Formation of multi-planetary systems in turbulent disks

Details Formation of multi-planetary systems in turbulent disks Formation of multi-planetary systems in turbulent disks

2009-04-27

arxiv.org/abs/0904.4160v1

EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP Conference Proceedings,

Astronomy and Astrophysics

Astrophysics

Earth and Planetary Astrophysics

4 pages, 2 figures, 2nd Subaru International Conference on Exoplanets and Disks: Their Formation and Diversity, Keauhou - Hawa

Scientific paper

10.1063/1.3215915

We summarize the analytic model and numerical simulations of stochastically forced planets in a turbulent disk presented in a recent paper by Rein and Papaloizou. We identify two modes of libration in systems with planets in mean motion resonance which react differently to random forces. The slow mode, which mostly corresponds to motion of the angle between the apsidal lines of the two planets, is converted to circulation more readily than the fast mode which is associated with oscillations of the semi-major axes. We therefore conclude that stochastic forcing due to disk turbulence may have played an important role in shaping the configuration of observed systems in mean motion resonance. For example, it naturally provides a mechanism for accounting for the HD128311 system for which the fast mode librates and the slow mode does not.

Affiliated with

Also associated with

No associations

Rating

Formation of multi-planetary systems in turbulent disks does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Formation of multi-planetary systems in turbulent disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of multi-planetary systems in turbulent disks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-322866