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On the Origin of Orbits in Extrasolar Planetary Systems - PowerPoint PPT Presentation


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Outline. Observations show that extrasolar planetary systems fill the (a,e) planePlanet migration with disk torques and planet scattering is successful, but raises several issues: [1] Eccentricity damping vs excitation [2] Turbulence potentially compromises mean motion resonance. . MIGRATIO

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