| Preface A cknowledgments 1 Historical notes on planet formation Peter Bodenheimer 1.1 IntrOductiOn 1.2 Descartes and von Weizsficker：vortices 1.3 Magnetic effects l.4 Gravitational instability 1.5 Core accretion：gas capture 1.6 Planet searches 2 The Formation and Evolution of Planetary Systems：placing our Solar System in context Jeroen Bouwman，Michael R.Meyer,Jinyoung Serena Kim， Murray D.Silverstone，John M.Carpenter,and Dean C.Hines 2.1 IntrOductiOn 2.1.1 The formation of planets：from protoplanetary towards debris disk systems 2.1.2 The Spitzer Space Telescope and the formation and evolution of planetary systems legacy program 2.2 From protoplanetary to debris disks：processing and dispersion of the inner dust disk 2.3 Debris disks：Asteroid or Kuiper Belt？ 3 Destruction of protoplanetary disks by photoeVapOration Sabine Richling.David Hollenbach and Harold W.Yorke 3.1 IntrOductiOn 3.2 PhotoevaD0ratiOn and other dispersal mechanisms 3.3 PhotoevaDoration by external radiation 3.4 PhotoevaDoratiOn by the central star 3.5 PhOtoevaDOratiOn and dust evolution 3.6 Conclusions Acknowledgments 4 Turbulence in protoplanetary accretion disks：driving mechanisms and role in planet formation Hubert Klahr,,Michal R62yczka，Natalia Dziourkevitch，Richard Wiinsch，and Anders Johansen 4.1 IntroductiOn 4.1.1 Protostellar collapse and formation of disks 4.1.2 Observations of accretion in protoplanetary systems 4.1.3 Self-gravity and the early evolution of disks 4.1.4 Viscous evolution 4.2 Magnetohydrodynamic turbulence 4.2.1 Non-ideal magnetohydrodynamics 4.2.2 0hmic dissipation 4.2.3 Ambipolar diflusion 4.2.4 Hall term 4.3 Layered accretion 4.3.1 Ionization structure 4.3.2 Layered disk evolution 4.4 Alternative instabilities in the dead zone 4.5 Transport by turbulence 4.5.1 Dust dynamics 4.5.2 Dust—trapping mechanisms 4.5.3 Turbulent diflusion 4.6 Conclusions 5 The origin of solids in the early Solar System Mario Trielo∥and Herbert Palme 5.1 Introduction：geoscience meets astronomy 5.2 Meteorites：remnants of planetesimal formation 4.6 billion years ago in the asteroid belt 5.3 Calcium—aluminum—rich inclusions and chondrules：remnants from the earliest Solar System 5.4 Compositional variety of chondrites：planetesimal formation occurred at a variety of conditions in the protoplanetary disk 5.4.1 Metal abundance and oxidation state 5.4.2 Ratio of refractory to volatile elements 5.4.3 Major element ffactionations：Mg.Si.Fe 5.4.4 Oxygen isotopes …… 6 Experiments on planetesimal formation 7 Dust coagulation in protoplanetary 8 The accretion of giant planet cores 9 Planetary transits ： a first direct vision of extrasolar planets 10 The core accretion-gas capture model for gas-giant planet formation 11 Properties of exoplanets ： a Doppler study of 1330 stars 12 Giant-planet formation ： theories meet observations 13 From hot Jupiters to hot Neptunes and below 14 Disk-planet interaction and migration 15 The brown dwarf-planet relation 16 Exoplanet detection techniques - from astronomy to astrobiology 17 Overview and prospective in theory and observation of planet formation |
内容加载中，请稍后...
商品评论（0条）