Remarks on modeling the formation of Uranus and Neptune

Icarus

Volumn 153, Issue 1, 2001, Pages 224-228

  Levison, Harold F ^a   Stewart, Glen R ^b  

^a SOUTHWEST RESEARCH INSTITUTE   (United States)

^b UNIVERSITY OF COLORADO   (United States)

Author keywords

Formation; Solar system

Indexed keywords

EID: 0035189966     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.2001.6672     Document Type: Article

References (26)

1. Velocity distributions among colliding asteroids
2. Numerical simulations of the accretion of Uranus and Neptune
3. Protoplanetary formation I. Neptune
4. A multiple time step symplectic alogrithm for integrating close encounters
5. Orbital expansion and resonant trapping during the late accretion stages of the outer planets
6. High-accuracy statistical simulation of planetary accretion: II. Comparison with N-body simulation
7. Orbital migration of Neptune and the orbital distribution of trans-neptunian objects
8. Dynamical processes of macro-accretion of Uranus and Neptune-A first look
9. Symplectically integrating close encounters with the Sun
10. Growth of planet from planetesimals
11. Formation of the Neptune system
12. Collision probabilities with the planets and the distribution of interplanetary mater
13. Symplectic integration with variable stepsize
14. On the formation of Uranus and Neptune
15. Growth of a migrating protoplanet
16. The formation of Uranus and Neptune in the Jupiter-Saturn region of the Solar System
17. Resonant relaxation in protoplanetary disks
18. On disk-planet interactions and orbital eccentricities
19. Density waves in the solar nebula-Planetesimal velocities
20. On planetesimal formation: The role of collective particle behavior
21. Disk tides and accretion runaway
22. Dynamics of the trans-neptunian region: Apsidal waves in the Kuiper belt
23. The origin of comets in the solar nebula: A unified model
24. Formation of planetesimals in the solar nebula
25. Formation of planetary embryos - Effects of fragmentation, low relative velocity, and independent variation of eccentricity and inclination
26. Symplectic maps for the n-body problem