Ridge-hotspot interaction along the Mid-Atlantic Ridge between 37°30' and 40°30'N: the U sbnd Th disequilibrium evidence
Abstract
This study reports U sbnd Th disequilibrium data obtained by mass spectrometry for basaltic glasses collected along the Azores platform portion of the Mid-Atlantic Ridge (37°30'-40°30'N), a region characterized by both a geochemical and bathymetric gradient. High Th and U concentrations, as well as Th/U ratios, document an enriched geochemical signature. ( 230Th 238U ) activity ratios range from 1.20 to 1.35 and are thus systematically larger than most EPR MORBs reported in the literature. ( 230Th 232Th ) activity ratios show remarkable homogeneity for multiple samples taken from single dredge hauls. Additionally, samples with the highest Th concentrations (2.4 ppm) have among the highest Th isotope ratios. Taken together, these observations rule out assimilation of 230Th-rich sediment as an explanation for the 230Th sbnd 238U systematics. The relatively large 230Th excesses in the erupted lavas may be related to the influence of the enriched Azores mantle plume source. The lack of observed correlations between 230Th excess and trace element and isotopic indices of source enrichment, however, rules out source composition as an explanation for the variations in ( 230Th 238U ). Excess 230Th is correlated with the axial depth of the ridge in the study area, with the shallowest portions showing the largest extents of disequilibrium. This may reflect more melting in the presence of garnet for the shallow segments, and suggests that melting begins well within the garnet peridotite stability field (∼ 35 kbar) in the mantle beneath the Azores segment of the MAR. At the ridge segment scale, 230Th excesses tend to be smaller near segment boundaries. This could reflect differences in the melting process or less frequent magmatism in these zones. These results demonstrate the potential for U sbnd Th systematics to constrain the depth and degree of melting as well as the rate of mantle upwelling, even in the presence of source chemical heterogeneity.
- Publication:
-
Earth and Planetary Science Letters
- Pub Date:
- July 1996
- DOI:
- 10.1016/0012-821X(96)00092-1
- Bibcode:
- 1996E&PSL.142..175B