Tetragonal almandine pyrope phase (TAPP): retrograde Mg-perovskite from subducted oceanic crust

LS Armstrong, MJ Walter

Research output: Contribution to journalArticle (Academic Journal)peer-review

21 Citations (Scopus)

Abstract

Laser heated diamond-anvil cell experiments performed on a “tetragonal almandine pyrope phase” (TAPP) bulk composition constrain high-temperature phase relations between 6 and 48 GPa. Phase assemblages determined by synchrotron X-ray diffraction consist of TAPP + garnet ± pseudobrookite ± enstatite from 6-10 GPa, garnet from 13-22 GPa, Mg-perovskite + garnet from 23-30 GPa, and Mg-perovskite above 30 GPa. TAPP has the same structure at 1 atm and at high pressure based on in situ X-ray diffraction data, and is stable at a maximum pressure of 10-13 GPa at 1300-1700 K. These results rule out direct incorporation of TAPP in diamond at transition zone or lower mantle pressures. Possible origins of TAPP are (1) entrapment by diamonds in the upper mantle, and (2) retrograde formation from a high-pressure garnet or Mg-perovskite precursor. We suggest that single-phase TAPP inclusions and possibly composite TAPP-bearing inclusions originated as Mg-Pv in the lower mantle in mafic protoliths, and that TAPP forms upon retrograde conversion at pressures below 13 GPa upon exhumation of the diamonds from the lower mantle to shallower depths of less than 400 km.
Translated title of the contributionTetragonal almandine pyrope phase (TAPP): retrograde Mg-perovskite from subducted oceanic crust
Original languageEnglish
JournalEuropean Journal of Mineralogy
DOIs
Publication statusPublished - 2012

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