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Microlite crystallization during eruptions at Mt. Mazama: implications for magma ascent

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Abstract

Large silicic eruptions can be preceded by small eruptions of different styles and volumes. The Holocene Llao Rock, Cleetwood, and climactic eruptions of Mt. Mazama, OR, USA, were sourced from the same magma and followed this pattern. The Llao Rock and Cleetwood eruptions are both relatively small, have pyroclasts with microlites and a wide range of vesicularities, and each consisted of an explosive phase followed by an effusive phase. The climactic eruption had no effusive phase and created highly vesicular pyroclasts with no microlites. We analyzed microlite crystallization using phase equilibria and decompression experiments. Comparing the results to the pyroclasts from the Llao Rock and Cleetwood eruptions, we find that the differences between the small and climactic eruptions are likely caused by different magma ascent dynamics. Our experiments show that plagioclase and pyroxene microlites crystallize only during decompressions that are most likely too slow to result in explosive eruptions. The Llao Rock magma likely stalled at shallow depths before continuing fast ascent, which allowed for microlite crystallization that might have also caused explosive eruptions. The Cleetwood magma likely took two separate ascent paths, a majority fraction that ascended quickly from high pressure without stalling and a minority fraction that stalled at shallow depths before continuing ascent along with the majority fraction. These ascent dynamics of the Llao Rock and Cleetwood magmas led to the creation of obsidian pyroclasts from sidewall sintering of fragmented majority-fraction ash. The climactic magma did not stall at shallow depths and instead ascended from depth quickly to the surface, creating the conditions necessary for caldera collapse.

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All data obtained during this study and collated from previous studies are included in this published article.

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Acknowledgements

This research was conducted with the support of US National Science Foundation grant EAR-1725186, The University of Texas at Austin Graduate School, and US National Park Service scientific research and collecting permit CRLA-2018-SCI-0005. We thank Nicole Guinn, Wade Aubin, Thomas Giachetti, and Josh Wiejaczka for their assistance in the field, and Charlie Bacon for advice on the eruption. We also thank Dr. Jonathan M. Castro and an anonymous reviewer for their helpful comments in preparing this manuscript.

Funding

This work was supported by US National Science Foundation grant EAR-1725186 and The University of Texas at Austin Graduate School.

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Both authors contributed to the study concept and design. Samples were collected by both authors. Sample preparation, data collection and analyses were performed by SBO. The first draft of the manuscript was written by SBO and was subsequently revised by both authors.

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Correspondence to Sean B. O’Donnell.

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The authors have no competing interests to declare that are relevant to the content of this article.

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Communicated by Gordon Moore.

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O’Donnell, S.B., Gardner, J.E. Microlite crystallization during eruptions at Mt. Mazama: implications for magma ascent. Contrib Mineral Petrol 177, 105 (2022). https://doi.org/10.1007/s00410-022-01971-0

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