Garnet-perovskite transformation under conditions of the Earth's lower mantle: an analytical transmission electron microscopy study

Citation
N. Miyajima et al., Garnet-perovskite transformation under conditions of the Earth's lower mantle: an analytical transmission electron microscopy study, PHYS E PLAN, 116(1-4), 1999, pp. 117-131
Citations number
31
Categorie Soggetti
Earth Sciences
Journal title
PHYSICS OF THE EARTH AND PLANETARY INTERIORS
ISSN journal
00319201 → ACNP
Volume
116
Issue
1-4
Year of publication
1999
Pages
117 - 131
Database
ISI
SICI code
0031-9201(199912)116:1-4<117:GTUCOT>2.0.ZU;2-G
Abstract
Natural pyrope garnets with three different chemical compositions have been transformed at 30-60 GPa in the laser-heated diamond-anvil cell (DAC). Rec overed samples were examined by analytical transmission electron microscopy (ATEM). For all three pyropes, the dominant post-garnet phase was Mg-rich orthorhombic silicate perovskite, The Al content of Mg-perovskite increased significantly with increasing pressure and temperature, and its chemical c omposition became close to that of the starting material. Mg-perovskite wit h Al2O3 content less than 25 mol% was quenched as a single phase of orthorh ombic perovskite at ambient conditions, whereas Mg-perovskite with Al2O3 co ntent of 25-28 mol% transformed into the alternating lamellae of orthorhomb ic perovskite and lithium niobate phases. With further increasing the Al2O3 content, Mg-perovskite converted into a single phase of the lithium niobat e structure with polysynthetic twinning on {1012} at ambient conditions. Th e high Al content may also induce the stabilization of Fe3+ in the perovski te structure accompanied by metallic iron. Two Al-rich phases, corundum and a new Al-rich phase (the NAL phase) were recognized with Mg-perovskite mos tly at lower pressures. The NAL phase is close to M3Al4Si1.5O12 (M = Mg, Fe , Ca, Na, K), i.e., the middle of A(2)O(3) and AB(2)O(4) type compounds, an d is accompanied by stishovite. The electron diffraction patterns are consi stent with the space group P6(3)/m or P6(3) with a = 8.85 (2) Angstrom, c = 2.78 (2) Angstrom, V = 188 (1) Angstrom(3). The existence of large cations such as Ca, K, and Na seems to stabilize the NAL phase relative to the cor undum phase, but excess Ca and Na contents are likely to induce the formati ons of Ca-rich cubic perovskite and the calcium ferrite phase, respectively . (C) 1999 Elsevier Science B.V. All rights reserved.