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The Smithers Divide : ウィキペディア英語版 | The Smithers Divide
In Binary Systems containing one or more planets, if , the planet's orbit is almost always unstable, where is the ratio of planetary semi-major axis to stellar semi-major axis, and is the stellar orbital eccentricity. However, when , the planetary orbits appear to be stable. The Smithers Divide is this phenomenon, and is currently a topic of ongoing research at the University of California, Santa Cruz. It is named after Benjamin Smithers, a student at the University of California, Santa Cruz, California, United States.〔Smithers, et al. March 2015. The Smithers Divide〕 ==References==
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