The non-radial component of the solar wind and motion of dust near mean motion resonances with planets
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20078752/pdf
Reference35 articles.
1. Capture in Exterior Mean-Motion Resonances Due to Poynting-Robertson Drag
2. Brouwer, D., & Clemence, G. M. 1961, Methods of Celestial Mechanics (New York: Academic Press)
3. The ring around us
4. Radial evolution of solar wind intermittency in the inner heliosphere
5. A circumsolar ring of asteroidal dust in resonant lock with the Earth
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1. Dust grains in mean motion orbital resonances with a planet;Planetary and Space Science;2020-03
2. Locations of stationary/periodic solutions in mean motion resonances according to the properties of dust grains;Monthly Notices of the Royal Astronomical Society;2016-04-17
3. Orbital evolution of dust in the Edgeworth–Kuiper belt zone;Monthly Notices of the Royal Astronomical Society;2015-04-17
4. The effect of Poynting–Robertson drag on the triangular Lagrangian points;Icarus;2015-04
5. On the stability of dust orbits in mean-motion resonances perturbed by from an interstellar wind;Celestial Mechanics and Dynamical Astronomy;2014-08-02
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