Formation, Orbital and Internal Evolutions of Young Planetary Systems

@article{Baruteau2016FormationOA,
  title={Formation, Orbital and Internal Evolutions of Young Planetary Systems},
  author={C. Baruteau and X. Bai and C. Mordasini and P. Molli{\`e}re},
  journal={Space Science Reviews},
  year={2016},
  volume={205},
  pages={77-124}
}
  • C. Baruteau, X. Bai, +1 author P. Mollière
  • Published 2016
  • Physics
  • Space Science Reviews
  • The growing body of observational data on extrasolar planets and protoplanetary disks has stimulated intense research on planet formation and evolution in the past few years. The extremely diverse, sometimes unexpected physical and orbital characteristics of exoplanets lead to frequent updates on the mainstream scenarios for planet formation and evolution, but also to the exploration of alternative avenues. The aim of this review is to bring together classical pictures and new ideas on the… CONTINUE READING
    30 Citations

    Figures and Tables from this paper

    The contribution of the ARIEL space mission to the study of planetary formation
    • 6
    • Highly Influenced
    • PDF
    Migrating low-mass planets in inviscid dusty protoplanetary discs
    • PDF
    Pebble Accretion in Turbulent Protoplanetary Disks
    • 22
    • PDF
    Effects of the Planetary Temperature on the Circumplanetary Disk and on the Gap
    • 21
    • PDF
    Catching drifting pebbles. I. Enhanced pebble accretion efficiencies for eccentric planets
    • 25
    • PDF

    References

    SHOWING 1-10 OF 285 REFERENCES
    Theoretical models of planetary system formation: mass vs. semi-major axis
    • 93
    • PDF
    Planet-Disk Interaction and Orbital Evolution
    • 362
    • PDF
    Toward a Deterministic Model of Planetary Formation. VII. Eccentricity Distribution of Gas Giants
    • 109
    • PDF
    Dynamical Outcomes of Planet-Planet Scattering
    • 500
    • PDF
    The structure of protoplanetary discs around evolving young stars
    • 146
    • PDF
    The growth of planets by pebble accretion in evolving protoplanetary discs
    • 167
    • PDF
    Models of giant planet formation with migration and disc evolution
    • 438
    • PDF