From Gas to Satellitesimals: Disk Formation and Evolution

被引：21

作者：

Coradini, A. ^{[1
]}

Magni, G. ^{[2
]}

Turrini, D. ^{[1
]}

机构：

[1] INAF IFSI, I-00133 Rome, Italy

[2] INAF IASF, I-00133 Rome, Italy

来源：

SPACE SCIENCE REVIEWS | 2010年 / 153卷 / 1-4期

关键词：

Solar system: formation; Planets and satellites: formation; Accretion disks; Planets and satellites: Jupiter; Planets and satellites: Saturn; CRITICAL MASS; PLANETS; DIVERSITY; JUPITER; SYSTEMS;

D O I：

10.1007/s11214-009-9611-9

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The subject of satellite formation is strictly linked to the one of planetary formation. Giant planets strongly shape the evolution of the circum-planetary disks during their formation and thus, indirectly, influence the initial conditions for the processes governing satellite formation. In order to fully understand the present features of the satellite systems of the giant planets, we need to take into account their formation environments and histories and the role of the different physical parameters. In particular, the pressure and temperature profiles in the circum-planetary nebulae shaped their chemical gradients by allowing for the condensation of ices and noble gases. These chemical gradients, in turn, set the composition of the satellitesimals, which represent the building blocks of the present regular satellites.

引用

页码：411 / 429

页数：19

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[1] Neptune's capture of its moon Triton in a binary-planet gravitational encounter [J].