Slow diffusion and effective stability of dust particles orbiting asteroids

DOI10.1023/A:1019966826421zbMATH Open1027.70018OpenAlexW53119150MaRDI QIDQ1870178

Harry J. Dankowicz

Publication date: 11 May 2003

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

Full work available at URL: https://doi.org/10.1023/a:1019966826421

zbMATH Keywords

restricted three-body problemradiation pressureeffective stabilitynormal-form transformationspersistent periodic orbits

Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15) Dynamical systems in classical and celestial mechanics (37N05) Waves and radiation in optics and electromagnetic theory (78A40)

Related Items (1)

Chaotic Di?usion of Asteroids

Recommendations

• Motion of dust in mean motion resonances with planets 👍 👎
• Dust motions in quasi-statically charged binary asteroid systems 👍 👎
• Slow and fast diffusion in asteroid-belt resonances: A review 👍 👎
• Chaotic Di?usion of Asteroids 👍 👎
• Diffusion characters of the orbits in the asteroid motion 👍 👎
• Title not available (Why is that?) 👍 👎
• Title not available (Why is that?) 👍 👎
• Title not available (Why is that?) 👍 👎
• Title not available (Why is that?) 👍 👎

This page was built for publication: Slow diffusion and effective stability of dust particles orbiting asteroids

Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q1870178)