Anders Johansen
Professor
Giant Planet Formation and Migration
Author
Summary, in English
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.
Department/s
- Lund Observatory - Has been reorganised
Publishing year
2018-02-01
Language
English
Publication/Series
Space Science Reviews
Volume
214
Issue
1
Document type
Journal article review
Publisher
Springer
Topic
- Astronomy, Astrophysics and Cosmology
Keywords
- Planet-disc interactions
- Planets and satellites: formation
- Planets and satellites: gaseous planets
- Protoplanetary discs
Status
Published
ISBN/ISSN/Other
- ISSN: 0038-6308