Pages that link to "Item:Q1311632"
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The following pages link to Long period variations of the motion of a satellite due to non-resonant tesseral harmonics of a gravity potential (Q1311632):
Displaying 7 items.
- Long-period variations of the eccentricity vector valid also for near circular orbits around a non-spherical body (Q817659) (← links)
- Satellite motion in a non-singular gravitational potential (Q973715) (← links)
- An analytical theory for tesseral gravitational harmonics (Q1593009) (← links)
- Closed-form perturbation theory in the restricted three-body problem without relegation (Q2138494) (← links)
- Exploring the long-term dynamics of perturbed Keplerian motion in high degree potential fields (Q2207731) (← links)
- Dynamics of a satellite orbiting a planet with an inhomogeneous gravitational field (Q2641622) (← links)
- Dynamics of artificial satellite orbits with tesseral resonances including the effects of luni- solar perturbations (Q4237735) (← links)