Article

The Fusion Crust of the Winchcombe Meteorite: A Preserved Record of Atmospheric Entry Processes

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Citation

Genge MJ, Alesbrook LS, Almeida NV, Bates HC, Bland PA, Boyd MR, Burchell MJ, Collins GS, Cornwell LT, Daly L, Devillepoix HAR, van Ginneken M, Greshake A, Hallatt D & Schroeder C (2023) The Fusion Crust of the Winchcombe Meteorite: A Preserved Record of Atmospheric Entry Processes. Meteoritics and Planetary Science. https://doi.org/10.1111/maps.13937

Abstract
Fusion crusts form during the atmospheric entry heating of meteorites and preserve a record of the conditions that occurred during deceleration in the atmosphere. The fusion crust of the Winchcombe meteorite closely resembles those of other stony meteorites, and in particular CM2 chondrites, since it is dominated by olivine phenocrysts set in a glassy mesostasis with magnetite, and is highly vesicular. Dehydration cracks are unusually abundant in Winchcombe. Failure of this weak layer is an additional ablation mechanism to produce large numbers of particles during deceleration, consistent with observation of pulses of plasma in videos of the Winchcombe fireball. Calving events might provide an observable phenomenon related to meteorites that are particularly susceptible to dehydration. Oscillatory zoning is observed within olivine phenocrysts the fusion crust, in contrast to other meteorites, perhaps owing to temperature fluctuations resulting from calving events. Magnetite monolayers are found in the crust, and have also not been previously reported, and form discontinuous strata. These features grade into magnetite-rims formed on the external surface of the crust and suggest trapping of surface magnetite by collapse of melt. Magnetite monolayers may be a feature of meteorites that undergo significant degassing. Silicate warts with dendritic textures were observed and are suggested to be droplets ablated from another stone in the shower. They, therefore, represent the first evidence for inter-shower transfer of ablation materials and are consistent with the other evidence in the Winchcombe meteorite for unusually intense gas loss and ablation, despite its low entry velocity.

Keywords
Ablation; Fusion crust; Bolide(s)

Notes
Output Status: Forthcoming/Available Online Additional co-authors: Christopher Hamann, Lutz Hecht, Laura E. Jenkins, Diane Johnson, Rosie Jones, Ashley J. King, Haithem Mansour, Sarah McMullan, Jennifer T. Mitchell, Gavyn Rollinson, Sara S. Russell, Natasha R. Stephen, Martin D. Suttle, Jon D. Tandy, Patrick Trimby, Eleanor K. Sansom, Vassilia Spathis, Francesca M. Willcocks, Penelope J. Wozniakiewicz

Journal
Meteoritics and Planetary Science

StatusEarly Online
Publication date online02/01/2023
Date accepted by journal24/10/2022
URLhttp://hdl.handle.net/1893/34710
ISSN1086-9379
eISSN1945-5100

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