April 2, 2007 (Press Release) --
The findings will help geologists as they seek to understand how heat is transferred through the planet's interior, which drives all geologic processes like earthquakes and volcanoes, and Earth's magnetic field.
Robert van der Hilst of MIT and his colleagues studied an region under Central America by monitoring earthquake-generated seismic waves in real time. The speed of the seismic waves indicates the chemical and physical properties of the material they encounter.
The waves penetrate thousands of miles beneath Earth's surface, effectively taking the temperature of the boundary between Earth's core and the surrounding mantle by combining this seismic data with mineral physics. The team calculated the temperature at this boundary as well as above and below it.
Specifically, a mineral called perovskite transforms into so-called post-perovskite at certain temperatures and pressures. The location of the core-mantle boundary, a place where abrupt temperature and pressure changes occur, can be identified by locating the exact spot of this mineral transition. The scientists' calculations put this temperature at about 6,650 degrees. Scientists estimate Earth's inner core to be about 9,000 degrees.
Combined with a past study that estimated heat loss in an area beneath the Pacific Ocean, the research team suggests Earth's total heat loss at the core-mantle boundary is about 7.5 to 15 terawatts, much higher than previous estimates. Global energy use by humans is about 13 terawatts.
From their measurements, the scientists estimate about one-third of the heat that radiates from Earth's surface into the atmosphere -- estimated to be 42 terawatts -- comes from our planet's core.
The new temperature measurements will also help geoscientists refine their understanding our planet's magnetic field, which protects us from cosmic rays and solar storms. The field fluctuates over time, for reasons not fully understood, and now and then it even shrinks to zero before flipping polarity entirely.
The turbulent flow is the result of convection, and a higher rate of heat loss indicates more convection and a faster flow. With computer simulations, scientists have estimated the amount of energy needed to maintain the magnetic field. But this study is arguably the first to nail down concrete estimates, not computer-modeled ones, of these temperatures, van der Hilst said.
"The heat flow that we measure is larger than what is needed to drive the geo-dynamo, so there is actually more energy down there than people thought," van der Hilst told LiveScience.
The findings are reported in the March 30 issue of the journal Science.
Source: http://news.xinhuanet.com/
Robert van der Hilst of MIT and his colleagues studied an region under Central America by monitoring earthquake-generated seismic waves in real time. The speed of the seismic waves indicates the chemical and physical properties of the material they encounter.
The waves penetrate thousands of miles beneath Earth's surface, effectively taking the temperature of the boundary between Earth's core and the surrounding mantle by combining this seismic data with mineral physics. The team calculated the temperature at this boundary as well as above and below it.
Specifically, a mineral called perovskite transforms into so-called post-perovskite at certain temperatures and pressures. The location of the core-mantle boundary, a place where abrupt temperature and pressure changes occur, can be identified by locating the exact spot of this mineral transition. The scientists' calculations put this temperature at about 6,650 degrees. Scientists estimate Earth's inner core to be about 9,000 degrees.
Combined with a past study that estimated heat loss in an area beneath the Pacific Ocean, the research team suggests Earth's total heat loss at the core-mantle boundary is about 7.5 to 15 terawatts, much higher than previous estimates. Global energy use by humans is about 13 terawatts.
From their measurements, the scientists estimate about one-third of the heat that radiates from Earth's surface into the atmosphere -- estimated to be 42 terawatts -- comes from our planet's core.
The new temperature measurements will also help geoscientists refine their understanding our planet's magnetic field, which protects us from cosmic rays and solar storms. The field fluctuates over time, for reasons not fully understood, and now and then it even shrinks to zero before flipping polarity entirely.
The turbulent flow is the result of convection, and a higher rate of heat loss indicates more convection and a faster flow. With computer simulations, scientists have estimated the amount of energy needed to maintain the magnetic field. But this study is arguably the first to nail down concrete estimates, not computer-modeled ones, of these temperatures, van der Hilst said.
"The heat flow that we measure is larger than what is needed to drive the geo-dynamo, so there is actually more energy down there than people thought," van der Hilst told LiveScience.
The findings are reported in the March 30 issue of the journal Science.
Source: http://news.xinhuanet.com/

Scientists have stuck a thermometer in the Earth's inner core and found it's really, really hot -- about 9,000 degrees Farhrenheit, just 1,000 degrees cooler than the sun's surface.
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