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The eclogite engine: Chemical geodynamics as a Galileo thermometer

Anderson, Don L. (2007) The eclogite engine: Chemical geodynamics as a Galileo thermometer. In: Plates, Plumes, and Planetary Processes. Special papers (Geological Society of America). No.430. Geological Society of America , Boulder, CO, pp. 47-64. ISBN 9780813724300.

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Migrating and incipient ridges and triple junctions sample the heterogeneous mantle created by plate tectonics and crustal stoping. The result is a yo-yo vertical convection mode that fertilizes, cools, and removes heat from the mantle. This mode of mantle convection is similar to the operation of a Galileo thermometer (GT). The GT mode of small-scale convection, as applied to the mantle, differs from the Rayleigh-Taylor (RT) instability of a homogeneous fluid in a thermal boundary layer. It involves stoping of over-thickened continental crust and the differences in density and melting behavior of eclogites and peridotites in the mantle. The fates of subducted and delaminated crust, underplated basalt, and peridotite differ because of differences in scale, age, temperature, melting temperature, chemistry, thermal properties, and density. Cold subducted oceanic crust—as eclogite—although denser than ambient mantle at shallow depths, may become less dense or neutrally buoyant somewhere in the upper mantle and transition zone, and may be gravitationally trapped to form mafic eclogite-rich blobs or layers. Detached lower continental crust starts out warmer; it thermally and gravitationally equilibrates at shallower depths than do slabs of cold mature lithosphere. The density jumps at the depths of 400 and 650 km act as barriers. Trapped eclogite is heated by conduction from the surrounding mantle and its own radioactivity. It is displaced, entrained, and melted as it warms up to ambient mantle temperature. Both the foundering and the re-emergence of mafic and ultramafic blobs create midplate magmatism and uplift. Mantle upwellings and partially molten blobs need not be hotter than ambient mantle or from a deep thermal boundary layer. The fertile blobs drift slowly in the opposite direction to plate motions—the counterflow model—thereby maintaining age progressions and small relative motions between hotspots. Large-scale midplate volcanism is due to mantle fertility anomalies, such as large chunks of delaminated crust or subducted seamount chains, or to the release of accumulated underplate when the plate experiences flexure or pre-breakup extension. Eclogite can have lower shear velocities than volatile-free peridotite and will show up in seismic tomograms as low-velocity, or red, regions, even when cold and dense. This model removes the paradoxes associated with deep thermal RT instabilities, propagating cracks and small-scale thermal convection. It explains such observations as relative fixity of melting spots, even though the fertile blobs are shallow.

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Additional Information:© 2007 Geological Society of America. Manuscript accepted by the Society 31 January 2007. This article is one of a series on implications of the top-down hypothesis for mantle dynamics and geochemistry. The top-down, or plate, hypothesis is being developed in collaboration with Jim Natland, Anders Meibom, and Gillian Foulger. Interactions with Dean Presnall, Jerry Winterer, Warren Hamilton, Seth Stein, Alan Smith, Cin-Ty Lee, and contributors to have been, and continue to be, invaluable. Jim Natland reviewed the preliminary manuscript and stimulated a complete rewrite, as did the reviewers of the present article. My interest in delamination was started by a series of discussion seminars at Rice University, Houston, and by conversations with Alan Levander, Adrian Lenardic, Richard Gordon, Gene Humphreys, and Cin-Ty Lee. The manuscript benefited enormously from comments and reprints by Dave Green, John Hernlund, and Jim Natland. The information on density borrows heavily from papers by Cin-Ty Lee and Dave Green.
Subject Keywords:delamination, small-scale convection, plumes, blobs, LIPs, eclogite
Series Name:Special papers (Geological Society of America)
Issue or Number:430
Record Number:CaltechAUTHORS:20121018-084451644
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Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34963
Deposited By: Tony Diaz
Deposited On:18 Oct 2012 16:54
Last Modified:03 Oct 2019 04:23

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