Nitrogen in strongly peraluminous granites reveals a significant increase in biomass burial and O2 production prior to the Neoproterozoic oxygenation event

Fawn S.M. Holland*, Eva E. Stüeken, Wei Dan, Wenxiang Zhang, Yu Zhu, Sami Mikhail

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

Strongly Peraluminous Granites (SPGs) are mostly formed by the partial melting of Al-rich sedimentary rocks and can reflect the chemical properties of their sedimentary protoliths. Recent work suggests that the nitrogen content ([N]) of SPGs preserve changes in biomass burial over time (Mikhail et al., 2024). This mechanism occurs because in unaltered samples, SPGs with elevated [N] are thought to reflect the elevated [N] of their sedimentary protolith, and this additional nitrogen would come from sediment-hosted biomass. This archive reveals an increase in biomass burial by a factor of 5- to 8-fold between 1.4–0.5 Ga. In this study, we analysed the nitrogen abundances and isotopic values of SPG samples from 1.0 to 0.7 Ga to better resolve the period when biomass burial increased. We find that SPG [N] increases 2.4-fold across the Mesoproterozoic-Neoproterozoic boundary at 1.0 Ga and 2.8-fold across the Neoproterozoic-Phanerozoic boundary at 0.5 Ga. Therefore, with consideration of the time lag from biomass burial to SPG formation, we suggest that biomass burial first began to increase in the late Mesoproterozoic. Biomass burial removes organic carbon, a reductant, from Earth’s surface, causing a net production of O2. Therefore, these data permit us to calculate an increase in O2 production from biomass burial starting in the Mesoproterozoic, yielding an additional 6.3 × 1020 to 30 × 1020 moles of O2 throughout the Neoproterozoic, possibly contributing to the Neoproterozoic Oxygenation Event and to the chain of events which resulted in an environment capable of supporting animal life in the Cambrian.
Original languageEnglish
Article number119890
Pages (from-to)1-10
Number of pages10
JournalEarth and Planetary Science Letters
Volume679
Early online date6 Feb 2026
DOIs
Publication statusE-pub ahead of print - 6 Feb 2026

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