Add to ORKGUsing a semi-analytical approach, domains of possible motion for Trojan asteroids were established. It is shown that stable librating motion is possible for both high inclination and high eccentricity. Frequency distributions were also produced for real Trojan asteroids, against differing libration amplitudes and libration periods
We present a series of numerical integrations of observed and fictitious Jupiter Trojan asteroids, u...
In this paper, we focus on the stability of the Trojan asteroids for the planar restricted three-bod...
Trojan asteroids are minor planets that share the orbit of a planet about the Sun and librate around...
Jupiter Trojans are a remnant of outer solar system planetesimals captured into stable or quasistabl...
DraftJupiter’s Trojan asteroids fulfill the prediction of Lagrange that orbits can be stable when a ...
working version of a paper planned for Planetary and Space ScienceJupiter’s Trojan asteroids fulfill...
Context.We have known about the Trojan group of asteroids since 1906. With a suspected number compar...
Aims. In this paper, we analyze the collisional and dynamical evolution of the population of L4 Jovi...
We have numerically explored the mechanisms that destabilize Jupiter's Trojan orbits outside the sta...
A mechanism to replenish the Apollo and Amor groups by resonant asteroid-orbit transformation is sug...
In this paper we develop a semianalytical model to describe the long-term motion of Trojan asteroids...
The Jupiter Trojans constitute an important asteroidal population both in number and also in relatio...
In this case of the 5:2 commensurability with the motion of Jupiter, an asteroid can reach the orbit...
Trojan asteroids are small bodies orbiting around the L or L Lagrangian points of a Sun-planet syste...
In this paper, I construct a program to map the evolution of the potential in a planet-star system w...
We present a series of numerical integrations of observed and fictitious Jupiter Trojan asteroids, u...
In this paper, we focus on the stability of the Trojan asteroids for the planar restricted three-bod...
Trojan asteroids are minor planets that share the orbit of a planet about the Sun and librate around...
Jupiter Trojans are a remnant of outer solar system planetesimals captured into stable or quasistabl...
DraftJupiter’s Trojan asteroids fulfill the prediction of Lagrange that orbits can be stable when a ...
working version of a paper planned for Planetary and Space ScienceJupiter’s Trojan asteroids fulfill...
Context.We have known about the Trojan group of asteroids since 1906. With a suspected number compar...
Aims. In this paper, we analyze the collisional and dynamical evolution of the population of L4 Jovi...
We have numerically explored the mechanisms that destabilize Jupiter's Trojan orbits outside the sta...
A mechanism to replenish the Apollo and Amor groups by resonant asteroid-orbit transformation is sug...
In this paper we develop a semianalytical model to describe the long-term motion of Trojan asteroids...
The Jupiter Trojans constitute an important asteroidal population both in number and also in relatio...
In this case of the 5:2 commensurability with the motion of Jupiter, an asteroid can reach the orbit...
Trojan asteroids are small bodies orbiting around the L or L Lagrangian points of a Sun-planet syste...
In this paper, I construct a program to map the evolution of the potential in a planet-star system w...
We present a series of numerical integrations of observed and fictitious Jupiter Trojan asteroids, u...
In this paper, we focus on the stability of the Trojan asteroids for the planar restricted three-bod...
Trojan asteroids are minor planets that share the orbit of a planet about the Sun and librate around...