from Kepler. IX. Catalog of the Full Long-cadence Data Set. Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets. SOPHIE velocimetry of Kepler transit candidates. III.

Kepler-39b is a confirmed extrasolar object discovered orbiting the F-type star Kepler-39. It is formerly known as KOI 423b. Lets get to know more about Kepl...

Kepler-39 b is an exoplanet orbiting the star Kepler-39, located about 3446.8 light-years (1056.8 pc) away from Solar System. Its discovery was publicly announced on 2011. The host star Kepler-39 has apparent magnitude of 14.3, with absolute magnitude of 4.2. It is 1.3 times more massive and 1.2 times bigger compared with our Sun.

2017年8月29日 · Using Kepler photometry, we examined the brown dwarf Kepler-39b and the warm Saturn Kepler-427b. We could not reliably constrain the oblateness of Kepler-39b. We find transit depth variations for Kepler-427b at 90.1% significance ( 1.65σ) consistent with a precession period of Pprec = 5.45+0.46−0.37 years and an oblateness, f = 0.19+0.32−0.16.

Kepler-39b, formerly known as KOI-423b, is a Jupiter-like planet discovered in the orbit of F-type star Kepler-39. Kepler-39b is eighteen times more massive than Jupiter, and is about a five fourths its size.