The formation of Uranus and Neptune in the Jupiter–Saturn region of the Solar System

作者: Edward W. Thommes , Martin J. Duncan , Harold F. Levison

DOI: 10.1038/45185

关键词:

摘要: Planets are believed to have formed through the accumulation of a large number small bodies1,2,3,4. In case gas-giant planets Jupiter and Saturn, they accreted significant amount gas directly from protosolar nebula after accumulating solid cores about 5–15 Earth masses5,6. Such models, however, been unable produce smaller ice giants7,8 Uranus Neptune at their present locations, because in that region Solar System planetary bodies will more widely spaced, less tightly bound gravitationally Sun. When applied current Jupiter–Saturn zone, recent theory predicts that, addition two or three other comparable mass likely formed9. Here we report results model calculations demonstrate such scattered outwards as Jupiter, perhaps nebular gas. The orbits these then evolve into resemble those Neptune, result gravitational interactions with outer disk nebula.

参考文章(23)
Harold F. Levison, Jack J. Lissauer, Martin J. Duncan, Modeling the Diversity of Outer Planetary Systems The Astronomical Journal. ,vol. 116, pp. 1998- 2014 ,(1998) , 10.1086/300557
Craig B Agnor, Robin M Canup, Harold F Levison, On the Character and Consequences of Large Impacts in the Late Stage of Terrestrial Planet Formation Icarus. ,vol. 142, pp. 219- 237 ,(1999) , 10.1006/ICAR.1999.6201
Stuart J. Weidenschilling, Francesco Marzari, Gravitational scattering as a possible origin for giant planets at small stellar distances Nature. ,vol. 384, pp. 619- 621 ,(1996) , 10.1038/384619A0
Frederic A. Rasio, Eric B. Ford, Dynamical Instabilities and the Formation of Extrasolar Planetary Systems Science. ,vol. 274, pp. 954- 956 ,(1996) , 10.1126/SCIENCE.274.5289.954
Peter Bodenheimer, James B. Pollack, Calculations of the accretion and evolution of giant planets: The effects of solid cores Icarus. ,vol. 67, pp. 391- 408 ,(1986) , 10.1016/0019-1035(86)90122-3
Eiichiro Kokubo, Shigeru Ida, Oligarchic growth of protoplanets Icarus. ,vol. 131, pp. 171- 178 ,(1998) , 10.1006/ICAR.1997.5840
Harold F. Levison, Martin J. Duncan, From the Kuiper Belt to Jupiter-Family Comets: The Spatial Distribution of Ecliptic Comets Icarus. ,vol. 127, pp. 13- 32 ,(1997) , 10.1006/ICAR.1996.5637
James B. Pollack, Olenka Hubickyj, Peter Bodenheimer, Jack J. Lissauer, Morris Podolak, Yuval Greenzweig, Formation of the Giant Planets by Concurrent Accretion of Solids and Gas Icarus. ,vol. 124, pp. 62- 85 ,(1996) , 10.1006/ICAR.1996.0190
Renu Malhotra, Joseph M. Hahn, Orbital Evolution of Planets Embedded in a Planetesimal Disk The Astronomical Journal. ,vol. 117, pp. 3041- 3053 ,(1999) , 10.1086/300891