Generalized perturbation equations of celestial mechanics
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Abstract
Generalized perturbation equations of celestial mechanics in terms of orbital elements are derived. The most general case is considered: Keplerian motion of two bodies caused by gravitational forces between them is disturbed by disturbing acceleration acting on each of the bodies separately and by changes of masses of these bodies. It is also pointed out why derivation presented in Klačka (1992a) is completely physically correct only for constant masses.
Keywords
Gravitational Force Constant Mass Orbital Element Celestial Mechanic Perturbation Equation
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References
- Klačka, J.: 1992a, ‘Perturbation Equations of Celestial Mechanics’,Earth, Moon and Planets 59, 23–39.Google Scholar
- Klačka, J.: 1992b, ‘Interplanetary Dust Particles: Disintegration and Orbital Motion’,Earth, Moon and Planets 60, 17–21 (1993).Google Scholar
- Klačka, J. and Saniga, M.: 1992a, ‘Interplanetary Dust Particles and Solar Wind’,Earth, Moon and Planets 60, 23–29 (1993).Google Scholar
- Klačka, J. and Saniga, M.: 1992b, ‘Interplanetary Dust Particles and Impact Erosion’,Earth, Moon and Planets 59, 103–110.Google Scholar
Copyright information
© Kluwer Academic Publishers 1993