Pb-Pb mineral isochrons were determined for three cumulate eucrites (Moama, Moore County, and Serra de Mage) and three noncumulate eucrites (Nuevo Laredo, Bouvante, and Stannern). Two noncumulate eucrites (Bereba and Cachari) show disturbed Pb isotope patterns. The mineral isochron ages of cumulate eucrites range from 4.40 Ga to 4.48 Ga. The latter is the age of Moore County (4.484 +/- 0.019 Ga), which was also dated by the Sm-Nd method at 4.456 +/- 0.025 Ga. Nuevo Laredo and Bouvante give the same Pb-Pb age: 4.514 +/- 0.015 Ga and 4.510 +/- 0.004 Ga, respectively. The Pb isochron of Stannern corresponds to 4.128 +/- 0.016 Ga, which is a reequilibration age. Both Cachari and Bereba show evidence of isotope resetting at about 4 Ga. A Pb-Pb multicorrelation approach is introduced and applied to the data.

B and Nb concentrations and B isotope composition were determined for lavas covering the entire length of the Kurile are. B/Nb and beta(11)B of these lavas show clear across-are Variations in which both are highest at the trench side and continuously decrease as the slab depth increases. B/Nb in the volcanic front lavas (8-25) is significantly higher than those of MORB and OIB, indicating that the mantle wedge is extensively metasomatized by B-rich fluid derived from the subducting slab. The frontal delta(11)B values are also out of the range of MORB and OIB, and systematic difference exists between Northern Kurile (NK: + 5.4 +/- 0.5 parts per thousand) and Central and Southern Kurile (CSK: + 4.3 +/- 0.3 parts per thousand). However, these two parameters approach or coincide with mantle values at the most back-are side. The delta(11)B and Sr-87/Sr-86 linearly correlate with Nb/B, suggesting control by simple mixing of two isotopically homogeneous components; that is, slab-derived fluid and mantle wedge. The estimated delta(11)B and Sr-87/Sr-86 of the fluid are +7.0 +/- 0.6 parts per thousand and 0.70326 +/- 0.00005 for NK, and + 6.3 +/- 0.3 parts per thousand and > 0.7033 for CSK, respectively. These fluid compositions are consistent with a source constituted by > 95% altered oceanic crust and < 5% oceanic sediment, with the slight difference between NK and CSK resulting from the different lithologies of subducting sediments. The mantle wedge beneath the Kurile are has B, Sr and Nd isotope compositions identical with MORB but shows significantly higher B/Nb. The above trends bear a close resemblance to those observed in the Izu are, strongly suggesting their universality in the are system. The across-are decline of B/Nb observed both in Kurile and Izu implies that the fluid flux from the slab continuously decreases as the slab depth increases. However, this relates only to a final stage of slab dehydration since most of the volatile components are lost at the fore-are region. In contrast to B, K is uniformly enriched across the are. This requires control by a K-bearing mineral phase either in the slab (phengite) or the mantle wedge (phlogopite), although such a mineral is responsible for only a small part of the whole fluid transport. (C) 1997 Elsevier Science B.V.

Nb/B ratios and delta(11)B values of Mariana lavas reveal the involvement of two isotopically distinct slab-derived fluids in the magma genesis. The evidence of one type of fluid is observed in lavas of the islands of Anatahan, Alamagan, Agrigan, and Uracas, in which simple mixing between fluid with very homogeneous delta(11)B values (+5.40 parts per thousand +/- 0.05 parts per thousand) and the mantle wedge controls the magma compositions. In lavas of the islands of Guguan, Asuncion, and Pagan, however, the fluids that mixed with the mantle wedge are significantly heterogeneous in delta(11)B (+5.4 parts per thousand to +7.6 parts per thousand) even within a single island. The compositional difference between these two types of fluid can result from different ratios of sediment to altered oceanic crust (AOC) in the slabs, and this hypothesis is consistent,vith the Sr, Nd, and Pb isotope data. We propose that the variable isotope compositions of the latter fluid may be derived from local changes in sediment/AOC ratios of the slab that are caused by subduction of the Magellan seamounts beneath the Mariana are.

