Celestial Mechanics & Dynamical Astronomy

Papers
(The TQCC of Celestial Mechanics & Dynamical Astronomy is 3. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2021-05-01 to 2025-05-01.)
ArticleCitations
Planetary systems with forces other than gravitational forces35
Three families of 5-body central configurations in the plane21
Analysis of the natural orbits around Io18
Tidal evolution for any rheological model using a vectorial approach expressed in Hansen coefficients16
Mascon distribution techniques for asteroids and comets16
Automated tour design in the Saturnian system14
Accelerating binary asteroid system propagation via nested interpolation method14
Detection of separatrices and chaotic seas based on orbit amplitudes14
Satellite transfers between Keplerian orbits13
The nature of the Laplace resonance between the Galilean moons13
Transfers from the Earth to $$L_2$$ Halo orbits in the Earth–Moon bicircular problem11
Ellipsoidal equilibrium figure and Cassini states of rotating planets and satellites deformed by a tidal potential in the spatial case11
Orbit determination from one position vector and a very short arc of optical observations10
Invariant manifolds near $$L_1$$ and $$L_2$$ in the quasi-bicircular problem10
Asymptotic behaviour of orbit determination for hyperbolic maps10
Correction: Bifurcation of frozen orbits in a gravity field with zonal harmonics10
Asteroid families: properties, recent advances, and future opportunities9
Orbit averaging applied to inverse-square perturbations8
Sensitivity analysis of polar orbiter motion to lunar viscoelastic tidal deformation8
Identification of asteroid groups in the $$z_1$$ and $$z_2$$ nonlinear secular resonances through genetic algorithms7
Periodic orbits in a galactic potential7
Regularized phase-space volume for the three-body problem7
Orbits of charged particles with an azimuthal initial velocity in a dipole magnetic field7
Lagrange’s planetary equations with time-dependent secular perturbations7
Regular n-gon rotating equilibria with logarithm gravitational interaction7
A LiDAR-less approach to autonomous hazard detection and avoidance systems based on semantic segmentation7
Realizations of the interior spherical Bessel harmonic coefficients of a polyhedral body within the Brillouin sphere6
GANBISS: a new GPU accelerated N-body code for binary star systems6
Tidal evolution and spin–orbit dynamics for bodies in the viscous regime6
Correction: Mars orientation and rotation angles6
Dynamics around the Earth–Moon triangular points in the Hill restricted 4-body problem6
Framework for the full N-body problem in SE(3) and its reduction to the circular restricted full three-body problem6
Generalization of a method by Mossotti for initial orbit determination5
Design of satellite orbits in the Sun–Earth–Moon system5
“Twist vectors" for central configuration equations5
Orbit determination of the moons of the Pluto–Charon system5
Bifurcation of frozen orbits in a gravity field with zonal harmonics5
Revisiting Earth tide parameters used in the development of planetary and lunar ephemeris5
Kepler equation solution without transcendental functions or lookup tables5
Stability analysis of apsidal alignment in double-averaged restricted elliptic three-body problem5
Closed-form perturbation theory in the restricted three-body problem without relegation5
A new perturbative solution to the motion around triangular Lagrangian points in the elliptic restricted three-body problem4
An attempt to build a dynamical catalog of present-day solar system co-orbitals4
Low-energy Earth–Moon transfers via Theory of Functional Connections and homotopy4
Determination of the doubly symmetric periodic orbits in the restricted three-body problem and Hill’s lunar problem4
Regularization of the Hill four-body problem with oblate bodies4
Extension of the creep tide theory to exoplanet systems with high stellar obliquity. The dynamic tide of CoRoT-3b4
On the effect of the sun on Kordylewski clouds4
Rapid and accurate methods for computing whiskered tori and their manifolds in periodically perturbed planar circular restricted 3-body problems4
Spatial equilateral chain central configurations of the five-body problem with a homogeneous potential4
Correction: Chaotic coexistence of librational and rotational dynamics in the averaged planar three-body problem4
Evolution of the characteristic curves in the restricted three-body problem in terms of the mass parameter4
Secular orbital dynamics of the innermost exoplanet of the $$\upsilon $$-Andromedæ system4
The negative energy N-body problem has finite diameter4
Assessment of dynamical models for transitioning from the Circular Restricted Three-Body Problem to an ephemeris model with applications4
The capture probability of Dawn into ground-track resonances with Vesta4
Bounds on energy and angular momentum loss in the full n-body problem3
The power spectrum indicator, a new and fast method for the early detection of chaos3
An application of symplectic integration for general relativistic planetary orbitography subject to non-gravitational forces3
The Manifold Of Variations: impact location of short-term impactors3
Overlong simulations of the solar system dynamics with two alternating step-lengths3
On the global families of periodic solutions of a generalized Sitnikov problem3
Relegation-free closed-form perturbation theory and the domain of secular motions in the restricted three-body problem3
Chaos identification through the autocorrelation function indicator $$({\textit{ACFI}})$$3
Spin–orbit coupling of the primary body in a binary asteroid system3
Gaia-DR2 asteroid observations and INPOP planetary ephemerides3
Application of the theory of functional connections to the perturbed Lambert’s problem3
Reducing roundoff errors in numerical integration of planetary ephemeris3
Resonance perturbation of (5026) Martes and 2005 WW113 asteroid pair3
Librations of a body composed of a deformable mantle and a fluid core3
Understanding flow around planetary moons via finite-time Lyapunov exponent maps3
Melnikov method for non-conservative perturbations of the restricted three-body problem3
A hidden barrier surface complementary to the zero velocity surface in the circular restricted three-body problem3
Orbiting below the Brillouin sphere using shifted spherical harmonics3
The phase-space architecture in extrasolar systems with two planets in orbits of high mutual inclination3
Transit and capture in the planar three-body problem leveraging low-thrust invariant manifolds3
Exploring more solutions for low-energy transfers to lunar distant retrograde orbits3
Mars orientation and rotation angles3
Orbital dynamics of smart dust with Poynting–Robertson and solar wind drag3
An implicit symplectic solver for high-precision long-term integrations of the Solar System3
Implementation and study of a drag model for an N-body problem simulator3
Invariant manifolds near $$L_1$$ and $$L_2$$ in the Sun–Jupiter elliptic restricted three-body problem I3
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