Magmatic plumbing at Lucky Strike volcano based on olivine‐hosted melt inclusion compositions. (20th January 2015)

• Record Type: Journal Article
• Authors: Wanless, V. D.; Shaw, A. M.; Behn, M. D.; Soule, S. A.; Escartín, J.; Hamelin, C.
• Is Part Of: Geochemistry, geophysics, geosystems. Volume 16:Number 1(2015:Jan.)
• Page Start: 126
• Page End: 147
• Publication Date: 2015-01-20
• Subjects: Geochemistry -- Periodicals; Geophysics -- Periodicals; Earth sciences -- Periodicals; 550.5
• DOI: 10.1002/2014GC005517
• Languages: English
• ISSNs: 1525-2027

Abstract

<abstract abstract-type="main"> <title>Abstract</title> <p>Here we present volatile, major, and trace element concentrations of 64 olivine‐hosted melt inclusions from the Lucky Strike segment on the mid‐Atlantic ridge. Lucky Strike is one of two locations where a crustal melt lens has been seismically imaged on a slow‐spreading ridge. Vapor‐saturation pressures, calculated from CO<sub>2</sub> and H<sub>2</sub>O contents of Lucky Strike melt inclusions, range from approximately 300–3000 bars, corresponding to depths of 0.5–9.9 km below the seafloor. Approximately 50% of the melt inclusions record crystallization depths of 3–4 km, corresponding to the seismically imaged melt lens depth, while an additional ∼35% crystallize at depths > 4 km. This indicates that while crystallization is focused within the melt lens, significant crystallization also occurs in the lower crust and/or upper mantle. The melt inclusions span a range of major and trace element concentrations from normal to enriched basalts. Trace element ratios at all depths are heterogeneous, suggesting that melts are not efficiently homogenized in the mantle or crust, despite the presence of a melt lens. This is consistent with the transient nature of magma chambers proposed for slower‐spreading ridges. To investigate the petrogenesis of the melt inclusion compositions, we compare the measured trace element compositions to theoretical melting calculations that consider variations in the melting geometry and heterogeneities in the mantle source. The full range of compositions can be produced by slight variations in the proportion of an Azores plume and depleted upper mantle components and changes in the total extent of melting.</p> </abstract>