Simulation of the full two rigid body problem using polyhedral mutual potential and potential derivatives approach
From MaRDI portal
Publication:861398
DOI10.1007/s10569-006-9045-6zbMath1116.70014OpenAlexW2121246281MaRDI QIDQ861398
Eugene G. Fahnestock, Daniel J. Scheeres
Publication date: 29 January 2007
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-006-9045-6
Celestial mechanics (70F15) Orbital mechanics (70M20) Dynamics of a rigid body and of multibody systems (70E99)
Related Items (14)
Mutual potential between two rigid bodies with arbitrary shapes and mass distributions ⋮ Figure-figure interaction between bodies having arbitrary shapes and mass distributions: a power series expansion approach ⋮ Generating function of the inertial integrals for small celestial bodies ⋮ Accelerating binary asteroid system propagation via nested interpolation method ⋮ Dynamic limits on planar libration-orbit coupling around an oblate primary ⋮ The two-body interaction potential in the STF tensor formalism: an application to binary asteroids ⋮ Energy and stability in the full two body problem ⋮ Extended two-body problem for rotating rigid bodies ⋮ Vector potentials for the gravitational interaction of extended bodies and laminas with analytical solutions for two disks ⋮ A finite element method for computational full two-body problem. I: The mutual potential and derivatives over bilinear tetrahedron elements ⋮ The two rigid body interaction using angular momentum theory formulae ⋮ Dust motions in quasi-statically charged binary asteroid systems ⋮ The planar two-body problem for spheroids and disks ⋮ The spin–spin model and the capture into the double synchronous resonance
Cites Work
This page was built for publication: Simulation of the full two rigid body problem using polyhedral mutual potential and potential derivatives approach
