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
... Earth's Dust Ring Exercise Questions Appendix A : Solar System Data Introduction Astronomical Constants Julian Date A.4 Orbital Elements of the Planets and Their Variation A.5 Planets , Satellites , and Rings A.6 Asteroids , Centaurs ...
... Earth's Dust Ring Exercise Questions Appendix A : Solar System Data Introduction Astronomical Constants Julian Date A.4 Orbital Elements of the Planets and Their Variation A.5 Planets , Satellites , and Rings A.6 Asteroids , Centaurs ...
الصفحة 2
... Earth were in the ratio 1 : 2 : 3 ( Bernal 1969 ) . The importance of whole numbers to members of the Pythagorean school led them to believe that the distances of the heavenly bodies from the Earth corresponded to a sequence of musical ...
... Earth were in the ratio 1 : 2 : 3 ( Bernal 1969 ) . The importance of whole numbers to members of the Pythagorean school led them to believe that the distances of the heavenly bodies from the Earth corresponded to a sequence of musical ...
الصفحة 6
... Earth 1 Mars 2 Ceres 3 Jupiter 4 Saturn 5 0.39 0.72 1.00 1.52 2.77 5.20 9.54 Uranus 6 19.18 Neptune 7 30.06 Pluto 39.44 8 Semi - major Titius - Bode Axis ( AU ) Law ( AU ) calculation . However , if every value of i is filled we should ...
... Earth 1 Mars 2 Ceres 3 Jupiter 4 Saturn 5 0.39 0.72 1.00 1.52 2.77 5.20 9.54 Uranus 6 19.18 Neptune 7 30.06 Pluto 39.44 8 Semi - major Titius - Bode Axis ( AU ) Law ( AU ) calculation . However , if every value of i is filled we should ...
الصفحة 9
... Earth . Most of the major , natural satellites in the solar system are in a 1 : 1 or synchronous spin - orbit resonance . However , other spin - orbit states are also possible and radar observations of Mercury by Pettengill & Dyce ...
... Earth . Most of the major , natural satellites in the solar system are in a 1 : 1 or synchronous spin - orbit resonance . However , other spin - orbit states are also possible and radar observations of Mercury by Pettengill & Dyce ...
الصفحة 14
... interplanetary dust particles in the solar system . It has now been shown that the Earth is embedded in a dust ring composed of asteroidal particles temporarily trapped in a series of strong orbit - orbit. 14 1 Structure of the Solar ...
... interplanetary dust particles in the solar system . It has now been shown that the Earth is embedded in a dust ring composed of asteroidal particles temporarily trapped in a series of strong orbit - orbit. 14 1 Structure of the Solar ...
المحتوى
LXVIII | 261 |
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LXXI | 274 |
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LXXIV | 289 |
LXXV | 293 |
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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