• Intro
  • Diversity
    • Extra Solar Planets
      • Upsilon And
  • History
    • Dole Fig
  • Outline
  • Disclaimer
  • Methods
    • Load M vs a
      • Load M vs e
  • Methods (cont)
    • Pollack et al.
  • Instabilities in Systems
    • Movie 1
    • Run 6b
  • Are We Constructing Reasonable Systems?
    • zeta vs dl
  • Characteristics of Outer Planetary Systems
    • Histogram
    • Run 12b
    • Run 14a
    • Run 6b again
    • Run 15a
    • Run 9a
    • Run 11a
  • Characteristics of Outer Planetary Systems (cont.)
    • Run 11a again
      • Critical Argument
    • Run 4a
      • Critical Argument
    • Run 10a
      • Critical Argument
    • Run 7b
    • Movie 2
    • Orb El Run 7b
  • Conclusions

  • Formation of Uranus and Neptune
    • Ip 89 1
      • Ip 89 3
    • No drag: e vs t
    • M vs a
      • anim
  • Can drag keep the system cold enough to allow accretion?
    • M vs a
      • anim

  • A New Idea
    • Run 4f Animation
      • Last Frame Run 4f
  • Talking About?
    • Oligarchic Growth
      • KI fig
    • M vs t
    • a,q,Q(t) of run 4f
  • The Runs
    • Series I top
      • Series I bottom
    • Run 10a frame 1
      • Run 10a Animation
        • Last Frame Run 10a
    • Series II top
      • Series II bottom
    • Run 12f frame 1
      • Run 12f Animation
        • Last Frame Run 12f
    • Series III top
      • Series III bottom
  • Observational support
  • Conclusions
  • Back to Other Systems