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开普勒-36:一对轨道相邻但密度不同的行星。

Kepler-36: a pair of planets with neighboring orbits and dissimilar densities.

机构信息

Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA.

出版信息

Science. 2012 Aug 3;337(6094):556-9. doi: 10.1126/science.1223269. Epub 2012 Jun 21.

Abstract

In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in giant planets around other stars was the first clue that this pattern is not universal and that planets' orbits can change substantially after their formation. Here, we report another violation of the orbit-composition pattern: two planets orbiting the same star with orbital distances differing by only 10% and densities differing by a factor of 8. One planet is likely a rocky "super-Earth," whereas the other is more akin to Neptune. These planets are 20 times more closely spaced and have a larger density contrast than any adjacent pair of planets in the solar system.

摘要

在太阳系中,行星的组成随轨道距离而变化,靠近轨道的是岩石行星,而较远轨道的是低密度的气态巨行星。在其他恒星周围发现近距离的巨行星,这首先表明这种模式并非普遍存在,而且行星的轨道在形成后可能会发生实质性变化。在这里,我们报告了另一种违反轨道-组成模式的情况:两颗行星围绕同一颗恒星运行,轨道距离仅相差 10%,密度相差 8 倍。其中一颗行星可能是岩石“超级地球”,而另一颗则更类似于海王星。这两颗行星的间距是太阳系中任何相邻行星对的 20 倍,密度差异也更大。

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