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The sailboat island and the New Horizons trajectory
(Elsevier B.V., 2015)
Relaxation-chaos phenomena in celestial mechanics. I. On wisdom's model for the 3/1 kirkwood gap
(1987-05-01)
Sudden eccentricity increases of asteroidal motion in 3/1 resonance with Jupiter were discovered and explained by J. Wisdom through the occurrence of jumps in the action corresponding to the critical angle (resonant ...
Chaotic diffusion caused by close encounters with several massive asteroids The (4) Vesta case
(Edp Sciences S A, 2012-07-01)
Context. Close encounters with massive asteroids are known to be a mechanism of dynamical mobility that can significantly alter proper elements of minor bodies, and they are the main source of dynamical mobility for ...
Resonance capture at arbitrary inclination
(Oxford Univ Press, 2015)
Dynamical evolution of V-type asteroids in the central main belt
(Oxford University Press, 2014)
Stable retrograde orbits around the triple system 2001 SN263
(Oxford Univ Press, 2015)
The stable archipelago in the region of the Pallas and Hansa dynamical families
(Wiley-Blackwell, 2010-10-11)
Among highly inclined asteroids, the region of the central main belt between the 3J:-1A and 5J:-2A mean-motion resonances has long been known to host the Pallas and Hansa dynamical families. This region is characterized ...
Secular dynamics and family identification among highly inclined asteroids in the Euphrosyne region
(Wiley-Blackwell, 2012-02-01)
Among highly inclined asteroids the external region of the main belt beyond the 5J:2A mean-motion resonance with Jupiter has long been known to host the Euphrosyne and Alauda families. The region is confined in semimajor ...
A possible stellar metallic enhancement in post-T Tauri stars by a planetesimal bombardment
(Blackwell Publishing, 2007-07-11)
The photospheres of stars hosting planets have larger metallicity than stars lacking planets. This could be the result of a metallic star contamination produced by the bombarding of hydrogen-deficient solid bodies. In the ...