Читать книгу Mantle Convection and Surface Expressions - Группа авторов - Страница 13

Convection in Earth’s mantle is linked to plate tectonic processes and controls the fluxes of heat and material between deep mantle reservoirs, the surface, and the atmosphere over billions of years. A better understanding of these mantle material cycles and their impact on the long‐term evolution of our planet, as well as their potential role on other planetary bodies, requires integrated approaches that involve all disciplines studying the solid Earth.

Over the past decades, the rise in geophysical data has provided increasingly sharp images of the deep mantle, including direct images of sinking slabs and rising plumes. Increasingly accurate and novel types of geochemical data of hotspot lavas provide a detailed account of the spectrum and origin of mantle heterogeneity. Models of mantle convection make predictions on the distribution of this heterogeneity through time, and on the evolution of our planet from accretion to the present‐day. In turn, mineral physics provides increasingly realistic material properties needed to interpret the geophysical observables and constrain geodynamic models. This profound progress in the deep Earth Sciences has even advanced neighboring fields such as Planetary Sciences, Cosmochemistry, and Astrobiology, for example by providing insight into the conditions for habitability on the timescales of biological evolution, and thus, for the sustainability of higher life.

This AGU book unifies researchers with an expertise in different solid Earth disciplines, including observational geophysics, numerical modelling, geochemistry and mineral physics, to outline current concepts on dynamic processes occurring in the mantle and associated material cycles. Since each sub‐discipline is restricted by fundamental uncertainties, true progress is increasingly made at the intersection between different sub‐disciplines. The present book is hence devoted to synergetic multi‐disciplinary work, motivated by the vision of a holistic picture of the deep Earth.

Despite the common call for trans‐disciplinary research, only limited work has been done that truly and quantitatively integrates different approaches. Sometimes, just the lack of a common language, with different jargon across discipline boundaries, prevents any directed and sustainable progress. It is our hope that this AGU book can help to bridge the gaps between different Earth Science communities, resolve some semantic issues, and foster future collaborations. We attempted to ensure that chapters are written in a style accessible for researchers from all sub‐disciplines. It is up to the reader to decide if we succeeded.

This book does not aim to provide a comprehensive overview of all relevant research strands. Instead, we aim to cover a wide range of relevant topics and emphasize the interdisciplinary connection between them. As the overarching idea of the book is to bridge between the disciplines, the subsections of the book are not sorted by discipline, but instead by guiding research questions.

The first part of the book summarizes the current state of the mantle, its properties and dynamic evolution. This is followed by part two, which discusses the transport of heat and material through the mantle, as constrained by geophysical observations and geodynamic model predictions. The final part of the book focuses on the surface expressions of mantle dynamics and its control on planetary evolution and habitability.