A new analysis of the GJ581 extrasolar planetary system (2012)
- Authors:
- USP affiliated authors: MELLO, SYLVIO FERRAZ DE - IAG ; MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- Unidade: IAG
- Subjects: PLANETAS; MECÂNICA CELESTE
- Language: Inglês
- Imprenta:
- Publisher: Sociedade Astronômica Brasileira
- Publisher place: São Paulo
- Date published: 2012
- Conference titles: Reunião Anual da Sociedade Astronômica Brasileira
-
ABNT
SANTOS, Marcos Tadeu dos et al. A new analysis of the GJ581 extrasolar planetary system. 2012, Anais.. São Paulo: Sociedade Astronômica Brasileira, 2012. . Acesso em: 03 mar. 2026. -
APA
Santos, M. T. dos, Silva, G. G. da, Ferraz-Mello, S., & Michtchenko, T. A. (2012). A new analysis of the GJ581 extrasolar planetary system. In . São Paulo: Sociedade Astronômica Brasileira. -
NLM
Santos MT dos, Silva GG da, Ferraz-Mello S, Michtchenko TA. A new analysis of the GJ581 extrasolar planetary system. 2012 ;[citado 2026 mar. 03 ] -
Vancouver
Santos MT dos, Silva GG da, Ferraz-Mello S, Michtchenko TA. A new analysis of the GJ581 extrasolar planetary system. 2012 ;[citado 2026 mar. 03 ] - Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects
- On the V-type asteroids outside the Vesta family I. Interplay of nonlinear secular resonances and the Yakovsky effect: the cases of 956 Elisa and 809 Lundia
- Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt
- Dynamic portrait of the planetary 2/1 mean-motion resonace: I. systems with a more massive outer planet
- Dynamics of two planets in the 2:1 and 3:2 ressonances
- Resonant Structure of the outer solar system in the neighborhood of the planets
- Determinação da órbita de exoplanetas com inferência estatística
- Study of diffusive phenomena within 2/1 and 3/2 asteroidal resonances
- Determination of dynamical and physical parameters of the system CoRoT 3
- The role of close encounters with (4) Vesta in the origin of the basaltic NEAs
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
