Astrophysics of planet formation:
"The study of planet formation has been revolutionized by recent observational breakthroughs, which have allowed the detection and characterization of extrasolar planets, the imaging of protoplanetary disks, and the discovery of the Solar System's Kuiper Belt. Written for beginning graduat...
Gespeichert in:
1. Verfasser: | |
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Format: | Buch |
Sprache: | English |
Veröffentlicht: |
Cambridge [u.a.]
Cambridge Univ. Press
2010
|
Ausgabe: | 1. publ. |
Schlagworte: | |
Online-Zugang: | Inhaltsverzeichnis |
Zusammenfassung: | "The study of planet formation has been revolutionized by recent observational breakthroughs, which have allowed the detection and characterization of extrasolar planets, the imaging of protoplanetary disks, and the discovery of the Solar System's Kuiper Belt. Written for beginning graduate students, this textbook provides a basic understanding of the astrophysical processes that shape the formation of planetary systems. It begins by describing the structure and evolution of protoplanetary disks, moves on to the formation of planetesimals, terrestrial and gas giant planets, and concludes by surveying new theoretical ideas for the early evolution of planetary systems. Covering all phases of planet formation - from protoplanetary disks to the dynamical evolution of planetary systems - this introduction can be understood by readers with backgrounds in planetary science, observational and theoretical astronomy. It highlights the physical principles underlying planet formation and the areas where more research and new observations are needed"--Provided by publisher "The study of planet formation has a long history. My goals in writing this text are to provide a concise introduction to the classical theory of planet formation and to more recent developments spurred by new observations"--Provided by publisher |
Beschreibung: | Hier auch später erschienene, unveränderte Nachdrucke |
Beschreibung: | X, 284 S. Ill., graph. Darst. |
ISBN: | 9780521887458 0521887453 |
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520 | 3 | |a "The study of planet formation has been revolutionized by recent observational breakthroughs, which have allowed the detection and characterization of extrasolar planets, the imaging of protoplanetary disks, and the discovery of the Solar System's Kuiper Belt. Written for beginning graduate students, this textbook provides a basic understanding of the astrophysical processes that shape the formation of planetary systems. It begins by describing the structure and evolution of protoplanetary disks, moves on to the formation of planetesimals, terrestrial and gas giant planets, and concludes by surveying new theoretical ideas for the early evolution of planetary systems. Covering all phases of planet formation - from protoplanetary disks to the dynamical evolution of planetary systems - this introduction can be understood by readers with backgrounds in planetary science, observational and theoretical astronomy. It highlights the physical principles underlying planet formation and the areas where more research and new observations are needed"--Provided by publisher | |
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Datensatz im Suchindex
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adam_text | Titel: Astrophysics of planet formation
Autor: Armitage, Philip J.
Jahr: 2010
Contents
Préface page ix
1 Observations of planetary Systems 1
1.1 Solar System planets 2
1.1.1 The minimum mass Solar Nebula 4
1.2 Minor bodies in the Solar System 6
1.3 Radioactive dating of the Solar System 8
1.4 The snowline in the Solar Nebula 12
1.5 Chondritic météorites 13
1.6 Extrasolar planetary Systems 14
1.6.1 Direct imaging 15
1.6.2 Radial velocity searches 17
1.6.3 Astrometry 23
1.6.4 Transits 24
1.6.5 Gravitational microlensing 27
1.7 Properties of extrasolar planets 29
1.8 Further reading 33
2 Protoplanetary disk structure 34
2.1 Disks in the context of star formation 34
2.1.1 Classification of Young Stellar Objects 36
2.2 Vertical structure 38
2.3 Radial force balance 41
2.4 Radial température profile of passive disks 42
2.4.1 Razor-thin disks 43
