Modeling the 5: 2 mean-motion resonance in the Jupiter-Saturn Planetary System (2001)
- Authors:
- USP affiliated authors: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- Assunto: SISTEMA SOLAR
- Language: Inglês
- Imprenta:
- Source:
-
ABNT
MICHTCHENKO, Tatiana Alexandrovna e FERRAZ-MELLO, Sylvio. Modeling the 5: 2 mean-motion resonance in the Jupiter-Saturn Planetary System. Icarus, v. 149, p. 357-374, 2001Tradução . . Acesso em: 21 maio 2024. -
APA
Michtchenko, T. A., & Ferraz-Mello, S. (2001). Modeling the 5: 2 mean-motion resonance in the Jupiter-Saturn Planetary System. Icarus, 149, 357-374. -
NLM
Michtchenko TA, Ferraz-Mello S. Modeling the 5: 2 mean-motion resonance in the Jupiter-Saturn Planetary System. Icarus. 2001 ; 149 357-374.[citado 2024 maio 21 ] -
Vancouver
Michtchenko TA, Ferraz-Mello S. Modeling the 5: 2 mean-motion resonance in the Jupiter-Saturn Planetary System. Icarus. 2001 ; 149 357-374.[citado 2024 maio 21 ] - Planetary masses and orbital parameters from radial velocity measurements
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- Detectability and error estimation in orbital fits of resonant extrasolar planets
- Retrato dinâmico do cinturão asteroidal interior
- Detectability and error estimation in orbital fits of resonant extrasolar planets
- Dynamics of two planets in the 2:1 and 3:2 mean motion resonances
- On the depletion of the Hecuba gap in the asteroidal belt
- 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: II. systems with a more massive inner planet
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