Scaling of convection in high-pressure ice layers of large icy moons and implications for habitability
The existence of a high-pressure (HP) ice layer between the silicate core and the liquid ocean in large icy moons and ocean worlds is usually seen as a barrier to habitability, preventing a direct contact and therefore transfer of nutrients from the core to the liquid ocean. More recently, several s...
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Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2023-05, Vol.396, p.115494, Article 115494 |
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