cosmogony;
numerical simulations;
outer planets;
solar system;
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
The present status of our knowledge about the accretion process of Uranus and Neptune is discussed, emphasising in the possible origin of the orbital structure at the time of formation of the outer solar system. The most important influences of this process over the entire solar system are also discussed: in the inner planetary region, contributing to the formation. of the planetary atmospheres and water reservoirs; in the asteroid and Kuiper belts, sculpting their primordial structures, and in the outer edge of the solar system, building up the Oort cloud of comets.
机构:
LPG Nantes UMR 6112, Lab Planetol & Geodynam, 2 Rue Houssiniere, F-44322 Nantes 03, FranceLPG Nantes UMR 6112, Lab Planetol & Geodynam, 2 Rue Houssiniere, F-44322 Nantes 03, France
Grasset, O.
Castillo-Rogez, J.
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h-index: 0
机构:
CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USALPG Nantes UMR 6112, Lab Planetol & Geodynam, 2 Rue Houssiniere, F-44322 Nantes 03, France
Castillo-Rogez, J.
Guillot, T.
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h-index: 0
机构:
Observ Cote Azur, Bd Observ, F-06304 Nice 4, FranceLPG Nantes UMR 6112, Lab Planetol & Geodynam, 2 Rue Houssiniere, F-44322 Nantes 03, France
Guillot, T.
Fletcher, L. N.
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h-index: 0
机构:
Univ Leicester, Dept Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, EnglandLPG Nantes UMR 6112, Lab Planetol & Geodynam, 2 Rue Houssiniere, F-44322 Nantes 03, France
Fletcher, L. N.
Tosi, F.
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h-index: 0
机构:
INAF IAPS Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00133 Rome, ItalyLPG Nantes UMR 6112, Lab Planetol & Geodynam, 2 Rue Houssiniere, F-44322 Nantes 03, France