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Motions of Celestial Bodies: Computer simulations [Kietas viršelis]

(St Petersburg State University, Russia)
  • Formatas: Hardback, 240 pages, aukštis x plotis x storis: 254x178x14 mm, With figures in colour and black and white
  • Serija: IOP Expanding Physics
  • Išleidimo metai: 15-Oct-2014
  • Leidėjas: Institute of Physics Publishing
  • ISBN-10: 0750311010
  • ISBN-13: 9780750311014
Kitos knygos pagal šią temą:
  • Formatas: Hardback, 240 pages, aukštis x plotis x storis: 254x178x14 mm, With figures in colour and black and white
  • Serija: IOP Expanding Physics
  • Išleidimo metai: 15-Oct-2014
  • Leidėjas: Institute of Physics Publishing
  • ISBN-10: 0750311010
  • ISBN-13: 9780750311014
Kitos knygos pagal šią temą:
Preface ix
Author biography xi
1 Introduction: getting started 1-1
1.1 List of the simulation programs 1-1
1.2 How to operate the simulation programs 1-2
1.3 Keplerian motions in celestial mechanics 1-3
1.4 Numerical and analytical methods 1-6
Part I Review of the simulations 2-1
2 Kepler's laws 2-3
2.1 Kepler's first law 2-3
Questions and problems 2-7
2.2 Kepler's second law 2-8
Questions and problems 2-10
2.3 Kepler's third law 2-11
Questions and problems 2-14
2.4 The approximate nature of Kepler's laws 2-15
Questions and problems 2-16
3 Hodograph of the velocity vector for Keplerian motion 3-1
3.1 Hodograph of the velocity for closed orbits 3-1
3.2 Hodograph of the velocity for open orbits 3-3
Questions and problems 3-5
4 Orbits of satellites and trajectories of missiles 4-1
4.1 Families of Keplerian orbits 4-2
4.1.1 Orbits with various directions of the initial velocities 4-2
4.1.2 Satellites with equal magnitudes of the initial velocities 4-5
4.1.3 Orbits of satellites launched in one direction with different magnitudes of the initial velocities 4-7
Questions and problems 4-9
4.2 Evolution of an orbit in the atmosphere 4-10
4.2.1 Evolution of an elongated elliptical orbit 4-11
4.2.2 Late stage of the evolution and the aerodynamical paradox 4-12
4.2.3 Air density over the Earth 4-14
Questions and problems 4-17
5 Active maneuvers in space orbits 5-1
5.1 How to operate the program 5-1
5.2 Space flights and orbital maneuvers 5-4
5.2.1 Designing a space flight 5-4
5.2.2 The way back from space to the Earth 5-5
Questions and problems 5-9
5.3 Relative motion of bodies in space orbits 5-9
5.3.1 The motion of a small body ejected from the orbital station 5-10
5.3.2 Numerical estimates 5-12
5.3.3 The secular component of the relative motion 5-13
5.4 Space probes and relative motion 5-15
5.4.1 Space probes in inner orbits 5-15
5.4.2 Space probes in outer orbits 5-17
Questions and problems 5-19
5.5 Rendezvous in space and interplanetary flights 5-20
Questions and problems 5-21
6 Precession of an equatorial orbit 6-1
Questions and problems 6-5
7 Binary stars—the two-body problem 7-1
Questions and problems 7-5
8 Three-body systems 8-1
8.1 The restricted three-body problem 8-1
8.2 Managing the program 'Planet with a Satellite' 8-2
8.3 Satellites of a planet that orbits a star 8-3
8.4 Exact particular solutions to the three-body problem 8-8
8.4.1 A system with equal masses of heavy bodies 8-8
8.4.2 Satellites at the triangular libration points 8-10
8.4.3 The collinear libration points 8-12
8.5 A space flight over the back side of the Moon 8-18
8.6 Lunar perturbations of a satellite's orbit 8-20
8.7 A space voyage to a distant planet and back 8-21
8.8 Comets—interplanetary vagabonds 8-25
8.9 A double star with a planet 8-28
Questions and problems 8-32
9 Many-body systems in celestial mechanics 9-1
9.1 Planetary system—a many-body problem 9-1
9.2 A model of the Solar System 9-4
9.2.1 The kinematics of planetary motion 9-4
9.2.2 Kinematics of the inferior planets 9-7
9.3 Hypothetical planetary systems and heavenly catastrophes 9-7
9.4 Multiple stars 9-11
9.5 Exact particular solutions to the many-body problem 9-13
9.5.1 A star with two planets of equal mass 9-13
9.5.2 A 'round dance' of identical planets 9-15
9.5.3 Keplerian motions in equilateral configurations 9-16
9.5.4 A remarkable three-body motion along a figure-eight 9-20
Questions and problems 9-21
Part II The simulated phenomena 10-1
10 Phenomena and concepts in celestial mechanics—an introductory approach 10-3
10.1 Newton's law of universal gravitation 10-3
10.2 Potential energy of a body in the Newtonian gravitational field 10-5
10.3 Circular velocity and escape velocity 10-6
10.4 Geometric properties of Keplerian orbits 10-8
10.5 Initial conditions and parameters of Keplerian orbits 10-10
10.6 A satellite in the atmosphere 10-13
10.7 Trajectories of a landing module 10-16
10.8 A space probe 10-19
10.9 Space rendezvous 10-21
10.10 Kepler's laws and the solar system 10-24
10.11 An approximate approach to the restricted three-body problem 10-25
Questions for further thought 10-28
11 Theoretical background 11-1
11.1 Angular momentum and areal velocity 11-1
11.2 Dynamical derivation of Kepler's first law 11-3
11.3 Kepler's third law 11-6
11.4 A hodograph of the velocity vector for Keplerian motion 11-8
11.5 Another derivation of Kepler's first law 11-11
11.6 A family of orbits with equal energies and a common initial point 11-14
11.6.1 The envelope surface for the family of orbits 11-14
11.6.2 Applications of the envelope surface 11-17
11.7 Relative orbital motion 11-19
11.8 The gravitational field of a distorted planet 11-23
11.8.1 A planet with additional masses at the poles 11-24
11.8.2 A planet with an equatorial bulge 11-25
11.9 The two-body problem 11-26
11.9.1 Reduced mass and relative motion 11-27
11.9.2 An alternative approach to the two-body problem 11-29
11.10 Exact particular solutions to the three-body problem 11-30
11.11 The non-restricted three-body problem 11-35
11.11.1 A star with two identical planets 11-36
11.11.2 The regular Keplerian motions of three different bodies in the equilateral configuration 11-37
11.12 The sphere of gravitational action 11-40
11.13 The oceanic tides 11-42
11.13.1 The origin of tidal forces: an elementary approach 11-44
11.13.2 Tidal forces at an arbitrary point near the Earth 11-47
11.13.3 The horizontal and vertical components of the tidal force 11-48
11.13.4 The static distortion of the water surface 11-50
11.13.5 Tidal forces on the rotating Earth 11-51
11.13.6 The potential function for tidal forces 11-53
11.13.7 The natural wave and the driving tidal forces 11-54
11.13.8 The tides as forced oscillations of the ocean 11-56
11.13.9 A mathematical description of the forced oscillations 11-57
11.13.10 Real-world complications 11-59
11.13.11 The evolution of orbital motions and spins of celestial bodies induced by tidal forces 11-60
12 Glossary 12-1