Origin and Formation of Planetary Systems
Artikel i vetenskaplig tidskrift, 2010

To estimate the occurrence of terrestrial exoplanets and maximize the chance of finding them, it is crucial to understand the formation of planetary systems in general and that of terrestrial planets in particular. We show that a reliable formation theory should not only explain the formation of the Solar System, with small terrestrial planets within a few AU and gas giants farther out, but also the newly discovered exoplanetary systems with close-in giant planets. Regarding the presently known exoplanets, we stress that our current knowledge is strongly biased by the sensitivity limits of current detection techniques (mainly the radial velocity method). With time and improved detection methods, the diversity of planets and orbits in exoplanetary systems will definitely increase and help to constrain the formation theory further. In this work, we review the latest state of planetary formation in relation to the origin and evolution of habitable terrestrial planets.

giant planets

solar nebula

protoplanetary disks


orbital migration

mass planets

Planet formation

stellar x-ray



Gas giants



Terrestrial exoplanets

Ice giants


Y. Alibert

Universität Bern

Observatoire de Besancon

C. Broeg

Universität Bern

W. Benz

Universität Bern

G. Wuchterl

Thüringer Landessternwarte Tautenburg

O. Grasset

CNRS Centre National de la Recherche Scientifique

C. Sotin

CNRS Centre National de la Recherche Scientifique

C. Eiroa

Universidad Autonoma de Madrid (UAM)

T. Henning

Max Planck-institutet

T. Herbst

Max Planck-institutet

L. Kaltenegger

Harvard-Smithsonian Center for Astrophysics

A. Leger

Universite Paris-Sud XI

René Liseau

Chalmers, Institutionen för radio- och rymdvetenskap, Radioastronomi och astrofysik

H. Lammer

Institut fur Weltraumforschung

C. Beichman

Jet Propulsion Laboratory, California Institute of Technology

W. Danchi

NASA Goddard Space Flight Center

M. Fridlund


J. Lunine

University of Arizona

F. Paresce

Istituto Nazionale Di Astrofisica, Rome

A. Penny

Rutherford Appleton Laboratory

Royal Observatory

A. Quirrenbach

Landessternwarte Heidelberg

H. Rottgering

Universiteit Leiden

F. Selsis

Universite de Bordeaux

J. Schneider

Observatoire de Paris-Meudon

D. Stam

Netherlands Institute for Space Research (SRON)

G. Tinetti

University College London (UCL)

G. J. White

Rutherford Appleton Laboratory

Open University


1531-1074 (ISSN)

Vol. 10 19-32


Astronomi, astrofysik och kosmologi


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