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 assinatura
- Este artigo NÃO é de acesso aberto
- Cor do Acesso Aberto: closed
-
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: 14 jan. 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 jan. 14 ] 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 jan. 14 ] Available from: https://doi.org/10.1006/icar.2002.6871 - Tidal evolution of a close-in planet with a more massive outer companion
- Orbital evolution of asteroids in the hecuba gap
- Evolution of migrating planet pairs in resonance
- Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12
- Modeling close encouters with massive asteroids: a Markovian approach. An aplication to the Vesta family
- Stationary orbits in resonant extrasolar planetary systems
- Resonances and stability of extra-solar planetary systems
- The role of close encounters with (4) Vesta in the origin of the basaltic NEAs
- Secular behavior of a pair of coplanar planets
- Modeling the 3-D secular planetary three-body problem discussion on the outer 'úpsilon' Andromedae planetary system
Informações sobre o DOI: 10.1006/icar.2002.6871 (Fonte: oaDOI API)
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