Abstract

Heavy noble gases can record long-lasting heterogeneities in the mantle, because Ne, Ar, and Xe isotopes are produced from extant (U, Th, K) and extinct (129I and 244Pu) radionuclides. However, the presence of ubiquitous atmospheric contamination in basalts, particularly for ocean island basalts (OIBs) that sample the Earth's deep mantle, have largely hampered precise characterization of the mantle source compositions. Here we present new high-precision noble gas data from gas-rich basalts erupted along the Rochambeau Rift (RR) in the northwestern corner of the Lau Basin. The strong influence of a deep mantle plume in the Rochambeau source is apparent from low 4He/3He ratios down to 25,600 (3He/4He of 28.1RA).We find that the Rochambeau source is characterized by low ratios of radiogenic to non-radiogenic nuclides of Ne, Ar, and Xe (i.e., low 21Ne/22Ne, 40Ar/36Ar, and 129Xe/130Xe) compared to the mantle source of mid-ocean ridge basalts (MORBs). High-precision xenon isotopic measurements indicate that the lower 129Xe/130Xe ratios in the Rochambeau source cannot be explained solely by mixing atmospheric xenon with MORB-type xenon; nor can fission-produced Xe be added to MORB Xe to produce the compositions seen in the Rochambeau basalts. Deconvolution of fissiogenic xenon isotopes demonstrate a higher proportion of Pu- fission derived Xe in the Rochambeau source compared to the MORB source. Therefore, both I/Xe and Pu/Xe ratios are different between OIB and MORB sources. Our observations require heterogeneous volatile accretion and a lower degree of processing for the plume source compared to the MORB source. Since differences in 129Xe/130Xe ratios have to be produced while 129I is still alive, OIB and MORB sources must have been processed at different rates for the first 100 million years (Myr) of Solar System history, and subsequent to this period, the two reservoirs have not been homogenized.In combination with recent results from the Iceland plume, our noble gas observations require the formation and preservation of less-degassed, early-formed (pre-4.45Ga) heterogeneities in the Earth's deep mantle. Consequently, the primitive noble gas reservoir sampled by mantle plumes cannot be created solely through sequestration of recycled slabs or undegassed melts at the base of the mantle during the past 4.4Ga. Finally, if the more primitive, less degassed heterogeneities reside in the Large Low Shear Wave Velocity Provinces (LLSVPs), then LLSVPs must be long-lasting features of the deep mantle and are not composed exclusively of recycled material.

Highlights

  • The noble gas compositions of mantle-derived basalts provide information on the degassing history, style of mantle convection, and volatile exchange between the deep Earth and exosphere

  • We find that the Rochambeau source is characterized by low ratios of radiogenic to non-radiogenic nuclides of 20 Ne, Ar, and Xe compared to the mantle source of mid-ocean ridge basalts (MORBs)

  • Our observations demonstrate that MORBs and 293 plumes have small but distinct differences in 129Xe/136Xe ratios

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Summary

Introduction

The noble gas compositions of mantle-derived basalts provide information on the degassing history, style of mantle convection, and volatile exchange between the deep Earth and exosphere. Lower ratios of radiogenic 51 to non-radiogenic Xe isotopes (129Xe/130Xe) are found in Hawaii, Samoa, Iceland and Reunion (e.g., Mukhopadhyay 2012; Poreda and Farley, 1992; Trieloff et al, 2000; Trieloff et al, 2002) These noble gas signatures in OIBs are commonly attributed to sampling parts of Earth’s mantle that are significantly less degassed than the MORB source (e.g., Allegre et al, 1987; Graham, 2002; Gonnermann and Mukhopadhyay, 2009; Kurz et al, 1982; Kurz et al, 2009; Porcelli and Wasserburg, 1995; Staudacher and Allegre, 1982). The low 40Ar/36Ar and 129Xe/130Xe ratios in OIBs may arise from recycled atmospheric Ar and Xe and not from a less degassed reservoir (Holland and Ballentine, 2006: Kendrick et al, 2011; Trieloff and Kunz, 2005)

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