Zobrazeno 1 - 10
of 16
pro vyhledávání: '"D. C. Mourão"'
Exomoons are a missing piece of exoplanetary science. Recently, two promising candidates were proposed, Kepler-1625 b-I and Kepler-1708 b-I. While the latter still lacks a dynamical analysis of its stability, Kepler-1625 b-I has already been the subj
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e0eee69f1bf43fe223d06e0a058bc729
http://arxiv.org/abs/2301.10730
http://arxiv.org/abs/2301.10730
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2022-05-01T08:15:10Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-09-01 Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) Recent observations of stellar occultations have revealed rings of pa
Autor:
R. Vilhena de Moraes, J. P. S. Carvalho, D. C. Mourão, Antonio F. B. A. Prado, Othon C. Winter
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2018-12-11T17:29:44Z (GMT). No. of bitstreams: 0 Previous issue date: 2016-10-01 An exoplanet, or extrasolar planet, is a planet that does not orbit the Sun, but is around a different star, stellar remnant, or brown dwarf.
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2018-12-11T16:53:05Z (GMT). No. of bitstreams: 0 Previous issue date: 2018-04-21 The G ring arc hosts the smallest satellite of Saturn, Aegaeon, observed with a set of images sent by Cassini spacecraft. Along with Aegaeon,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2698ad12b56505240e9b815e8263bb3
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 430:2761-2767
Impacts of micrometeoroids on the surfaces of the plutonian small satellites Nix and Hydra can generate dust particles. Even in this region so far from the Sun these tiny ejected particles are under the effects of the solar radiation pressure. In thi
Autor:
D. C. Mourão, Antonio F. B. A. Prado, Othon C. Winter, J. P. S. Carvalho, R. Vilhena de Moraes
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2018-12-11T17:26:47Z (GMT). No. of bitstreams: 0 Previous issue date: 2016-01-01 Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8f028ba398b319f016fb20e2f17360f6
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 380:L54-L57
Since the Voyager flybys, embedded moonlets have been proposed to explain some of the surprising structures observed in Saturn's narrow F ring. Experiments conducted with the Cassini spacecraft support this suggestion. Images of the F ring show brigh
Publikováno v:
Physica D: Nonlinear Phenomena. 225:112-118
In the present work we analyse the behaviour of a particle under the gravitational influence of two massive bodies and a particular dissipative force. The circular restricted three body problem, which describes the motion of this particle, has five e
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Context: Co-orbital systems are bodies that share the same mean orbit. They can be divided into different families according to the relative mass of the co-orbital partners and the particularities of their movement. Janus and Epimetheus are unique in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d9a48faafc9e17b394473b2851a58ed
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 372:1614-1620
In the present work, we study the stability of hypothetical satellites that are coorbital with Enceladus and Mimas. We performed numerical simulations of 50 particles around the triangular Lagrangian equilibrium points of Enceladus and Mimas taking i