Neptunes Resonances With Kuiper Belt Objects and What It Tells Us About the Early Solar System The Origin of Plutos Orbit: Implications for the Solar System Beyond Neptune Renu Malhotra A signature of Planetary Migration: The Origin of Asymmetric Capture in the 2:1 Resonance Ruth A. Murray-Clay & Eugene I. Chiang On the Plutinos and Twotinos of the Kuiper Belt E.I. Chiang & A.B. Jordan Resonant and Secular Families of the Kuiper Belt E.I. Chiang The Effect of Neptunes Accretion on Pluto and the Plutinos Paul Wiegert Horseshoe Orbit Stationary frame | Rotating frame Janus & Epimetheus The Migration of the Planets Initial orbit (AU)MigrationFinal orbit Jupiter Saturn Uranus Neptune Pluto migrates out as a result of being in resonance with Neptune Eccentricity final from Eccentricity initial, resonance, and initial and final semi-major axes of the migrating planet Groupings of the test particles Semi-major axis, eccentricity, and inclination over the period 0 to 10 8 years resonance angle argument of perihelion ColdHot e=0.001, sini=e/2e=0.1, sini=e/2 Eccentricity and inclination of the known Plutinos, and of the simulated particles under hot conditions Different distributions reveal the rate of migration 10 7 yrs10 6 yrs Known PlutinosSimulated Particles Dione A Jupiter-mass planet spends 50,000 years of migrating from 1 AU to 4 AU. As its exterior resonances swept through a group of planetesimals, it excited their orbits and captured them into resonances. Rotating Frame images of the orbits of the captured particles.
