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13 - Carbon-Bearing Phases in the Mantle

Published online by Cambridge University Press:  19 December 2020

Simon Mitton
Affiliation:
University of Cambridge
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Summary

Earth is the only known habitable planet in the solar system. Although there are half a dozen planetary moons that may have habitable zones beneath their surfaces, astronomers have yet to find an exoplanet with conditions deemed suitable for life on its surface. From a geological point of view, Earth’s distinctive features include the presence of life, the abundance of liquid water, the long-term tectonic system and the profusion of organic carbon in contact with the oxygen-bearing atmosphere. The carbon cycle inextricably binds biological life at the surface with carbon on the move in the interior. Through laboratory experiments, we have discovered that, following subduction, carbon-bearing materials undergo great transformation in the high-pressure hothouse of the mantle. Earth’s subduction factory plays a key role in the deep carbon cycle by feeding the mantle with different carbon phases, four-fifths of which are carbonates and one-fifth organic carbon, proportions that have remained relatively stable since Earth’s biosphere became established.

Type
Chapter
Information
From Crust to Core
A Chronicle of Deep Carbon Science
, pp. 261 - 281
Publisher: Cambridge University Press
Print publication year: 2020

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References

Bridgman, P. W. The measurement of high hydrostatic pressure. II. A secondary mercury resistance gauge. Proceedings of the American Academy of Arts and Sciences 44, 221251 (1909).CrossRefGoogle Scholar
Bridgman, P. W. Rough compression of 177 substances to 40,000 kg/cm2. Proceedings of the American Academy of Arts and Sciences 76, 7187 (1948).CrossRefGoogle Scholar
Bridgman, P. W. An experimental contribution to the problem of diamond synthesis. The Journal of Chemical Physics 15, 9298 (1947).CrossRefGoogle Scholar
Hazen, R. M. The Diamond Makers (Cambridge University Press, 1999).Google Scholar
Bridgman, P. W. Synthetic diamonds. Scientific American 193, 4247 (1955).CrossRefGoogle Scholar
Coes, L. A new dense crystalline silica. Science 118, 131132 (1953).Google Scholar
Hall, H. T. Personal experiences in high pressure. The Chemist July, 276–279 (1970).Google Scholar
Goldschmidt, V. M. Geochemistry. 78 (LWW, 1954).Google Scholar
Yoder, H. S. Planned Invasion of Japan, 1945: The Siberian Weather Advantage. 223 (American Philosophical Society, 1997).Google Scholar
Ernst, W. G., Hazen, R. M. and Mysen, B. Biographical Memoir of S. Yoder Jr. (1921–2003) (National Academy of Sciences, 2014).Google Scholar
Yoder, H. S. Generation of Basaltic Magma (National Academies, 1976).Google Scholar
Yoder, H. S. Jr and Tilley, C. E. Origin of basalt magmas: an experimental study of natural and synthetic rock systems. Journal of Petrology 3, 342532 (1962).CrossRefGoogle Scholar
Holmes, A. The thermal history of the earth. Journal of the Washington Academy of Sciences 23, 169195 (1933).Google Scholar
Bridgman, P. W. The Physics of High Pressure (G. Bell & Sons, 1931).Google Scholar
Tammann, G. Aggregatzustände: Die Zustandsänderungen der Materie in Abhängigkeit von Druck und Temperatur (Leopold Voss, 1923).Google Scholar
Gutenberg, B. and Richter, C. F. On supposed discontinuities in the mantle of the earth. Bulletin of the Seismological Society of America 21, 216223 (1931).CrossRefGoogle Scholar
Li, J. et al. Deep carbon cycle through five reactions. American Mineralogist 104, 465467 (2019).CrossRefGoogle Scholar
Moody, J. B. Serpentinization: a review. Lithos 9, 125138 (1976).CrossRefGoogle Scholar
Strutt, R. J. Measurements of the rate at which helium is produced in thorianite and pitchblende, with a minimum estimate of their antiquity. Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character 84, 379388 (1910).Google Scholar
Hazen, R. M. et al. Mineral evolution. American Mineralogist 93, 16931720 (2008).Google Scholar
Hazen, R. M., Downs, R. T., Kah, L. and Sverjensky, D. Carbon mineral evolution. Reviews in Mineralogy and Geochemistry 75, 79107 (2013).CrossRefGoogle Scholar
Hazen, R. M., Grew, E. S., Downs, R. T., Golden, J. and Hystad, G. Mineral ecology: chance and necessity in the mineral diversity of terrestrial planets. The Canadian Mineralogist 53, 295324 (2015).Google Scholar
Grew, E. S. and Hazen, R. M. Beryllium mineral evolution. American Mineralogist 99, 9991021 (2014).CrossRefGoogle Scholar
Hazen, R. M. et al. Earth’s “missing” minerals. American Mineralogist 100, 23442347 (2015).Google Scholar
Hazen, R. M., Hummer, D. R., Hystad, G., Downs, R. T. and Golden, J. J. Carbon mineral ecology: predicting the undiscovered minerals of carbon. American Mineralogist 101, 889906 (2016).CrossRefGoogle Scholar
Jefferson, T. Letter to Daniel Salmon (1808).Google Scholar
The Carbon Mineral Challenge. Rock&Gem (2016).Google Scholar
Shahar, A., Driscoll, P., Weinberger, A. and Cody, G. What makes a planet habitable? Science 364, 434435 (2019).CrossRefGoogle ScholarPubMed

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