TY - GEN
T1 - Analysis of The Asteroid Deflection Effect Considering Impact Uncertainties
AU - Yang, Xiaomin
AU - Zhang, Jianying
AU - Zhang, Feng
AU - Qia, Dong
AU - Li, Xiangyu
N1 - Publisher Copyright:
© Press of Acta Aeronautica et Astronautica Sinica 2026.
PY - 2026
Y1 - 2026
N2 - The potential hazard of asteroids on the impact of Earth has drawn increasing attention in recent years. The instantaneous moment alteration via impact is the most feasible deflection technique. However, there are a number of factors that influence the impact of progress. Some of them are still not understood, which causes a large uncertainty of the change of velocity after impact and affects the performance of orbit deflection. In this work, we investigate the effects of planetary perturbation and orbital uncertainty on the defense effectiveness of kinetic energy impact missions. Based on the real ephemeris model, a dynamic model considering the gravitational perturbation of many bodies is established. A virtual asteroid orbit with Earth impact characteristics is constructed by the inverse orbit integration method. the state transition tensor (STT) method is employed to calculate the influence of the impact direction uncertainty on orbit deflection. Research results demonstrate that the optimal asteroid impact moment appears in perihelion, which not only enhances orbital dis-placement but also suppresses perturbations in deflection outcomes induced by velocity direction errors. Crucially, our study also reveals that close planets flyby after impact will also influence the deflection performance significantly. This suggests that specialized orbital analysis of such gravitational interactions is necessary in actual mission design to ensure a reliable defense strategy.
AB - The potential hazard of asteroids on the impact of Earth has drawn increasing attention in recent years. The instantaneous moment alteration via impact is the most feasible deflection technique. However, there are a number of factors that influence the impact of progress. Some of them are still not understood, which causes a large uncertainty of the change of velocity after impact and affects the performance of orbit deflection. In this work, we investigate the effects of planetary perturbation and orbital uncertainty on the defense effectiveness of kinetic energy impact missions. Based on the real ephemeris model, a dynamic model considering the gravitational perturbation of many bodies is established. A virtual asteroid orbit with Earth impact characteristics is constructed by the inverse orbit integration method. the state transition tensor (STT) method is employed to calculate the influence of the impact direction uncertainty on orbit deflection. Research results demonstrate that the optimal asteroid impact moment appears in perihelion, which not only enhances orbital dis-placement but also suppresses perturbations in deflection outcomes induced by velocity direction errors. Crucially, our study also reveals that close planets flyby after impact will also influence the deflection performance significantly. This suggests that specialized orbital analysis of such gravitational interactions is necessary in actual mission design to ensure a reliable defense strategy.
KW - Asteroid
KW - Kinetic impact
KW - State transition tensor
KW - Uncertainty
UR - https://www.scopus.com/pages/publications/105021829148
U2 - 10.1007/978-981-95-3010-6_39
DO - 10.1007/978-981-95-3010-6_39
M3 - Conference contribution
AN - SCOPUS:105021829148
SN - 9789819530090
T3 - Lecture Notes in Mechanical Engineering
SP - 570
EP - 583
BT - Proceedings of the 2nd Aerospace Frontiers Conference (AFC 2025) - Volume III
PB - Springer Science and Business Media Deutschland GmbH
T2 - 2nd Aerospace Frontiers Conference, AFC 2025
Y2 - 11 April 2025 through 14 April 2025
ER -