MSA AWARD LECTURE: CALIBRATING THE EFFECT OF WATER ON SEISMIC DISCONTINUITIES IN THE EARTH'S MANTLE
Due to the high solubility of H2O in the mineral wadsleyite it has been recognized that the presence of H2O in the mantle could influence the depth and depth interval of the olivine to wadsleyite phase transformation. This depth interval or width arises because the transformation occurs in a multi-component system, and is therefore smeared out over a pressure interval. The width of the 410 appears to vary regionally in the mantle from values of <4 km to over 30 km. To quantify the expansion of the wadsleyite stability field as a result of the presence of H2O, multianvil experiments were performed in the Mg2SiO4-H2O system. At 1200oC the wadsleyite stability field was found to expand to lower pressures by approximately 1 GPa under H2O saturated conditions. At 1400oC the expansion was approximately 0.4 GPa and no expansion was detected at 1600oC. When these results are combined with phase relations in the Mg2SiO4-Fe2SiO4 system it can be shown that significant effects on the pressure and pressure interval of the olivine to wadsleyite transformation are only expected at lower than ambient mantle temperatures and for H2O concentrations that are substantially greater than 0.2 weight %. Areas of the mantle where the 410-km discontinuity appears to occur over a depth interval of over 20 km can only be explained if the temperature in these regions is at or below 1200oCC and water concentrations are close to the level where olivine would become H2O saturated (i.e. >0.5 wt %). A broad discontinuity may not just arise from the presence of H2O however. The presence of ferric Fe can also broaden the olivine-wadsleyite transformation and there is significant evidence to argue that ferric iron is more likely to be the cause of broad 410 observations.