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The Anglo-Australian planet search XX: a solitary ice-giant planet orbiting HD 102365

机译:英澳行星搜寻XX:一颗环绕HD 102365的巨型冰巨行星

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摘要

We present 12 years of precision Doppler data for the very nearby G3 star HD 102365, which reveals the presence of a Neptune-like planet with a 16.0 M Earth minimum mass in a 122.1 day orbit. Very few 'Super Earth' planets have been discovered to date in orbits this large and those that have been found reside in multiple systems of between three and six planets. HD 102365 b, in contrast, appears to orbit its star in splendid isolation. Analysis of the residuals to our Keplerian fit for HD 102365 b indicates that there are no other planets with minimum mass above 0.3 M Jup orbiting within 5 AU and no other 'Super Earths' more massive than 10 M Earth orbiting at periods shorter than 50 days. At periods of less than 20 days these limits drop to as low as 6 M Earth. There are now 32 exoplanets known with minimum mass below 20 M Earth, and interestingly the period distributions of these low-mass planets seem to be similar whether they orbit M-, K-, or G-type dwarfs.
机译:我们为附近的G3恒星HD 102365提供了12年的精确多普勒数据,该数据揭示了在122.1天的轨道中存在最小质量为16.0 M的海王星状行星。迄今为止,很少有“超地球”行星在如此大的轨道上被发现,而被发现存在于三到六颗行星的多个系统中。相比之下,HD 102365 b似乎以出色的隔离性绕其恒星运行。对我们的适用于HD 102365 b的开普勒拟合残差的分析表明,没有其他行星的最小质量超过0.3 M焦距的轨道在5 AU之内,并且没有其他“超级地球”的质量大于10 M的地球在不到50天的时间内轨道运行。在不到20天的时间里,这些限制降至地球6M。现在已知有32个系外行星,其最小质量在20 M地球以下,有趣的是,这些低质量行星的周期分布似乎都围绕M型,K型或G型矮星运行。

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