Crash test for the Copenhagen problem with oblateness
EE Zotos - Celestial Mechanics and Dynamical Astronomy, 2015 - Springer
The case of the planar circular restricted three-body problem where one of the two primaries
is an oblate spheroid is investigated. We conduct a thorough numerical analysis on the …
is an oblate spheroid is investigated. We conduct a thorough numerical analysis on the …
Single-averaged model for analysis of frozen orbits around planets and moons
JPS Carvalho, T Yokoyama, DC Mourão - Celestial Mechanics and …, 2022 - Springer
Let us consider the restricted three-body problem. Analysis of the orbital motion of a
spacecraft around planets or moons is presented taking into account the nonsphericity of the …
spacecraft around planets or moons is presented taking into account the nonsphericity of the …
How does the oblateness coefficient influence the nature of orbits in the restricted three-body problem?
EE Zotos - Astrophysics and Space Science, 2015 - Springer
We numerically investigate the case of the planar circular restricted three-body problem
where the more massive primary is an oblate spheroid. A thorough numerical analysis takes …
where the more massive primary is an oblate spheroid. A thorough numerical analysis takes …
Exploring the equilibrium dynamics of an infinitesimal body in the perturbed problem of five bodies
MS Suraj, EI Abouelmagd, M Bhushan… - Chaos, Solitons & …, 2025 - Elsevier
This work aims to analyze the dynamics of the restricted five-body problem when the
primaries are non-spherical spheroids. We explored numerically three different scenarios:(i) …
primaries are non-spherical spheroids. We explored numerically three different scenarios:(i) …
Orbital dynamics in the post-Newtonian planar circular restricted Sun–Jupiter system
EE Zotos, FL Dubeibe - International Journal of Modern Physics D, 2018 - World Scientific
The theory of the post-Newtonian (PN) planar circular restricted three-body problem is used
for numerically investigating the orbital dynamics of a test particle (eg a comet, asteroid …
for numerically investigating the orbital dynamics of a test particle (eg a comet, asteroid …
Orbital dynamics in the planar Saturn-Titan system
EE Zotos - Astrophysics and Space Science, 2015 - Springer
We use the planar circular restricted three-body problem in order to numerically investigate
the orbital dynamics of orbits of a spacecraft, or a comet, or an asteroid in the Saturn-Titan …
the orbital dynamics of orbits of a spacecraft, or a comet, or an asteroid in the Saturn-Titan …
Effects of the planetary migration on some primordial satellites of the outer planets-I. Uranus' case
Context. During the first hundred million years after the formation of our solar system, the
four giant planets are believed to have migrated significantly (by up≈ 20 AU). The current …
four giant planets are believed to have migrated significantly (by up≈ 20 AU). The current …
Orbit classification in the planar circular Pluto-Charon system
EE Zotos - Astrophysics and Space Science, 2015 - Springer
We numerically investigate the orbital dynamics of a spacecraft, or a comet, or an asteroid in
the Pluto-Charon system in a scattering region around Charon using the planar circular …
the Pluto-Charon system in a scattering region around Charon using the planar circular …
On the classification of orbits in the three-dimensional Copenhagen problem with oblate primaries
The character of motion for the three-dimensional circular restricted three-body problem with
oblate primaries is investigated. The orbits of the test particle are classified into four types …
oblate primaries is investigated. The orbits of the test particle are classified into four types …
[HTML][HTML] Oblateness Effect of Saturn on Halo Orbits of L1 and L2 in Saturn-Satellites Restricted Three-Body Problem
N Pushparaj, RK Sharma - International Journal of Astronomy and …, 2016 - scirp.org
The Circular Restricted Three-Body Problem (CRTBP) with more massive primary as an
oblate spheroid with its equatorial plane coincident with the plane of motion of the primaries …
oblate spheroid with its equatorial plane coincident with the plane of motion of the primaries …