Planet-Disc Interactions and Early Evolution of Planetary Systems

  title={Planet-Disc Interactions and Early Evolution of Planetary Systems},
  author={C. Baruteau and A. Crida and S. Paardekooper and F. Masset and J. Guilet and B. Bitsch and R. Nelson and W. Kley and J. Papaloizou},
  journal={arXiv: Earth and Planetary Astrophysics},
The great diversity of extrasolar planetary systems has challenged our understanding of how planets form, and how their orbits evolve as they form. Among the various processes that may account for this diversity, the gravitational interaction between planets and their parent protoplanetary disc plays a prominent role in shaping young planetary systems. Planet-disc forces are large, and the characteristic times for the evolution of planets orbital elements are much shorter than the lifetime of… Expand

Figures from this paper

The dispersal of planet-forming discs: theory confronts observations
Empirical constraints on disc evolution and dispersal are reviewed with special emphasis on transition discs, a subset of discs that appear to be caught in the act of clearing out planet-forming material. Expand
Planetary Migration in Protoplanetary Disks.
The known exoplanet population displays a great diversity of orbital architectures, and explaining the origin of this is a major challenge for planet formation theories. The gravitational interactionExpand
Planet formation and disk-planet interactions
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 anExpand
From Disks to Planets: The Making of Planets and Their Early Atmospheres. An Introduction
This paper is an introduction to volume 56 of the Space Science Series of ISSI, “From disks to planets—the making of planets and their proto-atmospheres”, a key subject in our quest for the originsExpand
The structure of protoplanetary discs around evolving young stars
The formation of planets with gaseous envelopes takes place in protoplanetary accretion discs on time scales of several million years. Small dust particles stick to each other to form pebbles,Expand
Forming Planets via Pebble Accretion
The detection and characterization of large populations of pebbles in protoplanetary disks have motivated the study of pebble accretion as a driver of planetary growth. This review covers all aspectsExpand
The growth of planets by pebble accretion in evolving protoplanetary discs
The formation of planets depends on the underlying protoplanetary disc structure, which in turn influences both the accretion and migration rates of embedded planets. The disc itself evolves on timeExpand
A new and simple prescription for planet orbital migration and eccentricity damping by planet–disc interactions based on dynamical friction
During planet formation gravitational interaction between a planetary embryo and the protoplanetary gas disc causes orbital migration of the planetary embryo, which plays an important role in shapingExpand
Migrating low-mass planets in inviscid dusty protoplanetary discs
Disc-driven planet migration is integral to the formation of planetary systems. In standard, gas-dominated protoplanetary discs, low-mass planets or planetary cores undergo rapid inwards migrationExpand


Celestial Mechanics and Dynamical Astronomy Equations for the orbital elements : Hidden symmetry
We revisit the Lagrange and Delaunay systems of equations for the orbital elements, and point out a previously neglected aspect of these equations: in both cases the orbit resides on a certainExpand