Preprints
https://doi.org/10.5194/egusphere-2025-928
https://doi.org/10.5194/egusphere-2025-928
20 Mar 2025
 | 20 Mar 2025

Diffusion kinetics of 3He in pyroxene and plagioclase and applications to cosmogenic exposure dating and paleothermometry in mafic rocks

Marie Bergelin, Andrew Gorin, Greg Balco, and William Cassata

Abstract. In this study, we investigate the diffusivity of cosmogenic 3He in a variety of plagioclase and pyroxene compositions, and its application to paleothermometry and exposure dating in these minerals, through stepwise degassing experiments. While cosmogenic 3He has been utilized for exposure dating in pyroxene for decades due to its retentivity, plagioclase, often found along with pyroxene in mafic rocks, is generally less retentive of cosmogenic noble gas. However, the diffusivity of 3He in either plagioclase or pyroxene has not yet been measured quantitatively. A challenge in measuring diffusion kinetics by step-degassing experiments in poorly retentive minerals is the fact that significant amounts of He can be lost prior to the experiment. To address this issue, we apply a forward ‘multiple diffusion domain’ (MDD) inversion model that includes model predictions of initial gas loss during irradiation and storage of the samples to account for this observation and add constraints to the diffusion parameters. We find that 3He diffusivity in plagioclase appears to be highly variable. This variability can be explained by the MDD inversion models’ inability to constrain the diffusion parameters when significant gas has been lost during irradiation and/or prolonged storage prior to experiment analysis, resulting in an overestimation of 3He retentivity. Plagioclase samples that were kept frozen after irradiation to limit the initial gas loss yielded the most reliable estimate of diffusion kinetics. We find that 3He in plagioclase is diffusively lost at Earth’s surface temperatures on a timescale of hundred years, and therefore, unsuitable for surface temperature paleothermometry. Contrary, we find cosmogenic 3He in pyroxene to be retentive at Earth’s surface temperatures on a million-year-timescale.

Competing interests: At least one of the (co-)authors is a member of the editorial board of Geochronology. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Marie Bergelin, Andrew Gorin, Greg Balco, and William Cassata

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2025-928', Anonymous Referee #1, 08 May 2025
    • AC1: 'Reply on RC1', Marie Bergelin, 11 Jun 2025
  • RC2: 'Comment on egusphere-2025-928', Florian Hofmann, 15 May 2025
    • AC2: 'Reply on RC2', Marie Bergelin, 11 Jun 2025

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2025-928', Anonymous Referee #1, 08 May 2025
    • AC1: 'Reply on RC1', Marie Bergelin, 11 Jun 2025
  • RC2: 'Comment on egusphere-2025-928', Florian Hofmann, 15 May 2025
    • AC2: 'Reply on RC2', Marie Bergelin, 11 Jun 2025
Marie Bergelin, Andrew Gorin, Greg Balco, and William Cassata
Marie Bergelin, Andrew Gorin, Greg Balco, and William Cassata

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Short summary
Helium gas accumulates over time in minerals, but loss can occur depending on temperature. If partially retained, its loss can potentially be used for determining past surface temperatures. This study uses a model that accounts for complex gas loss to analyze helium retention in two minerals commonly found on the surface of Antarctica. We find one of the minerals retains helium while the other loses nearly all of the gas within hundred years, making it unsuitable as a climate reconstruction.
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