Geochronology of zircon megacrysts from nepheline-bearing gneisses as constraints on tectonic setting: implications for resetting of the U-Pb and Lu-Hf isotopic systems
dc.contributor.author | Ashwal, L. D. | |
dc.contributor.author | Armstrong, Richard | |
dc.contributor.author | Roberts, R.J. | |
dc.contributor.author | Schmitz, Mark | |
dc.contributor.author | Corfu, Fernando | |
dc.contributor.author | Hetherington, C.J. | |
dc.contributor.author | Burke, K. | |
dc.contributor.author | Gerber, M. | |
dc.date.accessioned | 2015-12-07T22:24:52Z | |
dc.date.issued | 2007 | |
dc.date.updated | 2015-12-07T09:29:34Z | |
dc.description.abstract | Nepheline-bearing gneisses from the 75 km2 Tambani body in the Mozambique Belt of southern Malawi, are miaskitic biotite-nepheline monzodiorites, reflecting an absence of K-feldspar, alkali amphiboles or pyroxenes, and contain euhedral zircon megacrysts up to 5 cm across. The zircons contain U = 1-1,860 ppm, Th = 0-2,170 ppm and Y = 400-1,100 ppm, and very low concentrations of all other measured trace elements except Hf (HfO2 = 0.53-0.92 wt. %). Cathodoluminescence images reveal oscillatory sector growth zoning and no evidence for xenocrystic cores, indicating that the zircons represent primary magmatic crystallization products that have survived amphibolite grade metamorphism. U-Pb isotopic analyses (by TIMS) yield an upper intercept age of 730 ± 4 Ma (MSWD = 1.7), which we interpret as the time of magmatic crystallization of the zircons. This is coincident with 11 SHRIMP spot analyses, which yield a mean age of 729 ± 7 Ma (MSWD = 0.37). Metamorphism, at 522 ± 17 Ma as suggested by monazite, caused partial Pb-loss during local recrystallization of zircon. Lu-Hf isotopic data for three whole-rock samples of nepheline-bearing gneiss are collinear with those for zircon megacrysts, and correspond to an age of 584 ± 17 Ma (MSWD = 0.37. We interpret the Lu-Hf array to represent a mixing line defined by the Hf isotopic signature of primary zircon and that of the rock-forming minerals reset during metamorphic (re-)crystallization; hence the 584 Ma age is likely geologically meaningless. Given the well-defined association of nepheline syenites (and phonolitic volcanic equivalents) with continental rifting, we suggest that the Tambani body represents a magmatic product formed at 730 Ma during the break-up of the Rodinia supercontinent. The 522 Ma age is akin to other Pan-African metamorphic ages that record collisional suturing events during the final assembly of Gondwana. Zircon-bearing nepheline gneisses thus preserve a record of intra-continental rifting and of continental collision in southern Malawi. | |
dc.identifier.issn | 0010-7999 | |
dc.identifier.uri | http://hdl.handle.net/1885/21020 | |
dc.publisher | Springer | |
dc.source | Contributions to Mineralogy and Petrology | |
dc.subject | Keywords: cathodoluminescence; collision zone; geochronology; gneiss; Gondwana; isotopic composition; megacryst; metamorphism; recrystallization; SHRIMP dating; tectonic setting; trace element; uranium-lead dating; zircon; Africa; East Africa; Malawi; Mozambique Be | |
dc.title | Geochronology of zircon megacrysts from nepheline-bearing gneisses as constraints on tectonic setting: implications for resetting of the U-Pb and Lu-Hf isotopic systems | |
dc.type | Journal article | |
local.bibliographicCitation.lastpage | 403 | |
local.bibliographicCitation.startpage | 389 | |
local.contributor.affiliation | Ashwal, L. D., University of the Witwatersrand | |
local.contributor.affiliation | Armstrong, Richard, College of Physical and Mathematical Sciences, ANU | |
local.contributor.affiliation | Roberts, R.J., University of the Witwatersrand | |
local.contributor.affiliation | Schmitz, Mark, Carnegie Institution of Washington | |
local.contributor.affiliation | Corfu, Fernando, University of Oslo | |
local.contributor.affiliation | Hetherington, C.J., University of Massachusetts | |
local.contributor.affiliation | Burke, K., University of Houston | |
local.contributor.affiliation | Gerber, M., University of the Witwatersrand | |
local.contributor.authoremail | u4029979@anu.edu.au | |
local.contributor.authoruid | Armstrong, Richard, u4029979 | |
local.description.embargo | 2037-12-31 | |
local.description.notes | Imported from ARIES | |
local.identifier.absfor | 040203 - Isotope Geochemistry | |
local.identifier.absfor | 040313 - Tectonics | |
local.identifier.ariespublication | u4027924xPUB15 | |
local.identifier.citationvolume | 153 | |
local.identifier.doi | 10.1007/s00410-006-0153-9 | |
local.identifier.scopusID | 2-s2.0-33847687615 | |
local.identifier.uidSubmittedBy | u4027924 | |
local.type.status | Published Version |
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