2.4.2 Flared disks 45
2.4.3 Radiative equilibrium disks 47
2.4.4 The Chiang-Goldreich model 50
2.4.5 Spectral energy distributions 50
vi Contents
2.5 Opacity 52
2.5.1 Opacity in the optically thin outer disk 54
2.5.2 Analytic opacities 55
2.6 The condensation séquence 56
2.7 Ionization state of protoplanetary disks 58
2.7.1 Thermal ionization 59
2.7.2 Nonthermal ionization 60
2.8 Further reading 64
3 Protoplanetary disk évolution 65
3.1 Observations of disk évolution 65
3.2 Surface density évolution of a thin disk 68
3.2.1 The viscous time scale 69
3.2.2 Solutions to the disk évolution équation 70
3.2.3 Température profile of accreting disks 74
3.3 Vertical structure of protoplanetary disks 76
3.3.1 The central température of accreting disks 77
3.3.2 Shakura-Sunyaev a prescription 78
3.3.3 Vertically averaged solutions 80
3.4 Angular momentum transport mechanisms 82
3.4.1 The Rayleigh criterion 82
3.4.2 The magnetorotational instability 82
3.4.3 Disk winds and magnetic braking 87
3.4.4 Hydrodynamic turbulence 90
3.5 Effects of partial ionization on disk évolution 95
3.5.1 Layered disks 97
3.6 Disk dispersai 101
3.6.1 Photoevaporation 101
3.6.2 Viscous évolution with photoevaporation 103
3.7 Magnetospheric accretion 105
3.8 Further reading 108
4 Planetesimal formation 109
4.1 Aerodynamic drag on solid particles 1 10
4.1.1 Epstein drag 110
4.1.2 Stokes drag 111
4.2 Dustsettling 112
4.2.1 Single particle settling with coagulation 113
4.2.2 Settling in the présence of turbulence 116
4.3 Radial drift of solid particles 118
4.3.1 Radial drift with coagulation 121
4.3.2 Particle concentration at pressure maxima 122
Contents vii
4.3.3 Turbulent radial diffusion 123
4.4 Diffusion of large particles 125
4.5 Planetesimal formation via coagulation 128
4.5.1 Coagulation équation 131
4.5.2 Sticking efficiencies 132
4.6 Goldreich-Ward mechanism 134
4.6.1 Gravitational stability of a particle layer 134
4.6.2 Application to planetesimal formation 140
4.6.3 Self-excited turbulence 142
4.7 Routes to planetesimal formation 144
4.8 Further reading 145
Terrestrial planet formation 146
5.1 Physics of collisions 147
5.1.1 Gravitational focusing 147
5.1.2 Shear versus dispersion dominated encounters 148
5.1.3 Accretion versus disruption 152
5.2 Statistical models of planetary growth 156
5.2.1 Approximate treatment 157
5.2.2 Shear and dispersion dominated limits 159
5.2.3 Isolation mass 164
5.3 Velocity dispersion 165
5.3.1 Viscous stirring 166
5.3.2 Dynamical friction 169
5.3.3 Gas drag 169
5.4 Analytic formulae for planetary growth 171
5.5 Collisional damping and turbulent excitation 176
5.6 Coagulation équation 178
5.7 Final assembly 182
5.8 Further reading 184
Giant planet formation 185
6.1 Core accretion 186
6.1.1 Core/envelope structure 191
6.1.2 Critical core mass 195
6.1.3 Growth of giant planets 198
6.2 Disk instability 203
6.2.1 Fragmentation conditions 204
6.2.2 Disk cooling time scale 206
6.3 Comparison with observations 210
6.4 Further reading 217
viii Contents
7 Early évolution of planetary Systems 218
7.1 Migration in gaseous disks 219
7.1.1 Résonant torques 222
7.1.2 Type 1 migration 226
7.1.3 Type 2 migration 229
7.1.4 Applications 234
7.2 Résonant évolution 238
7.2.1 Résonant capture 241
7.2.2 Kozai résonance 244
7.3 Migration in planetesimal disks 247
7.3.1 Application to the outer Solar System 25 1
7.3.2 The Nice Model 252
7.3.3 Application to extrasolar planetary Systems 253
7.4 Planetary System stability 253
7.4.1 Hill stability 255
7.4.2 Planet-planet scattering 259
7.5 Further reading 262
Appendix 1 Physical and astronomical constants 263
Appendix 2 N-body methods 264
Références 273
Index 281
|
any_adam_object | 1 |
author | Armitage, Philip J. 1971- |
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dewey-full | 523.4 |
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dewey-ones | 523 - Specific celestial bodies and phenomena |
dewey-raw | 523.4 |
dewey-search | 523.4 |
dewey-sort | 3523.4 |
dewey-tens | 520 - Astronomy and allied sciences |
discipline | Physik |
edition | 1. publ. |
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publisher | Cambridge Univ. Press |
record_format | marc |
