Are Clay Minerals Systematically the Products of Aqueous Alteration in Cosmic Bodies?

Author:

El Albani Abderrazak1,Chraiki Ibtissam1ORCID,Aoudjehane Hasnaa2ORCID,Ghnahalla Mohamed1ORCID,Abdelfadel Fatima3,Elmola Ahmed4ORCID,Bankole Olabode1ORCID,Ikouanga Julie1,El Khoury Anna15ORCID,Fontaine Claude1,Bouougri El6,Westall France7,Meunier Alain1

Affiliation:

1. Institut de Chimie des Milieux et Matériaux, Université de Poitiers and CNRS, 86073 Poitiers, France

2. GAIA Laboratory, Faculty of Sciences Ain Chock, Hassan II University of Casablanca, km 8 Route d’El Jadida, Casablanca 20150, Morocco

3. National Institute for Scientific and Technological Research in Water, City of Innovation Souss Massa, Ibn Zohr University, Agadir 80000, Morocco

4. The James Hutton Institute, Craigiebuckler, Aberdeen AB15 8QH, UK

5. Nanoscopium Beamline, Synchrotron Soleil, 91192 Gif-sur-Yvette, France

6. Department of Geology, Faculty of Sciences-Semlalia, Cadi Ayyad University, Marrakesh 40000, Morocco

7. CNRS-Centre de Biophysique Moléculaire, 45100 Orléans, France

Abstract

The formation of chondrite materials represents one of the earliest mineralogical processes in the solar system. Phyllosilicates are encountered at various stages of the chondrule formation, from the initial stages (IDP agglomerates) to the final steps (chondrule internal alteration). While typically linked to aqueous alteration, recent studies reveal that phyllosilicates could precipitate directly from residual fluids in post-magmatic or deuteric conditions and under a wide range of temperatures, pressures, water/rock ratios, and H2/H2O ratio conditions. This study re-examined the formation of hydrated phyllosilicates in chondrules and associated fine-grained rims (FGRs) using published petrographical, mineralogical, and chemical data on carbonaceous chondrites. Given that chondrules originate from the melting of interplanetary dust particles, the water liberated by the devolatilization of primary phyllosilicates, including clay minerals or ice melting, reduces the melting temperature and leads to water dissolution into the silicate melt. Anhydrous minerals (e.g., olivine and diopside) form first, while volatile and incompatible components are concentrated in the residual liquid, diffusing into the matrix and forming less porous FGRs. Serpentine and cronstedtite are the products of thermal metamorphic-like mineral reactions. The mesostasis in some lobated chondrules is composed of anhydrous and hydrous minerals, i.e., diopside and serpentine. The latter is probably not the alteration product of a glassy precursor but rather a symplectite component (concomitant crystallization of diopside and serpentine). If so, the symplectite has been formed at the end of the cooling process (eutectic-like petrographical features). Water trapped inside chondrule porosity can lead to the local replacement of olivine by serpentine without external water input (auto-alteration). In the absence of water, hydrated phyllosilicates do not crystallize, forming a different mineral assemblage.

Funder

La Région Nouvelle Aquitaine

l’Agence Nationale de la Recherche Scientifique

French government program

Publisher

MDPI AG

Reference110 articles.

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