A physicist's journey to the centre of the Earth

It is a paradox that, despite it being the planet on which all our experience is founded, the bulk Earth is as inaccessible as a remote galaxy. In South African diamond mines, man has penetrated about 3 km into the solid Earth; intact core from boreholes has been recovered from about 7 km and, in th...

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Veröffentlicht in:Physics education 1999-07, Vol.34 (4), p.167-167
1. Verfasser: Hipkin, Roger
Format: Artikel
Sprache:eng
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Zusammenfassung:It is a paradox that, despite it being the planet on which all our experience is founded, the bulk Earth is as inaccessible as a remote galaxy. In South African diamond mines, man has penetrated about 3 km into the solid Earth; intact core from boreholes has been recovered from about 7 km and, in the Kola Peninsula of northern Russia, drill chippings have been sluiced up from about 13 km. Nevertheless, even if we had the resources to pepper the outer layer with exploratory boreholes, direct observation of the remaining 99% of the Earth's volume will always remain an impossibility. And yet we know some quite detailed properties of the interior of the Earth. Contrary to primitive cosmologies inspired by watching volcanoes erupt, and although below 2890 km there is a core of molten steel, we know that only in rare, shallow and isolated pockets are the rocks of the Earth's interior molten. The interior of the Earth is like an onion-skin: properties (density, electrical conductivity, sound speed etc) change mainly with depth. Taking the Earth's response to stress as one example, the material behaves like a brittle elastic solid only to depths of about 10-20 km. Below that, Earth materials exhibit the properties of both a solid and a liquid: to short-period effects like sound waves, they respond as a conventional solid but, when subjected to long-period stress, they can also flow like a liquid with a very high viscosity. Viscosity is initially controlled by the increasing mobility of atoms as temperature increases (viscosity decreases from about 1025 Pa s in the upper 20 km to about 1020 Pa s at a depth of 250 km); but atomic mobility is then offset by the counteracting effects of increasing pressure (viscosity increases to perhaps 1023 Pa s at 2500 km). We also have a quantitative physical picture of Earth behaviour stretching back over 4.5 billion years, despite having only 4500 years of recorded scientific observations about the Earth. Using the same physics that designed the platework of ships and bridges, we see the upper elastic layer of the Earth bending under the loads applied by mountains and ice sheets: about 11 000 years ago, a 2 km load of ice melted, and Scandinavia and northern Canada are still springing back into shape at about 10 mm per year. About 100 million years ago, the plate supporting North America and Europe fractured, and we can measure their continuing separation with lasers and microwaves at a few cm per year. We are now just able to m
ISSN:0031-9120
1361-6552
DOI:10.1088/0031-9120/34/4/001