Fusion crust of stony meteorites: From the observation spectrum to the initial meteoroid matter

1Evgeniya V. Petrova,1Victor I. Grokhovsky,2Anna Kartashova
Icarus (inPress) Link to Article [https://doi.org/10.1016/j.icarus.2026.117147]
1Ural Federal University, Mira Str., 19/5, 620002 Ekaterinburg, Russia
2Institute of Astronomy RAS, Pyatnitskaya Str., 48, 119017 Moscow, Russia
Copyright Elsevier

Fragmentation, ablation and significant loss of mass occur when the meteoroid passes through the Earth’s atmosphere. There a combined action of melting and shearing takes place, so a fusion crust is forming on the surface of the fragments. It combined a subsurface layer of heated matter and an outer layer consisting of remaining melted meteoroid substance.
In this publication we focused on the process of ablation from different points of view: i – registered spectra of fireballs; ii – fusion crust composition study; iii – ablation modeling ground experiments.

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