Geometry of freezing impacts ice composition: implications for icy satellites
Geometry of freezing impacts ice composition: implications for icy satellites
Date
2023-03-14
Authors
Buffo, Jacob J.
Meyer, Colin R.
Chivers, Chase J.
Walker, Catherine C.
Huber, Christian
Schmidt, Britney E.
Meyer, Colin R.
Chivers, Chase J.
Walker, Catherine C.
Huber, Christian
Schmidt, Britney E.
Linked Authors
Person
Person
Person
Person
Person
Files
Alternative Title
Citable URI
As Published
Date Created
Location
DOI
10.1029/2022JE007389
Related Materials
Replaces
Replaced By
Keywords
Ice-ocean worlds
Ice-brine systems
Europa
Multiphase solidification
Ice-brine systems
Europa
Multiphase solidification
Abstract
Non‐ice impurities within the ice shells of ocean worlds (e.g., Europa, Enceladus, Titan, Ganymede) are believed to play a fundamental role in their geophysics and habitability and may become a surface expression of subsurface ocean properties. Heterogeneous entrainment and distribution of impurities within planetary ice shells have been proposed as mechanisms that can drive ice shell overturns, generate diverse geological features, and facilitate ocean‐surface material transport critical for maintaining a habitable subsurface ocean. However, current models of ice shell composition suggest that impurity rejection at the ice‐ocean interface of thick contemporary ice shells will be exceptionally efficient, resulting in relatively pure, homogeneous ice. As such, additional mechanisms capable of facilitating enhanced and heterogeneous impurity entrainment are needed to reconcile the observed physicochemical diversity of planetary ice shells. Here we investigate the potential for hydrologic features within planetary ice shells (sills and basal fractures), and the unique freezing geometries they promote, to provide such a mechanism. By simulating the two‐dimensional thermal and physicochemical evolution of these hydrological features as they solidify, we demonstrate that bottom‐up solidification at sill floors and horizontal solidification at fracture walls generate distinct ice compositions and provide mechanisms for both enhanced and heterogeneous impurity entrainment. We compare our results with magmatic and metallurgic analogs that exhibit similar micro‐ and macroscale chemical zonation patterns during solidification. Our results suggest variations in ice‐ocean/brine interface geometry could play a fundamental role in introducing compositional heterogeneities into planetary ice shells and cryoconcentrating impurities in (re)frozen hydrologic features.
Description
Author Posting. © American Geophysical Union, 2023. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research: Planets 128(3), (2023): e2022JE007389, https://doi.org/10.1029/2022JE007389.
Embargo Date
Citation
Buffo, J. J., Meyer, C. R., Chivers, C. J., Walker, C. C., Huber, C., & Schmidt, B. E. (2023). Geometry of freezing impacts ice composition: implications for icy satellites. Journal of Geophysical Research: Planets, 128(3), e2022JE007389.