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E-raamat: Formation and Evolution of Exoplanets [Wiley Online]

Edited by (University of Arizona, Tucson, USA)
  • Formaat: 320 pages
  • Ilmumisaeg: 17-Feb-2010
  • Kirjastus: Blackwell Verlag GmbH
  • ISBN-10: 3527629769
  • ISBN-13: 9783527629763
Teised raamatud teemal:
  • Wiley Online
  • Hind: 185,03 €*
  • * hind, mis tagab piiramatu üheaegsete kasutajate arvuga ligipääsu piiramatuks ajaks
Formation and Evolution of ExoplanetsSuurem pilt
  • Formaat: 320 pages
  • Ilmumisaeg: 17-Feb-2010
  • Kirjastus: Blackwell Verlag GmbH
  • ISBN-10: 3527629769
  • ISBN-13: 9783527629763
Teised raamatud teemal:
Wiley Online e-raamatudRohkem infot Wiley Online kohta
Raamatu kodulehekülg: https://onlinelibrary.wiley.com/doi/book/10.1002/9783527629763
This single, coherent review of the theory behind extrasolar planet formation and interaction systematically covers all aspects of the topic, including different formation processes, planet-planet scattering, giant planets and brown dwarfs. With a chapter on observation, careful referencing and an elaborate bibliography at the end of each chapter, this is indispensable reading for researchers, theorists and observers alike.
Preface xi
List of Contributors
xiii
Exoplanet Observations
1(26)
Jacob L. Bean
Introduction
1(1)
Orbital Properties
1(10)
Orbital Periods and Eccentricities
2(4)
Multiplanet Systems
6(2)
Planets in Multiple Star Systems
8(1)
Spin-Orbit Alignment
9(2)
Physical Properties
11(4)
Mass Distribution
11(2)
Masses and Radii of Transiting Planets
13(2)
Host Star Properties
15(6)
Planet-Stellar Composition Correlation
16(3)
Planet-Stellar Mass Correlation
19(2)
Conclusion
21(6)
References
21(4)
Further Reading
25(2)
Pinpointing Planets in Circumstellar Disks
27(22)
Alice C. Quillen
Introduction
27(1)
Signatures of Extrasolar Planets Imprinted on Dusty Disks
28(1)
Morphological Features of Circumstellar Disks
29(5)
Clearings
30(1)
Spiral Arms
31(1)
Clumps
31(1)
Important Timescales
32(2)
The Role of Mean Motion Resonances
34(4)
General Theory for First-Order Mean Motion Resonances
35(3)
When are Spiral Density Waves Important?
38(1)
The Chaotic Zone Boundary
38(1)
Minimum Gap Opening Planet Masses
39(1)
Fomalhaut
40(3)
Summary
43(1)
References
43(6)
Planet-Planet Interactions
49(22)
Rory Barnes
Introduction
49(1)
Review of Orbital Theory
49(8)
Analytic Methods
50(1)
Secular Theory
50(3)
Resonant Interactions
53(1)
N-Body Integrations
54(1)
Dynamical Stability and Chaos
55(2)
Distributions of Dynamical Properties
57(7)
Types of Interactions
58(1)
Frequency of Mean Motion Resonances
58(1)
Apsidal Motion
59(1)
Proximity to Dynamical Instability
60(4)
Conclusions
64(7)
References
64(6)
Further Reading
70(1)
Formation via Disk Instability
71(30)
Lucio Mayer
Introduction-Basic Notions of Disk Instability
71(3)
Simulations of Disk Instability
74(3)
Disk Thermodynamics and Fragmentation
77(3)
Beyond the Fragmentation Stage
80(6)
Masses, Numbers, and Evolution of Clumps Produced by Fragmentation
80(5)
Orbits and Orbital Evolution
85(1)
Comparison with Solar and Extrasolar Giant Planets
86(3)
From Gas Giants to Ice Giants and Super-Earths
86(1)
Fragmentation around Different Stellar Types
87(1)
The Correlation between Metallicity of Host Star and Planet Frequency
87(2)
The Solid Content of Planets Formed by Disk Instability
89(2)
Disk Formation and Disk Masses-a Key Issue
91(2)
The Role of Stellar Companions and Interactions
93(1)
Looking into the Future
94(7)
References
95(3)
Further Reading
98(3)
Core-accretion Model
101(22)
Olenka Hubickyj
Introduction
101(1)
Historical Background of the Development of the Core Accretion Model
101(2)
Observational Constraints
103(1)
General Description of the Core-accretion Model
104(1)
The Model and the Computer Code
105(5)
The Code Components
106(2)
The Code Boundary Conditions
108(1)
The Code Assumptions
109(1)
Results
110(5)
Opacity
112(1)
Core Mass
113(2)
MMSN or not MMSN
115(1)
Discussion
115(8)
Migration
116(1)
Metallicity
117(1)
Observational Predictions for New Planets
118(1)
References
118(4)
Further Reading
122(1)
