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Earth interior model

Simplified model of the Earth’s interior and its global dynamics featuring a solid inner and a fluid outer core, a viscous partially molten but not fluid mantle, and characteristic surface topography.

Simplified model of the Earth interior and its global dynamics featuring a solid inner and a fluid outer core, a viscous partially molten but not fluid mantle, with hot material rising from the core-mantle boundary in form of active mantle plumes and cold material, including oceanic surface plates, sinking back into the mantle in a process called subduction. The dynamics in the Earth interior crucially shapes the rocky surface of the planet, creating mountain ranges and deep-sea trenches.

  • Creator: Fabio Crameri
  • This version: 06.10.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri adjusted from Crameri & Tackley (2016) is available via the open-access s-ink.org repository.
  • Related reference: Crameri, F., and P. J. Tackley (2016), Subduction initiation from a stagnant lid and global overturn: new insights from numerical models with a free surface, Progress in Earth and Planetary Science, 3(1), 1–19, doi:10.1186/s40645-016-0103-8
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Planetary interior

Comparison of suggested mantle convection in the Earth (mobile-lid mode) and Venus (inefficient short slab mode).

Comparison of suggested mantle convection in Earth and Venus. Mobile-lid mantle convection in the Earth involves most surface plates (dark brown), which are recycled by sinking back into the deep mantle, where large low shear-wave velocity provinces (LLSVPs) exist (whitish). The ongoing plate destruction causes a more heterogeneous mantle and a surface of variable age, with young and thin oceanic plates and old and thick continental plates that remain at the surface. Mantle plumes (light red) tend to occur far away from sinking plates. By contrast, the mode of mantle convection on Venus is suggested to consist of a nearly immobile, mostly stagnant lid, and only localised, short sinking plate portions that are formed by (and thus spatially coincide with) hot mantle upwelling (light red). The resulting surface deformation matches observations from coronae on Venus. The short sinking portions do not, in contrast to Earth, significantly move their tail ends at the surface, which explains the uniformly aged, relatively thick surface plate (dark brown).

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Slab-gap dynamics

Sketch of an evolution of an opening and sinking slab gap during oceanic subduction and the resulting surrounding mantle flow.

Evolution of an opening and sinking slab gap during oceanic subduction. This conclusive image is based on analog models of subduction, where the slab surface was monitored by 3-D scanning and the mantle flow was imaged using PIV technique. The opening slab gap allows mantle to flow from the sub-slab area to the mantle wedge area. However, this flow might only have an effect on the surface when the slab gap is near-surface and has a significant vertical extent.

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Volcanic arc creation

A conceptual view of a volcanic arc growing through the evolution of magmatism in subduction zones controlled by fluid and melt fluxes.

A series of schematic cartoons (both as still and animated images) to show how a volcanic arc grows through the evolution of magmatism in subduction zones controlled by fluid and melt fluxes.

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Deep geologic water cycle

A schematic cartoon of the deep water cycle in the Earth’s mantle.

A schematic cartoon of the deep water cycle. Water percolates through the oceanic tectonic plates at the surface, hydrating the oceanic crust and lithospheric mantle below it. When the oceanic plates subduct, part of the water is released at shallow depths (<250 km) into the mantle wedge above the slab. This triggers mantle melting and the formation of volcanic arcs at the surface, in the overriding plate. The rest of the water stays in the slab and is carried deep down into the mantle. Depending on the subduction dynamics, this water can either be released at the mantle transition zone (410-660 km), where large amount of water can be stored in nominally anhydrous minerals, or go even deeper, up to the core-mantle boundary. Part of the water present in the mantle can then be released at the surface again by melt at intraplate volcanoes and mid-ocean ridges as it is transported by plumes and mantle convection.

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Earth processes

A schematic highlighting some of the most relevant Earth processes.

