Origins of Pb-210-Ra-226 disequilibria in basalts

New insights from the 1978 Asal Rift eruption

Simon Turner*, Mark Reagan, Nathalie Vigier, Bernard Bourdon

*Corresponding author for this work

Research output: Contribution to journalArticle

9 Citations (Scopus)
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Abstract

There has been much debate as to whether 210Pb-226Ra disequilibria in young volcanic rocks result from partial melting, cumulate interaction or magma degassing. Here we present new data from basalts erupted in 1978 from Ardoukoba volcano in the Asal Rift. The (210Pb/ 226Ra)t ratios are very low (0.2 to 0.6) and appear to correlate negatively with (226Ra/230Th). Invariant ( 230Th/238U) and (231Pa/235U) ratios require similar melting rates, porosities, and extents for all parental magmas. Thus, the range in (226Ra/230Th), which is negatively correlated with Th concentration, reflects fractional crystallization over millennia after the magmas were emplaced into the crust. This precludes the 210Pb deficits from resulting from partial melting. Instead, the 210Pb deficits must have formed subsequent to magma differentiation and are interpreted to reflect several decades of magma degassing. Many young basalts erupted in a variety of tectonic settings are similarly depleted in 210Pb with respect to 226Ra, suggesting that they continuously degas over a period of a few to several decades, perhaps reflecting the time required to rise to the surface from deeper reservoirs. In some of these basalts, gas accumulation leads to the shallowest, most evolved, and earliest erupting magmas having the highest (210Pb/226Ra) ratios and sometimes 210Pb excesses.

Original languageEnglish
Article numberQ07002
Pages (from-to)1-8
Number of pages8
JournalGeochemistry, Geophysics, Geosystems
Volume13
Issue number7
DOIs
Publication statusPublished - 6 Jul 2012

Bibliographical note

Copyright AGU 2012. Originally published in Geochemistry Geophysics Geosystems, Vol.13, Q07002. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.

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