Coreless Terrestrial Exoplanets

TL;DR

This paper predicts the existence of coreless terrestrial exoplanets, formed through oxidation processes during accretion, which lack metallic cores and have implications for interpreting exoplanet compositions.

Contribution

It introduces the concept of coreless terrestrial planets formed via oxidation, challenging the assumption that all differentiated planets have metallic cores.

Findings

Coreless planets are possible through oxidation during formation.

Such planets would have different interior density profiles.

Impacts interpretation of exoplanet mass-radius data.

Abstract

Differentiation in terrestrial planets is expected to include the formation of a metallic iron core. We predict the existence of terrestrial planets that have differentiated but have no metallic core--planets that are effectively a giant silicate mantle. We discuss two paths to forming a coreless terrestrial planet, whereby the oxidation state during planetary accretion and solidification will determine the size or existence of any metallic core. Under this hypothesis, any metallic iron in the bulk accreting material is oxidized by water, binding the iron in the form of iron oxide into the silicate minerals of the planetary mantle. The existence of such silicate planets has consequences for interpreting the compositions and interior density structures of exoplanets based on their mass and radius measurements.