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The Smithers Divide

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File:Smithers' Divide.jpg
A plot demonstrating The Smithers Divide, created using scipy and matplotlib.

In Binary Systems containing one or more planets, if ϕPaSaϵ<0.75, the planet's orbit is almost always unstable, where ϕPaSa is the ratio of planetary semi-major axis to stellar semi-major axis, and ϵ is the stellar orbital eccentricity. However, when ϕϵ=0.25, 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.[1]

References

  1. Smithers, et al. March 2015. The Smithers Divide

External links



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