Formation of the Kirkwood gaps in the asteroid belt

DOI10.1007/BF01235812zbMath0571.70005OpenAlexW4249559053MaRDI QIDQ3687763

Anne Lemaitre

Publication date: 1984

Published in: Celestial Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01235812

zbMATH Keywords

dissipationresonancesKirkwood gapadiabatic invariant theoryasteroids beltrestricted circular and planar 3-body problem

Mathematics Subject Classification ID

Three-body problems (70F07)

Related Items (6)

Critical point families at the 3:1 resonance ⋮ The critical inclination problem ? 30 years of progress ⋮ Secular resonances in the primitive solar nebula ⋮ The elliptic restricted problem at the 3:1 resonance ⋮ A perturbation method for problems with two critical arguments ⋮ Asteroid motion near the 3:1 resonance

Cites Work

• A second fundamental model for resonance
• High-order resonances in the restricted three-body problem
• Capture into resonance: An extension of the use of adiabatic invariants
• The gravitational potential due to uniform disks and rings

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