Equations of state of Na-K-Al host phases and implications for MORB density in the lower mantle

Details Equations of state of Na-K-Al host phases and implications for MORB density in the lower mantle Equations of state of Na-K-Al host phases and implications for MORB density in the lower mantle

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004pepi..143..107g&link_type=abstract

Physics of the Earth and Planetary Interiors, Volume 143, p. 107-128.

Physics

20

Scientific paper

We report equations of state (EoS) of two important silicate phases known to store Na, K, and Al, at pressures and temperatures prevailing in the Earth's lower mantle. Using laser heated diamond anvil cell, we produced the Ca-ferrite type (CF) and the new aluminum rich (NAL) phases using different synthetic and natural starting materials, at pressures ranging from 23 to 65GPa. Unit cell volumes were investigated by means of angle dispersive X-ray diffraction at the ID30 beamline of the ESRF synchrotron ring (Grenoble, France). CF-phases were synthesized in NaAlSiO4-MgAl2O4 and NaAlSiO4-(Mg,Fe)2SiO4 systems, and for a natural mid-ocean ridge basalt (MORB). The insertion of MgAl2O4 in the NaAlSiO4-based lattice has reduced effects on the CF-phase EoS, whereas that of (Mg,Fe)2SiO4 is mainly to increase the room pressure volume. CF-phases most relevant to the Earth's mantle show compression behavior comparable to the pure NaAlSiO4-CF-phase, with bulk moduli values close to K0=190GPa and K0'=4. We also synthesized (NAL) phases in NaAlSiO4-MgAl2O4 system, and using CaNa- and K-rich silicate glasses as starting materials. All NAL-compounds investigated show similar compression behavior, except for one anomalously NaAlSiO4-rich composition. For NAL-phase with the most ``natural'' conditions relevant composition, we refine bulk moduli of K0=182GPa and K0'=6.
We then model the density profiles expected for the CF and NAL-phases, using our newly determined EoS and the most accurate chemical compositions reported in the literature. These two phases appear significantly less dense than a pyrolitic type material at all lower mantle pressures and 300K. However, the density profiles calculated for mineral assemblages corresponding to typical MORB compositions point out to denser MORBs compared to the pyrolite. This is due to the high Fe-content in MORB, yielding a densest Fe-rich perovskite that counterbalances the lower densities of the CF and NAL-phases. The density gap is calculated between 0.4 and 4.0% depending on the starting MORB composition and pressure.

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