Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt (2002)
- Authors:
- USP affiliated authors: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- DOI: 10.1006/icar.2002.6871
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
MICHTCHENKO, Tatiana Alexandrovna et al. Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt. Icarus, v. 158, p. 343-359, 2002Tradução . . Disponível em: https://doi.org/10.1006/icar.2002.6871. Acesso em: 03 mar. 2026. -
APA
Michtchenko, T. A., Lazzaro, D., Ferraz-Mello, S., & Roig, F. (2002). Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt. Icarus, 158, 343-359. doi:10.1006/icar.2002.6871 -
NLM
Michtchenko TA, Lazzaro D, Ferraz-Mello S, Roig F. Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt [Internet]. Icarus. 2002 ; 158 343-359.[citado 2026 mar. 03 ] Available from: https://doi.org/10.1006/icar.2002.6871 -
Vancouver
Michtchenko TA, Lazzaro D, Ferraz-Mello S, Roig F. Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt [Internet]. Icarus. 2002 ; 158 343-359.[citado 2026 mar. 03 ] Available from: https://doi.org/10.1006/icar.2002.6871 - 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
- 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
- Symmetric and asymmetric quasi satellite orbits in the planetary three-body problem
Informações sobre o DOI: 10.1006/icar.2002.6871 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
