Planetary Systems | p. 1 |
Introduction | p. 1 |
The Plurality of Worlds: A Question as Old as the Hills | p. 1 |
From Antiquity to the Copernican Revolution | p. 1 |
The First Theories on the Formation of the World | p. 3 |
First Searches for Other Worlds | p. 5 |
The First Astrometric Searches | p. 6 |
The Velocimetry Method | p. 6 |
The First Results and the Problems Raised | p. 9 |
Planets Around Pulsars | p. 10 |
The Search for Protoplanetary Disks | p. 12 |
The Solar System: A Typical Planetary System? | p. 13 |
The Sun as an Average Star | p. 14 |
Brown Dwarfs: Between Stars and Planets | p. 15 |
A Specific Planetary System: The Solar System | p. 15 |
The Formation of the Planets by Nucleation | p. 15 |
Terrestrial and Giant Planets | p. 18 |
Bibliography | p. 20 |
Detection Methods | p. 21 |
The Extent of the Problem | p. 21 |
Contrast Between Star and Planet | p. 21 |
Angular Separation Between the Objects | p. 22 |
Environment of the Earth and Exoplanets | p. 23 |
The Indirect Detection of Exoplanets | p. 24 |
The Effect of a Planet on the Motion of Its Star | p. 24 |
The Effect a Planet has on Photometry of Its Star | p. 36 |
Comparison of the Different Indirect Methods | p. 46 |
Direct Detection of Exoplanets | p. 46 |
Choice of Spectral Region | p. 47 |
Coronagraphic Methods and Adaptive Optics | p. 48 |
Interferometry | p. 55 |
Interferometry and Imagery: Hypertelescopes | p. 62 |
Detection by Radio | p. 65 |
Bibliography | p. 67 |
Extrasolar Planets, 12 Years After the First Discovery | p. 69 |
Exoplanets and Exoplanetary Systems | p. 70 |
The Mass-Distribution of Exoplanets | p. 70 |
The Distance-Distribution of Exoplanets | p. 74 |
The Relationship Between the Mass of Exoplanets and Their Distance from Their Star | p. 76 |
Orbital Eccentricity Among Exoplanets | p. 78 |
Exoplanets and Their Parent Stars | p. 80 |
Mass/Diameter Ratio | p. 82 |
Characteristics of Extrasolar Planetary Atmospheres | p. 83 |
Bibliography | p. 84 |
What we Learn from the Solar System | p. 85 |
Observational Methods | p. 85 |
The Observational Data | p. 87 |
Orbits that are Essentially Co-Planar and Concentric | p. 87 |
Terrestrial Planets and Giant Planets | p. 88 |
The Small Bodies | p. 89 |
Dating the Solar System Through Radioactive Decay | p. 91 |
The Emergence of a 'Standard Model' | p. 91 |
The Nebular Theory | p. 91 |
The Standard Model: The Chronology of Events | p. 92 |
The Physical and Chemical Properties of Solar-System Objects | p. 100 |
The Electromagnetic Spectrum of the Objects in the Solar System | p. 100 |
Planetary Atmospheres | p. 101 |
The Terrestrial Planets | p. 106 |
The Giant Planets | p. 110 |
Rings and Satellites in the Outer Solar System | p. 120 |
Small Bodies in the Solar System | p. 125 |
Conclusions: The Solar System Compared with Other Planetary Systems | p. 130 |
The Scenario for the Formation of the Solar System | p. 130 |
Objects in the Planetary Systems Observable from Earth | p. 131 |
Bibliography | p. 132 |
Stellar Formation and Protoplanetary Disks | p. 135 |
The First Stages in Stellar Formation | p. 135 |
Properties of the Interstellar Medium | p. 135 |
The Formation of Molecular Clouds | p. 137 |
Collapse of a Molecular Cloud | p. 138 |
Observation of Young Stars | p. 138 |
Structure and Evolution of Protoplanetary Disks | p. 141 |
Observation of Protoplanetary Disks | p. 141 |
Stellar Accretion Flux | p. 144 |
The Rotation of T-Tauri Stars | p. 145 |
The Formation of Binary Systems | p. 146 |
The Principal Stages of Stellar Formation | p. 147 |
Later Stages of Stellar Evolution: Evolution Towards the Main Sequence | p. 151 |
The Structure of Protoplanetary Disks | p. 153 |
Composition of the Gas and Dust | p. 157 |
Planetary Disks and Debris Disks | p. 158 |
Observation of the Disk of HR 4796A | p. 159 |
Observation of the Disk of ß Pic | p. 160 |
