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Analysis of the secular problem for triple star systems
(2013-01-01)
The long-term dynamics of the three-body problem is studied. The goal is to study the motion of a planet (m1) around a star (m0) that is perturbed by a third-body (m2) (a planet or a brown dwarf star). The gravitational ...
Dynamic portrait of the planetary 2/1 mean-motion resonance - I. Systems with a more massive outer planet
(WILEY-BLACKWELL, 2008)
We analyse the global structure of the phase space of the planar planetary 2/1 mean-motion resonance in cases where the outer planet is more massive than its inner companion. Inside the resonant domain, we show the existence ...
A new insight into the Galactic potential: A simple secular model for the evolution of binary systems in the solar neighbourhood
(EDP Sciences, 2017-04)
Context. Among the main effects that the Milky Way exerts in binary systems, the Galactic tide is the only one that is not probabilistic and can be deduced from a potential. Therefore, it is possible to perform an analysis ...
Possible effects of secular resonances in Phobos and Triton
(Elsevier B.V., 2002-01-01)
Due to the tides, the orbits of Phobos and Triton are contracting. While their semi major axes are decreasing, several possibilities of secular resonances involving node, argument of the pericenter and mean motion of the ...
Possible effects of secular resonances in Phobos and Triton
(Elsevier B.V., 2002-01-01)
Due to the tides, the orbits of Phobos and Triton are contracting. While their semi major axes are decreasing, several possibilities of secular resonances involving node, argument of the pericenter and mean motion of the ...
Relating The South Atlantic Anomaly And Geomagnetic Flux Patches
(Elsevier B.V., 2017)
Análisis dinámico del grupo de asteroides Hungaria
(2019)
Entre el planeta Marte y el borde interno del cinturón principal de asteroides se encuentra la región de asteroides Hungaria (1,77 UA < a < 2,06 UA). Estos objetos se hallan rodeados por las resonancias seculares ν5 , ν6 ...
Ação de forças gravitacionais e não gravitacionais sobre o movimento orbital de satélites artificiais
(Universidade Estadual Paulista (Unesp), 2007-04)
Uma teoria para estudar o movimento orbital de satélites artificiais sobre efeitos do arrasto atmosférico e da pressão de radiação solar direta - considerando a sombra da Terrae alguns termos do geopotencial - é desenvolvida ...
Ação de forças gravitacionais e não gravitacionais sobre o movimento orbital de satélites artificiais
(Universidade Estadual Paulista (Unesp), 2007-04)
Uma teoria para estudar o movimento orbital de satélites artificiais sobre efeitos do arrasto atmosférico e da pressão de radiação solar direta - considerando a sombra da Terrae alguns termos do geopotencial - é desenvolvida ...