Journal
NATURE COMMUNICATIONS
Volume 12, Issue 1, Pages -Publisher
NATURE PORTFOLIO
DOI: 10.1038/s41467-021-26710-0
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Funding
- U.S-Israel Binational Science Foundation (BSF) [2018152]
- National Aeronautics and Space Administration Habitable Worlds programme [FP062796-A/NNX16AR85G]
- Divn Of Social and Economic Sciences
- Direct For Social, Behav & Economic Scie [2018152] Funding Source: National Science Foundation
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The deep ocean of Europa, covered by a thick icy shell, has the potential to harbor extraterrestrial life. This study added critical elements to previous ocean dynamics research, revealing that the ocean is weakly stratified and dominated by salinity variations, exhibiting strong transient convection and eddies.
The deep (similar to 100 km) ocean of Europa, Jupiter's moon, covered by a thick icy shell, is one of the most probable places in the solar system to find extraterrestrial life. Yet, its ocean dynamics and its interaction with the ice cover have received little attention. Previous studies suggested that Europa's ocean is turbulent using a global model and taking into account non-hydrostatic effects and the full Coriolis force. Here we add critical elements, including consistent top and bottom heating boundary conditions and the effects of icy shell melting and freezing on ocean salinity. We find weak stratification that is dominated by salinity variations. The ocean exhibits strong transient convection, eddies, and zonal jets. Transient motions organize in Taylor columns parallel to Europa's axis of rotation, are static inside of the tangent cylinder and propagate equatorward outside the cylinder. The meridional oceanic heat transport is intense enough to result in a nearly uniform ice thickness, that is expected to be observable in future missions.
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