Journal of Petrology | Pages |
© 1998 Oxford University Press |
A 1996 conference on `shallow level processes in ocean island magmatism' drew attention to the controversy that is developing on the possible extent of crustal contamination for oceanic island basalts (Bohrson et al., 1997). This controversy is important because most studies of oceanic island basalts have assumed that these lavas provide a direct indication of the geochemical and isotopic composition of mantle (e.g. Zindler & Hart, 1986). This assumption has been questioned in several recent studies (e.g. Eiler et al., 1996a; Thirlwall et al., 1997) and it has been suggested that even the most primitive basalts from some oceanic islands were contaminated by crustal materials (e.g. Hemond et al., 1993). Resolution of this controversy will have fundamental implications for our understanding of the magmatic history of oceanic island basalts and for the composition of the mantle. Oxygen isotopes are a potentially powerful tool to help resolve this debate because [delta]18O values of magma can be substantially modified by assimilation of rocks that have interacted with the hydrosphere (e.g. Taylor, 1974). Many oceanic island basalts have [delta]18O[dagger] values somewhat below the assumed mantle range, based on studies of mantle xenoliths and lunar rocks (4·6-5·3%o vs 5·5-6·0%o; e.g. Taylor & Sheppard, 1986; Mattey et al., 1994; Harmon & Hoefs, 1995) and mid-ocean ridge basalts (MORB; 5·7 ± 0·2%o; Ito et al., 1987). Many of these oceanic island basalts are mafic (>6·5 wt % MgO) and display no obvious signs of crustal contamination (Garcia et al., 1989b). Thus, it has been argued that the mantle is heterogeneous in [delta]18O (Harmon & Hoefs, 1995), which would make recognition of crustal contamination more difficult. Correlations have been noted between low [delta]18O values of olivine and whole-rock ratios of 206Pb/204Pb in Hawaiian basalts, which have been interpreted to reflect assimilation of hydrothermally altered oceanic crust (Eiler et al., 1996a). The same correlation for clinopyroxene and whole rocks with low [delta]18O values from the Canary Islands has been related to either recycling of ancient altered oceanic crust or crustal contamination (Thirlwall et al., 1997). Therefore, the role of crustal contamination in oceanic island magma petrogenesis is equivocal based on these previous studies. Hawaiian tholeiitic glasses have yielded a considerable range of [delta]18O values (4·6-5·8%o; Kyser et al., 1982; Garcia et al., 1989b, 1993), which overlaps with the range for MORB. Some of the low [delta]18O values are for submarine Hawaiian tholeiites that apparently assimilated hydrothermally altered crust because these rocks have elevated [delta]D values (-33 to -52%o vs mantle values of -60%o to -96%o; Kyser & O'Neil, 1984), boron concentrations and [delta]11B values (Chaussidon & Jambon, 1994). These lavas also have obvious petrographic signs of assimilation and complicated magmatic histories (Clague et al., 1995). There are, however, submarine Hawaiian tholeiitic lavas with a range of [delta]18O values (4·9-5·8%o) and mantle-like [delta]D (-61 to -88%o; Kyser & O'Neil, 1984; Garcia et al., 1989b). Thus, the large variation in [delta]18O values for these Hawaiian tholeiitic glasses apparently supports the interpretation from other isotopic work on Hawaiian tholeiites (e.g. West et al., 1987) that at least two isotopically distinct reservoirs are present in the source for Hawaiian magmas. We embarked on this study to evaluate whether the oxygen isotope variation in fresh Hawaiian tholeiitic basalts was indeed caused by mantle source heterogeneity or crustal contamination. To simplify this effort, we focused our attention on the pristine basalts from the current Puu Oo eruption of Kilauea Volcano on the island of Hawaii. This eruption is the best studied, longest lived (14 years and continuing), most voluminous (~1·5 km3) and one of the most compositionally variable (5·7-10·1 wt % MgO) historical eruptions of Kilauea Volcano. Unlike most previous studies on oceanic island basalts, our approach was to determine [delta]18O values of both glassy matrix material (95 to >99 vol. % of these rocks) and olivine (0·1-3 vol. %) for all the compositional variants from this eruption and to check for temporal variation. Olivine analyses are a critical component of this study because olivine is the liquidus mineral in Hawaiian tholeiitic magmas (Wright, 1971) and it is thought to be resistant to oxygen exchange, even at magmatic temperatures (Cole & Ohmoto, 1986). Thus, the olivine analyses should provide a good record of the early oxygen isotope history of Puu Oo magmas. Our results for Puu Oo lavas show a temporal variation in matrix [delta]18O values (4·56-5·25%o) that correlates with changes in vent location and eruption style. A sharp increase in matrix [delta]18O (~0·4%o) occurred following such a change but the [delta]18O of the coexisting olivines decreased slightly. The small difference between [delta]18O for olivines and host matrix [[Delta](ol-m)] in many Puu Oo lavas (>-0·4%o) is indicative of disequilibrium. Thus, although the Puu Oo lavas are pristine and have no other apparent geochemical evidence of crustal assimilation, the [delta]18O disequilibrium records the effects of crustal contamination and oxygen exchange, which occurred after the crystallization of some of the olivine crystals. Our results indicate that caution should be exercised in interpreting low [delta]18O values for basalts (<5·0%o), especially without oxygen isotope data for coexisting minerals, and that time series studies are important for interpreting geochemical processes. The Puu Oo eruption started in January 1983 (episode 1) and is continuing vigorously with typical eruption rates of (0·3-0·5) * 106 m3/day (Kauahikaua et al., 1996). Between 1983 and the end of 1996, the eruption produced ~1·5 km3 of lava (dense rock equivalent). The initial episode of the eruption formed a `curtain of fire' along an 8-km-long, discontinuous fissure system which intermittently produced lava for 20 days (Wolfe et al., 1987). During the next 3·5 years (episodes 2-47), eruptive activity was episodic with repose periods of 8-65 days during which magma accumulated and fractionated in a shallow reservoir under the Puu Oo vent (Fig. 1). These eruptive episodes were usually short (5-100 h) with lava fountains of variable height (tens of meters to 400 m high).INTRODUCTION
BRIEF HISTORY OF THE PUU OO ERUPTION