MANTLE NEON AND ATMOSPHERIC CONTAMINATION

dc.contributor.authorFarley K.A.
dc.contributor.authorPoreda R.J.
dc.date.accessioned2020-11-11T06:16:58Z
dc.date.available2020-11-11T06:16:58Z
dc.date.issued1993
dc.description.abstractThe apparent distinction between atmospheric and mantle²⁰Ne²²Ne ratios may provide a technique to quantify air contamination in mantle-derived materials. In the absence of mantle nuclear reactions, which produce either²⁰Ne or²²Ne in substantial quantities, it is likely that the entire mantle is characterized by a single, uniform²⁰Ne²²Ne ratio; a value of around 12.5 is suggested by analyses of MORBs, OIBs, diamonds and xenoliths. If this premise is correct, then any measured²⁰Ne²²Ne ratios in mantle samples that are lower than this must result from addition of an air component, with²⁰Ne²²Ne= 9.8. This is most likely a syn- or post-eruptive contaminant. The degree of air contamination inferred from²⁰Ne²²Ne ratios is generally small for diamonds, but is increasingly significant for MORBs and OIBs; many OIB's may carry > 90% air neon. We calculated “air-neon corrected”²¹Ne²²Ne and⁴⁰Ar³⁶Ar ratios for the highly degassed MORB mantle and for the less degassed (high³He⁴He) “plume” reservoir. The inferred MORB composition is indistinguishable from measurements of some gas-rich glasses. The calculated plume composition is similar to the least air-like measurements from ocean islands, but is less air-like than has been proposed previously. This plume composition is not consistent with a completely undegassed reservoir.
dc.identifierhttps://elibrary.ru/item.asp?id=31598469
dc.identifier.citationEarth and Planetary Science Letters, 1993, , 2, 325-339
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/18926
dc.titleMANTLE NEON AND ATMOSPHERIC CONTAMINATION
dc.typeСтатья

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