Fusion crust is a thin (few millimetres) dark layer which cover the surface of all fresh-fall meteorites, and form by vigorous interactions with the Earth atmosphere during their entry. However, remains still controversial the redox state during fusion crust formation. In order to better understand these chemical processes, in this work, we present a chemical and mineralogical surface study of the Tagish Lake (C2-Ung) meteorite fusion crust.

XPS, SEM, and micro-Raman investigations of Tagish Lake (C2-ung) meteorite fusion crust / X. Shehaj, S. Caporali, B. Cortigiani, M. Ricci, G. Giuli, E. Palomba, G. Pratesi. - ELETTRONICO. - (2024), pp. 0-0. (Intervento presentato al convegno XIX Congresso Nazionale di Scienze Planetarie).

XPS, SEM, and micro-Raman investigations of Tagish Lake (C2-ung) meteorite fusion crust

X. Shehaj;S. Caporali;B. Cortigiani;M. Ricci;G. Pratesi
2024

Abstract

Fusion crust is a thin (few millimetres) dark layer which cover the surface of all fresh-fall meteorites, and form by vigorous interactions with the Earth atmosphere during their entry. However, remains still controversial the redox state during fusion crust formation. In order to better understand these chemical processes, in this work, we present a chemical and mineralogical surface study of the Tagish Lake (C2-Ung) meteorite fusion crust.
2024
XIX Congresso Nazionale di Scienze Planetarie
XIX Congresso Nazionale di Scienze Planetarie
X. Shehaj, S. Caporali, B. Cortigiani, M. Ricci, G. Giuli, E. Palomba, G. Pratesi
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1349912
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