Context. Close encounters with (1) Ceres and (4) Vesta, the two most massive bodies in the main belt, are known to be a mechanism of dynamical mobility able to significantly alter proper elements of minor bodies, and they ...

Context. Close encounters with (1) Ceres and (4) Vesta, the two most massive bodies in the main belt, are known to be a mechanism of dynamical mobility able to significantly alter proper elements of minor bodies, and they ...

Neste trabalho, apresentamos um estudo sobre a formação dos satélites irregulares de Júpiter por meio da captura gravitacional de asteróides binários. Analisamos as condições de ruptura/captura para um dos membros de um ...

Neste trabalho, apresentamos um estudo sobre a formação dos satélites irregulares de Júpiter por meio da captura gravitacional de asteróides binários. Analisamos as condições de ruptura/captura para um dos membros de um ...

In this paper we search for photometric data of asteroids in the outer region of the Hecuba gap in the Moving Object Catalogue of the Sloan Digital Sky Survey to find the spectrophotometric characteristics of small members ...

Asteroid families are groups of asteroids that are identifiable in domains of proper elements. They may be the outcome of a collision, or the product of rotational fission. Among collisional families, young asteroid families ...