Giant Planet Formation and Migration

被引：0
作者：
Sijme-Jan Paardekooper
Anders Johansen
机构：
[1] University of London,Astronomy Unit, School of Physics and Astronomy, Queen Mary
[2] Lund University,Lund Observatory, Department of Astronomy and Theoretical Physics
来源：
Space Science Reviews | 2018年 / 214卷
关键词：
Planet-disc interactions; Planets and satellites: formation; Planets and satellites: gaseous planets; Protoplanetary discs;
D O I：
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学科分类号：
摘要：
Planets form in circumstellar discs around young stars. Starting with sub-micron sized dust particles, giant planet formation is all about growing 14 orders of magnitude in size. It has become increasingly clear over the past decades that during all stages of giant planet formation, the building blocks are extremely mobile and can change their semimajor axis by substantial amounts. In this chapter, we aim to give a basic overview of the physical processes thought to govern giant planet formation and migration, and to highlight possible links to water delivery.
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