Unveiling Mars: The Hidden Molten Layers Beneath

Geophysical evidence from seismic data collected by the NASA InSight mission suggests the presence of an enriched molten silicate layer, known as the basal mantle layer (BML), above Mars's core. This BML, which is strongly enriched in iron and heat-producing elements, acts as a buffer between the core and mantle, reducing heat transfer and influencing Mars's thermochemical evolution. The presence of the BML explains the observed seismic reflections occurring above the core-mantle boundary (CMB) and suggests a smaller and denser core than previously inferred. These findings challenge the assumption of a homogeneous Martian mantle and provide new insights into the internal structure of Mars.
- Geophysical evidence for an enriched molten silicate layer above Mars’s core Nature.com
- Mars Conceals a Radioactive Sea of Magma Under Its Surface The New York Times
- Mars hides a core of molten iron deep inside Ars Technica
- Scientists identify molten layer deep within interior of Mars Reuters
- Evidence for a liquid silicate layer atop the Martian core Nature.com
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