Numerical efficiency of the elliptic function expansions of the first-order intermediary for general planetary theory
1996 ◽
Vol 172
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pp. 101-104
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Keyword(s):
We compare numerical efficiency of the two kinds of series for the first-order intermediate orbit for general planetary theory: (1) the classical expansion involving mean longitudes of the planets; (2) an expansion resulting from the theory of elliptic functions. We conclude that mutual perturbations of close couples of planets (the ratio of major semi-axes ∼ 1) can be represented in more compact form with the aid of the second kind of series.
1994 ◽
Vol 59
(1)
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pp. 1-36
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1997 ◽
Vol 66
(4)
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pp. 345-363
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1973 ◽
Vol 25
(2)
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pp. 271-354
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1997 ◽
pp. 301-306
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Keyword(s):
2011 ◽
Vol 25
(14)
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pp. 1931-1939
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