Ultra-Mafic Cumulates From Kaupulehu, Hualālai Volcano, Hawai'i: Geochemical Resetting of Mantle-Inherited Olivine
| dc.contributor.author | Dujardin, A. D. | en |
| dc.contributor.author | Demouchy, S. | en |
| dc.contributor.author | Alard, O. | en |
| dc.contributor.author | Gardés, E. | en |
| dc.contributor.author | Laubier, M. | en |
| dc.contributor.author | Barou, F. | en |
| dc.date.accessioned | 2026-01-02T09:41:26Z | |
| dc.date.available | 2026-01-02T09:41:26Z | |
| dc.date.issued | 2025 | en |
| dc.description.abstract | We characterized the chemical composition and microstructure of six ultramafic cumulates from the Kaupulehu lava flow, Hualālai (Hawai'i Island), to decipher their origin. The samples are mostly wehrlites with poikilitic textures. The chemical compositions obtained from electron probe microanalyses and laser ablation inductively coupled plasma mass spectrometry confirm the magmatic origin of pyroxenes. Olivines display homogeneous compositions in major, minor and trace elements. Their Fo# (81–88) are typical of magmatic compositions, but first row transition element concentrations are intermediate between mantle and magmatic olivine compositions. Rare Earth element (REE) patterns are similar to those of mantle olivine, but Kaupulehu olivines are more enriched in heavy REE than mantle specimens. Results from Fourier transform infrared spectroscopy showed that nominally anhydrous minerals are very poor in hydrogen: 1.3–2.2 ppm H2O by weight in olivine, 6.4 in orthopyroxene, and 12.6–48.2 in clinopyroxene. Nevertheless, fluid inclusions and bubbles evidenced by scanning electron microscopy demonstrate the presence of volatiles, which are expected to exsolve during degassing. Despite the undeniable magmatic imprint in these ultra-mafic cumulates, electron backscatter diffraction maps evidence subgrain boundaries in olivine, important internal misorientation (>10°), and Crystallographic preferred orientation (CPO) (axial [010], orthorhombic and transitional toward axial-[001]), not associated with shape preferred orientation or euhedral olivine shape. All these features are evidence of high temperature dislocation creep within the asthenospheric mantle, prior to melt percolation and chemical resetting, well before their mobilization by the volcanic eruption. We conclude that olivines are mantle-inherited, whereas clinopyroxenes result from crystallization of percolating melt. | en |
| dc.description.sponsorship | C. Nevado and D. Delmas are thanked for providing high-quality sections for FTIR and EBSD; J.L. Devidal for assistance with EPMA analyses; A. Tommasi and B. Ildefonse are deeply thanked for scientific discussions at an early stage of this project. The EBSD-SEM national facility at Geoscience Montpellier, the EPMA and SEM-FIB-STEM CarMa facility at Laboratoire Magmas et Volcans are all supported by the Institut National de Sciences de l'Univers (INSU), Centre National de la Recherche Scientifique (CNRS, France). We acknowledge funding from ANR H-Deep-ISO to S. Demouchy, from ANU-Research School of Earth Sciences to O. Alard, and from ARC- DP220100709 to O. Alard and S. Demouchy, from program TelluS of the Institut National des Sciences de l\u2019Univers\u2014CNRS, from PHC FASIC ECPD 2025 project N\u00B053572VF, from the French government initiative \u201Cprogramme d'investissements d'avenir\u201D managed by the Agence Nationale de la Recherche (ANR) under Grant ANR-20-SFRI-0003 project CAP GS, and from the University Clermont Auvergne via its Centre International de Recherche Catastrophes Naturelles et D\u00E9veloppement Durable (CIR4) program (InMelt project) to S. Demouchy. This is CIR4-ClerVolc publication N\u00B0678. C. Nevado and D. Delmas are thanked for providing high\u2010quality sections for FTIR and EBSD; J.L. Devidal for assistance with EPMA analyses; A. Tommasi and B. Ildefonse are deeply thanked for scientific discussions at an early stage of this project. The EBSD\u2010SEM national facility at Geoscience Montpellier, the EPMA and SEM\u2010FIB\u2010STEM CarMa facility at Laboratoire Magmas et Volcans are all supported by the Institut National de Sciences de l'Univers (INSU), Centre National de la Recherche Scientifique (CNRS, France). We acknowledge funding from ANR H\u2010Deep\u2010ISO to S. Demouchy, from ANU\u2010Research School of Earth Sciences to O. Alard, and from ARC\u2010 DP220100709 to O. Alard and S. Demouchy, from program TelluS of the Institut National des Sciences de l\u2019Univers\u2014CNRS, from PHC FASIC ECPD 2025 project N\u00B053572VF, from the French government initiative \u201Cprogramme d'investissements d'avenir\u201D managed by the Agence Nationale de la Recherche (ANR) under Grant ANR\u201020\u2010SFRI\u20100003 project CAP GS, and from the University Clermont Auvergne via its Centre International de Recherche Catastrophes Naturelles et D\u00E9veloppement Durable (CIR4) program (InMelt project) to S. Demouchy. This is CIR4\u2010ClerVolc publication N\u00B0678. | en |
| dc.description.status | Peer-reviewed | en |
| dc.format.extent | 24 | en |
| dc.identifier.issn | 1525-2027 | en |
| dc.identifier.scopus | 105011340745 | en |
| dc.identifier.uri | https://hdl.handle.net/1885/733802449 | |
| dc.language.iso | en | en |
| dc.provenance | This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. | en |
| dc.rights | © 2025 The Author(s). Geochemistry, Geophysics, Geosystems published by Wiley Periodicals LLC on behalf of American Geophysical Union. | en |
| dc.source | Geochemistry, Geophysics, Geosystems | en |
| dc.subject | cumulates | en |
| dc.subject | EBSD | en |
| dc.subject | Hawaii | en |
| dc.subject | LA-ICP-MS | en |
| dc.subject | mantle | en |
| dc.subject | olivine | en |
| dc.title | Ultra-Mafic Cumulates From Kaupulehu, Hualālai Volcano, Hawai'i: Geochemical Resetting of Mantle-Inherited Olivine | en |
| dc.type | Journal article | en |
| dspace.entity.type | Publication | en |
| local.bibliographicCitation.lastpage | 24 | en |
| local.bibliographicCitation.startpage | 1 | en |
| local.contributor.affiliation | Dujardin, A. D.; CNRS | en |
| local.contributor.affiliation | Demouchy, S.; Geosciences Montpellier, Université de Montpellier | en |
| local.contributor.affiliation | Alard, O.; Geochemistry, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | Gardés, E.; Université Clermont Auvergne | en |
| local.contributor.affiliation | Laubier, M.; Université Clermont Auvergne | en |
| local.contributor.affiliation | Barou, F.; Geosciences Montpellier, Université de Montpellier | en |
| local.identifier.citationvolume | 26 | en |
| local.identifier.doi | 10.1029/2024GC012128 | en |
| local.identifier.pure | 17e3778b-a278-48b7-9630-9e5b6d70fc95 | en |
| local.identifier.url | https://www.scopus.com/pages/publications/105011340745 | en |
| local.type.status | Published | en |
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