Pages that link to "Item:Q1804302"
From MaRDI portal
The following pages link to Gravitational potential harmonics from the shape of an homogeneous body (Q1804302):
Displaying 14 items.
- Small body surface gravity fields via spherical harmonic expansions (Q469033) (← links)
- The exact transformation from spherical harmonic to ellipsoidal harmonic coefficients for gravitational field modeling (Q531174) (← links)
- Determination of the potential of homogeneous polyhedral bodies using line integrals (Q697121) (← links)
- Ellipsoids, material points and material segments (Q868490) (← links)
- The temporal variation of the spherical and Cartesian multipoles of the gravity field: the generalized MacCullagh representation. (Q1862555) (← links)
- Evaluation of the spherical harmonic coefficients for the external potential of a polyhedral body with linearly varying density (Q2005594) (← links)
- Mixed-model gravity representations for small celestial bodies using mascons and spherical harmonics (Q2005632) (← links)
- Stability of the planar synchronous full two-body problem -- the approach of periodic orbits (Q2160937) (← links)
- Genealogy and stability of periodic orbit families around uniformly rotating asteroids (Q2205687) (← links)
- Uncertainties in the gravity spherical harmonics coefficients arising from a stochastic polyhedral shape (Q2210845) (← links)
- Uncertainty maps for motion around binary asteroids (Q2675574) (← links)
- A method for modelling the surface of irregular celestial bodies (Q3826141) (← links)
- The spin–spin model and the capture into the double synchronous resonance (Q4986213) (← links)
- Spin-orbit coupling of the primary body in a binary asteroid system (Q6609744) (← links)
