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Ancient melt depletion overprinted by young carbonatitic metasomatism in the New Zealand lithospheric mantle

  • J. M. Scott
  • , A. Hodgkinson
  • , J. M. Palin
  • , T. E. Waight
  • , Q. H.A. van der Meer
  • , A. F. Cooper

Rannsóknarafurð: Framlag til fræðitímaritsGreinritrýni

Útdráttur

Spinel facies dunite, harzburgite, lherzolite and wehrlite mantle xenoliths from a cluster of Miocene volcanoes in southern New Zealand preserve evidence of the complex evolution of the underlying continental mantle lithosphere. Spinel Cr# records melt extraction with some values indicative of near complete removal of clinopyroxene. LREE-enriched, low Ti/Eu and low Al2O3 clinopyroxene and rare F-, LREE-rich apatite indicates subsequent interaction between peridotite and a metasomatising carbonatitic melt. The clearest metasomatic signature occurs in the formerly highly depleted samples because there was little or no pre-existing clinopyroxene to dilute the carbonatite signature. For the same reason, the isotopic character of the metasomatising agent is best observed in the formerly highly depleted peridotites (87Sr/86Sr = 0.7028-0.7031; 143Nd/144Nd = 0.5129; 206Pb/204Pb = 20.2-20.3). These isotope ratios are very close to, but slightly less radiogenic than, the HIMU end-member mantle reservoir. Nd isotope data imply carbonatite metasomatism occurred within the last several hundred million years, with ubiquitous pyroxene core-to-rim Al diffusion zoning indicating that it must pre-date cooling of the lithospheric mantle following Late Cretaceous-Eocene rifting of Zealandia from Gondwana. Metasomatism was significantly younger than ancient Re-depletion ages of ~2 Ga and shows that decoupling of peridotite isotope systems has occurred.

Upprunalegt tungumálEnska
Númer greinar963
Síður (frá-til)1-17
Síðufjöldi17
FræðitímaritContributions to Mineralogy and Petrology
Bindi167
Númer tölublaðs1
DOI
ÚtgáfustaðaÚtgefið - jan. 2014

Athugasemd

Funding Information: Acknowledgments We thank the Foundation for Research, Science and Technology for contract UOOX1004 to JMS; the AUSIMM for a scholarship to AH; the Carlsberg Foundation and Danish Research Council for Nature and Universe for research grants to TEW; A. Riches, C. Perinelli and C. Ballhaus for comments on the text.

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