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The Stability of the Solar System and of Small Stellar Systems
Sur un Invariant Intégral du Problème des n Corps: Conséquence de L’homogénéité du Potentiel
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Author(s):
L. Losco
Publication date
(Print):
1974
Publisher:
Springer Netherlands
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The Analytical Foundations of Celestial Mechanics
A. WINTNER
,
A Wintner
(1941)
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Note concerning a conjecture by A. Wintner
J Waldvogel
(1972)
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Les méthodes nouvelles de la mécanique céleste
H. Poincaré
(1957)
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Book Chapter
Publication date (Print):
1974
Pages
: 249-255
DOI:
10.1007/978-94-010-9877-9_35
SO-VID:
7c23aeb1-32e4-4938-92c0-30e52312b30f
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Book chapters
pp. 1
Stability Theory in Celestial Mechanics
pp. 11
Modern Dynamical Systems Theory
pp. 19
The Present State of the n-Body Problem
pp. 21
Bode’s Law
pp. 23
Distribution of the Mean Motions of Planets and Satellites and the Development of the Solar System
pp. 25
Can the Solar System be Quantized?
pp. 37
On the Original Distribution of the Asteroids
pp. 57
The Origin of Commensurabilities in the Satellite Systems
pp. 59
The Origin of the Asteroid Ring
pp. 63
Orbits of Trojan Asteroids
pp. 71
The Role of Saturn’s Oblateness in the Mimas-Tethys Resonance
pp. 77
Stability of Asteroidal Motion in the Hecuba Gap
pp. 81
Secular Perturbations for Asteroids Belonging to Families
pp. 83
The Formation of Disks by Inelastic Collisions of Gravitating Particles. Applications to the Dynamics of the Saturn’s Ring and to the Formation of the Solar System
pp. 95
Stationary Solutions of the Averaged Three-Body Problem and Some Problems of Planet Motion Stability
pp. 117
Integrable Cases of Satellite Problem with the Third Body and the Oblate Planet
pp. 125
The Global Solution in the Problem of the Critical Inclination
pp. 129
Retrograde Satellites in the Circular Plane Restricted Three-Body Problem
pp. 131
A Note on a Separation of Equations of Variation of the Elliptic Restricted Three-Body Problem into Hill’s Equations
pp. 133
Comet Schwassmann-Wachmann 3 (1930 VI)
pp. 135
The Motion of Comet Westphal in 1852–1974
pp. 137
The Motion of Comet Encke-Backlund over 1901–1970
pp. 139
An Iterative Method of General Planetary Theory
pp. 157
On the Calculation of Secular Perturbations in the Case of Close Commensurability
pp. 165
Long Period Terms in the Solar System
pp. 167
On the Theory of the Galilean Satellites of Jupiter
pp. 185
Conditions for Escape and Retention
pp. 201
Influence of the Dynamical Figure of the Moon on its Rotational-Translational Motion
pp. 209
A Comparison of the Mean-Value and Initial-Value Solutions of the Ideal Resonance Problem with an Application in Rigid-Body Mechanics
pp. 211
Statistics of Three-Body Experiments
pp. 225
The Role of Binaries in Cluster Dynamics
pp. 231
On the Stability of Small Clusters or Cluster Remnants
pp. 239
The Dynamical Evolution of Trapezium Systems
pp. 247
The Stability of Triple Stellar Systems
pp. 249
Sur un Invariant Intégral du Problème des n Corps: Conséquence de L’homogénéité du Potentiel
pp. 257
Numerical Experiments on Expanding Gravitational Systems
pp. 259
Numerical Experiments on the Stability of Spherical Stellar Systems
pp. 261
On the ‘Thermodynamics’ of Self-Gravitating N-Body Systems
pp. 273
Dynamics and Clusters of Galaxies
pp. 285
Dynamical Friction Effects on the Motion of Stars in Rotating Spherical Clusters
pp. 297
On the Disappearance of Isolating Integrals in Dynamical Systems with More than Two Degrees of Freedom
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