Solar System DynamicsCambridge University Press, 1999 - 592 頁 The force of gravity acting over eons has provided the solar system with an intricate dynamical structure, much of it revealed by recent space missions. This comprehensive introduction to the dynamical features of the solar system also provides all the mathematical tools and physical models needed for a complete understanding of the subject. Clearly written and well illustrated coverage shows how a basic knowledge of the two- and three-body problems and perturbation theory can be combined to understand features as diverse as the tidal heating of Jupiter's moon Io, the origin of the Kirkwood gaps in the asteroid belt, and the radial structure of Saturn's rings. Problems at the end of each chapter and a free Internet Mathematica® software package help students to fully develop their understanding of the subject. This volume provides an authoritative textbook for advanced undergraduate and graduate courses on planetary dynamics and celestial mechanics. It also equips students with the mathematical tools to tackle broader courses on dynamics, dynamical systems, applications of chaos theory and nonlinear dynamics. Written by two leading figures in planetary dynamics, it is a benchmark publication in the field and destined to become a classic. |
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... , Satellites , and Rings 529 530 A.6 Asteroids , Centaurs , Trans - Neptunian Objects , and Comets 535 Appendix B : Expansion of the Disturbing Function 539 References 557 Index 577 Preface What is a Man , If his chief good.
... , Satellites , and Rings 529 530 A.6 Asteroids , Centaurs , Trans - Neptunian Objects , and Comets 535 Appendix B : Expansion of the Disturbing Function 539 References 557 Index 577 Preface What is a Man , If his chief good.
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內容
II | 1 |
III | 2 |
IV | 3 |
V | 4 |
VI | 5 |
VII | 9 |
VIII | 15 |
IX | 17 |
LXVIII | 261 |
LXIX | 264 |
LXX | 270 |
LXXI | 274 |
LXXII | 279 |
LXXIII | 283 |
LXXIV | 289 |
LXXV | 293 |
X | 19 |
XI | 22 |
XII | 23 |
XIII | 25 |
XIV | 32 |
XV | 37 |
XVI | 42 |
XVII | 45 |
XVIII | 48 |
XIX | 54 |
XX | 57 |
XXI | 60 |
XXII | 63 |
XXIII | 64 |
XXIV | 68 |
XXV | 71 |
XXVI | 74 |
XXVII | 77 |
XXVIII | 83 |
XXIX | 95 |
XXX | 97 |
XXXI | 102 |
XXXII | 107 |
XXXIII | 110 |
XXXIV | 115 |
XXXV | 121 |
XXXVI | 128 |
XXXVII | 130 |
XXXVIII | 131 |
XXXIX | 136 |
XL | 140 |
XLI | 149 |
XLII | 153 |
XLIII | 155 |
XLIV | 158 |
XLV | 160 |
XLVI | 166 |
XLVII | 174 |
XLVIII | 175 |
XLIX | 178 |
L | 183 |
LI | 186 |
LII | 189 |
LIII | 194 |
LIV | 200 |
LV | 210 |
LVI | 215 |
LVII | 217 |
LVIII | 222 |
LIX | 225 |
LX | 226 |
LXI | 228 |
LXII | 233 |
LXIII | 238 |
LXIV | 246 |
LXV | 248 |
LXVI | 251 |
LXVII | 253 |
LXXVI | 299 |
LXXVII | 302 |
LXXVIII | 307 |
LXXIX | 309 |
LXXX | 314 |
LXXXI | 317 |
LXXXII | 318 |
LXXXIII | 321 |
LXXXIV | 326 |
LXXXV | 328 |
LXXXVI | 332 |
LXXXVII | 334 |
LXXXVIII | 337 |
LXXXIX | 341 |
XC | 364 |
XCI | 371 |
XCII | 373 |
XCIII | 375 |
XCIV | 385 |
XCV | 387 |
XCVI | 390 |
XCVII | 394 |
XCVIII | 396 |
XCIX | 399 |
C | 402 |
CI | 405 |
CII | 406 |
CIII | 409 |
CIV | 410 |
CV | 413 |
CVI | 421 |
CVII | 428 |
CVIII | 448 |
CIX | 452 |
CX | 456 |
CXI | 466 |
CXII | 469 |
CXIII | 471 |
CXIV | 474 |
CXV | 475 |
CXVI | 481 |
CXVII | 492 |
CXVIII | 495 |
CXIX | 512 |
CXX | 515 |
CXXI | 518 |
CXXII | 520 |
CXXIII | 522 |
CXXIV | 524 |
CXXV | 526 |
CXXVI | 527 |
CXXVII | 529 |
CXXVIII | 530 |
CXXIX | 535 |
CXXX | 539 |
CXXXI | 557 |
577 | |
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常見字詞
amplitude angle angular momentum approximate asteroid asteroid belt Astron body calculate centre of mass chaotic circular consider denote density derived Dermott disturbing function dynamics Earth eccentricity and inclination effect ellipse encounter equations of motion equilibrium points evolution exact resonance expansion expression force given in Eq Goldreich gravitational Hamiltonian Hence horseshoe orbits inner Jacobi constant Jupiter Kepler's libration longitude of pericentre m₁ mean motion Mimas Murray Note orbital elements orbital period outer pericentre planet planetary planetary rings plot potential precession quantities r₁ radial radius resonant argument restricted three-body problem rings of Uranus rotating satellite Saturn Sect secular perturbations semi-major axis separatrix shown in Fig solar system solution spin surface of section synchronous Table tadpole orbits test particle theory tide timescale torque trajectory uranian Uranus values variation velocity zero-velocity curves