Stable stationary solutions to an unrestricted three body problem at the second order resonance and oblateness of a central planet.

Details Stable stationary solutions to an unrestricted three body problem at the second order resonance and oblateness of a central planet. Stable stationary solutions to an unrestricted three body problem at the second order resonance and oblateness of a central planet.

Aug 1998

adsabs.harvard.edu/abs/1998kosis..36..446s

Kosmicheskie Issledovaniia, Tom 36, No. 4, p. 446 - 448

Physics

Three-Body Problem: Planets, Three-Body Problem: Resonances, Three-Body Problem: Oblateness

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