The chemical separation (Yierpan et al., 2018) and instrumental measurement techniques (Kurrawa et al., 2017) established in this project allow for unprecedented precision of Se isotope and Se-Te elemental analysis of geological materials such as mafic rocks (Yierpan et al., 2019), chondritic meteorites (Labidi et al., 2018) and single sulfides (König et al., 2019) with as low as 3 ng total Se.
In contrast to all previously published studies, our technique allows for the first time to resolve Se isotope variations between different chondritic meteorites (Labidi et al., 2018), with cosmochemical implications for the understanding of sulfide formation in the early solar nebula and potential for discriminating between meteorites as building materials for Earth and the origin of terrestrial volatiles.
Origin of Earth's volatile elements from the Outer Solar System could be constrained for the first time from the perspective of stable isotopes of a highly siderophile and volatile element (Varas-Reus et al. (2020, Nature Geoscience).
High-precision isotope measurements of the volatile element selenium in hot spot volcanic rocks showed that ancient surface oxidation signatures were transferred into the deep mantle by subduction where they survived for billions of years. Within the framework of most recent models based on Se systematics, the results further imply that our atmosphere ~1–2 billion years ago probably contained much more oxygen than widely assumed in the scientific community. In addition, these newly constrained selenium isotope systematics highlight how exactly volatile elements in the Earth’s atmosphere, continents and mantle are linked by a large geological cycle (Yierpan et al., 2020, Science Advances). Moreover, selenium isotopes show the highly oxidized nature of slab fluids in modern subduction zone systems (König et al., 2021, Geochemical Perspectives Letters).
Together with the possibility to analyse Os isotopes of the same dissolved sample material, it is expected that, for the first time, robust Os isotope minimum ages can be obtained for a given Se isotope signature. This will push the limits in exploring the terrestrial volatile and redox evolution from the perspectives of single and deep mantle sulfides through Earth's geological history. Another significant finding is that selenium isotopes may contribute to trace the existence of deep microbial life (Cabral et al., 2021, Geology).