Dry peralkaline felsic liquids and carbon dioxide flux through the Kenya rift zone
Dry peralkaline felsic liquids and carbon dioxide flux through the Kenya rift zone
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通讯作者:
Editor B. o. Mysen;D. K. Bailey;R. Macdonald
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作者:
Editor B. o. Mysen;D. K. Bailey;R. Macdonald
-Around Lake Naivasha, at the topographic culmination of the Kenya rift, a wide range of peralkaline felsic magmas erupted in the Holocene. Glassy samples are abundant. Volcanological and petrographic evidence indicates that these glasses reflect characteristically low concentrations of H 2 0 in the melts, and this relationship is confirmed by experimental and chemical information. Distinct magma types, trachytes, comendites and pantellerites, erupted almost exclusively from different centres, even though these are sufficiently close for intercalation of the erupted products from adjacent volcanoes. This individuality is maintained in chemical variation diagrams where the products from different centres form separate groups, with no gradational compositions. In some diagrams smaller clusters appear within the main groups. These distinctive patterns indicate that there is no continuous evolution of the melts below the rift, and that each centre represents the outpouring of a different melt. Batches within the same centre could also represent different episodes of melt generation. Generation ofthese melts in a regional context can best be explained by melting ofdifferent sources during the influx of a CO 2 -rich fluid. Trachytes, pantellerites and comendites could then be the products of a flux/melting cycle as it climbs progressively through mantle, mafic deep crust, and sialic crust. The high concentrations of sodium and iron in the melts call for enhancement of these elements in the source rocks:this could be achievedby regional metasomatism resultingfrom prolonged activity through the rift segment over the past 23 Ma. Incompatible trace element variations cannot be attributed to solid-melt interactions but could be imparted by the fluid during melting.