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 76
الصفحة
... . Heis anassociate editorof the journals Icarus and Celestial Mechanicsand Dynamical Astronomy aswellasbeing a member of the Imaging Team ofthe Cassinimission to Saturn. Asteroid 5598 was officially named Carlmurray in recognition of.
... . Heis anassociate editorof the journals Icarus and Celestial Mechanicsand Dynamical Astronomy aswellasbeing a member of the Imaging Team ofthe Cassinimission to Saturn. Asteroid 5598 was officially named Carlmurray in recognition of.
الصفحة i
... asteroid belt , the radial structure of Saturn's A ring , and the long - term stability of the solar system . Problems at the end of each chapter and a free Internet Mathematica® software package ( that includes animations and ...
... asteroid belt , the radial structure of Saturn's A ring , and the long - term stability of the solar system . Problems at the end of each chapter and a free Internet Mathematica® software package ( that includes animations and ...
الصفحة 5
... asteroid ( 1 ) Ceres in 1801 at 2.77 AU ( i = 3 ) were considered triumphs of the " law " ( see Table 1.1 and Nieto 1972 ) . Such was the success of the Titius - Bode " law " that both John Couch Adams ( 1847 ) and Urbain Le Verrier ...
... asteroid ( 1 ) Ceres in 1801 at 2.77 AU ( i = 3 ) were considered triumphs of the " law " ( see Table 1.1 and Nieto 1972 ) . Such was the success of the Titius - Bode " law " that both John Couch Adams ( 1847 ) and Urbain Le Verrier ...
الصفحة 9
... asteroid orbits and more than 500 reliable orbits for comets . Numerous bodies have been discovered with orbits beyond that of Pluto in the Edgeworth - Kuiper belt . Some estimates suggest that there may be as many as 2 × 108 objects ...
... asteroid orbits and more than 500 reliable orbits for comets . Numerous bodies have been discovered with orbits beyond that of Pluto in the Edgeworth - Kuiper belt . Some estimates suggest that there may be as many as 2 × 108 objects ...
الصفحة 13
... Asteroid Belt The asteroid belt also exhibits resonant structure . Explaining the gaps in the radial distribution of the asteroid orbits remains an important problem in solar system dynamics . Using a sample of < 100 asteroids ...
... Asteroid Belt The asteroid belt also exhibits resonant structure . Explaining the gaps in the radial distribution of the asteroid orbits remains an important problem in solar system dynamics . Using a sample of < 100 asteroids ...
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