High-pressure diamond-cell experiments indicate that the iron-magnesiu
m partitioning between (Fe,Mg)SiO3-perovskite and magnesiowustite in E
arth's lower mantle depends on the pressure, temperature, bulk iron/ma
gnesium ratio, and ferric iron content, The perovskite stability field
expands with increasing pressure and temperature. The ferric iron com
ponent preferentially dissolves in perovskite and raises the apparent
total iron content but had little effect on the partitioning of the fe
rrous iron, The ferrous iron depletes in perovskite at the top of the
lower mantle and gradually increases at greater depth. These changes i
n iron-magnesium composition should affect geochemical and geophysical
properties of the deep interior.