Online Resource
Cambridge University Press (CUP)
;
1996
In:
Symposium - International Astronomical Union Vol. 172 ( 1996), p. 57-60
In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 172 ( 1996), p. 57-60
Abstract:
The motion of the Jovian planets is investigated using Hamiltonian perturbation theory and numerical integrations. Experiments varying the mass of Neptune exhibit 1:1 secular resonance between the perihelion motions of Jupiter and Uranus.
Type of Medium:
Online Resource
ISSN:
0074-1809
DOI:
10.1017/S0074180900127135
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1996
SSG:
16,12
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