Insights into the construction of the Oruanui magma reservoir from a comparison of zircon hosted in plagioclase and whole-rock
• We report new 238 U- 230 Th ages and trace-element data for both rims and interiors of zircons separated from whole-rock and plagioclase. • Whole-rock zircon surfaces define two clear compositional groups. • Preservation of these two groups requires assembly of the erupted magma within 2 kyr of eruption. • Plagioclase-hosted zircon rim data indicate heating and magma mixing ∼40 kyr prior to eruption. • These data provide new insights about the processes leading to large silicic eruptions. Silicic magmatic systems play a critical role in the evolution of continental crust, and their eruptions could pose significant hazard to modern civilization. However, the processes of silicic magma storage and assembly prior to eruption are not well understood. We report new 238 U- 230 Th ages and trace-element data for both rims and interiors of zircons separated from whole-rock (WR) samples and from bulk plagioclase separates from the 25.4 ka Oruanui eruption, Taupo Volcanic Zone, New Zealand. These data provide petrologic context and a more complete record of zircon crystallization than previous analyses of whole-rock hosted zircon interiors. In particular, whole-rock zircon surfaces are more restricted in composition than other zircon groups and define two clear compositional groups. Preservation of these two distinct compositional groups requires that the zircon must have been incorporated into the erupted Oruanui rhyolite at most ∼2 kyrs prior to eruption. In addition, systematic variations in Eu/Eu*, Hf, and Sc with Ti-in-zircon temperature and 238 U- 230 Th age recorded in plagioclase-hosted zircon surfaces indicate that a shift to higher temperatures and less evolved compositions began at ∼40 ka and continued until amalgamation of the final erupted magma body. These new data demonstrate the additional insights available from detailed microanalytical investigations and support other studies indicating that large volumes of silicic magma accumulate in the crust via amalgamation of multiple smaller compositionally distinct portions of the broader magma reservoir.
Authors
- Adam J.R. Kent (ORCID: https://orcid.org/0000-0003-3564-6285)
- Tyler D. Schlieder (ORCID: https://orcid.org/0000-0002-4382-6537)
- Amissabah Johnson
- C. D. Deering (ORCID: https://orcid.org/0000-0002-3768-2258)
- Kari M. Cooper (ORCID: https://orcid.org/0000-0003-0636-6292)
- Darren M. Gravley (ORCID: https://orcid.org/0000-0003-4451-9210)
- Seth Rubin
Institutions
- Michigan Technological University (US)
- Planetary Science Institute (US)
- Oregon State University (US)
- University of Canterbury (NZ)
- University of California, Davis (US)
Publication Details
- Journal
- Earth and Planetary Science Letters
- Published
- 2025-06-16
- DOI
- https://doi.org/10.1016/j.epsl.2025.119495
- Primary Topic
- Geological and Geochemical Analysis
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Science Foundation