Gravitational perturbations correlated with the asteroid kinetic impact deflection technique

This paper presents the use of the kinetic impact technique to deflect asteroids that may present some risk of collision with Earth. Within the work to be developed here, we intend to evaluate in more detail the possibility to deflect the orbit of the asteroid 101955 Bennu by applying variations in its velocity (Δ v) at different positions along its orbital period and measuring effects of close encounters with planet Earth. We will see that, in a relatively long period of time, the asteroid has several close encounters with the planet, thus suffering a natural gravitational perturbation. With the application of the impulses, the relative distances change, causing variations in the energy of the asteroid and a large variation in the relative distance between the asteroid and Earth over a long period after the impulse. We present results related to the magnitude of the impulse applied, which is important because its defines the mass and velocity of the impactor to be considered. Then, we mapped the positions of the impulses along a period of the orbit of the asteroid. We finish by explaining what happens to the orbit of the asteroid during the periods of gravitational perturbation, since the close encounters amount to “Swing Bys” that intensify the variations of the relative distances between the bodies after the impulse is applied. © 2022, The Author(s).

Authors
Chagas B.S. , Prado A.F.B.A. , Winter O.C.
Publisher
Nature Publishing Group
Issue number
1
Language
English
State
Published
Number
11721
Volume
12
Year
2022
Organizations
  • 1 Grupo de Dinâmica Orbital e Planetologia, São Paulo State University (UNESP), SP, Guaratinguetâ, Brazil
  • 2 Academy Engineering, RUDN University Miklukho-Maklaya, Street 6, Moscow, 117198, Russian Federation
  • 3 INPE: National Institute for Space Research, SP, São Josẽ dos Campos, Brazil
Keywords
article; astronomy
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