The Formation of Planetesimals and Planetary Embryos | p. 163 |
From Microscopic Particles to Centimetre-Sized Grains | p. 163 |
From Centimetre-Sized Grains to Kilometre-Sized Bodies | p. 164 |
From Protoplanets to Planets | p. 165 |
Bibliography | p. 167 |
The Dynamics of Planetary Systems | p. 171 |
Characteristics of the Orbits | p. 171 |
Calculation of Radial Velocities | p. 171 |
Orbital Characteristics from Radial-Velocity Curves | p. 172 |
Multiple Systems Case | p. 174 |
Exoplanets and Known Multiple Systems | p. 175 |
Rotation of the Planets | p. 178 |
Migration | p. 179 |
Migration in the Solar System | p. 179 |
Migration in Exosystems | p. 181 |
The Different Migration Mechanisms | p. 182 |
Observational Indications | p. 184 |
The End of the Migration and Tidal Effects | p. 186 |
Stability of Planetary Systems | p. 187 |
Dynamical Categories | p. 187 |
The GJ 876 System | p. 189 |
The HD 82943 System | p. 190 |
The v Andromedae System | p. 190 |
The HD 202206 System: A Circumbinary Planet? | p. 191 |
The HD 69830 System: Three Neptunes and a Ring of Dust | p. 193 |
Planetary Systems Around Pulsars | p. 193 |
The Dynamics of Debris Disks | p. 195 |
Bibliography | p. 198 |
Structure and Evolution of an Exoplanet | p. 199 |
The Internal Structure of Giant Exoplanets | p. 200 |
The Observable Features | p. 200 |
The Equations of Internal Structure | p. 201 |
Rotation Effects | p. 203 |
Equations of State | p. 203 |
Construction of Models of Internal Structure | p. 205 |
Evolutionary Models | p. 208 |
The Internal Structure of Terrestrial-Type Exoplanets and Ocean Planets | p. 210 |
Terrestrial-Type Exoplanets | p. 211 |
Ocean Planets | p. 213 |
The Atmospheres of Exoplanets: Their Structure, Evolution and Spectral Characteristics | p. 216 |
Giant Exoplanets | p. 216 |
Terrestrial Planets and Habitable Planets | p. 227 |
Hot Neptunes, Super-Earths, and Ocean Planets | p. 241 |
Bibliography | p. 244 |
Present and Future Instrumental Projects | p. 247 |
Indirect Methods of Detection | p. 248 |
Velocimetry | p. 248 |
Astrometry | p. 252 |
The Study of Planetary Transits | p. 257 |
Searching for Microlensing Events | p. 268 |
Direct Methods of Detection | p. 272 |
Imaging | p. 272 |
Interferometry | p. 281 |
Direct Detection of Radio Waves | p. 291 |
Bibliography | p. 293 |
The Search for Life in Planetary Systems | p. 295 |
What is Life? | p. 295 |
How Should Life be Defined? | p. 295 |
The Role of Carbon and of Liquid Water | p. 296 |
The Building-Block of Life: Macromolecules | p. 298 |
Nucleic Acids | p. 300 |
The Role of the Cell | p. 300 |
Prebiotic Material in the Universe | p. 301 |
Organic Material in the Universe | p. 301 |
The Synthesis of Organic Molecules: Miller and Urey's Experiment | p. 302 |
Transport of Complex Organic Molecules to the Primordial Earth | p. 305 |
Stages on the Road to Complexity | p. 308 |
Polymers and Macromolecules | p. 308 |
The Formation of Membranes | p. 309 |
RNA and DNA | p. 311 |
The Appearance of Life on the Primitive Earth | p. 311 |
Favourable Conditions | p. 311 |
The Environment of the Primitive Earth: The Hydrosphere and Atmosphere | p. 312 |
The Search for Habitable Locations in the Solar System | p. 314 |
The Planet Mars | p. 314 |
The Satellites of the Outer Planets | p. 318 |
The Search for Life on Exoplanets | p. 322 |
Exoplanets' Habitable Zones | p. 322 |
How May Life on an Exoplanet be Detected? | p. 324 |
The Search for Extraterrestrial Civilisations | p. 327 |
The Drake and Sagan Equation | p. 327 |
Communication by Radio Waves | p. 327 |
The State of SETI and CETI Searches | p. 327 |
Bibliography | p. 329 |
p. 331 | |
Star or Planet? | p. 331 |
Gravitation and Kepler's Laws | p. 332 |
A.3 | p. 332 |
The Hertzsprung-Russell Diagram and the Spectral Classification of Stars | p. 334 |
Resonances | p. 336 |
Index | p. 339 |
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