Planet Formation and Disk-Planet Interactions

Publication typeBook Chapter
Publication date2019-02-02
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ISSN18617980, 18618227
Abstract
This review is based on lectures given at the 45th Saas-Fee Advanced Course “From Protoplanetary Disks to Planet Formation” held in March 2015 in Les Diablerets, Switzerland. Starting with an overview of the main characterictics of the Solar System and the extrasolar planets, we describe the planet formation process in terms of the sequential accretion scenario. First the growth processes of dust particles to planetesimals and subsequently to terrestrial planets or planetary cores are presented. This is followed by the formation process of the giant planets either by core accretion or gravitational instability. Finally, the dynamical evolution of the orbital elements as driven by disk-planet interaction and the overall evolution of multi-object systems is presented.
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Kley W. Planet Formation and Disk-Planet Interactions // Saas-Fee Advanced Courses. 2019. pp. 151-260.
GOST all authors (up to 50) Copy
Kley W. Planet Formation and Disk-Planet Interactions // Saas-Fee Advanced Courses. 2019. pp. 151-260.
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RIS Copy
TY - GENERIC
DO - 10.1007/978-3-662-58687-7_2
UR - https://doi.org/10.1007/978-3-662-58687-7_2
TI - Planet Formation and Disk-Planet Interactions
T2 - Saas-Fee Advanced Courses
AU - Kley, Wilhelm
PY - 2019
DA - 2019/02/02
PB - Springer Nature
SP - 151-260
SN - 1861-7980
SN - 1861-8227
ER -
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@incollection{2019_Kley,
author = {Wilhelm Kley},
title = {Planet Formation and Disk-Planet Interactions},
publisher = {Springer Nature},
year = {2019},
pages = {151--260},
month = {feb}
}