Deflecting an Asteroid on a Collision Course with Earth Using a Powered Swing-By Maneuver

The deflection of potentially dangerous asteroids has been treated with great intensity and has gained more and more attention in scientific research. Different techniques are developed over the years. Among these techniques, we found the kinetic impact deflection technique to be the most viable at...

Full description

Bibliographic Details
Authors: Chagas, Bruno S. [UNESP], Prado, Antonio Fernando Bertachini de Almeida, Winter, Othon Cabo [UNESP]
Format: article
Status:Published version
Publication Date:2022
Country:Brasil
Institution:Universidade Estadual Paulista (UNESP)
Repository:Repositório Institucional da UNESP
Language:English
OAI Identifier:oai:repositorio.unesp.br:11449/242254
Online Access:http://dx.doi.org/10.3390/sym14081658
http://hdl.handle.net/11449/242254
Access Level:Open access
Keyword:asteroid collision
astrodynamics
deflect asteroids
planetary defense
swing by
Description
Summary:The deflection of potentially dangerous asteroids has been treated with great intensity and has gained more and more attention in scientific research. Different techniques are developed over the years. Among these techniques, we found the kinetic impact deflection technique to be the most viable at the moment. In this work we address the kinetic impact deflection technique, but in a scenario where we have a short time to deflect an asteroid that will collide with Earth. For this, we also use a maneuver similar to a powered gravity-assisted maneuver with Earth in a previous passage to change the trajectory of the asteroid to avoid the collision. We apply this technique in three scenarios: (i) impulse before the close encounter, (ii) impulse during the close encounter, and (iii) impulse after the close encounter. We observe that some trajectories are symmetric with respect to the line Sun–Earth, and others are asymmetric. We show that, using this technique, it is possible to change the trajectory of the asteroid, even in a short period, to avoid the collision without using a large variation of velocity in the orbit of the asteroid.