On the stability of the zodiacal cloud

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1994 English Publisher:Springer Science and Business Media LLCJournal:Earth, Moon, and Planets, volume 64, pages 95-98 (issn: 0167-9295, eissn: 1573-0794,

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Authors: J. Klačka;

doi: 10.1007/bf00608207

On the stability of the zodiacal cloud

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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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