If we took a journey from Earth’s surface to the center, the midway point is roughly at 1900 km depth in the lower mantle. The lower mantle ranges from 660 to 2900 km depth and occupies 55% of our planet by volume. The chemical composition of the lower mantle is rather simple. It has long been pictured as being made up of 2 major minerals (~95%), namely bridgmanite and ferropericlase. Recently, this model was directly challenged by a set of discoveries in the lower mantle.
“One of the major lower mantle compositions, ferropericlase (Mg, Fe)O, turns into a pyrite-type structure upon meeting water. This intriguing chemical reaction only occurs at Earth’s deep lower mantle which is defined in depths between 1900 and 2900 km,” said Qingyang Hu from HPSTAR. “The reaction produces so-called oxygen excessive phases, or simply superoxides. The lower mantle is oxidized in the presence of water.” Generally, when all the oxygen atoms in a compound are bonded with metal atoms, they are called oxides. However, if a compound has paired oxygen atoms, like oxygen-oxygen bonding, it becomes a superoxide. Although superoxide is rarely found in nature, it might be common in Earth’s deep lower mantle.
“We also found that olivine and its high-pressure phase wadsleyite, the dominating minerals in the upper mantle, decompose to generate superoxides when subducting down into the deep mantle with water,” added by Jin Liu from at HPSTAR. Few approaches are available for scientists to probe the lower mantle mineralogy, given its depth. “Our experiments are very challenging. We input appropriate parameters like pressure, temperature, and starting minerals. Then we investigated the outputs including chemical reactions, new mineral assemblages, and their density profiles. Those parameters allow us to better constrain the nature of the lower mantle and its oxidation state. Contrary to the paradigm that the lower mantle is highly reduced, our results indicate that the deep lower mantle is at least locally oxidized wherever water is present.”
The team members proceeded with minerals existing on Earth’s surface, by squeezing them between two pieces of diamond anvils to generate about 100,000,000 times the atmospheric pressure at sea level, heating them up using an infrared laser, before analyzing the samples using a battery of X-ray and electron probes. The experiments have mimicked the extreme pressure-temperatures conditions found in Earth’s deep lower mantle.
Previous experiments explored a dry mineral assembly in the absence of water. Those experiments reported that bridgmanite (and/or post-bridgmanite) and ferropericlase are the most abundant and stable minerals throughout the lower mantle. However, when water is introduced, ferropericlase would be partially oxidized to superoxide under the deep lower mantle conditions. The superoxide is verified to stay in harmony with bridgmanite and post-bridgmanite.
This new water-mantle chemistry can be closely linked to the water cycling in the solid Earth. Every year, billions of tons of ocean water falls into the deep Earth at tectonic plate boundaries. While some water returns via underwater volcanoes and hot vents, some goes deep into the Earth’s interior. “Our experiments indicate the deep water is an essential part of mantle chemistry. The water cycling can extend to the deep lower mantle where water has extraordinary oxidation power, producing highly oxidized superoxide and releasing hydrogen,” suggested Dr. Ho-kwang Mao from HPSTAR. “The lower mantle can be oxidized and reduced at the same time.”
Qingyang Hu et al, Mineralogy of the deep lower mantle in the presence of H2O, National Science Review (2020). DOI: 10.1093/nsr/nwaa098
Note: The above post is reprinted from materials provided by Science China Press.