Kulanaokuaiki 3: Product of an Energetic, Diatreme-Like Eruption at Kilauea
Abstract
Kulanaokuaiki 3 (K-3), one of five units of the Kulanaokuaiki tephra, was erupted at ~AD 850 and blanketed large near-summit areas. Most complete remnants today are found in the Koa`e fault system and on the volcano`s south flank, S and SE of the summit. There, K-3 consists mostly of crystal-rich scoria lapilli contained in two sub-units, generally 1-8 cm thick, separated by a <1 cm "parting" of coarse ash and/or reticulite lapilli. Fine ash (<0.5 mm) makes up <3% of the two scoria units, increasing upward to ~10%. Dense lithic clasts are contained in both sub-units; ~85% of these consist of a wide variety of basalt (some enclosed in cored bombs), and ~12% are fine-coarse gabbro (some containing interstitial glass w/vesicles). The lithics are typically fresh, suggesting that the eruptive conduit pierced pristine parts of the volcano`s edifice rather than long-established, hydrothermally altered conduit systems. Erosion has stripped most K-3 from the south flank, leaving its lithics as scattered lags. Dense clasts, >4 kg and 18 cm across, are found as far as 7 km from the summit; progressively smaller clasts (~3-4 cm) fell at the coastline, 17 km away. The K-3 scoria deposits are unremarkable to the eye, but this belies cryptic vertical zonation that characterizes these units at widespread south-flank localities. The specific gravity of scoria lapilli (7-10 mm dia.) decreases upward in the lower sub-unit, accompanied by decreasing whole-rock MgO values. The pattern is reversed in the upper sub-unit, where specific gravity and MgO values increase upward. Available information suggests the specific gravity and MgO variations correlate with percentages of phenocrystic olivine. Preliminary geobarometry of pyroxene-glass pairs suggests that some gabbro was crystallizing at 5-7 km depth before exploding from the volcano-- far deeper than expected in a phreatomagmatic eruption. We interpret that CO2, known to be released in huge volumes from Kilauea`s summit, and which initially exsolves from basaltic magma at ~10 km depth, was the likely propellant for the diatreme-like K-3 eruption. While reaming a conduit to the surface, the streaming CO2, knicked the upper part of a magma body (likely dike-shaped), initiating its disintegration. The first pulse of the eruption released scoria that, along with spalled conduit wall rocks, erupted to form the lower K-3 sub-unit. Following a brief pause, when the air partly cleared to form the mid-K-3 parting, a second pulse entrained scoria originating from progressively deeper and more olivine-rich parts of the magma body. As a result, scoria containing greater percentages of phenocrystic olivine was erupted, and these were showered over the south flank to produce the observed upside-down "magma-chamber grading" in the upper K-3 sub-unit. Multi-mach exit velocities are visualized, and entrained lithic clasts may have been carried to heights of 15-20 km. These clasts were carried to the southeast as they fell through high-level northwesterly winds.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2006
- Bibcode:
- 2006AGUFM.V33B0647F
- Keywords:
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- 8404 Volcanoclastic deposits;
- 8428 Explosive volcanism;
- 8430 Volcanic gases;
- 8455 Tephrochronology (1145);
- 8486 Field relationships (1090;
- 3690)