Planet Formation行星的形成
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作者： Wolfgang Brandner著
出 版 社：
出版时间： 2006-6-1字数：版次： 1页数： 302印刷时间： 2006/06/01开本： 16开印次： 1纸张： 胶版纸I S B N ： 9780521860154包装： 精装内容简介
“This carefully organized text，represents a snapshot of the state of the art of the modern quest for the origins of worlds，a sense of excitement and scientific novelty persists in the many detailed passages，a definitive text for the shelves of researchers, students，and interested bystanders that should prove to be of considerable longevity。”Science
目录
Preface
A cknowledgments
1Historical notes on planet formation
Peter Bodenheimer
1.1 IntrOductiOn
1.2Descartes and von Weizsficker：vortices
1.3 Magnetic effects
l.4 Gravitational instability
1.5 Core accretion：gas capture
1.6 Planet searches
2The 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？
3Destruction 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