Formation of Terrestrial Planets
123(22)
Sean N. Raymond
Introduction
123(1)
Setting the Stage: Protoplanetary Disks
124(1)
Stages of Terrestrial Planet Growth
125(9)
From Dust to Planetesimals
126(1)
From Planetesimals to Planetary Embryos
127(5)
From Planetary Embryos to Terrestrial Planets
132(2)
Planetary Compositions and Habitability
134(3)
Compositions of Terrestrial Planets
134(1)
Prospects for Terrestrial and Habitable Planets in Exoplanet Systems
135(2)
Conclusions
137(8)
Acknowledgments
138(1)
References
139(4)
Further Reading
143(2)
Brown Dwarfs
145(12)
Kevin L. Luhman
Introduction
145(1)
Defining Brown Dwarfs and Giant Planets
145(1)
Distinguishing between Brown Dwarfs and Giant Planets
146(1)
Protoplanetary Disks around Brown Dwarfs
147(10)
The Least Massive Objects with Disks
147(1)
Disk Fractions and Lifetimes
148(2)
Disk Compositions
150(1)
Transitional Disks
151(1)
Disk Radii and Masses
152(1)
Implications of Disk Properties for Planet Formation
153(1)
Searches for Planets around Brown Dwarfs
153(1)
References
154(3)
Exoplanet Chemistry
157(30)
Katharina Lodders
Introduction
157(1)
A Goodly Gallery of Planets
157(3)
Elemental Ingredients of Planets
160(2)
Diagnostics from Elemental Abundance Fractionations
161(1)
Planetary Building Blocks
162(7)
Similarities between Gas-Giant Planets and Brown Dwarfs
169(14)
Chemistry in Gas-Giant Planets
173(3)
Condensate Clouds
176(5)
The Effects of Varying the C/O Ratio on Gas-Giant Planet Chemistry
181(1)
Gas Chemistry Variations through Changes in C/O Ratio
181(1)
Possible Scenarios to Alter C/O Ratios during Planetary Formation
182(1)
Outlook
183(4)
Acknowledgments
184(1)
References
184(2)
Further Reading
186(1)
Migration and Multiplicity Effects During Giant Planet Formation
187(16)
Edward W. Thommes
Introduction
187(1)
Type I Migration
188(3)
Type II Migration
191(1)
``Exotic'' Migration Scenarios
192(1)
Planet-Planet Interactions During Migration
193(1)
From Disk to Planets: Putting the Pieces Together
194(5)
Summary and Discussion
199(4)
References
200(3)
Planets in Mean-Motion Resonance
203(20)
Wilhelm Kley
Introduction
203(1)
Extrasolar Systems in Mean-Motion Resonance
203(4)
Planetary Migration
207(2)
Planet-Disk Interaction
207(2)
Resonant Capture through Convergent Migration
209(4)
Hydrodynamical Studies
209(3)
Forced Migration
212(1)
Matching Observed Systems
213(1)
GJ 876: A Case of Adiabatic Migration
213(1)
Formation of Systems HD 128311 and HD 73526 through Mixed Scenarios
214(2)
Capture in 3:2 Resonance
216(1)
Destruction of Resonances
217(1)
Summary
217(6)
Acknowledgments
218(1)
References
218(4)
Further Reading
222(1)
Planet-Planet Gravitational Scattering
223(20)
F. Marzari
Introduction
223(1)
Onset of Instability in Multiplanet Systems: the Gas-Free Scenario
224(8)
The Stability Limit
224(3)
Planet-Planet Scattering Dynamics
227(4)
Tidal Interaction with the Star and Formation of ``Hot'' Jupiters
231(1)
Kozai Oscillations
231(1)
Planet-Planet Scattering in Presence of the Gas Disk
232(5)
Planet-Planet Scattering in Binary Stars
237(2)
Summary
239(4)
References
240(1)
Further Reading
241(2)
Tides and Exoplanets
243(24)
Brian Jackson
Rory Barnes
Richard Greenberg
Introduction
243(1)
Tidal Physics
244(5)
Tidal Effects on Gaseous Exoplanets
249(4)
Orbital Evolution
249(3)
Tidal Heating
252(1)
Tidal Effects on Rocky Exoplanets
253(7)
Orbital Evolution and Habitability
254(1)
Effects of Tidal Heating
255(4)
Rotation and Habitability
259(1)
Conclusions
260(7)
References
260(5)
Further Reading
265(2)
Index 267
Dr. Rory Barnes is a researcher in the Astronomy Department and Astrobiology Program at the University of Washington in Seattle. He is an active participant in the theoretical side of one of the hottest topics in astrophysics - the science of exoplanets. He has published numerous papers that consider exoplanets from astrophysical, planetary science, and astrobiological points of view. For this book, he has brought together an august group of authors to detail current perspectives of the origins and properties of these fascinating worlds.
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