Interior Structure Models Of Venus
Oliver Shah, Ravit Helled, Yann Alibert, Klaus Mezger

TL;DR
This study models Venus's interior structure, exploring possible core sizes and compositions, and suggests future measurements could clarify its formation, evolution, and differences from Earth.
Contribution
It provides the first comprehensive range of Venus interior models considering various compositions and core segregation scenarios.
Findings
Core size estimated at 2930-4350 km.
Normalized moment of inertia (MoI) estimated at 0.317-0.351.
Solid inner core could exist under all modeled compositions.
Abstract
Venus' mass and radius are similar to those of Earth. However, dissimilarities in atmospheric properties, geophysical activity and magnetic field generation could hint towards significant differences in the chemical composition and interior evolution of the two planets. Although various explanations for the differences between Venus and Earth have been proposed, the currently available data are insufficient to discriminate among the different solutions. Here we investigate the possible range of Venus structure models. We assume that core segregation happened as a single-stage event. The mantle composition is inferred from the core composition using a prescription for metal-silicate partitioning. We consider three different cases for the composition of Venus defined via the bulk Si and Mg content, and the core's S content. Permissible ranges for the core size, mantle and core composition…
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Taxonomy
TopicsPlanetary Science and Exploration · Astro and Planetary Science · Space Exploration and Technology
