Zobrazeno 1 - 10
of 83
pro vyhledávání: '"Gomes, Rodney"'
Autor:
de Sousa, Rafael Ribeiro, Morbidelli, Alessandro, Gomes, Rodney, Neto, Ernesto Vieira, Izidoro, Andre, Alves, Abreuçon Atanasio
The Dwarf Planet Ceres revealed the presence of ammonia and other unique properties compared to other asteroids in the main belt which suggests that it was not formed in situ. We model the early dynamical evolution of the outer Solar System to study
Externí odkaz:
http://arxiv.org/abs/2202.09238
Autor:
Gomes, Rodney
The Classical Kuiper Belt is populated by a group of objects with low inclination orbits, reddish colors and usually belonging to a binary system. This so called Cold Classical Kuiper Belt is considered to have been formed in situ from primordial ice
Externí odkaz:
http://arxiv.org/abs/2009.12489
Autor:
de Sousa, Rafael Ribeiro, Morbidelli, Alessandro, Raymond, Sean N., Izidoro, Andre, Gomes, Rodney, Neto, Ernesto Vieira
Publikováno v:
ICARUS cite as https://doi.org/10.1016/j.icarus.2019.113605
The dynamical structure of the Solar System can be explained by a period of orbital instability experienced by the giant planets. While a late instability was originally proposed to explain the Late Heavy Bombardment, recent work favors an early inst
Externí odkaz:
http://arxiv.org/abs/1912.10879
Autor:
Banda-Huarca, Martin, Camargo, Julio, Desmars, Josselin, Ogando, Ricardo, Vieira-Martins, Roberto, Assafin, Marcelo, da Costa, Luiz, Bernstein, Gary, Kind, Matias Carrasco, Wagner, Alex Drlica, Gomes, Rodney, Gysi, Matheus, Ribas, Felipe Braga, Maia, Marcio, Gerdes, David, Hamilton, Stephanie, Wester, William, Abbot, Tim, Abdalla, Filipe, Allam, Sahar, Avila, Santiago, Bertin, Emmanuel, Brooks, David, Buckley-Geer, Elizabeth, Burke, David, Rossell, Aurelio Carnero, Carretero, Jorge, Cunha, Carlos, Davis, Christopher, de Vicente, Juan, Diehl, Thomas, Doel, Peter, Fosalba, Pablo, Frieman, Josh, Garcia-Bellido, Juan, Gaztanaga, Enrique, Gruen, Daniel, Gruendl, Robert, Gschwend, Julia, Gutierrez, Gaston, Hartley, Will, Hollowood, Devon, Honscheid, Klaus, James, David, Kuehn, Kyler, Kuropatkin, Nikolay, Menanteau, Felipe, Miller, Christopher, Miquel, Ramon, Plazas, Andres, Romer, Kathy, Sanchez, Eusebio, Scarpine, Vic, Schubnell, Michael, Serrano, Santiago, Sevilla, Ignacio, Smith, Mathew, Soares-Santos, Marcelle, Sobreira, Flavia, Suchyta, Eric, Swanson, Molly, Tarle, Gregory
Transneptunian objects (TNOs) are a source of invaluable information to access the history and evolution of the outer solar system. However, observing these faint objects is a difficult task. As a consequence, important properties such as size and al
Externí odkaz:
http://arxiv.org/abs/1811.10724
The link between the dynamical evolution of the giant planets and the Kuiper Belt orbital structure can provide clues and insight about the dynamical history of the Solar System. The classical region of the Kuiper Belt has two populations (the cold a
Externí odkaz:
http://arxiv.org/abs/1808.02146
Autor:
Cáceres, Jessica, Gomes, Rodney
The hypothesis of an additional planet in the outer Solar System has gained new support as a result of the confinement noted in the angular orbital elements of distant trans-Neptunian objects. Orbital parameters proposed for the external perturber su
Externí odkaz:
http://arxiv.org/abs/1808.01248
Autor:
Deienno, Rogerio, Izidoro, Andre, Morbidelli, Alessandro, Gomes, Rodney S., Nesvorny, David, Raymond, Sean N.
The main asteroid belt (MB) is low in mass but dynamically excited. Here we propose a new mechanism to excite the MB during the giant planet ('Nice model') instability, which is expected to have featured repeated close encounters between Jupiter and
Externí odkaz:
http://arxiv.org/abs/1808.00609
Autor:
Ribeiro de Sousa, Rafael, Morbidelli, Alessandro, Gomes, Rodney, Neto, Ernesto Vieira, Izidoro, Andre, Alves, Abreuçon Atanasio
Publikováno v:
In Icarus June 2022 379
The origin of the orbital structure of the cold component of the Kuiper belt is still a hot subject of investigation. Several features of the solar system suggest that the giant planets underwent a phase of global dynamical instability, but the actua
Externí odkaz:
http://arxiv.org/abs/1710.05178