Collisions with the Earth: the Moon's contribution
Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
---|---|
Data(s) |
20/05/2014
20/05/2014
01/01/2004
|
Resumo |
In the present work is analyzed the contribution of the Moon on the collisional process of the Earth with asteroids (NEOs). The dynamical system adopted is the restricted four-body problem Sun-Earth-Moon-particle. Using a simple analytical approach one can verify that, the orbit of an object can be significantly affected by the Moon's gravitational field when their relative velocity is smaller than 5 km/s. Therefore, the present work is based on hypothetical asteroids whose velocities relative to Moon are of the order of 1 km/s. In fact, there are several real objects (NEOs) with such velocities at the point they cross the Earth's orbit. The net results obtained indicate that the Moon helps to avoid collisions (2.6%) more than it contributes to extra collisions (0.6%). (C) 2003 COSPAR. Published by Elsevier Ltd. All rights reserved. |
Formato |
1534-1538 |
Identificador |
http://dx.doi.org/10.1016/S0273-1177(03)00459-9 Impact of Minor Bodies of Our Solar System on Planets and Their Middle and Upper Atmosphere. Kidlington: Pergamon-Elsevier B.V., v. 33, n. 9, p. 1534-1538, 2004. 0273-1177 http://hdl.handle.net/11449/39327 10.1016/S0273-1177(03)00459-9 WOS:000222364500014 |
Idioma(s) |
eng |
Publicador |
Elsevier B.V. |
Relação |
Impact of Minor Bodies of Our Solar System on Planets and Their Middle and Upper Atmosphere |
Direitos |
closedAccess |
Tipo |
info:eu-repo/semantics/article |