Astrophysics and Space Science

, Volume 192, Issue 2, pp 257–262 | Cite as

The formalism of the translational-rotational motion of a rigid body in the field of a gravitating and radiating centre

  • A. G. Mavraganis
Article
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Abstract

The author's aim is to formulate the problem of motion of a rigid body acted upon by the Newtonian attraction of a particle and the repulsive force of this particle radiation. These forces are taken to be proportional to each other in a way which extends this connection from the point-like description of a body to its actual picture.

Keywords

Radiation Rigid Body Repulsive Force Particle Radiation Actual Picture 

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References

  1. Duboshin, G. N.: 1963,Celestial Mechanics, Basic Problems and Methods, Fizmatgiz, Moscow (translation Div. Wright-Patterson Air Force Base, Fairborn, Ohio, 1969).Google Scholar
  2. Mavraganis, A. G.: 1991,Mech. Res. Com. (submitted).Google Scholar
  3. Ogorodnikov, K. F.: 1958,The Stellar Dynamics Systems, GIFML, Moscow.Google Scholar
  4. Simmons, J. F. L. et al.: 1985,Celest. Mech. 35, 145.Google Scholar
  5. Zhuravlev, S. G.: 1989,Soviet Astron. 33(6), 680.Google Scholar

Copyright information

© Kluwer Academic Publishers 1992

Authors and Affiliations

  • A. G. Mavraganis
    • 1
  1. 1.Department of Engineering Science, Section of MechanicsNational Technical University of AthensAthensGreece

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