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Cenozoic paleogeography (animation)

Global paleogeography with zoomed in figures showing the evolution of oceanic gateways active during the Cenozoic time.

Global paleogeography of Straume et al. (2020) with zoomed in figures showing the evolution of oceanic gateways active during the Cenozoic time (66 – 0 Ma).

  • High-res video format
  • Perceptually uniform colour map
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Paleo surface topography

Earth’s reconstructed global surface topography from the beginning of the Cenozoic era (66 Million years ago) until today.

Still images of the Earth’s global surface topography reconstructed through the Cenozoic time (66 – 0 Ma). Shown is the Straume et al. (2020) paleogeography model. The Scientific colour map ‘bukavu‘ is used to represent data accurately and to all readers.

  • Various time snapshots
  • Alternative map projections
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Paleo surface topography (animated)

Animations of the Earth’s global surface topography reconstructed through the Cenozoic time (66 – 0 Ma).

Animations of the Earth’s global surface topography reconstructed through the Cenozoic time (66 – 0 Ma). Shown is the Straume et al. (2020) paleogeography model. The Scientific colour map ‘bukavu‘ is used to represent data accurately and to all readers.

  • Alternative map projections
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  • Light & dark background versions
  • Perceptually uniform colour map
  • Colour-vision deficiency friendly
  • Readable in black&white

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3-D subduction mantle flow

3-D subduction dynamics and mantle flow model animation showing the time evolution of oceanic plate subduction and resulting mantle flow.

Animation of 3-D subduction dynamics and mantle flow showing the time evolution of oceanic plate subduction with a continental part in the middle and resulting mantle flow computed in a 3-D numerical model. Although only one specific geometry, this model is useful to visualise how slabs deform at depth, how mantle flows around their edges, and how back-arc basins form.

Description of the model evolution (see below for detailed legend) – In this model, the subducting plate is mostly oceanic, but has continental lithosphere in the middle and the overriding plate is continental (see top panels at Time 0 Myr). The oceanic slab (in blue) sinks into the mantle and, at Time 8.1 Myr, continental collision happens in the middle of the subduction zone. At this point, the trench stays quasi-stationary in the middle, but starts to retreat quickly at the sides and the slab significantly deforms at depth (from Time 9.8 Myr onward). This causes the mantle to quickly flow around the slab (see how the spheres move). The large trench retreat generates a significant amount of extension in the overriding plate that eventually causes the overriding plate to break (Time 28.4 Myr). At this point, the mantle material rises towards the surface and starts melting because of decompression in the back-arc region. Melt close to trench is due to the presence of fluids released from the slab and shows the location of the volcanic arc. As the slab keeps retreating, the opening of the back-arc basin, associated with mantle melting, continues creating a wider and wider basin that will be composed of new oceanic crust generated by mantle melting.

Legend – The 3 panels are showing different views of the same model: side/top view (top left panel), top view (top right panel), and front view (bottom panel). The slab is shown in blue, continental crust in grey. In the top view (top right panel), the subducting plate is on the left side and the overriding plate is the grey area to the left. The slab will subduct towards the right. The contour in the red-to-white colour map indicates the regions where the mantle melts and the amount of melt fraction. The spheres are tracers passively transported in the mantle and colour-coded by depth; they are useful to show how the mantle flows around the slab (toroidal flow).

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Global volcano distribution

Global distribution of active and inactive volcanoes as compiled in the NCEI Volcano Location Database.

Global distribution map of active and inactive volcanoes as compiled in the NCEI Volcano Location Database available at https://www.ngdc.noaa.gov/hazel/view/hazards/volcano/loc-data.

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Historic earthquake distribution

Global distribution map of large 5.8+ magnitude historic earthquakes derived from seismic wave measurements.

Global map showing the distribution of large 5.8+ magnitude historic earthquakes derived from seismic wave measurements after the compilation by Hayes (2018). Shown are individual epicentres coloured by depth. For a nice looking poster graphic, see s-ink.org/earthquake-distribution-map-poster .

The Scientific colour map ‘oslo‘ is used to represent earthquake depth accurately and to all readers.

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Light spectrum (approximation)

Approximate RGB values for the visible wavelengths of the light spectrum.

Approximate RGB values for the visible wavelengths of the light spectrum after Dan Bruton – Color Science.

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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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