Pulsating different curves of zero velocity around triangular equilibrium points in elliptical restricted three-body problem (Q355835)
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scientific article; zbMATH DE number 6191219
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Pulsating different curves of zero velocity around triangular equilibrium points in elliptical restricted three-body problem |
scientific article; zbMATH DE number 6191219 |
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Pulsating different curves of zero velocity around triangular equilibrium points in elliptical restricted three-body problem (English)
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25 July 2013
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Summary: The oblateness and the photogravitational effects of both the primaries on the location and the stability of the triangular equilibrium points in the elliptical restricted three-body problem have been discussed. The stability of the triangular points under the photogravitational and oblateness effects of both the primaries around the binary systems Achird, Lyeten, Alpha Cen-AB, Kruger 60, and Xi-Bootis, has been studied using simulation techniques by drawing different curves of zero velocity.
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