A sixth-order accurate scheme for solving two-point boundary value problems in astrodynamics
DOI10.1007/s10569-006-9047-4zbMath1116.70005OpenAlexW1967599676MaRDI QIDQ861394
Francesco Topputo, Roberto Armellin
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/s10569-006-9047-4
Restricted three-body problemBicircular four-body problemHalo orbitsNonlinear boundary value problem
Three-body problems (70F07) Computational methods for problems pertaining to mechanics of particles and systems (70-08) Control of mechanical systems (70Q05) Orbital mechanics (70M20)
Related Items (2)
Cites Work
- Numerical solution of two-point boundary value problems
- Sun-perturbed Earth-to-Moon transfers with low energy and moderate flight time
- High-order expansions of invariant manifolds of libration point orbits with applications to mission design
- Dynamics and Mission Design Near Libration Points
- BURRAU'S PROBLEM OF THREE BODIES
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