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Scattering V-type asteroids during the giant planet instability: a step for Jupiter, a leap for basalt
(Oxford Univ Press, 2017-06-01)
V-type asteroids are a taxonomic class whose surface is associated with a basaltic composition. The only known source of V-type asteroids in the Main Asteroid Belt is (4) Vesta, which is located in the inner part of the ...
Dynamic portrait of the region occupied by the Hungaria asteroids: the influence of Mars
(Oxford University Press, 2018-06)
The region occupied by the Hungaria asteroids has a high-dynamical complexity. In this paper, we analyse the main dynamic structures and their influence on the known asteroids through the construction of maps of initial ...
Excitation of a Primordial Cold Asteroid Belt as an Outcome of Planetary Instability
(Iop Publishing Ltd, 2018-09-01)
The main asteroid belt (MB) is low in mass but dynamically excited. Here we propose a new mechanism to excite the MB during the giant planet (the Nice model) instability, which is expected to feature repeated close encounters ...
APOPHIS - effects of the 2029 Earth's encounter on the surface and nearby dynamics (vol 510, pg 95, 2022)
(Oxford Univ Press, 2022-02-24)
Mapping stable direct and retrograde orbits around the triple system of asteroids (45) Eugenia
(2017-12-01)
It is widely accepted that knowing the composition and the orbital evolution of asteroids might help us to understand the process of formation of the Solar system. It is also known that asteroids can represent a threat to ...
Exploring S-type orbits in the Pluto-Charon binary system
(Wiley-Blackwell, 2010-05-01)
This work generates, through a sample of numerical simulations of the restricted three-body problem, diagrams of semimajor axis and eccentricity which defines stable and unstable zones for particles in S-type orbits around ...
Exploring S-type orbits in the Pluto-Charon binary system
(Wiley-Blackwell, 2010-05-01)
This work generates, through a sample of numerical simulations of the restricted three-body problem, diagrams of semimajor axis and eccentricity which defines stable and unstable zones for particles in S-type orbits around ...
On the oldest asteroid families in the main belt
(2016-03-17)
Asteroid families are groups of minor bodies produced by high-velocity collisions. After the initial dispersions of the parent bodies fragments, their orbits evolve because of several gravitational and non-gravitational ...