We investigate the stability of motion close to the Lagrangian equilibrium points L 4 and L 5
in the framework of the spatial, elliptic, restricted three-body problem, subject to the radial …

The term 'α-meteoroid'was introduced to describe a group of micrometeoroids with certain
dynamical properties, which–alongside the group of the β-meteoroids–had been identified …

A new algorithm is presented for the numerical integration of second-order ordinary
differential equations with perturbations that depend on the first derivative of the dependent …

We perform an analysis of the dynamics of the circular, restricted, planar three-body problem
under the effect of different kinds of dissipation (linear, Stokes and Poynting–Robertson …

We investigate the combined effect of solar wind, Poynting–Robertson drag, and the frozen-
in interplanetary magnetic field on the motion of charged dust grains in our solar system. For …

Third and fourth order mean motion resonances are studied in the model of the restricted
three-body problem by numerical methods for mass parameters corresponding …

In the frame work of Saturn–Titan system, the resonant orbits of first-order are analyzed for
three different families of periodic orbits, namely, interior resonant orbits, exterior resonant …

In this paper, we investigate the action of solar wind on an arbitrarily shaped interplanetary
dust particle. The final relativistically covariant equation of motion of the particle also …

We present some analytical results about the existence of periodic orbits for the planar
restricted three body problem with dissipation considered recently by Celletti et al.(CMDA …

Eccentricity evolution of a dust particle in a mean motion orbital resonance with a planet in
circular orbit is investigated. The action of solar electromagnetic and corpuscular radiation …