spelling | Armitage, Philip J. 1971- Verfasser (DE-588)140139613 aut Astrophysics of planet formation Philip J. Armitage 1. publ. Cambridge [u.a.] Cambridge Univ. Press 2010 X, 284 S. Ill., graph. Darst. txt rdacontent n rdamedia nc rdacarrier Hier auch später erschienene, unveränderte Nachdrucke "The study of planet formation has been revolutionized by recent observational breakthroughs, which have allowed the detection and characterization of extrasolar planets, the imaging of protoplanetary disks, and the discovery of the Solar System's Kuiper Belt. Written for beginning graduate students, this textbook provides a basic understanding of the astrophysical processes that shape the formation of planetary systems. It begins by describing the structure and evolution of protoplanetary disks, moves on to the formation of planetesimals, terrestrial and gas giant planets, and concludes by surveying new theoretical ideas for the early evolution of planetary systems. Covering all phases of planet formation - from protoplanetary disks to the dynamical evolution of planetary systems - this introduction can be understood by readers with backgrounds in planetary science, observational and theoretical astronomy. It highlights the physical principles underlying planet formation and the areas where more research and new observations are needed"--Provided by publisher "The study of planet formation has a long history. My goals in writing this text are to provide a concise introduction to the classical theory of planet formation and to more recent developments spurred by new observations"--Provided by publisher Planets Origin Astrophysics Planetenentstehung (DE-588)4174796-3 gnd rswk-swf Extrasolarer Planet (DE-588)4456110-6 gnd rswk-swf Entstehung (DE-588)4156614-2 gnd rswk-swf Staub (DE-588)4057011-3 gnd rswk-swf Planetologie (DE-588)4233970-4 gnd rswk-swf Planetensystem (DE-588)4126386-8 gnd rswk-swf Aggregation (DE-588)4000728-5 gnd rswk-swf Akkretionsscheibe (DE-588)4312917-1 gnd rswk-swf Planetenentstehung (DE-588)4174796-3 s Akkretionsscheibe (DE-588)4312917-1 s Staub (DE-588)4057011-3 s Aggregation (DE-588)4000728-5 s 1\p DE-604 Extrasolarer Planet (DE-588)4456110-6 s 2\p DE-604 Planetensystem (DE-588)4126386-8 s Entstehung (DE-588)4156614-2 s 3\p DE-604 Planetologie (DE-588)4233970-4 s 4\p DE-604 HBZ Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=019003117&sequence=000004&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 3\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 4\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
spellingShingle | Armitage, Philip J. 1971- Astrophysics of planet formation Planets Origin Astrophysics Planetenentstehung (DE-588)4174796-3 gnd Extrasolarer Planet (DE-588)4456110-6 gnd Entstehung (DE-588)4156614-2 gnd Staub (DE-588)4057011-3 gnd Planetologie (DE-588)4233970-4 gnd Planetensystem (DE-588)4126386-8 gnd Aggregation (DE-588)4000728-5 gnd Akkretionsscheibe (DE-588)4312917-1 gnd |
subject_GND | (DE-588)4174796-3 (DE-588)4456110-6 (DE-588)4156614-2 (DE-588)4057011-3 (DE-588)4233970-4 (DE-588)4126386-8 (DE-588)4000728-5 (DE-588)4312917-1 |
title | Astrophysics of planet formation |
title_auth | Astrophysics of planet formation |
title_exact_search | Astrophysics of planet formation |
title_full | Astrophysics of planet formation Philip J. Armitage |
title_fullStr | Astrophysics of planet formation Philip J. Armitage |
title_full_unstemmed | Astrophysics of planet formation Philip J. Armitage |
title_short | Astrophysics of planet formation |
title_sort | astrophysics of planet formation |
topic | Planets Origin Astrophysics Planetenentstehung (DE-588)4174796-3 gnd Extrasolarer Planet (DE-588)4456110-6 gnd Entstehung (DE-588)4156614-2 gnd Staub (DE-588)4057011-3 gnd Planetologie (DE-588)4233970-4 gnd Planetensystem (DE-588)4126386-8 gnd Aggregation (DE-588)4000728-5 gnd Akkretionsscheibe (DE-588)4312917-1 gnd |
topic_facet | Planets Origin Astrophysics Planetenentstehung Extrasolarer Planet Entstehung Staub Planetologie Planetensystem Aggregation Akkretionsscheibe |
url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=019003117&sequence=000004&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
work_keys_str_mv | AT armitagephilipj astrophysicsofplanetformation |