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Althea Moorhead: Reproducing a vs. e
2005: Giant planet migration through the action of disk torques and planet-planet scattering
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Type II migration damps the semi-major axes a, while planet
scattering increases the orbital eccentricities ε. Our
experiments (red squares) fill the a - ε plane (shown), in
rough agreement with observations (black stars). |
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Giant planet migration through the action of disk torques and planet-planet scattering, (A. V.
Moorhead and F. C. Adams), Icarus 178, 517-539 (2005).
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