Earth's core is rotating much slower than previously believed


Scientists believe they have achieved the first accurate estimate of how much faster Earth's core is rotating compared to the rest of the planet. University of Cambridge study has discovered that earlier estimates of one degree quicker each year were wrong. The core is actually moving much slower than previously believed – approximately one degree faster every million years.

Material from the fluid outer core solidifies onto its surface, making Earth's inner core grows very slowly over time. During this process, an east-west hemispherical difference in velocity is frozen into the structure of the inner core.

Lead researcher Lauren Waszek, a PhD student from the university's Department of Earth Sciences, said:

'The faster rotation rates are incompatible with the observed hemispheres in the inner core because it would not allow enough time for the differences to freeze into the structure. 'This has previously been a major problem, as the two properties cannot co-exist. 'However, we derived the rotation rates from the evolution of the hemispherical structure, and thus our study is the first in which the hemispheres and rotation are inherently compatible.'

Scientists used seismic body waves which pass through the inner core – 5 200km beneath the surface of the Earth – and compared their travel time to waves which reflect from the inner core surface. The difference between the travel times of these waves provided them with the velocity structure of the uppermost 90 km of the inner core.

Because the inner core grows over time the deeper structure is therefore older. The shift in the boundaries between the two hemispheres results in the inner core rotating with time. As the inner core grows, the heat released during solidification drives convection in the fluid in the outer core. This result is the first observation of such a slow inner core rotation rate.

This convection generates the Earth's geomagnetic field which protects our planet from solar radiation.

'It therefore provides a confirmed value which can now be used in simulations to model the convection of Earth's fluid outer core, giving us additional insight into the evolution of our magnetic field.'

The scientists' findings are published in the journal Nature Geoscience.

Featured image: Ilustration of inner core. Credit: NASA


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