Filippov Sliding Dynamics of Cosmic Dust Atmospheric Entry: Survival Boundaries, Asymptotic Mass Loss, and Inverse Problem Limits
Md Shahrier Islam Arham, Prasun Panthi, Min Heo
Abstract
We develop a mathematically rigorous framework for modelling the atmospheric entry of micrometeoroids with radii $r_{0}\in[0.5,1000]μm$ at hypervelocity speeds $v_{0}\in[11.2,72]km/s$. The governing four-state ODE system coupling altitude, speed, temperature, and radius has a discontinuous right-hand side at the ablation threshold $T=T_{melt}$, making it a Filippov dynamical system. We prove three original results. First, the empirical survival boundary $r_{0}^{crit}\propto v_{0}^{-3}$ (known since Love & Brownlee 1991) is the sliding bifurcation locus of the Filippov system: the locus in parameter space where particle trajectories first touch the attracting sliding region on the switching surface. This gives the $v_{0}^{-3}$ scaling its first rigorous dynamical-systems derivation. Second, a matched perturbation expansion with small parameter $δ_ε=3Λρ_{0}H/(8Q^{*}ρ_{p}r_{0}\sin γ)$ yields a closed-form mass-loss formula with numerically confirmed $\mathcal{O}(δ_ε^{2})$ error bound. Third, the transfer matrix K mapping entry distributions to stratospheric surface outcomes has a null space in its surviving-particle submatrix $K_{surv}$ determined by the full-ablation manifold A. For iron and cometary compositions (high vo, large ro), A is non-empty and contains particles permanently invisible to stratospheric collectors regardless of sample size. Fate maps for silicate and iron compositions are validated against Love & Brownlee (1991). Global Sobol analysis confirms entry speed as the dominant parameter. A regularised nonnegative inversion demonstrates partial recovery of the pre-atmospheric flux distribution.
