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Models for noble gases in mantle geochemistry: Some observations and alternatives

Meibom, Anders and Sleep, Norman H. and Zahnle, Kevin and Anderson, Don L. (2005) Models for noble gases in mantle geochemistry: Some observations and alternatives. In: Plates, Plumes, and Paradigms. Special papers (Geological Society of America). No.388. Geological Society of America , Boulder, CO, pp. 347-363. ISBN 9780813723884 http://resolver.caltech.edu/CaltechAUTHORS:20121018-081134753

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Abstract

Models for noble gases in the Earth's mantle are evaluated against a number of observational constraints: (1) high ^3He/^4He ratios do not correlate with high (initial) ^3He concentrations; (2) the ^3He/^4He data for mid-ocean ridge basalts and ocean island basalts do not represent two different distributions (Anderson 2001); (3) globally robust correlations between ^3He/^4He ratios and lithophile isotopic systems are not observed; (4) diverse local correlations exist that are broadly linear; (5) large, local geographical ^3He/^4He variations are observed, which are inconsistent with a strongly localized (i.e., plume-stem) flux of high-^3He/^4He material; and (6) dramatic temporal ^3He/^4He variations are observed on very short time scales (10^2 years). Layered (reservoir) models for noble gases, in which a deep and radially constrained region of the Earth's mantle preserves unradiogenic He and Ne isotopic compositions because of a high noble gas concentration, do not seem consistent with these observations. Heterogeneous (nonlayered) mantle models for noble gases, in which the carrier of unradiogenic He is a relatively noble gas–poor component scattered in the (upper) mantle, appear more consistent with the constraints. We propose that the carrier of unradiogenic noble gases is primarily olivine. Olivine-rich lithologies, produced in previous partial melting events, are a natural part of the statistical upper mantle assemblage (SUMA), a highly heterogeneous assemblage of small- to moderate-scale (∼1–100 km) enriched and depleted lithologies with a wide range of chemical composition, fertility, age, and isotopic signatures (Meibom and Anderson, 2004). The isotopic signatures of oceanic basalts, including noble gases, are obtained by partial melting of the SUMA under slightly different pressure and temperature (P-T) conditions, i.e., different degrees of partial melting and different degrees of homogenization prior to eruption (Morgan and Morgan, 1999; Meibom and Anderson, 2004; Rudge et al., 2005; Ito and Mahoney, 2005). Unradiogenic noble gas isotopic compositions are not tracers of deep-mantle components in the source materials of oceanic basalts. Noble gas isotopic compositions may, however, indirectly indicate potential temperature, because the order in which different upper-mantle lithologies melt depends on the P-T conditions.


Item Type:Book Section
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http://dx.doi.org/10.1130/0-8137-2388-4.347DOIUNSPECIFIED
http://specialpapers.gsapubs.org/content/388/347.abstractPublisherUNSPECIFIED
Additional Information:© 2005 Geological Society of America. Manuscript accepted by the Society January 3, 2005. This work was supported in part by National Science Foundation Grant EAR-0309414 and by the U.S. National Aeronautics and Space Administration Planetary Atmospheres Program. A.M. is grateful for inspiring discussions with Jim Natland, Pete Burnard, Francis Albarede, Don DePaolo, and his students Tom Sisson. John Eiler, Alan Brandon, Garrett Ito, and Cin-Ty Lee. We thank Don DePaolo for sharing his compiled database from the Hawaiian Scientific Drilling Project. Constructive and thorough reviews were provided by Dave Graham, Chris Ballentine, Paul Tackey, and Gillian Foulger. Their efforts are greatly appreciated.
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Funding AgencyGrant Number
NSFEAR-0309414
NASA Planetary Atmospheres ProgramUNSPECIFIED
Subject Keywords:noble gases, mantle geochemistry, reservoirs, SUMA, plumes
Record Number:CaltechAUTHORS:20121018-081134753
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20121018-081134753
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34961
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:18 Oct 2012 22:16
Last Modified:18 Oct 2012 22:16

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