2000/05/05 by J. Klačka, Jozef Klacka, Klacka, Jozef
Physics and Astronomy · #Astrophysics (astro-ph) #Experimental and Theoretical Physics Studies #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0005100
arxiv created 2000/05/05 · openalex publication_date 2000/05/05 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
A simple model for motion of dust particle (meteoroid) under the action of (solar) electromagnetic radiation is presented. The particle of the form of plane mirror is taken into account and exact analytical results are presented. As for long-term orbital evolution, particle may spiral outwards the central body (Sun); initial conditions are important. As a consequence, motion of real dust particles may differ from that generally considered.