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期刊名:Celestial mechanics & dynamical astronomy

缩写:CELEST MECH DYN ASTR

ISSN:0923-2958

e-ISSN:1572-9478

IF/分区:1.4/Q3

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共收录本刊相关文章索引3344
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Rahil Makadia,Davide Farnocchia,Steven R Chesley et al. Rahil Makadia et al.
We present a new method for computing the state transition matrix of a nonlinear dynamical system. The proposed method does not require the implementation of complex partial derivatives or auto-differentiation of the dynamics, while removin...
Maximilian Zimmermann,Elke Pilat-Lohinger Maximilian Zimmermann
We present a GPU accelerated N-body integrator using the Bulirsch-Stoer method, called GANBISS (GPU accelerated n-body code for binary star systems). It is designed to simulate the dynamical evolution of planetesimal disks in binary star sy...
Barak Kol Barak Kol
The three-body problem is a fundamental long-standing open problem, with applications in all branches of physics, including astrophysics, nuclear physics and particle physics. In general, conserved quantities allow to reduce the formulation...
Luke Bury,Jay McMahon Luke Bury
The circular restricted three-body model is widely used for astrodynamical studies in systems where two major bodies are present. However, this model relies on many simplifications, such as point-mass gravity and planar, circular orbits of ...
C S Arnot,C R McInnes,R J McKay et al. C S Arnot et al.
This paper presents rich new families of relative orbits for spacecraft formation flight generated through the application of continuous thrust with only minimal intervention into the dynamics of the problem. Such simplicity facilitates imp...
C Burger,T I Maindl,C M Schäfer C Burger
Collisions between large, similar-sized bodies are believed to shape the final characteristics and composition of terrestrial planets. Their inventories of volatiles such as water are either delivered or at least significantly modified by s...
Alice C Quillen,Yuan-Yuan Chen,Benoît Noyelles et al. Alice C Quillen et al.
A Hamiltonian model is constructed for the spin axis of a planet perturbed by a nearby planet with both planets in orbit about a star. We expand the planet-planet gravitational potential perturbation to first order in orbital inclinations a...