Mafic High-Pressure Rocks Are Preferentially Exhumed From Warm Subduction Settings

Peter E. van Keken, Ikuko Wada, Geoffrey A. Abers, Bradley R. Hacker, Kelin Wang

Research output: Contribution to journalArticlepeer-review

29 Scopus citations


The oceanic crust that enters a subduction zone is generally recycled to great depth. In rare and punctuated episodes, however, blueschists and eclogites derived from subducted oceanic crust are exhumed. Compilations of the maximum pressure-temperature conditions in exhumed rocks indicate significantly warmer conditions than those predicted by thermal models. This could be due to preferential exhumation of rocks from hotter conditions that promote greater fluid productivity, mobility, and buoyancy. Alternatively, the models might underestimate the forearc temperatures by neglecting certain heat sources. We compare two sets of global subduction zone thermal models to the rock record. We find that the addition of reasonable amounts of shear heating leads to less than 50 °C heating of the oceanic crust compared to models that exclude this heat source. Models for young oceanic lithosphere tend to agree well with the rock record. We test the hypothesis that certain heat sources may be missing in the models by constructing a global set of models that have high arbitrary heat sources in the forearc. Models that satisfy the rock record in this manner, however, fail to satisfy independent geophysical and geochemical observations. These combined tests show that the average exhumed mafic rock record is systematically warmer than the average thermal structure of mature modern subduction zones. We infer that typical blueschists and eclogites were exhumed preferentially under relatively warm conditions that occurred due to the subduction of young oceanic lithosphere or during the warmer initial stages of subduction.

Original languageEnglish (US)
Pages (from-to)2934-2961
Number of pages28
JournalGeochemistry, Geophysics, Geosystems
Issue number9
StatePublished - Sep 2018

Bibliographical note

Funding Information:
We thank Sarah Penniston-Dorland for providing an updated data set of the exhumed rock record and Michael Brown for providing his new compilation of the exhumed rock record before publication. We also thank Sarah Penniston-Dorland and Michael Brown for discussion and constructive reviews of an earlier version of this manuscript. We thank Bruno Reynard, Donna Whitney, and Philippe Agard for discussions. We are grateful to Simon Wallis, J?rg Hermann, and Taras Gerya for their very helpful and constructive reviews. In supporting information Data Set S1 we provide text files that describe the thermal structure of the oceanic crust as predicted from our models.


  • geodynamics
  • metamorphic petrology
  • modeling
  • seismology
  • shear heating
  • subduction zone thermal structure

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