Planet Formation : Theory, Observations, and Experiments.

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When this book was published in 2006, it had been just over ten years since the first planet outside our solar system was detected. Since then, much work has focused on understanding how extrasolar planets may form, and discovering the frequency of potentially habitable Earth-like planets. This volu...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Brandner, Wolfgang
Otros Autores: Klahr, Hubert, Jakosky, Bruce
Formato: Electrónico eBook
Idioma:Inglés
Publicado: West Nyack : Cambridge University Press, 2006.
Colección:Cambridge astrobiology.
Temas:
Planets > Origin.
Space biology.
Planètes > Origines.
Biologie spatiale.
Planets > Origin
Space biology
Acceso en línea:Texto completo

MARC

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245 1 0 |a Planet Formation :  |b Theory, Observations, and Experiments. 
260 |a West Nyack :  |b Cambridge University Press,  |c 2006. 
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505 0 |a Cover; Half-title; Series-title; Title; Copyright; Dedication; Contents; Preface; Acknowledgments; 1 Historical notes on planet formation; 1.1 Introduction; 1.2 Descartes and von Weizsäcker: vortices; 1.3 Magnetic effects; 1.4 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; 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. 
505 8 |a 2.2 From protoplanetary to debris disks: processing and dispersion of the inner dust disk2.3 Debris disks: Asteroid or Kuiper Belt?; 3 Destruction of protoplanetary disks by photoevaporation; 3.1 Introduction; 3.2 Photoevaporation and other dispersal mechanisms; 3.3 Photoevaporation by external radiation; 3.4 Photoevaporation by the central star; 3.5 Photoevaporation and dust evolution; 3.6 Conclusions; Acknowledgments; 4 Turbulence in protoplanetary accretion disks: driving mechanisms and role in planet formation; 4.1 Introduction; 4.1.1 Protostellar collapse and formation of disks. 
505 8 |a 4.1.2 Observations of accretion in protoplanetary systems4.1.3 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 Ohmic dissipation; 4.2.3 Ambipolar diffusion; 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 diffusion; 4.6 Conclusions; 5 The origin of solids in the early Solar System. 
505 8 |a 5.1 Introduction: geoscience meets astronomy5.2 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 fractionations: Mg, Si, Fe; 5.4.4 Oxygen isotopes; 5.5 Isotopic homogeneity of Solar-System materials. 
505 8 |a 5.5.1 Heterogeneity inherited from the interstellar medium: restricted to rare individual grains5.5.2 Heterogeneous or homogeneous distribution of short-lived nuclides: mixed evidence; 5.6 Dating accretion, heating, and cooling of planetesimals; 5.7 A timescale of early Solar-System events; 5.8 Formation of terrestrial planets; 5.9 Disk dissipation, Jupiter formation and gas-solid fractionation; 5.10 Summary; Acknowledgments; 6 Experiments on planetesimal formation; 6.1 Introduction; 6.2 Two-body collisions and the growth of aggregates in dust clouds; 6.2.1 Hit-and-stick collisions. 
500 |a 6.2.1.1 Measurements of adhesion forces. 
520 |a When this book was published in 2006, it had been just over ten years since the first planet outside our solar system was detected. Since then, much work has focused on understanding how extrasolar planets may form, and discovering the frequency of potentially habitable Earth-like planets. This volume addresses fundamental questions concerning the formation of planetary systems in general, and of our solar system in particular. Drawing from advances in observational, experimental and theoretical research, it summarises our understanding of the planet formation processes, and addresses major op. 
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650 0 |a Planets  |x Origin. 
650 0 |a Space biology. 
650 6 |a Planètes  |x Origines. 
650 6 |a Biologie spatiale. 
650 7 |a Planets  |x Origin  |2 fast 
650 7 |a Space biology  |2 fast 
700 1 |a Klahr, Hubert. 
700 1 |a Jakosky, Bruce. 
776 0 8 |i Print version:  |a Brandner, Wolfgang.  |t Planet Formation : Theory, Observations, and Experiments.  |d West Nyack : Cambridge University Press, ©2006  |z 9780521860154 
830 0 |a Cambridge astrobiology. 
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