2004
DOI: 10.1023/b:cele.0000028165.34272.d9
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Electromagnetic Radiation and Motion of a Particle

Abstract: Abstract. We consider the motion of uncharged dust grains of arbitrary shape including the effects of electromagnetic radiation and thermal emission. The resulting relativistically covariant equation of motion is expressed in terms of standard optical parameters.Explicit expressions for secular changes of osculating orbital elements are derived in detail for the special case of the Poynting-Robertson effect. Two subcases are considered: (i) central acceleration due to gravity and the radial component of radiat… Show more

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Cited by 40 publications
(75 citation statements)
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“…The effect of electromagnetic radiation on spherical micron-sized dust particles yields, in general, a shift of perihelion, while the evolution of the semi-major axis and eccentricity may be calculated within an approximation of constant optical properties (see Eqs. (64)- (65), (102)- (103), with the corresponding initial conditions (58)- (63) in Klačka 2004). The statement about the semi-major axis and eccentricity hold when heliocentric distances are not smaller than about 0.1 AU.…”
Section: Numerical Resultsmentioning
confidence: 94%
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“…The effect of electromagnetic radiation on spherical micron-sized dust particles yields, in general, a shift of perihelion, while the evolution of the semi-major axis and eccentricity may be calculated within an approximation of constant optical properties (see Eqs. (64)- (65), (102)- (103), with the corresponding initial conditions (58)- (63) in Klačka 2004). The statement about the semi-major axis and eccentricity hold when heliocentric distances are not smaller than about 0.1 AU.…”
Section: Numerical Resultsmentioning
confidence: 94%
“…where f β 0 is a true anomaly (all orbital elements relates to the central acceleration G M (1 − β 0 ), also a true anomaly; corresponding quantities are denoted by subscript β 0, to be consistent with Klačka 2004). Using the fact that the semi-major axis and eccentricity exhibit small changes during one period − 1 6.58E-3 1.89E-3 7.51E-4 −1.08E-3…”
Section: Discussionmentioning
confidence: 97%
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