4.7 Article

Solubilities of nitrogen and noble gases in silicate melts under various oxygen fugacities: Implications for the origin and degassing history of nitrogen and noble gases in the earth

Journal

GEOCHIMICA ET COSMOCHIMICA ACTA
Volume 68, Issue 2, Pages 387-401

Publisher

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/S0016-7037(03)00484-8

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Solubility experiments for nitrogen and noble gases (Ar and Ne) in silicate melts were conducted using two experimental configurations: one was conducted at I atmospheric pressure, T = 1300degreesC and oxygen fugacity (fO(2)) of IW + 0.9 (i.e., 0.9 log units higher than the iron-wustite buffer) and the other at high pressures (P-total similar to 2 x 10(8) Pa), 1500degreesC and fO(2) similar to IW + 6. For the former experiment, isotopically labeled-nitrogen ((NN)-N-15-N-15-enriched) was used to distinguish dissolved nitrogen from contaminating atmospheric or organic nitrogen and to examine dissolution mechanisms of nitrogen in silicate melts. The results obtained for the two series of experiments are consistent with each other, suggesting that Henry's law is satisfied for fN(2) of up to similar to250 atm (2.5 x 10(7) Pa). The results are also consistent with our earlier results (Miyazaki et al., 1995) obtained at highly oxidizing conditions (fO(2) similar to IW + 10). All these results support physical dissolution of nitrogen as N-2 molecules in silicate melts for fO(2) from similar toIW + 10 down to similar toIW. The observed solubility (Henry's constant) of nitrogen (3-5 x 10(-9) mol/g/atm) is comparable to that of Ar (2-4 x 10(-9) mol/g/atm), and much lower than that of Ne (11-14 x 10(-9) mol/g/atm) at 1300degreesC. A preliminary experiment was also performed for partitioning of nitrogen and noble gases between clinopyroxene (cpx) and basaltic melt using a piston cylinder-type apparatus at 1.5 GPa and at 1270 to 1350degreesC. The obtained cpx/melt partition coefficient of nitrogen is 0.06, slightly lower than those of noble gases (similar to0.1 for Ne to Xe), suggesting that nitrogen is as incompatible as or even slightly more incompatible than noble gases. The present results imply that a large nitrogen/Ar fractionation would not be produced by magmatic processes. Therefore, the two orders of magnitude difference between the N-2/Ar-36 ratios in the Earth's atmosphere (similar to10(4)) and that in the mantle (similar to10(6)) must be explained by some other processes, such as incomplete segregation of metal blobs into the core and their later oxidation. Copyright (C) 2004 Elsevier Ltd.

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