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. |
من داخل الكتاب
النتائج 1-5 من 73
الصفحة ix
... Resonant Perturbations Introduction 8 8.1 8.2 8.3 8.4 Variation of Orbital Elements 8.5 Resonance in the Circular Restricted Three - Body Problem 8.6 The Pendulum Model 8.7 Libration Width 8.8 The Hamiltonian Approach 8.9 The 2 : 1 ...
... Resonant Perturbations Introduction 8 8.1 8.2 8.3 8.4 Variation of Orbital Elements 8.5 Resonance in the Circular Restricted Three - Body Problem 8.6 The Pendulum Model 8.7 Libration Width 8.8 The Hamiltonian Approach 8.9 The 2 : 1 ...
الصفحة 9
... resonance . In basic terms a resonance can arise when there is a simple numerical relationship between frequencies or periods . The periods involved could be the rotational and orbital periods of a single body , as in the case of spin ...
... resonance . In basic terms a resonance can arise when there is a simple numerical relationship between frequencies or periods . The periods involved could be the rotational and orbital periods of a single body , as in the case of spin ...
الصفحة 10
... resonance between their orbital periods , which French astronomers called la grande inégalité ( the great inequality ) . Although the two planets are not actually in a 5 : 2 resonance they are sufficiently close to it for significant ...
... resonance between their orbital periods , which French astronomers called la grande inégalité ( the great inequality ) . Although the two planets are not actually in a 5 : 2 resonance they are sufficiently close to it for significant ...
الصفحة 11
... resonance ensures that when a conjunction takes place between any pair of satellites , the third satellite is always at least 60 ° away . The 2 : 1 Io - Europa resonance is directly responsible for the active vulcanism on Io that was ...
... resonance ensures that when a conjunction takes place between any pair of satellites , the third satellite is always at least 60 ° away . The 2 : 1 Io - Europa resonance is directly responsible for the active vulcanism on Io that was ...
الصفحة 13
... resonance ( Murray & Thompson 1990 ) and Cordelia and Ophelia bound the narrow e ring by means of a 24:25 and a 14:13 resonance with its inner and outer edges ( Porco & Goldreich 1987 ) . Cordelia is also involved in resonances with ...
... resonance ( Murray & Thompson 1990 ) and Cordelia and Ophelia bound the narrow e ring by means of a 24:25 and a 14:13 resonance with its inner and outer edges ( Porco & Goldreich 1987 ) . Cordelia is also involved in resonances with ...
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