CV Lattes
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Ministério da Ciência, Tecnologia e Inovação (Brasil). Instituto Nacional de Pesquisas Espaciais (INPE) (Institutional affiliation from the last research proposal) Birthplace: Brazil
Research Scientist at Southwest Research Institute (SwRI - Boulder/CO, 2017-Present). Pos-doctorate at Instituto de Pesquisas Espaciais (2014-2017). Pos-doctorate fellow at Observatories de la Côte d'Azur, Nice, France (2016). PhD in Engineering and Space Technology at the Instituto Nacional de Pesquisas Espaciais (2014) with split-site PhD (as intern) at Southwest Research Institute - Boulder/CO (05/2013-11/2013). Holds a Master in Physics in the area of Applied Physics at the Universidade Estadual Paulista Júlio de Mesquita Filho (2010), Bachelor Degree in Physics from the Universidade Estadual Paulista Júlio de Mesquita Filho (2008) and graduated in Full Degree in Physics from the Universidade Estadual Paulista Júlio de Mesquita Filho (2007). Has experience in the field of Astronomy, with emphasis on Celestial Mechanics and Dynamical Astronomy. (Source: Lattes Curriculum)
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It is commonly accepted that the Asteroid Belt was formed by the partial agglutination of solid material available in that region, which was halted before the formation of a planet, due to the simultaneous appearance of Jupiter. However, for a more complete understanding of the scenario of asteroids formation, one must also take into account their characteristics and implications for the …
In the Nice Model (Tsiganis et al, 2005) there is a consensus that the regular satellites are primordial and resisted the migration, while the irregular ones were captured a posteriori or during the migration. Although this never was tested in a rigorous way, in Deienno (2010), Deienno et al (2010), this problem was exaustively studied in the case of Uranus system. What is observed is th…
The planetary instability, as proposed by the most recent model of planetary migration, known as jumping-Jupiter, can explain many features of the evolution of the giants planets. This instability is characterized by the fact that the giants planets in the outer solar system, formed in a multi-resonant orbital configuration, underwent several close encounters with one another, after being…
In the Nice model (Tsiganis et al 2005 - NiceI) it is accepted that the regular satellites survived to the planetary migration and the irregulars were captured after or during the migration itself. Nesvorný et al 2007 studied the capture process of irregular satellites during the phase of the planetary close encounters. In this work, the authors can successfully explain how Uranus and Nep…
| 3 / 2 | Completed scholarships in Brazil |
| 2 / 2 | Completed scholarships abroad |
| 5 / 4 | All Scholarships |
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