Collisions with the Earth: the Moon's contribution


Autoria(s): Domingos, R. C.; Winter, O. C.; Neto, E.; Jenniskens, P.; Cellino, A. Q.; Price, S.
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