𝔖 Bobbio Scriptorium
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Poynting-Robertson effect: ‘Circular’ orbit

✍ Scribed by J. Klačka; J. Kaufmannová


Publisher
Springer Netherlands
Year
1992
Tongue
English
Weight
243 KB
Volume
59
Category
Article
ISSN
1573-0794

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✦ Synopsis


Time evolution of the interplanetary dust particle under the action of the solar electromagnetic radiation (Poynting-Robertson effect) is investigated. Evolution of the initially circular orbit in terms of the orbital elements present in the standard equations for their secular changes is considered. It is pointed out that the osculating eccentricity is practically constant during the motion in spite of generally accepted opinion that the standard equations for the secular changes of orbital elements represent time evolution of the osculating elements.


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Grains orbiting a star experience orbital decay due to Poynting-Robertson drag and can become trapped in commensurability resonances with a planet. We examine conditions for trapping in the circular restricted three-body problem, and derive criteria for trapping in terms of the radiation pressure fa