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Growth and interaction of planets

Published online by Cambridge University Press:  26 May 2016

Pawel Artymowicz
Pawel Artymowicz*
Affiliation:
Stockholm Observatory, SE-13336 Saltsjöbaden, Sweden, [email protected]

Abstract

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We discuss theories of origin and evolution of the newly discovered extrasolar planetary systems. As these systems failed to fulfill prior expectations concerning their orbital structure, we are challenged to extend and/or revise many preexisting theories. Important extensions include migration of bodies in disks and planetary eccentricity pumping by planet-planet interaction and primordial disk-planet interaction. Progress in observational techniques will allow us to find which of these two types of interaction is responsible for the observed variety of orbits and masses of planets. New insights into the formation of giant planets in our system can be obtained by asking why Jupiter and Saturn are not larger, closer to the sun and/or do not follow noticeably elliptic orbits.

Type
Part II: Progress in the theory of planet formation
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 149 - 158
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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