Insights into the dynamics of a complex system are often gained by focusing on large
fluctuations. For the financial system, huge databases now exist that facilitate the analysis of …

In this work, we study the stability of hypothetical satellites of extrasolar planets. Through
numerical simulations of the restricted elliptic three-body problem we found the borders of …

It has been thought,, that the capture of irregular moons—with non-circular orbits—by giant
planets occurs by a process in which they are first temporarily trapped by gravity inside the …

We investigate the stability of prograde versus retrograde planets in circular binary systems
using numerical simulations. We show that retrograde planets are stable up to distances …

In this paper we use recently developed phase-space transport theory coupled with a so-
called classical spectral theorem to develop a dynamically exact and computationally …

Target of NASA's DART mission, the system of Didymos and Dimorphos will once again be
visited by a space mission—ESA's Hera mission, scheduled to be launch in 2024. Hera will …

The stability evolution of family f of the planar circular restricted three-body problem in the
Earth–Moon case is explored numerically using the Poincaré surface of section. It is shown …

In a previous work, Giuliatti Winter et al. found several stable regions for test particles in orbit
around Pluto associated with families of periodic orbits obtained in the circular, restricted …

This work generates, through a sample of numerical simulations of the restricted three-body
problem, diagrams of semimajor axis and eccentricity which defines stable and unstable …

In the present work we explore regions of distant direct stable orbits around the Moon. First,
the location and size of apparently stable regions are searched for numerically, adopting the …