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Estudo de formação de satélites regulares de planetas gigantes usando integração numérica hidrodinâmica bidimensional com perturbação da estrela
(Universidade Estadual Paulista (Unesp), 2018-03-28)
A formação de satélites em um disco circumplanetário é tida como sendo similar a formação de planetas em um disco protoplanetário, especialmente super Terras rochosas. Dessa forma, é possível utilizar sistemas com satélites ...
Study of optical properties and spatial distribution of cirrus clouds over S??o Paulo, Brazil, using CALIPSO level 2 data
(Universidad de Magallanes, 2022)
The 'breaking the chains' migration model for super-Earth foation: The effect of collisional fragmentation
(2022-01-01)
Planets between 1 and 4 R (Earth radius) with orbital periods <100 d are strikingly common. The migration model proposes that super-Earths migrate inwards and pile up at the disc inner edge in chains of mean motion resonances. ...
The eccentricity distribution of giant planets and their relation to super-Earths in the pebble accretion scenario
(2020-11-01)
Observations of the population of cold Jupiter planets (r >1 AU) show that nearly all of these planets orbit their host star on eccentric orbits. For planets up to a few Jupiter masses, eccentric orbits are thought to be ...
Orbital propagation for Brazilian satellites using NORAD models
(Elsevier B.V., 2014)