A schematic highlighting some of the most relevant Earth processes. Illustrated are an early Earth (without a fully developed solid inner core, left) that evolves into a dynamic, present-day-style Earth (right), which generates and erases geologic records of its transforming states and is now experiencing unprecedented environmental change. The arcuate lines surrounding globe illustrate the protective geomagnetic field that arises from the fluid dynamics within the outer core (light grey, illustrated with curled lines). The solid inner core is shown to scale as a darker grey. The mantle and crust (continental rocks are light brown, ocean floor basalts are dark brown; thicknesses greatly exaggerated, with mantle thickness to scale) is a single system driven by convection within the mantle that arises from radioactive decay of heat-producing elements and the loss of the deeply buried planet’s formational energy through cooling of the core. The lithosphere (crust and coldest mantle) is broken into separating and colliding plates whose distribution influence critical element distribution, earthquakes, volcanism, topography, critical zone, climate, water cycle, biogeochemistry, and biodiversity. The Earth is blanketed in a thin atmosphere (light blue). The profile of a landscape highlights Earth surface processes, the sedimentary record of Earth’s history, human influence, and geohazards to people. Displacement on faults may produce sudden strong earthquakes (creating significant hazards) or develop slowly with virtually imperceptible earthquakes. Landslides and coastal retreat, sea level rise, and tsunamis also present hazards to the coastal community. Uplifted hills will experience weathering (light brown) such that dense bedrock develops porosity and holds moisture and groundwater (light blue) that is exploited by vegetation. Deep groundwater aquifers (blue) are key water resources. Precipitation (blue lines) is returned to the atmosphere by evaporation and transpiration (blue dots) with excess water recharging groundwater or running off. Biologically-mediated gas exchange with the atmosphere occurs across the planet. Older sedimentary rocks (stippled brown) and young to contemporary sediments provide records of Earth’s evolving climate, biogeochemistry, and biodiversity. Humans are acting as geologic agents and affecting Earth processes in many ways, including through climate change (via urbanization, release of greenhouse gases, and vegetation change); nutrient input to terrestrial aquatic systems and the oceans (from agriculture and urban wastewater); changes in erosion and sedimentation (from land use change, dams, and other influences on river flow and sediment load); modification of the geographic distribution of biodiversity (from climate and land use change); and exacerbation of hazards (through rising sea level, more intense storms, land use change, and drought-induced wildland fires).

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Slab retreat dynamics

Three different ways to allow for fast subduction trench retreat.

Sketch of three different ways to allow for fast subduction trench retreat that are flattening of the slab from side view (top left), curvature of the slab from top view for narrow (top centre) and wide subduction zones (bottom), and partial slab damage (i.e., slab window) from side view (top right). Shown are initial (grey) and end position (black) of the plate and corresponding mantle flow (blue) that displaces mantle material from its initial region (orange) to its final region (green).

  • Creator: Fabio Crameri
  • This version: 12.09.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri from Crameri and Tackley (2014) is available via the open-access s-Ink repository.
  • Related reference: Crameri, F., and P.J. Tackley (2014), Spontaneous development of arcuate single-sided subduction in global 3-D mantle convection models with a free surface, J. Geophys. Res. Solid Earth, 119(7), 5921-5942, doi:10.1002/2014JB010939
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Subduction seismic anisotropy

Illustration of constraints on subduction zone seismic anisotropy from a global compilation of shear-wave splitting measurements.

Illustration of constraints on subduction zone seismic anisotropy from shear-wave splitting measurements from the compilation presented in Long (2013). The subduction trenches compiled by Bird (2003) are shown in black. The anisotropic signals of the wedge (orange) and back-slab regions (blue) are shown separately. Blue arrows indicate average fast directions for the back-slab splitting signal from SKS (seismic waves traveling through the Outer Core), local S, and source-side tele-seismic S-splitting measurements (Long and Silver, 2009; Paczkowski, 2012). Orange arrows indicate average fast directions for wedge anisotropy from local S splitting (Long and Wirth, 2013). In regions where multiple fast directions are shown, splitting patterns exhibit a mix of trench-parallel, trench-perpendicular, and oblique fast directions.

  • Creator: Fabio Crameri
  • This version: 01.09.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri after Crameri and Tackley (2014) and Long (2013) is available via the open-access s-Ink repository.
  • Related references:
    Crameri, F., and P.J. Tackley (2014), Spontaneous development of arcuate single-sided subduction in global 3-D mantle convection models with a free surface, J. Geophys. Res. Solid Earth, 119(7), 5921-5942, doi:10.1002/2014JB010939
    Long, M. D. (2013), Constraints on subduction geodynamics from seismic anisotropy, Rev. Geophys., 51, 76–112, doi:10.1002/rog.20008
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Slab tearing

Time-evolution of subduction slab break-off shown in a global spherical 3-D model.

Evolution of subduction slab tearing and eventual slab break-off shown in a global spherical 3-D model by contours of viscosity. The stiff down-going plate (yellow) is moving towards the observer before subduction and is starting to laterally tear apart at depth, while the remaining intact part continues to subduct.

  • Creator: Fabio Crameri
  • This version: 01.09.2021
  • License: Attribution-ShareAlike 4.0 International (CC BY-SA 4.0)
  • Specific citation: This graphic by Fabio Crameri from Crameri and Tackley (2014) is available via the open-access s-Ink repository.
  • Related reference: Crameri, F., and P.J. Tackley (2014), Spontaneous development of arcuate single-sided subduction in global 3-D mantle convection models with a free surface, J. Geophys. Res. Solid Earth, 119(7), 5921-5942, doi:10.1002/2014JB010939
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