| Revista: | Computational & applied mathematics |
| Base de datos: | PERIÓDICA |
| Número de sistema: | 000267935 |
| ISSN: | 1807-0302 |
| Autors: | Domingos, R. C1 Winter, O. C2 |
| Institucions: | 1Instituto Nacional de Pesquisas Espaciais, Sao Jose dos Campos, Sao Paulo. Brasil 2Universidade Estadual Paulista "Julio de Mesquita Filho", Grupo de Dinamica Orbital e Planetologia, Guaratingueta, Sao Paulo. Brasil |
| Any: | 2005 |
| Període: | Ene-Abr |
| Volum: | 24 |
| Número: | 1 |
| Paginació: | 99-107 |
| País: | Brasil |
| Idioma: | Inglés |
| Tipo de documento: | Artículo |
| Enfoque: | Analítico, descriptivo |
| Resumen en inglés | Considering hypothetical co-orbital asteroids with the Earth, Tatum (1997) presented a study about the necessary radial distance in order to produce collision. He adopted an analysis considering a composition of circular two-body systems, Sun-Earth and Sun-Asteroid. He found that asteroids with radial positions between 0.9943 and 1.0057 AU would necessarily collide with the Earth. In the present work, we show that this problem cannot be treated in this way. Adopting the circular restricted three-body problem, we verified that asteroids in the supposed region of collision with the Earth have stable horseshoe trajectories. Therefore, in the co-orbital region the dynamical system has to be studied as a restricted three-body problem since the composition of two-body problems gives a misleading result |
| Disciplines | Matemáticas, Física y astronomía |
| Paraules clau: | Matemáticas aplicadas, Astronomía, Asteroides, Colisiones, Distancia radial, Planeta Tierra, Modelos matemáticos |
| Keyword: | Mathematics, Physics and astronomy, Applied mathematics, Astronomy, Asteroids, Collisions, Radial distance, Earth planet, Mathematical models |
| Text complet: | Texto completo (Ver HTML) |
