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 x
... Objects , and Comets Appendix B : 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 ...
... Objects , and Comets Appendix B : 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 ...
الصفحة 2
... objects in the solar system can be traced to early Greece , although it may have had its roots in Babylonian astronomy . Anaximander of Miletus ( 611-547 B.C. ) claimed that the relative distances of the stars , Moon , and Sun from the ...
... objects in the solar system can be traced to early Greece , although it may have had its roots in Babylonian astronomy . Anaximander of Miletus ( 611-547 B.C. ) claimed that the relative distances of the stars , Moon , and Sun from the ...
الصفحة 12
... objects in their orbits by means of a 1 : 1 orbit - orbit resonance . The satellites Janus and Epimetheus move on horseshoe orbits and periodically change their radial positions ( either closer or further from Saturn ) owing to their 1 ...
... objects in their orbits by means of a 1 : 1 orbit - orbit resonance . The satellites Janus and Epimetheus move on horseshoe orbits and periodically change their radial positions ( either closer or further from Saturn ) owing to their 1 ...
الصفحة 14
... Objects in the Edgeworth - Kuiper belt were first detected in 1992 and more than sixty such objects are currently known to exist . Curiously enough , knowledge of their orbits suggests that almost a third of these could be involved in a ...
... Objects in the Edgeworth - Kuiper belt were first detected in 1992 and more than sixty such objects are currently known to exist . Curiously enough , knowledge of their orbits suggests that almost a third of these could be involved in a ...
الصفحة 15
... objects ? This particularly fruitful question was first examined by Roy and Ovenden ( 1954 ) and subsequently by Goldreich ( 1965 ) . These authors considered commensurabilities of the form ( 1.17 ) where n1 and n2 are the mean motions ...
... objects ? This particularly fruitful question was first examined by Roy and Ovenden ( 1954 ) and subsequently by Goldreich ( 1965 ) . These authors considered commensurabilities of the form ( 1.17 ) where n1 and n2 are the mean motions ...
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