Abstract
AbstractSignificant quantities of shock‐induced melt are predicted to form during basin‐scale impact events and may contribute substantially to compositional variation in the lunar crust through differentiation processes. Knowledge of the evolution of impact melt sheets and the cooling and crystallization processes involved is therefore important to understanding the geology and petrology of the Moon. Here we perform a case study on the Orientale basin and investigate the possibility of differentiation of the impact melt sheet by assessing the thermal and physical processes that drive cooling and crystallization, focusing on crystal settling. Results predict that convective processes within the impact melt sheet enhance cooling and solidification and inhibit settling of crystals ~1.5 mm in diameter and smaller, preventing differentiation at or below this size. Impact melt sheet thickness is predicted to have minimal influence on crystallization history, suggesting that crystal size is the primary factor controlling lunar impact melt sheet differentiation.
Published Version (
Free)
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call