The formation of the terrestrial planets from lunar sized planetesimals
作者： Sverre J. Aarseth , Myron Lecar
DOI: 10.1017/S0252921100101745
关键词: Geology 、 Astrobiology 、 Eccentricity (behavior) 、 Secondary atmosphere 、 Terrestrial planet 、 Planetary migration 、 Inelastic collision 、 Planetesimal 、 Planetary mass 、 Protoplanet
摘要:
harvard.edu
sci-hub.st 参考文章(5)
Richard Greenberg, John F. Wacker, William K. Hartmann, Clark R. Chapman, Planetesimals to planets: Numerical simulation of collisional evolution Icarus. ,vol. 35, pp. 1- 26 ,(1978) , 10.1016/0019-1035(78)90057-X
T.A. Heppenheimer, Secular resonances and the origin of eccentricities of Mars and the asteroids Icarus. ,vol. 41, pp. 76- 88 ,(1980) , 10.1016/0019-1035(80)90160-8
Larry P. Cox, John S. Lewis, Numerical simulation of the final stages of terrestrial planet formation. Icarus. ,vol. 44, pp. 706- 721 ,(1980) , 10.1016/0019-1035(80)90138-4
William M. Kaula, Equilibrium velocities of a planetesimal population Icarus. ,vol. 40, pp. 262- 275 ,(1979) , 10.1016/0019-1035(79)90071-X
George W. Wetherill, Formation of the Terrestrial Planets Annual Review of Astronomy and Astrophysics. ,vol. 18, pp. 77- 113 ,(1980) , 10.1146/ANNUREV.AA.18.090180.000453