The Origin and Evolution of the Solar System

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The Graduate Series in AstronomySeries Editors:M Elvis, Harvard–Smithsonian Center for AstrophysicsA Natta, Osservatorio di Arcetri, FlorenceThe Graduate Series in Astronomy includes books on all aspects of theoreticaland experimental astronomy and astrophysics. The books are written at a levelsuitable for senior undergraduate and graduate students, and will also be useful topractising astronomers who wish to refresh their knowledge of a particular fieldof research.Other books in the seriesDust in the Galactic EnvironmentD C B WhittetObservational AstrophysicsR E White (ed)Stellar AstrophysicsR J Tayler (ed)Dust and Chemistry in AstronomyT J Millar and D A Williams (ed)The Physics of the Interstellar MediumJ E Dyson and D A WilliamsForthcoming titlesThe Isotropic Universe, 2nd editionD RaineDust in the Galactic Environment, 2nd editionD C B Whittet
Page 1: The Origin and Evolution of the Sol
Page 6 and 7: viiiContents1.6.5 Isotopic anomalie
Page 8 and 9: xContentsPART 3Current theories 141
Page 10 and 11: xiiContents10 Smaller planets and i
Page 13 and 14: IntroductionSince the time of Newto
Page 15 and 16: Chapter 1The structure of the Solar
Page 17: Planetary orbits and solar spin 5Fi
Page 24 and 25: 12 The structure of the Solar Syste
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40 The structure of the Solar Syste
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Chapter 2Observations and theories
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48 Observations and theories of sta
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Chapter 3What should a theory expla
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102 What should a theory explain?th
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104 What should a theory explain?sh
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106 What should a theory explain?3.
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108 What should a theory explain?ve
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112 Theories up to 1960Figure 4.1.
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114 Theories up to 1960III, De Revo
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118 Theories up to 1960the Shoemake
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120 Theories up to 1960etary clumps
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124 Theories up to 1960in which È
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132 Theories up to 1960have similar
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138 Theories up to 1960unrealistic
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140 Theories up to 1960The formatio
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144 A brief survey of modern theori
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Chapter 6The Sun, planets and satel
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158 The Sun, planets and satellites
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210 Planetary orbits and angular mo
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238 A planetary collisionFigure 8.1
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242 A planetary collisionIf the mag
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244 A planetary collisionTable 8.2.
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246 A planetary collision(iii) kine
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250 A planetary collisionIt has pre
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252 The MoonTable 9.1. The ratios o
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254 The Moonon the theory. For exam
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256 The MoonWith the two bodies wou
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258 The MoonFigure 9.3. The equatio
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260 The Moon9.1.4.1 Problems with,
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262 The Moonthis account because, b
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264 The Moonquillityite, an Fe-Ti s
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266 The MoonFigure 9.7. Thermal pro
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268 The MoonFigure 9.8. A view of t
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270 The MoonFigure 9.10. The abrade
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272 The Moonthe number of large obj
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274 The MoonFigure 9.13. The ideal
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276 The MoonTable 9.2. Estimated ex
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278 The Moon9.3.6 Calculations of t
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280 The MoonFigure 9.16. Present su
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282 The MoonCurves for the rate of
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284 The Moonsurface field was great
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286 The MoonTable 9.3. The position
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288 The MoonFigure 9.21. An idealiz
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290 The MoonFigure 9.22. A cross-se
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292 The MoonTable 9.4. The effect o
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Chapter 10Smaller planets and irreg
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296 Smaller planets and irregular s
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Chapter 11Asteroids, meteorites and
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318 Asteroids, meteorites and comet
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Chapter 12Comparisons of the main t
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The Proto-planet Theory reviewed 37
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The Solar Nebula Theory reviewed 37
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The Capture Theory reviewed 379goin
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The Capture Theory reviewed 381they
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General conclusion 383from a variet
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General conclusion 385Å ¬ and a p
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The Chandrasekhar limit, neutron st
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The Chandrasekhar limit, neutron st
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Appendix IIThe Virial TheoremThe Vi
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Appendix IIISmoothed particle hydro
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Smoothed particle hydrodynamics 395
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Smoothed particle hydrodynamics 397
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The Bondi and Hoyle accretion mecha
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Appendix VThe Poynting-Robertson ef
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References 403Cameron A G W 1973 Ic
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References 405Jones J H 1984 Geochi
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References 407Stewart G R and Wethe
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Index 409Bailey M E, 356, 362Barrin
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Index 411sticky particles in, 187-1
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Index 413isostacy, 272-273, 295, 30
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Index 415isotopic anomalies, 39-40,
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Index 417Pollack J B, 12polymict, 3
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Index 419radiation, 59Stewart G R,
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The Origin and Evolution of the Solar System

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