years (contingent on what we do), and the one after that, but at some point there could be some tectonic processes that make things more like the Cretacious — and there is probably some time horizon for the weather
of mantle convection, too, while the climate of the mantle (layered vs whole vs mixed convection, general descriptions of cell sizes and rates of motion) may be predicted for longer time frames.
For this effort the observed history of plate tectonics could be imposed as velocity boundary conditions in dynamic calculations
of mantle convection using a spherical geometry and realistic constitutive relations for geologic materials.
He calls this theory «top - down tectonics,» based on Kelvin's initial principles
of mantle convection.
The answer to this question is very important for us to understand the nature
of mantle convection,» explains lead author Mingming Li, who is pursuing his Ph.D. in geological sciences.
What we have done is to simulate the process
of mantle convection by solving the equations which controls the process
of mantle convection,» says Li.
«Based on our models
of mantle convection, the mantle may be removing as much as half of Earth's total convective heat budget from the core,» Rowley said.
Not exact matches
Hotspots were thought to be caused by a narrow stream
of hot
mantle convecting up from the
mantle - core boundary called a
mantle plume, the latest geological evidence is pointing to upper -
mantle convection as a cause.
«It gives us some insight into the connection between the slow circulation
of near - solid rock in Earth's
mantle caused by
convection currents carrying heat upwards from the planet's interior, and observed active plate tectonics at the surface.
Another possible scenario is that small - scale
convection is taking place within the channel as chunks
of mantle cool and sink.
«These images will help us understand how
convection connects Earth's surface with the bottom
of the
mantle,» said Associate Professor Tkalčić.
The plume's more southern location, Toomey said, adds fuel to his group's findings, at three different sites along the globe encircling mid-ocean ridge (where 85 percent
of Earth's volcanic activity occurs), that Earth's internal
convection doesn't always adhere to modeling efforts and raises new questions about how ocean plates at Earth's surface — the lithosphere — interact with the hotter, more fluid asthenosphere that sits atop the
mantle.
«Learning about the anatomy
of the
mantle tells us more about how the deep interior
of Earth works and what mechanisms are behind
mantle convection,» said Nicholas Schmerr, an assistant professor
of geology at UMD and co-author
of the Science Advances paper that addresses
mantle density and composition.
«There seems to be this critical filter and control on the movement
of slabs and therefore
convection of the
mantle,» Klein says.
«This seems to suggest there was a big change going back in Earth's history in terms
of how
mantle convection and plate tectonic processes would have happened.»
Jagoutz says the results suggest that sometime between 3 billion years ago and today, as the Earth's interior cooled, the
mantle switched from a one - layer
convection system, in which slabs flowed freely from upper to lower layers
of the
mantle, to a two - layer configuration, where slabs had a harder time penetrating through to the lower
mantle.
Meanwhile the MOLA data suggest that the elliptical northern hemisphere depression, some
of the flattest terrain ever mapped, may have been an ancient seabed shaped by vigorous
convection of the planet's
mantle or tectonic plate recycling during the planet's formative stages.
Although the heat from impacts may not have been a limiting factor for life, asteroid bombardment introduced numerous other challenges, affecting the climate, surface or even
convection of the
mantle.
Convection, or the flow
of mantle material transporting heat, drives plate tectonics.
It also was thought that planets were able to self - regulate their internal temperature via
mantle convection — the underground shifting
of rocks caused by internal heating and cooling.
Such diversity
of size and internal temperature would not hamper planetary evolution if there was self - regulating
mantle convection, Korenaga said.
Using Australia's National Computational Infrastructure's supercomputer Raijin, the team created high - resolution three - dimensional simulations
of mantle evolution over the past 200 million years to understand the coupling between
convection in the deep Earth and volcanism.
«The deflection
of the plumes into these finger - like channels represents an intermediate scale
of convection in the
mantle, between the large - scale circulation that drives plate motions and the smaller scale plumes, which we are now starting to image.»
Through
convection — slow movements
of material in the upper
mantle — the material was eventually mixed around and carried to the area
of the mid-ocean ridges and transported back to the surface in the lavas that make up MORBs.
But he adds, «If the ultra-low velocity pockets
of rock have a composition different from the ordinary
mantle rock, then
mantle convection would continually carry them to the edges
of piles where they collect.
This cooling and plate tectonics drives
mantle convection, the cooling
of the core, and Earth's magnetic field.
These ranged from global
mantle - scale
convection patterns, to the large thermochemical piles in the lower
mantle, and down to the very small - scale pockets
of ultra-low velocity zone at the bottom.
But this new study supports researchers» growing suspicion that
mantle convection somehow regulates the amount
of water in the oceans.
From there, the same
convection of mantle rock that produces plate tectonics could carry the water to the surface.
Now Yoshida and Madhava Santosh
of Kochi University, Japan, have modelled how
convection in the
mantle — including the superplumes — will drive plate motion over the next 250 million years.
slow movement
of Earth's solid
mantle caused by
convection currents transferring heat from the interior
of the Earth to the surface.
The team calculated the balance between tidal heating and heat transport by
convection in the
mantles of each planet.
In contrast, super-Earths with a similar concentration but larger absolute amount
of radioactive heat sources (i.e., uranium and thorium) than Earth would produce more internal heat, more vigorous
mantle convection, and faster plate tectonic action involving thinner plates, which may promote planetary habitability with lower mountain ranges but higher volcanic activity and an atmosphere with a greater relative composition
of volcanic and lighter gases (Sasselov and Valencia, Scientific American, August 2010; Valencia and O'Connell, 2009; and Valencia et al, 2007).
Scientists now recognize that macroscale behaviors, such as plate tectonics and
mantle convection, arise from the microscale properties
of Earth materials, including the smallest details
of their atomic structures.
My first article on the subject (published Sep. 2009) refers to the
convection in the underlying
mantle (as reflected in changes
of the area's magnetic intensity) is making significant contribution to the Atlantic basin climate change.
Convection of the
mantle is expressed at the surface through the motions
of tectonic plates.
The
mantle is not quite solid and consists
of magma which is in a state
of semi-perpetual
convection.
Kelvin modeled this as pure conduction, thinking
of the
mantle as too solid to admit
convection.
Source and sink
of heat, temperature at the start
of the 10 billion years, mechanism
of heat transfer through the
mantle (conduction or
convection?).
«The advent
of plate tectonics made the classical
mantle convection hypothesis even more untenable.
The evidence presented by Wegener and du Toit has been largely confirmed by global plate tectonics, and Holmes's causal account —
mantle convection — is now generally accepted as the cause
of plate tectonics.
Convection, or the flow
of mantle material transporting heat, drives plate tectonics.