Solar System DynamicsCambridge University Press, 13/02/2000 The Solar System is a complex and fascinating dynamical system. This is the first textbook to describe comprehensively the dynamical features of the Solar System and to provide students with all the mathematical tools and physical models they need to understand how it works. It is a benchmark publication in the field of planetary dynamics and destined to become a classic. Clearly written and well illustrated, Solar System Dynamics 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 are provided. Solar System Dynamics provides an authoritative textbook for 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 non-linear dynamics. |
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الصفحة viii
... Polynomials 71 74 77 83 95 97 102 107 110 115 121 128 130 130 131 136 140 149 153 155 158 160 166 174 175 178 183 186 189 189 189 194 200 210 215 217 222 225 225 226 228 6.4 Literal Expansion in Orbital Elements 6.5 Literal Expansion to.
... Polynomials 71 74 77 83 95 97 102 107 110 115 121 128 130 130 131 136 140 149 153 155 158 160 166 174 175 178 183 186 189 189 189 194 200 210 215 217 222 225 225 226 228 6.4 Literal Expansion in Orbital Elements 6.5 Literal Expansion to.
الصفحة ix
Carl D. Murray, Stanley F. Dermott. 6.4 Literal Expansion in Orbital Elements 6.5 Literal Expansion to Second Order 6.6 Terms Associated with a Specific Argument Use of the Disturbing Function 6.7 6.8 Lagrange's Planetary Equations 6.9 ...
Carl D. Murray, Stanley F. Dermott. 6.4 Literal Expansion in Orbital Elements 6.5 Literal Expansion to Second Order 6.6 Terms Associated with a Specific Argument Use of the Disturbing Function 6.7 6.8 Lagrange's Planetary Equations 6.9 ...
الصفحة x
... Expansion of the Disturbing Function References Index 399 402 405 406 409 409 410 413 421 428 448 452 456 466 469 471 474 474 475 481 492 495 512 515 518 520 522 524 526 526 526 527 529 530 535 539 557 577 Preface What is a Man , If his ...
... Expansion of the Disturbing Function References Index 399 402 405 406 409 409 410 413 421 428 448 452 456 466 469 471 474 474 475 481 492 495 512 515 518 520 522 524 526 526 526 527 529 530 535 539 557 577 Preface What is a Man , If his ...
الصفحة 18
... expansion to fourth order in the eccentricity and inclination of the standard perturbing potential experienced by one orbiting body due to another involves 79 separate cosine arguments and 144 terms ( see Appendix B ) . Consequently the ...
... expansion to fourth order in the eccentricity and inclination of the standard perturbing potential experienced by one orbiting body due to another involves 79 separate cosine arguments and 144 terms ( see Appendix B ) . Consequently the ...
الصفحة 35
... expansions for elliptical motion in more detail in Sect . 2.5 , where we derive expressions for the b , ( e ) terms ... expansion we can write 1 1 0 = ƒ ( E ; + € ) = ƒ ( E ; ) + « iƒ ' ( E ‚ ) + { e } ƒ " ( E ; ) + ' & ? ƒ " ( Ei ) + O ...
... expansions for elliptical motion in more detail in Sect . 2.5 , where we derive expressions for the b , ( e ) terms ... expansion we can write 1 1 0 = ƒ ( E ; + € ) = ƒ ( E ; ) + « iƒ ' ( E ‚ ) + { e } ƒ " ( E ; ) + ' & ? ƒ " ( Ei ) + O ...
المحتوى
LXVIII | 261 |
LXIX | 264 |
LXX | 270 |
LXXI | 274 |
LXXII | 279 |
LXXIII | 283 |
LXXIV | 289 |
LXXV | 293 |
19 | |
22 | |
23 | |
25 | |
32 | |
37 | |
42 | |
45 | |
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 |
CXVII | 475 |
CXVIII | 481 |
CXIX | 492 |
CXX | 495 |
CXXI | 512 |
CXXII | 515 |
CXXIII | 518 |
CXXIV | 520 |
CXXV | 522 |
CXXVI | 524 |
CXXVII | 526 |
CXXVIII | 527 |
CXXIX | 529 |
CXXX | 530 |
CXXXI | 535 |
CXXXII | 539 |
CXXXIII | 557 |
CXXXIV | 577 |
طبعات أخرى - عرض جميع المقتطفات
عبارات ومصطلحات مألوفة
amplitude angle angular approach approximate argument associated assume asteroid body calculate centre chaotic circle circular close consider constant corresponding curves defined denote derived determined direction distance disturbing function dynamics Earth eccentricity effect encounter energy equal equations equilibrium points evolution example expansion expression follows force frame function given gives gravitational Hamiltonian Hence inclination increase initial inner integration Jupiter libration longitude mass mean motion moving Note numerical objects observed obtain occur orbit origin outer particle path pericentre period perturbations planet planetary plot position possible potential problem quantities radial radius reference relation resonance respectively ring rotating satellite Saturn Sect secular semi-major axis shown in Fig solar system solution stable surface Table theory tidal tide trajectory values variation vector write