Geology is an amazing subject. Especially now when so much is happening around the world in terms of volcanic eruptions and seismic activities. Let’s review how the interior of the Earth is structured.
We'll take a journey into the depths of the Earth, down through the crust and mantle nearly to the core. We’ll use seismic waves to show the way, since they echo through the planet following an earthquake and reveal its internal structure, like radar waves. #ScienceUnmasked#EarthCore
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Do chemical leftovers from the early Earth sit near its core?
Let's take a journey into the depths of the Earth down through the crust and
mantle nearly to the core. We'll use seismic waves to show the way.
Since they echo through the planet following an earthquake and reveal its
internal structure like radar waves, down near the core there are zones where
seismic waves slow to a crawl. New research from the
University of Utah finds that these enigmatic and descriptively named
Modeling suggests that it's possible some of these zones are leftovers from
the processes that shaped the early Earth.
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Remnants of incomplete mixing like clumps of flour in the bottom of a bowl
of batter. Michael S Thorne, Associate Professor
in the Department of Geology and Geophysics said
that of all the features we know about in the deep mantle
ultra-low velocity zones represent what are probably the most extreme
features found anywhere on the planet. Into the mantle.
Let's review how the interior of the Earth is structured.
We live on the crust, a thin layer of solid rock.
Between the crust and the iron nickel core at the center of the planet is the
mantle. It's not an ocean of lava. Instead it's
more like solid rock but hot and with an ability to
move that drives plate tectonics at the surface.
How can we have an idea what's going on in the mantle and the core?
Seismic waves. As it ripples through the Earth after an earthquake scientists on
the surface can measure how and when the waves arrive at monitoring
stations around the world. From those measurements they can back
calculate how the waves were reflected and deflected by
structures within the Earth including layers of different densities.
That's how we know where the boundaries are between the crust
mantle and core and partially how we know
what they're made of. Ultra-low velocity zones sit at the bottom of the mantle
atop the liquid metal outer core. In these areas seismic waves slow
as much as half and density goes up by a third.
Scientists initially thought that these zones were areas where the mantle was
partially melted and might be the source of
magma for so-called hotspot volcanic regions like Iceland.
However Professor Thorne pointed out that most of the things we call
ultra-low velocity zones don't appear to be located beneath
hotspot volcanoes. So that cannot be the whole story. So he
and his team set out to explore an alternative hypothesis
that the ultra-low velocity zones may be regions
made of different rocks than the rest of the mantle and that their composition
may harken back into the early Earth. Professor Thorne believes that perhaps
ultra-low velocity zones could be collection of iron oxide
which we see as rust at the surface but that can behave as a metal in the deep
mantle. If that's the case pockets of iron oxide
just outside of the core might influence the Earth's
magnetic field that is generated just below.
Reverse engineering seismic waves. To get a clear picture the researchers studied
ultra-low velocity zones beneath the Coral Sea
between Australia and New Zealand. It's an ideal location because of abundance
of earthquakes in the area that provide a high resolution seismic picture
of the core mantle boundary. The hope was that high resolution observations could
reveal more about how ultra-low velocity zones are put together.
But getting a seismic image of something through nearly 1800 miles of crust and
mantle isn't easy. It's also not always conclusive. A thick
layer of low velocity material might reflect seismic waves the same way
as a thin layer of even lower velocity material.
So the team used a reverse engineering approach.
Pachai said that they can create a model of the Earth that includes ultra-low
wave speed reductions and then run a computer simulation
that shows what the seismic wave form would look like
if that is what the Earth actually looked like.
Then they would compare those predicted recordings with the recordings that
they actually have. Over hundreds of thousands of models run
the method called Bayesian inversion yields a mathematically robust model of
the interior with a good understanding of the
uncertainties and traders of different assumptions in the model.
One particular question that researchers wanted to answer is whether there are
internal structures such as layers within ultra-low velocity
zones. The answer according to the model is that
the layers are highly likely. This is a big deal because it shows that
the way to understanding how these zones came to be.
Looking back at the origins of the early Earth,
what does it mean that there are likely layers? More than four billion years ago
while dense iron was sinking to the core of the early Earth
and lighter materials were floating up into the mantle, a planetary object about
the size of Mars may have slammed into the
very early Earth. The collision may have thrown debris into Earth
orbit and that could have later formed the Moon.
It also raised the temperature of the early Earth significantly
as you might expect from two planets smashing into each other.
As a result, a large body of molten material known as magma ocean is formed.
The ocean would have consisted of rock, gases and crystals suspended in the
magma. The ocean would have sorted itself out as
it cooled with dense materials sinking and layering onto the bottom of the
mantle. Over the following billions of years as
the mantle churned and convected, the dense layers would have been
pushed into small patches showing up as the layer
ultra low velocity zones we see today. Patchi said that this finding changes
scientists view on the original and dynamics of ultra low velocity zones.
This type of ultra low velocity zone can be explained by chemical
heterogeneity is created at the very beginning of the Earth's history
and that they are still not well mixed after 4.5 billion years of mantle
convection. Not the final word. The study provides
some evidence of the origins of some ultra low velocity zones although
there's also evidence that suggests that different origins for
others such as the melting of the ocean's crust that's sinking back into
the mantle. But if at least some ultra low velocity
zones are leftovers from the early Earth, they preserve some of the history of the
planet that otherwise have been lost. This
discovery provides a tool to understand the initial
thermal and chemical status of Earth's mantle
and their long-term evolution. That's all from Science Unmasked. Remember to
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