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Magma forms far deeper than geologists previously thought, according to new research results.
A
team led by geologist Rajdeep Dasgupta of Rice University put very
small samples of peridotite, rock derived from Earth's mantle, under
high pressures in a laboratory.
The scientists found that the rock
can and does liquify, at least in small amounts, at pressures
equivalent to those found as deep as 250 kilometers down in the mantle
beneath the ocean floor.
Dasgupta said that this answers several questions about Earth's inner workings.
He is the lead author of a paper that appears today in the journal Nature. The research was funded by the National Science Foundation (NSF).
"The
results show that in some parts of the National Science Foundation (NSF). melting, or magma
formation, happens very deep beneath Earth's surface," said geologist
Jennifer Wade, a program director in NSF's Division of Earth Sciences,
which funded the research.
"It also means that some carbon dioxide
and water could come from different sources--and deeper within the
Earth--than we believed."
The mantle is the planet's middle layer, a buffer of rock between the crust--the top five miles or so--and the Earth's core.
If
one could compress millions of years of observation of the mantle to
mere minutes, the mantle would look like a rolling mass of rising and
falling material.
This slow but constant churning convection
brings materials from deep within the Earth to the surface, and higher,
through volcanic eruptions.
The team focused on the mantle beneath
the ocean because that's where crust is created and where, Dasgupta
said, "the connection between the interior and surface world is
established."
Magma rises with convective currents, then cools and spreads out to form ocean-floor crust.
The starting point for melting has long been thought to be at 70 kilometers beneath the seafloor.
That had confounded geologists who had suspected, but could not demonstrate, the existence of deeper magma, said Dasgupta.
For
example, when scientists try to determine the mantle's density, they do
so by measuring the speed of a seismic wave after an earthquake, from
its origin to other points on the planet.
Because such waves
travel faster through solids (e.g., crust) than through liquids (e.g.,
magma), geologists had been surprised to detect waves slowing down, as
though passing through liquid, in a zone that should be the mantle's
faster "express lane."
"Seismologists have observed anomalies in velocity data as deep as 200 kilometers beneath the ocean floor," Dasgupta said.
"It turns out that trace amounts of magma are generated at this depth, which would potentially explain that" slower velocity.
The research also offers clues to the electrical conductivity of the oceanic mantle.
"The
magma at such depths has a high enough concentration of dissolved
carbon dioxide that its conductivity is very high," Dasgupta said.
But,
because scientists have not yet been able to sample the mantle
directly, researchers have had to extrapolate from the properties of
rocks carried up to the surface.
So, in a previous study,
Dasgupta determined that melting in Earth's deep upper mantle is caused
by the presence of carbon dioxide.
The present study shows that
carbon helps to make silicate magma at significant depths. And, the
researchers also found that carbonated rock melts at significantly lower
temperatures than non-carbonated rock.
"This deep melting makes
the silicate differentiation [changes in silicate distribution that
range from the dense metallic core, to the less-dense silicate-rich
mantle, to the thinner crust] of the planet much more efficient than
previously thought," Dasgupta said.
"Deep magma is the main agent that brings all the key ingredients for life--water and carbon--to the surface of the Earth."
In
Dasgupta's high-pressure lab, volcanic rocks are windows to the
planet's interior. The researchers crush tiny rock samples that contain
carbon dioxide to find out how deep magma forms.
"We have all the
necessary tools to simulate very high pressures--to nearly 750,000
pounds per square inch--and temperatures," he said. "We can subject
small amounts of rock to these conditions to see what happens."
The
geologists use powerful hydraulic presses to partially melt rocks that
contain tiny amounts of carbon, simulating what they believe is
happening under equivalent pressures in the mantle.
"When rocks
come from deep in the mantle to shallower depths, they cross . . . the
solidus [boundary], where rocks begin to undergo partial melting and
produce magmas," Dasgupta said.
"Scientists knew the effect of a
trace amount of carbon dioxide or water would lower this boundary, but
our new estimation made it 150-180 kilometers deeper from the known
depth of 70 kilometers," he said.
"What we are now saying is that
with just a trace of carbon dioxide in the mantle, melting can begin as
deep as around 200 kilometers.
"When we incorporate the effect of trace water, the magma generation depth becomes at least 250 kilometers."
The
extent of magma generation is larger than previously thought, he said,
and, as a consequence, has the capacity to affect the geophysical and
geochemical properties of the entire planet.
Co-authors of the
paper are Ananya Mallik and Kyusei Tsuno at Rice University; Anthony
Withers and Marc Hirschmann at the University of Minnesota; and Greg
Hirth at Brown University.
The study was also supported by a Packard Fellowship to Dasgupta.
-NSF-
Media Contacts
Cheryl Dybas, NSF (703) 292-7734 cdybas@nsf.gov
Mike Williams, Rice University (713) 348-6728 mikewilliams@rice.edu
Mike Williams, Rice University (713) 348-6728 mikewilliams@rice.edu
The National Science Foundation (NSF) is an independent federal
agency that supports fundamental research and education across all
fields of science and engineering. In fiscal year (FY) 2012, its budget
is $7.0 billion. NSF funds reach all 50 states through grants to nearly
2,000 colleges, universities and other institutions. Each year, NSF
receives over 50,000 competitive requests for funding, and makes about
11,000 new funding awards. NSF also awards nearly $420 million in
professional and service contracts yearly.
Useful NSF Web Sites:
NSF Home Page: http://www.nsf.gov
NSF News: http://www.nsf.gov/news/
For the News Media: http://www.nsf.gov/news/newsroom.jsp
Science and Engineering Statistics: http://www.nsf.gov/statistics/
Awards Searches: http://www.nsf.gov/awardsearch/
NSF Home Page: http://www.nsf.gov
NSF News: http://www.nsf.gov/news/
For the News Media: http://www.nsf.gov/news/newsroom.jsp
Science and Engineering Statistics: http://www.nsf.gov/statistics/
Awards Searches: http://www.nsf.gov/awardsearch/
The National Science Foundation (NSF)
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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