Dynamical portrait of the Lixiaohua asteroid family

DOI10.1007/s10569-010-9263-9zbMath1291.70044OpenAlexW2113218884WikidataQ60164444 ScholiaQ60164444MaRDI QIDQ990341

J. Martínez

Publication date: 31 August 2010

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10569-010-9263-9

zbMATH Keywords

chaotic motionmean-motion resonancesasteroid familiesthree-body MMRYarkovsky-induced drift

Mathematics Subject Classification ID

Celestial mechanics (70F15)

Related Items (1)

Chirikov diffusion in the asteroidal three-body resonance \((5, - 2, - 2)\)

Uses Software

• VESTA

Cites Work

• Proposals for the masses of the three largest asteroids, the Moon-Earth mass ratio and the astronomical unit
• Secular perturbation theory and computation of asteroid proper elements
• Regular and stochastic motion
• Modeling close encounters with massive asteroids: a Markovian approach
• Synthetic proper elements for outer main belt asteroids

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