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A method for asteroid mass determination

Published online by Cambridge University Press:  25 May 2016

M. Kuzmanoski
M. Kuzmanoski*
Affiliation:
Faculty of Mathematics Studentski trg 16, 11000 Belgrade, Yugoslavia

Extract

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It is well known that the perturbing effects of any asteroid are negligible at all times, except during a close encounter. The influence of a perturbing asteroid on the motion of a perturbed one can be investigated by means of the differences of the right ascensions and declinations of the perturbed asteroid, as inferred from two numerical integrations, the one with and the other without taking into account the effects of the perturbing asteroid (Kuzmanoski and Knežević, 1994). These effects before reaching the epoch of the close encounter are very small, as expected. Beyond this epoch, the differences increase with time, due to the fact that the orbit is changed on account of the influence of the perturbing body during the close approach, so that perturbations by major planets act on it in a different way.

Type
Part IV - Asteroids: Theory and Ephemerides
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 207 - 208
Copyright
Copyright © Kluwer 1996 

References

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Kuzmanoski, M., Knežević, Z. (1994) Asteroid close encounters and mutual perturbations, Planet. Space Sci., 42, 297–299 CrossRefGoogle Scholar