Figure 11 from Multiple-planet Scattering and the Origin of Hot Jupiters

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 11.

Rare example of a planetary system showing clear effects of the Lidov–Kozai resonance. A Pop-II hot Jupiter formed in this simulation. Planetary masses were m ₁ = 1 M _Jup, m ₂ = 2 M _Jup, and m ₃ = 1 M _Jup.

Other Images in This Article

Copyright and Terms & Conditions