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Science is increasingly able to identify precautionary boundaries for critical Earth system processes, and the business world provides societies with important means for adaptive responses to global environmental risks. In turn, investors provide vital leverage on companies. Here, we report on our transdisciplinary science/business experience in applying the planetary boundaries framework (sensu Rockström et al., Ecol Soc 14, 2009) to define a boundary-compatible investment universe and analyse the environmental compatibility of companies. We translate the planetary boundaries into limits for resource use and emissions per unit of economic value creation, using indicators from the Carnegie Mellon University EIO‑LCA database. The resulting precautionary 'economic intensities' can be compared with the current levels of companies' environmental impact. This necessarily involves simplifying assumptions, for which dialogue between biophysical science, corporate sustainability and investment perspectives is needed. The simplifications mean that our translation is transparent from both biophysical and financial viewpoints, and allow our approach to be responsive to future developments in scientific insights about planetary boundaries. Our approach enables both sub‑industries and individual companies to be screened against the planetary boundaries. Our preliminary application of this screening to the entire background universe of all investable stock‑listed companies gives a selectivity of two orders of magnitude for an investment universe of environmentally attractive stocks. We discuss implications for an expanded role of environmental change science in the development of thematic equity funds.
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http://dx.doi.org/10.1007/s11625-018-0574-1 | DOI Listing |
Environ Pollut
September 2025
School of Environment, Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China; State Key Laboratory of Environmental Chemistry and Ecotoxicology, Research Center for Eco-Environmental Sciences, Chinese Academy of Sciences, Beijing 100085, China.
Ozone (O) is a primary pollutant affecting air quality in China, whose formation rate was non-linearly based on volatile organic compounds (VOCs) and nitrogen oxides (NOx). A comprehensive understanding of the key drivers governing O formation and its sensitivity to precursor variations presents a persistent research challenge, stemming from the complex interplay of underlying photochemistry, meteorology, and topography. To address this knowledge gap, we conducted synchronous measurements of O and its precursors at both an urban (JPU) and a mountain (LM) site in a typical city in eastern China, enabling concurrent evaluation of O formation sensitivity and diagnostic analysis of its underlying mechanisms.
View Article and Find Full Text PDFNature
September 2025
Institute for Geophysics, Jackson School of Geosciences, University of Texas at Austin, Austin, TX, USA.
For rocky planets, the presence of a solid inner core has notable implications on the composition and thermal evolution of the core and on the magnetic history of the planet. On Mars, geophysical observations have confirmed that the core is at least partially liquid, but it is unknown whether any part of the core is solid. Here we present an analysis of seismic data acquired by the InSight mission, demonstrating that Mars has a solid inner core.
View Article and Find Full Text PDFSci Rep
September 2025
Department of Earth and Planetary Sciences, ETH Zürich, Zürich, 8092, Switzerland.
The occurrence of tectonic plate reorganization events is evident throughout the geologic record and appears to be associated with the cessation of mature and/or initiation of new subduction. Subduction initiation that produced the bend in the Hawaii-Emperor seamount chain resulted in the most recent upheaval of plate motion and engendered dramatic changes in plate velocities. Here, applying a method for identifying plate boundaries in a numerical global mantle convection model, we calculate Euler vector time series of self-consistently generated plates over a period of approximately 144 Myr.
View Article and Find Full Text PDFSci Bull (Beijing)
August 2025
Key Laboratory of Continental Collision and Plateau Uplift, Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing 100101, China.
The northeastern (NE) Tibetan Plateau is extruding eastward at a rapid rate (∼15 mm a), but the role of the upper mantle in this process remains unclear. Early-Miocene primary melilitites from the leading edge of the extruding plateau provide critical insights into the upper mantle dynamics. Geochemical and Sr-Nd-Pb-Os isotopic data, supported by experimental melt comparisons, reveal that these melilitites originate from a hybrid source of CO-bearing mantle source, probably dominated by peridotite and pyroxenite/wehrlite lithologies.
View Article and Find Full Text PDFCommun Earth Environ
August 2025
Department of Earth and Planetary Sciences, Institute of Geochemistry and Petrology, ETH Zürich, Zürich, Switzerland.
Large Low Shear Velocity Provinces (LLSVPs) near the core-mantle boundary (CMB) are key yet enigmatic structures. Their origin is often linked to the accumulation of subducted mid-ocean ridge basalt (MORB), but computational models question MORB as the sole source due to its predicted high shear wave velocity compared to normal mantle. This uncertainty is compounded by the lack of direct sound velocity measurements at CMB pressures.
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