Abstract

This paper provides an effective approach for the prediction and estimation of space debris due to a vehicle breakup during uncontrolled reentry. For an advanced analysis of the time evolution of space debris dispersion, new efficient computational approaches are proposed. A time evolution of the dispersion of space pieces from a breakup event to the ground impact time is represented in terms of covariance ellipsoids, and in this paper, two covariance propagation methods are introduced. First, a derivative-free statistical linear regression method using the unscented transformation is utilized for performing a covariance propagation. Second, a novel Gaussian moment-matching method is proposed to compute the estimation of the covariance of a debris dispersion by using a Gauss-Hermite cubature-based numerical integration approach. Compared to a linearized covariance propagation method such as the Lyapunov covariance equation, the newly proposed Gauss-Hermite cubature-based covariance computation approach could provide high flexibilities in terms of effectively representing an initial debris dispersion and also precisely computing the time evolution of the covariance matrices by utilizing a larger set of sigma points representing debris components. In addition, we also carry out a parametric study in order to analyze the effects on the accuracy of the covariance propagation due to modeling uncertainties. The effectiveness of the newly proposed statistical linear regression method and the Gauss-Hermite computational approach is demonstrated by carrying out various simulations.

Highlights

  • In the past 50 years, over 16,000 metric tons of man-made space objects and unexpected asteroids have entered the Earth’s atmosphere

  • The locational difference between the final footprint impact locations of two different methods was about 2 km in the x direction, and 10 m in the y direction, that is, δx tfinal = 1 8980 km 0 00860 km 0 km. It is seen from the nominal trajectory plot that the uncertainties of the motion of the debris dispersion are captured more precisely by utilizing the Gauss-Hermite cubature technique compared to the unscented transformation method, and this is because the GHC method adopts a much larger set of sigma lattice points at the initial debris dispersion which leads to a more precise estimation of the debris dispersion

  • For advanced analysis of the time evolution of space debris dispersion due to the breakup during reentry, two effective computational approaches were proposed to estimate the statistical distribution of the debris dispersion

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Summary

Introduction

In the past 50 years, over 16,000 metric tons of man-made space objects and unexpected asteroids have entered the Earth’s atmosphere. The Lyapunov equation-based covariance propagation method is based on the linearization of the translational equations of motion of the reentering space debris and the equations of the atmospheric reentry is subject to unknown uncertainties; a high degree of neglected and truncated nonlinearities could lead to a degraded estimation of the debris dispersion [8, 9]. In order to compensate for the drawbacks of the Lyapunov-based estimation of the debris dispersion, alternative solutions could be employed by increasing the order of the Taylor-series expansion of the nonlinear system or by using an advanced numerical technique [9, 10] These efficient alternatives include the unscented transformation [11], the divided-difference numerical integration [12,13,14], and the cubature quadrature integration [15].

Reentry Equations of Motion
Algorithms for Estimation of Debris Dispersion
Simulation Results
10 Trajectory without wind
Summary and Conclusion
Full Text
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