The role of plumes in mantle helium fluxes

• Published in: Earth and Planetary Science Letters
• Main Authors: Kellogg, L. H., Wasserburg, G. J.
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: Elsevier 1990
• Subjects: Iceland
• Online Access: https://authors.library.caltech.edu/42094/; https://resolver.caltech.edu/CaltechAUTHORS:20131028-104549067

We present a simple model of ^3He and ^4He transport in the mantle using the appropriate rates of mass and species transfer and ^4He production. Previous workers have shown the presence of excess ^3He in hotspots such as Hawaii and Iceland and inferred that these hotspots tap a source with a higher ^3He ^4He ratio than the source region of mid-ocean ridge basalts (MORB). Hotspot ocean islands probably originate over upwelling plumes which carry material from the lower mantle to the upper mantle. Melting at hotspots and at mid-ocean ridges degasses the mantle of volatiles such as helium. The upper mantle is outgassed largely of helium due to melting at mid-ocean ridges and hotspots. We postulate that the excess ^3He seen in MORB originates in material that was carried from the lower mantle in plumes but not completely outgassed at hotspots. This helium is incorporated into the depleted upper mantle. Assuming that the upper mantle is in a quasi-steady-state with respect to helium, a simple model balancing ^3He and ^4He fluxes in the upper mantle indicates that the hotspots significantly outgas the lower mantle of ^3He. The concentration of ^4He in the plume source reservoir is 2–3 orders of magnitude lower than the concentration in carbonaceous chondrites. The residence time of helium in the upper mantle depends on the outgassing efficiency at hotspots, since the hotspots may outgas some upper mantle material which has been entrained in the plumes. The residence time of He in the upper mantle is about 1.4 × 10^9 yr. We conclude that the efficiency of outgassing of He from plumes is high and that the plumes dominate the present ^3He loss to the atmosphere. The ^4He in the less depleted layer of the mantle is not trapped “primordial” but is predominantly from in situ decay of U and Th in the depleted layer over ∼ 1.4 × 10^9 yr. The ^4He in the lower mantle is dominantly from in situ decay of U and Th over 4.4 × 10^9 yr. This model appears to explain the total Ar in the atmosphere as there is about the same amount of K in the depleted mantle as is in the continents.