Is Eruption Style Linked to Magma Residence Time at Kilauea Volcano? Results from Chemical Zoning in Olivine

Kilauea is generally characterized by its modern effusive activity, but the past 2500 years were dominated by cycles of explosive and effusive eruptions lasting 100's of years (Swanson et al. 2012). These different eruption styles may reflect variable volatile contents in the source that control magma ascent rate and storage durations (e.g., Sides et al. 2014). A detailed petrological study of the dominantly explosive Keanakako'i tephras (1500-1820 CE) was undertaken to better understand the storage and transport conditions preceding high-energy eruptions. Here, we focus on preliminary results for olivine from the 1500 CE Basal Reticulite (>600 m fountain; May et al. 2015). Olivine major (Fe, Mg), minor (Mn, Ca, Ni) and trace (Li, Na, Al, P, Sc, Ti, V, Cr, Co, Zn) element traverses and 2D maps were collected for 10 crystals and reveal two major populations. The dominant population has homogeneous Fo89 and Fo87 cores with thin (3-12 μm) rims of intermediate composition (Fo87.5-88.5). Normal, reverse, and complex trace element zoning (Al, P, Ti, Cr) is prominent in these otherwise homogenous (Fo, Ni, Ca, Mn) crystals. 2D maps reveal early skeletal growth and the progressive decrease of Cr from core to rim suggests olivine and Cr-spinel crystallization, which should produce significant Fo zoning. Absence of Fo zoning could imply significant storage time in a reservoir allowing homogenization. The majority of rim compositions are out of equilibrium with adhering glass, and Fe-Mg modeling indicates that their residence within the carrier melt was of a few days. A second population consists of strongly zoned (normal and reverse) crystals with a wide range of core Fo (78 to 89) and Fo82-84 rims. Timescales from Fe-Mg zoning are up to 1 year, and may record storage histories before interaction with the carrier melt. The diversity in olivine zoning suggests at least two stages of magma mixing, and a more complex evolution for the magmas that fed the reticulite eruptions than a simple closed-system and fast transport of a volatile-rich magma from the source to the surface.