uniform distribution
planar three body problem
formation
belt
adiabatic invariant theory
2021-11-01T17:56
1984-09-01
329-341
false
Kirkwood gaps
possible mechanism
invariant theory
origin
slow dissipation
means
nebula
three body problem
solar nebula
cases
1984-09
asteroid belt
gap
depletion
asteroids
article
resonance case
articles
distribution
solar system
theory
https://doi.org/10.1007/bf01235812
Formation of the Kirkwood gaps in the asteroid belt
dissipation
framework
en
body problem
system
A possible mechanism to explain the depletion of the Kirkwood gaps in the asteroid belt would be the slow dissipation of the solar nebula at the origin of the Solar System. The effects of this dissipation on a uniform distribution of asteroids are explored by means of the adiabatic invariant theory for the 2/1, 3/1 and 5/2 resonance cases. The framework is the restricted, circular and planar three body problem.
mechanism
problem
effect
https://scigraph.springernature.com/explorer/license/
34
Applied Mathematics
A.
Lemaitre
Springer Nature - SN SciGraph project
0923-2958
Celestial Mechanics and Dynamical Astronomy
Springer Nature
0008-8714
Department of Mathematics, Rempart de la Vierge, 8, 5000, Namur, Belgium
Department of Mathematics, Rempart de la Vierge, 8, 5000, Namur, Belgium
10.1007/bf01235812
doi
Mathematical Sciences
1-4
dimensions_id
pub.1014281022