The mantle perspective provided by radiogenic isotope geochemistry has evolved over the
last 40 years. Although the idea of an upper mantle depleted in incompatible elements by …

The Earth's mantle redox state regulates the fate and transfer of metals by magmatism,
buffers the igneous inputs of volcanic gases in the atmosphere and controls the depth of …

Aims. We present an inversion method based on Bayesian analysis to constrain the interior
structure of terrestrial exoplanets, in the form of chemical composition of the mantle and core …

The formation of Earth's core left behind geophysical and geochemical signatures in both
the core and mantle that remain to this day. Seismology requires that the core be lighter than …

The bulk chemical compositions of planets are uncertain, even for major elements such as
Mg and Si. This is due to the fact that the samples available for study all originate from …

The range in density and compressibility of Mercurian melt compositions was determined to
better understand the products of a possible Mercurian magma ocean and subsequent …

Context. The chemical composition of planets is an important constraint for planet formation
and subsequent differentiation. While theoretical studies try to derive the compositions of …

The final stage of terrestrial planet formation consists of several hundred approximately
lunar mass bodies accreting into a few terrestrial planets. This final stage is stochastic …

The two large low shear-wave velocity provinces (LLSVPs) that dominate lower-mantle
structure may hold key information on Earth's thermal and chemical evolution. It is generally …

Genetic contributions to the final stages of planetary growth, including materials associated
with the giant Moon-forming impact, late accretion, and late heavy bombardment are …