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The Qualitative Explanation of Observed Peculiarities of Hecuba and Hilda Asteroids Distribution by a Common Investigation

Published online by Cambridge University Press:  07 August 2017

Elena V. Alfimova  and
Igor A. Gerasimov
Elena V. Alfimova
Affiliation:
Shternberg State Astronomical Institute, Moscow, 119899, USSR. e-mail: SNN@SAI.MSK.SU
Igor A. Gerasimov
Affiliation:
Shternberg State Astronomical Institute, Moscow, 119899, USSR. e-mail: SNN@SAI.MSK.SU

Extract

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Let us consider the planar case of the circular restricted three-body problem. The mass of central body is unit, the radius of the circular orbit of perturbing point P′ (of mass μ = 1/1047.39 according to Jupiter's mass) is also unit and the other unit is such that the gravitational constant is equal to 1. The Keplerian elements of the perturbed mass point P (asteroid), with semi-major axis α < 1, are given by usual notations; the elements of P‘ are indicated with a prime (’).

Type
Part III - The Asteroidal Belt
Information
Symposium - International Astronomical Union , Volume 152: Chaos, Resonance and Collective Dynamical Phenomena in the Solar System , 1992 , pp. 139 - 144
Copyright
Copyright © Kluwer 1992 

References

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