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Abstract
We studied Caleta el Cobre 022, a nakhlite showing a high abundance of aqueous alteration products, commonly called “iddingsite” and compared it to eight other nakhlites, in order to constrain the composition and the history of the aqueous alteration of nakhlites. Olivine grains in nakhlites display planes of secondary fluid inclusions, composed of pyroxene, magnetite, and a void potentially filled by a fluid. They were formed by a first fluid alteration event, previous to the iddingsite alteration event, probably from a late magmatic fluid circulation. We observed magnetite–pyroxene symplectites in olivine grains in most nakhlites, related to the same fluid‐assisted tardi‐magmatic event as the crystallization of the secondary inclusion planes. Those secondary inclusions and symplectites can be observed at the center of iddingsite veins, inside the most altered nakhlites, and are thus interpreted as being weakness planes …
Original language | English |
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Pages (from-to) | 151-174 |
Number of pages | 24 |
Journal | Meteoritics & Planetary Science |
Volume | 60 |
Issue number | 2 |
DOIs | |
Publication status | Published - Feb 2025 |
Bibliographical note
Publisher Copyright:© 2024 The Meteoritical Society.
Projects
- 2 Active
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BASGO1: OZR Basisfinanciering voor Grote Onderzoeksgroepen - AMGC
1/01/24 → 31/12/29
Project: Fundamental