Abstract
The Poynting-Robertson effect (P-R effect) (Robertson, 1937), (Klacka, 1992) is generally considered to be the real effect which influences the motion of interplanetary dust particles (IDPs) — meteoroids, in the Solar System. The most general case of the validity of the P-R effect requires that Eq. (120) (or, Eq. (122) for the moving particle) in (Klaĉka, 1992) holds.
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© 2001 Springer Science+Business Media Dordrecht
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Klačka, J., Kocifaj, M. (2001). On the Stability of the Zodiacal Cloud. In: Pretka-Ziomek, H., Wnuk, E., Seidelmann, P.K., Richardson, D.L. (eds) Dynamics of Natural and Artificial Celestial Bodies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1327-6_58
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DOI: https://doi.org/10.1007/978-94-017-1327-6_58
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