Industrialization and urbanization around San Francisco Bay as well as mining and agriculture in the watersheds of the Sacramento and San Joaquin rivers have profoundly modified sedimentation patterns throughout the estuary. We provide some constraints on the onset of these erosional disturbances with Be-10 data for three sediment cores: two from Richardson Bay, a small embayment near the mouth of San Francisco Bay, and one from San Pablo Bay, mid-way between the river delta and the mouth. Comparison of pre-disturbance sediment accumulation determined from three C-14-dated mollusk shells in one Richardson Bay core with more recent conditions determined from the distribution of Pb-210, and Th-234 [Fuller, C.C., van Geen, A., Baskaran, M., Anima, R.J., 1999. Sediment chronology in San Francisco Bay, California, defined by Pb-210, Th-234, Cs-137, and Pu-239,Pu-240] shows that the accumulation rate increased by an order of magnitude at this particular site. All three cores from San Francisco Bay show subsurface maxima in Be-10 concentrations ranging in magnitude from 170 to 520 x 10(6) atoms/g. The transient nature of the increased Be-10 input suggests that deforestation and agricultural development caused basin-wide erosion of surface soils enriched in Be-10, probably before the turn of the century. (C) 1999 Elsevier Science B.V. All rights reserved.

We report measurements of the isotopic composition of lithium in basalts using a multicollector magnetic sector plasma-source mass spectrometer (MC-ICP-MS). This is the first application of this analytical technique to Li isotope determination. External precision of multiple replicate and duplicate measurements for a variety of sample types averages +/-1.1 parts per thousand (2 sigma population). The method allows for the rapid (similar to 8 min/sample) analysis of small samples (similar to 40 ng Li) relative to commonly used thermal ionization methods. The technique has been applied to a suite of samples from Kilauea Iki lava lake, Hawaii. The samples range from olivine-rich cumulitic lava to SiO2- and K2O-enriched differentiated liquids, and have delta(7)Li (per mil deviation of sample Li-7/Li-6 relative to the L-SVEC standard) of +3.0 to +4.8. The data indicate a lack of per mil-level Li isotope fractionation as a result of crystal-liquid fractionation at temperatures greater than 1050 degrees C, This conclusion has been tacitly assumed but never demonstrated, and is important to the interpretation of Li isotope results from such geochemically complex environments as island arcs. Copyright (C) 1999 Elsevier Science Ltd.

An evaluation of early solar system chronometry by the Pb-Pb and U-Pb methods is provided. Specifically, three consequential factors are examined: procedure of age calculation, extent of terrestrial Pb contamination, and initial Pb isotopic composition. On a Pb-Pb diagram, high temperature inclusions of the Allende meteorite are tightly organized into a well-defined line (inside a potentially dispersive mixing field), which is consistent with the inclusions containing initial Pb that is more primitive than that of Canon Diablo troilite (PAT). Consequences of the possible existence of a pre-PAT Pb to the evolution history of the solar nebula are discussed.

Trace element concentrations and B isotope compositions were determined for lavas from the Eastern Volcanic Front (EVF), the Central Kamchatka Depression (CKD), and the Sredinny Range (SR) in the Kamchatka are. Trace element ratios and delta B-11 values of the EVF lavas show across-arc variations that are consistent with those observed in the adjacent Kurile are: B/Nb, Pb/Nb, and delta B-11 are highest at the volcanic front (14 to 22, 2.0 to 2.4, and +4.9 to +5.6 parts per thousand, respectively) and systematically decrease with increasing slab depth (to similar to3, similar to0.9, and similar to2 parts per thousand, respectively) whereas Rb/Nb, Ba/Nb, K/Nb, Be/Nb, and Li/Zr do not vary significantly across the are. The values for the SR (B/Nb = 1.7 to 2.0, Pb/Nb = 0.9 to 1.2, and delta B-11 = -3.7 to -1.1 parts per thousand) located far behind the EVF are consistent with these across-are trends. However, the CKD lavas exhibit elevated B/Nb (6 to 13) and delta B-11 values (-0.6 to +3.6 parts per thousand) although the slab depths are greater than at the EVF, Despite variations in B/Nb and delta B-11, the values for all these three volcanic zones of Kamchatka can be explained in terms of simple mixing between a depleted mantle wedge and slab-derived aqueous fluids with a relatively homogeneous delta B-11 (+6.2 +/- 0.5 parts per thousand). This mixing trend resembles those observed in Kurile, Izu, and Mariana, suggesting that fluids derived from altered oceanic crust and/or serpentinized peridotite in the subducting slab predominate in the slab-mantle interaction beneath these western Pacific arcs. Given this mixing relationship, the high B/Nb and delta B-11 values observed in the CKD indicate particularly large fluid influx beneath this region, which may partly result from subduction of the altered crust of the Emperor seamount chain in addition to the altered Mid-Ocean Ridge Basalt (MORB) crust. The compositions of the SR lavas in this study are consistent with melting of a weakly fluid-metasomatized mantle. However, the origin of magma in this volcanic zone is complicated, judging from the variable chemical characteristics reported for the SR lavas, Copyright (C) 2001 Elsevier Science Ltd.