Kirkwood Gaps are gaps in the distribution of asteroid orbital periods which correspond to orbital resonances between Jupiter and the asteroids. Simplified explanations account for this effect by saying that Jupiter pulls on the asteroid at the same location each orbit, pulling it into a new orbit. However, in simulations what is found is simply an oscillation, with the orbital distance and eccentricity of the objects orbit never rising to a breaking point of the orbit. More detailed explanations are often summarized as “Chaos Theory”, which gives no intuitive idea of the actual cause. The goal of my research is to provide a pedagogical look at Kirkwood Gaps utilizing multiple levels of complexity to describe the origins of Kirkwood gap...
The formation of the Hecuba gap close to the 2:1 resonant asteroid mean motion with Jupiter is exami...
The collisional process between small bodies is one of the key processes in the formation and evolut...
extensive set of trajectories in both resonances. Moreover, we have included the 4/3 resonance in ou...
The problem of the Kirkwood gaps in the asteroid belt has introgued astronomers and mechanicians for...
Abstract. The study of the many body problem associated to the dynamics of the different elements of...
We study the evolution of asteroid orbits in a restricted threebody problem formulation consisting...
International audienceWe study the dynamics of the restricted planar three-body problem near mean mo...
The Hilda group is a collection of asteroids located in the asteroid belt between Mars and Jupiter t...
In this case of the 5:2 commensurability with the motion of Jupiter, an asteroid can reach the orbit...
International audienceThe asteroid belt is characterized by an extreme low total mass of material on...
In a previous paper we simulated the orbital evolution of dust particles from the Jupiter Trojan ast...
A comparative study of the evolution of the Sun–Jupiter–Asteroid system near the 4:1 and 7:2 resona...
International audienceContext. Statistical analysis of the orbits of distant Kuiper belt objects (KB...
Although analytical studies on the secular motion of the irregular satellites have been published re...
Kirkwood (Daniel). — The asteroids, or minor planets between Mars and Jupiter. Philadelphia, 1888. I...
The formation of the Hecuba gap close to the 2:1 resonant asteroid mean motion with Jupiter is exami...
The collisional process between small bodies is one of the key processes in the formation and evolut...
extensive set of trajectories in both resonances. Moreover, we have included the 4/3 resonance in ou...
The problem of the Kirkwood gaps in the asteroid belt has introgued astronomers and mechanicians for...
Abstract. The study of the many body problem associated to the dynamics of the different elements of...
We study the evolution of asteroid orbits in a restricted threebody problem formulation consisting...
International audienceWe study the dynamics of the restricted planar three-body problem near mean mo...
The Hilda group is a collection of asteroids located in the asteroid belt between Mars and Jupiter t...
In this case of the 5:2 commensurability with the motion of Jupiter, an asteroid can reach the orbit...
International audienceThe asteroid belt is characterized by an extreme low total mass of material on...
In a previous paper we simulated the orbital evolution of dust particles from the Jupiter Trojan ast...
A comparative study of the evolution of the Sun–Jupiter–Asteroid system near the 4:1 and 7:2 resona...
International audienceContext. Statistical analysis of the orbits of distant Kuiper belt objects (KB...
Although analytical studies on the secular motion of the irregular satellites have been published re...
Kirkwood (Daniel). — The asteroids, or minor planets between Mars and Jupiter. Philadelphia, 1888. I...
The formation of the Hecuba gap close to the 2:1 resonant asteroid mean motion with Jupiter is exami...
The collisional process between small bodies is one of the key processes in the formation and evolut...
extensive set of trajectories in both resonances. Moreover, we have included the 4/3 resonance in ou...