Volume 464, Number 1, March II 2007AMBER: Instrument description and first astrophysical results
|Page(s)||127 - 134|
|Published online||19 December 2006|
Poynting-Robertson effect and perihelion motion
Department of Astronomy, Physics of the Earth, and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University, Mlynská dolina, 842 48 Bratislava, Slovak Republic e-mail: [klacka;pavol.pastor]@fmph.uniba.sk
2 Astronomical Institute, Slovak Academy of Sciences, Dúbravská cesta 9, 845 04 Bratislava, Slovak Republic e-mail: firstname.lastname@example.org
Accepted: 17 October 2006
The effect of stellar electromagnetic radiation on the motion of homogeneous spherical dust particles, the Poynting-Robertson (P-R) effect, is investigated. The effect already produces a shift of pericenter/perihelion in the accuracy to the first order in , where is velocity of the particle with respect to the source of radiation and c is the speed of light. The advancement of pericenter occurs due to the fact that the P-R effect depends on radiation pressure efficiency factor , which is a function of optical properties of the particle. The particle orbiting a star moves in various distances from the star and the particle optical properties may vary with the distance, as they are functions of temperature.
Key words: scattering / solar system: general / interplanetary medium
© ESO, 2007
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