Orbits of near-earth asteroid triples 2001 SN263 and 1994 CC: properties, origin, and evolution
Three-body model fits to Arecibo and Goldstone radar data reveal the nature of two near-
Earth asteroid triples. The triple-asteroid system 2001 SN263 is characterized by a primary …
Earth asteroid triples. The triple-asteroid system 2001 SN263 is characterized by a primary …
Physical and dynamical properties of the main belt triple asteroid (87) Sylvia
We present the analysis of high angular resolution observations of the triple Asteroid (87)
Sylvia collected with three 8–10 m class telescopes (Keck, VLT, Gemini North) and the …
Sylvia collected with three 8–10 m class telescopes (Keck, VLT, Gemini North) and the …
Stability regions around the components of the triple system 2001 SN263
Abstract Space missions are an excellent way to increase our knowledge of asteroids. Near-
Earth asteroids (NEAs) are good targets for such missions, as they periodically approach the …
Earth asteroids (NEAs) are good targets for such missions, as they periodically approach the …
Evidence for differentiation of the most primitive small bodies
Context. Dynamical models of Solar System evolution have suggested that the so-called P-
and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit …
and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit …
A dynamical solution of the triple asteroid system (45) Eugenia
We present the first dynamical solution of the triple asteroid system (45) Eugenia and its two
moons Petit–Prince (diameter∼ 7km) and S/2004 (45) 1 (diameter∼ 5km). The two moons …
moons Petit–Prince (diameter∼ 7km) and S/2004 (45) 1 (diameter∼ 5km). The two moons …
Orbits, masses, and evolution of main belt triple (87) Sylvia
Sylvia is a triple asteroid system located in the main belt. We report new adaptive optics
observations of this system that extend the baseline of existing astrometric observations to a …
observations of this system that extend the baseline of existing astrometric observations to a …
Multiple asteroid systems (45) Eugenia and (87) Sylvia: sensitivity to external and internal perturbations
L Beauvalet, F Marchis - Icarus, 2014 - Elsevier
Satellites of asteroids are a widely used way to determine the masses and other dynamical
parameters of their systems. We make such a determination here, using data from the two …
parameters of their systems. We make such a determination here, using data from the two …
Free and forced inclinations of orbits perturbed by the central body's oblateness and an inclined third body
Q Zeng, Y Jiang, T Nie, X Liu - Celestial Mechanics and Dynamical …, 2024 - Springer
The effect of inclined third-body perturbation on the perturbed body's inclination evolution
has been investigated extensively. However, under various initial orbital elements, the exact …
has been investigated extensively. However, under various initial orbital elements, the exact …
Collisionally born family about 87 Sylvia
D Vokrouhlický, D Nesvorný, WF Bottke… - The Astronomical …, 2010 - iopscience.iop.org
There are currently more than 1000 multi-opposition objects known in the Cybele
population, adjacent and exterior to the asteroid main belt, allowing a more detailed analysis …
population, adjacent and exterior to the asteroid main belt, allowing a more detailed analysis …
Orbital stability near the (87) Sylvia system
The main goal of our work is to study the orbital dynamics of a spacecraft near the (87)
Sylvia system. Here, we consider a non-homogeneous mass distribution with a dense core …
Sylvia system. Here, we consider a non-homogeneous mass distribution with a dense core …