Figure 15 from Multiple-planet Scattering and the Origin of Hot Jupiters

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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 15.

Simulated evolution of the stellar spin–orbit angle and the hot Jupiter's semimajor axis over Gyr-long timescales. The red (black) circles show the results in the three-planet (four-planet case). These results were obtained by simulating the tidal effects with our semi-analytical model.

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