Some particularities in motion of retrograde satellites of Jupiter (Q1911226)
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scientific article; zbMATH DE number 866175
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Some particularities in motion of retrograde satellites of Jupiter |
scientific article; zbMATH DE number 866175 |
Statements
Some particularities in motion of retrograde satellites of Jupiter (English)
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16 February 1997
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Some peculiarities in the motion of retrograde satellites of Jupiter are investigated. The intermediate orbits are obtained by approximated solution of differential equations before transformation by the Zeipel's method. These orbits are non-Keplerian ellipses. For their construction, the secular motion of nodes, perijoves, and essential periodic perturbations are taken into account.
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motion of longitude of perijove
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Zeipel's method
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non-Keplerian ellipses
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secular motion of nodes
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periodic perturbations
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0.7824395298957825
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0.7735666632652283
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