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Three-dimensional retrograde periodic orbits of asteroids moving in mean motion resonances with Jupiter
(2022-01-01)
We study the dynamics of interior mean motion resonances of first, second and third order with Jupiter using the model of the restricted three-body problem with the Sun and Jupiter as primaries and we focus on asteroids ...
Results of the investigation of the asteroid (2121) Sevastopol based on photometric observations of mutual phenomena
(Pergamon-Elsevier Science Ltd, 2019-05)
The asteroid (2121) Sevastopol is a binary asteroid from the main belt. The duplicity of the asteroid was discovered based on photometric observations of mutual phenomena (eclipses and occultations) that were detected in ...
Asteroids' Size Distribution and Colors from HITS
(IOP, 2020)
We report the observations of solar system objects during the 2015 campaign of the High cadence Transient Survey (HiTS). We found 5740 bodies (mostly Main Belt asteroids), 1203 of which were detected in different nights ...
The resonant population of asteroids in librating states of the υ6 linear secular resonance
(2018-12-01)
We discuss the asteroid population evolving close by or into the υ6 secular resonance in the main asteroid belt. Using the analytical method of Yoshikawa, we estimate the actual domain of the υ6 resonance, which currently ...
Dynamical evolution of V-type asteroids in the central main belt
(Oxford University Press, 2014)
Morphological properties determination of main belt asteroids
(Instituto Nacional de Astrofísica, Óptica y Electrónica., 2019)
PECULIAR EUPHROSYNE
(Iop Publishing Ltd, 2014-09-01)
The asteroid (31) Euphrosyne is the largest body of its namesake family, and it contains more than 99% of the family mass. Among large asteroid families, the Euphrosyne group is peculiar because of its quite steep ...
The influence of Ceres on the dynamical evolution of the Zdenekhorsky/Nemesis asteroid family
(2019-01-01)
The Nemesis family, also identified as the Zdenekhorsky family by some authors, is an “incomplete” asteroid family in the central main belt, characterized by an asymmetric distribution between its left and right side, with ...