@Article{RoccoGonç:2017:SiTrDe,
author = "Rocco, Evandro Marconi and Gon{\c{c}}alves, Liana Dias",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Simulation of the trajectories described by a space vehicle around
the asteroid 243 Ida and its natural satellite Dactyl",
journal = "Journal of Physics: Conference Series",
year = "2017",
volume = "911",
pages = "012019",
abstract = "The asteroid 243 Ida located in the asteroid belt, between Mars
and Jupiter, is the fourth largest asteroid of the Koronis
asteroid family, with an average diameter of 31.3 km and a mass
around 4.2×1016 kg, and a small moon, Dactyl. In order to study
the dynamics of this system, orbital trajectories are simulated
around Ida considering, besides the gravitational attraction of
Dactyl, the non-central gravitational field of the asteroid,
defined by a polyhedral model that defines the shape and the
non-uniform mass distribution of the body. In this way, the
magnitude and the behaviour of such forces, and also their
influence on the orbital elements that define the trajectory of
the space vehicle, are evaluated and analysed.",
doi = "10.1088/1742-6596/911/1/012019",
url = "http://dx.doi.org/10.1088/1742-6596/911/1/012019",
issn = "1742-6588",
language = "en",
targetfile = "rocco_simulation.pdf",
urlaccessdate = "27 abr. 2024"
}