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Multiple-planet Scattering and the Origin of Hot Jupiters

  • Authors: C. Beaugé and D. Nesvorný

Beaugé & Nesvorný 2012 The Astrophysical Journal 751 119.

  • Provider: AAS Journals

Caption: Figure 10.

Same as Figure 9, but for a system that produced a hot Jupiter on a prograde orbit. Note that the scale of the middle plot has changed with respect to Figure 9. Also, in this case, planetary masses were m 1 = 1  M Jup, m 2 = 0.5  M Jup, and m 3 = 0.5  M Jup.

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