Core

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EARTH
Magnetosphere Exosphere Atmosphere
Ionosphere Thermosphere
Mesosphere
Hydrosphere Biosphere Stratosphere
Troposphere
Peplosphere
Pedosphere Lithosphere Crust Geosphere
Upper Crust
Lower Crust
Upper Mantle Lithospheric Mantle Mantle
Asthenosphere
Deeper Upper Mantle
Lower Mantle
Outer Core Core
Inner Core
Topics: Climate | Composition of the Earth | Formation of the Earth | Gaia Hypothesis | Geography | History of the Earth | Plate tectonics | Structure of the Earth


[edit] The Earth's Core

The average density of Earth is 5515 kg/m3, making it the densest planet in the Solar system. Since the average density of surface material is only around 3000 kg/m3, we must conclude that denser materials exist within Earth's core. Further evidence for the high density core comes from the study of seismology. In its earliest stages, about 4.5 billion years ago, melting would have caused denser substances to sink toward the center in a process called planetary differentiation, while less-dense materials would have migrated to the crust. As a result, the core is largely composed of iron (80%), along with nickel and one or more light elements, whereas other dense elements, such as lead and uranium, either are too rare to be significant or tend to bind to lighter elements and thus remain in the crust (see felsic materials).

Seismic measurements show that the core is divided into two parts, a solid inner core with a radius of ~1220 km and a liquid outer core extending beyond it to a radius of ~3400 km. The solid inner core was discovered in 1936 by Inge Lehmann and is generally believed to be composed primarily of iron and some nickel. Some have argued that the inner core may be in the form of a single iron crystal. (ref: [1]) The liquid outer core surrounds the inner core and is believed to be composed of iron mixed with nickel and trace amounts of lighter elements. It is generally believed that convection in the outer core, combined with stirring caused by the Earth's rotation (see: Coriolis effect), gives rise to the Earth's magnetic field through a process described by the dynamo theory. The solid inner core is too hot to hold a permanent magnetic field (see Curie temperature) but probably acts to stabilise the magnetic field generated by the liquid outer core.

Recent evidence has suggested that the inner core of Earth may rotate slightly faster than the rest of the planet. In August 2005 a team of geophysicists announced in the journal Science that, according to their estimates, Earth's inner core rotates approximately 0.3 to 0.5 degrees per year relative to the rotation of the surface.(ref [2] ) ~0-2°per year (ref. Neil F. Comins DEU-p.82)

It is estimated that due to the cooling of earth, the inner solid core increses in size each year (in the order of cm).

While the scientifically mainstream explanation for these temperature gradients is that the heat is simply left over from the planet's initial formation, a theory espoused by J. Marvin Herndon states that fast breeder nuclear reactor type reactions occur in the core of Earth. [ref [3])


[edit] Credits

This page incorporates material from Wikipedia which is available under the terms of the GNU Free Documentation License. Wikipedia url for material on this page:
http://en.wikipedia.org/wiki/Structure_of_the_Earth#Core
Retrieved from "http://www.palaeos.org/Core"
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