A mineralogical perspective on the granite alkali feldspar megacrysts paradox

Alkali feldspar megacrysts (commonly named K-feldspar) are a distinctive feature of many plutonic rocks. Yet, there is still no consensus on their origin. Two main contrasting explanations have been proposed so far: (i) the megacrysts form late during the crystallization history of the plutonic rock in which they occur and attain their large size in a melt-poor – even subsolidus – environment, or (ii) the megacrysts crystallize at an early stage and grow in the presence of large volumes of melt. In this article we address the applicability of these models to the alkali feldspar megacrysts of the Castellaccio Pluton (NW Sardinia, Italy). Petrographic observations and microstructural analysis of the megacrysts highlight the systematic occurrence of relict K-bearing mineral inclusions – biotite, muscovite and oligoclase – rimmed by anorthoclase and K-rich albite. We interpret these microstructures as evidence of reactions between partially assimilated K-bearing phases, likely from wall-rock, and the incoming melt. The chemical assimilation of K-bearing phases is proposed as the mechanism of K and Al enrichment necessary for the megacrysts growth. The temperatures of the megacrysts crystallization, calculated by Ti-in-K-feldspar thermometer, are estimated at c. 820 ± 60 or 780 ± 60 °C, depending on the calculated TiO 2 activity in the whole rock (0.47–0.62). Finally, the strong positive europium anomaly and enrichment in barium in the megacrysts with respect to the whole-rock compositions exclude significant plagioclase fractionation, thus supporting megacrysts formation at the early stage of the cooling history. All the results of our work point toward a magmatic origin and evolution of the K-feldspar megacrysts in the Castellaccio granite pluton. • A Variscan granite hosting alkali feldspar megacrysts is documented. • The megacrysts host relicts K– phases mantled by rims of anorthoclase/K-rich albite. • Microstructures indicate a reaction between wall–rock and granitic magma. • Megacrysts formed at high temperate during the early stage of granite.

Authors

Institutions

Publication Details

Journal
Lithos
Published
2025-09-04
DOI
https://doi.org/10.1016/j.lithos.2025.108229
Citations
1
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
1.87
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

A mineralogical perspective on the granite alkali feldspar megacrysts paradox

Alfredo Idini, Silvio Ferrero, Dario Fancello, Leonardo Casini et al.
1 citations
Lithos
Geological and Geochemical Analysis
1.87
article

A mineralogical perspective on the granite alkali feldspar megacrysts paradox

Alfredo Idini, Silvio Ferrero, Dario Fancello, Leonardo Casini, Paola Mameli, Stefano Cuccuru
article en
1 citations

Abstract

Alkali feldspar megacrysts (commonly named K-feldspar) are a distinctive feature of many plutonic rocks. Yet, there is still no consensus on their origin. Two main contrasting explanations have been proposed so far: (i) the megacrysts form late during the crystallization history of the plutonic rock in which they occur and attain their large size in a melt-poor – even subsolidus – environment, or (ii) the megacrysts crystallize at an early stage and grow in the presence of large volumes of melt. In this article we address the applicability of these models to the alkali feldspar megacrysts of the Castellaccio Pluton (NW Sardinia, Italy). Petrographic observations and microstructural analysis of the megacrysts highlight the systematic occurrence of relict K-bearing mineral inclusions – biotite, muscovite and oligoclase – rimmed by anorthoclase and K-rich albite. We interpret these microstructures as evidence of reactions between partially assimilated K-bearing phases, likely from wall-rock, and the incoming melt. The chemical assimilation of K-bearing phases is proposed as the mechanism of K and Al enrichment necessary for the megacrysts growth. The temperatures of the megacrysts crystallization, calculated by Ti-in-K-feldspar thermometer, are estimated at c. 820 ± 60 or 780 ± 60 °C, depending on the calculated TiO 2 activity in the whole rock (0.47–0.62). Finally, the strong positive europium anomaly and enrichment in barium in the megacrysts with respect to the whole-rock compositions exclude significant plagioclase fractionation, thus supporting megacrysts formation at the early stage of the cooling history. All the results of our work point toward a magmatic origin and evolution of the K-feldspar megacrysts in the Castellaccio granite pluton. • A Variscan granite hosting alkali feldspar megacrysts is documented. • The megacrysts host relicts K– phases mantled by rims of anorthoclase/K-rich albite. • Microstructures indicate a reaction between wall–rock and granitic magma. • Megacrysts formed at high temperate during the early stage of granite.

LithosVol. 516-517
University of Sassari (IT), University of Cagliari (IT)
Openalex Percentile: Top 15%
Geological and Geochemical Analysis
1.87
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.