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Abstract of article
Geology of Ore Deposits

 -  Vol. 47, No. 6, November-December 2005, pp. 455-468 Help

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Mantle Magmas as a Sensor of the Composition of Deep Geospheres
I. D. Ryabchikov
Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), Russian Academy of Sciences, Staromonetnyi per. 35, Moscow, 119017 Russia

Received July 15, 2005

It was shown that the material of deep plumes is characterized by ordinary contents of volatile components, similar to those of the bulk silicate Earth or even lower. The tight correlation of volatile components with certain nonvolatile incompatible components suggests that there is no large-scale additional input of volatile components, for instance, as deep fluid flows from the Earth's core. Even accounting for the presence of volatile components, the estimated temperatures of plume material during the initial stages of magma formation are much higher than temperatures in the upper part of the asthenosphere, which is in agreement with the thermal nature of mantle plumes. The finds of metallic phases in mantle xenoliths and a number of geochemical characteristics of plume-related magmas are compatible with the suggestion that the largest mantle plumes are generated at the core–mantle boundary. Magma-producing mantle plumes may form in the interiors of various planets through various mechanisms: the formation of low-density blocks in thermal boundary layers (D″ or the upper boundary of the lower mantle for the Earth) or deep mantle heterogeneity with respect to the distribution of radioactive elements inherited from the time of solidification of the early magma ocean (for Mars).

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PII: S1075701505060024

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