V22B-01:
Geochemical Diversity of the Mantle: 50 Years of Acronyms

Tuesday, 16 December 2014: 10:20 AM
Stanley R Hart, Woods Hole Oceanographic Institution, Department of Geology and Geophysics, Woods Hole, MA, United States
Abstract:
50 years ago, Gast, Tilton and Hedge demonstrated that the oceanic mantle is isotopically heterogeneous. 28 years ago, Zindler and Hart formalized the concept of geochemical mantle components, with an attendant, to some, odious, acronym soup. Work on a marriage of mantle geochemistry and dynamics continues unabated. We know unequivocally that the mantle is chemically heterogeneous; we do not know the scale lengths of these heterogeneities. We know unequivocally that these heterogeneities have persisted for eons (Gy); we do not know where they were formed or where they are stored. Through the kind auspices of the Plume Model, we plausibly have access to the whole mantle.

The most accessible and well understood mantle reservoir is the upper depleted MORB mantle (DMM). Classically, this mantle was depleted by extraction of oceanic and continental crust from a “chondritic” bulk silicate Earth. In this post-Boyet and Carlson world, the complementary enriched reservoir may instead be hidden in the deepest mantle. In this case, DMM will become an endangered acronym.

Hofmann and White (1982) argued that radiogenic Pb mantle (HIMU) is re-cycled ocean crust, and this is a comfortably viable model. It does require some ad hoc chemical manipulations during subduction. Given 2 Gy of aggregate mantle strains, the mafic component in HIMU may be of small length scale (< 50 m), possibly subsumed into the dominant peridotitic lithology. This mantle species is globally widespread.

Enriched mantles (EM1 and EM2) almost certainly reflect recycling of enriched continental material. This was splendidly verified by Jackson et al (2007), with 87Sr/86Sr in Samoan EM2 lavas up to 0.721. The lithology and length scale of EM1 and EM2 is unconstrained. EM1 is globally present; EM2 is confined to the SW Pacific hotspots.

FOZO is a work in progress; many would like to see it become extinct!

The trace element signatures of HIMU and FOZO mantles have been constrained using melting models; in both cases the spidergrams are “enriched” with peaks at Nb-Ta of 2x and 4x bulk silicate earth, respectively, but with quite different shapes. As is typical with OIB, the derived source compositions are incompatible with the isotopic signatures, requiring a fairly recent “enrichment” event (possibly auto-metasomatism).