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Third-order secular Solution of the variational equations of motion of a satellite in orbit around a non-spherical planet - MaRDI portal

Third-order secular Solution of the variational equations of motion of a satellite in orbit around a non-spherical planet (Q2443570)

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Third-order secular Solution of the variational equations of motion of a satellite in orbit around a non-spherical planet
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    Third-order secular Solution of the variational equations of motion of a satellite in orbit around a non-spherical planet (English)
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    8 April 2014
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    satellite Earth orbit
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    orbit perturbation
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    Lagrange equations of motion
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    Earth oblateness
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    secular variations
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