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How Does Ice Shell Geometry Shape Ocean Dynamics On Icy Moons? - Astrobiology

Summary by astrobiology.com
A poleward-thinning ice shell can drive circulation in the subsurface oceans of icy moons by imposing a meridional temperature gradient–colder at the equator than the pole–through the freezing point suppression due to pressure. This temperature gradient sets a buoyancy gradient, whose sign depends on the thermal expansion coefficient determined by ocean salinity. Together with vertical […] The post How Does Ice Shell Geometry Shape Ocean Dynamic…
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Twenty years of Cassini data are coming back to life – and with it a surprising discovery. A European team of scientists has reprocessed the data and discovered complex organic molecules. These substances come from geysers on Saturn's moon Enceladus, which shoot material from its interior into space....

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New Space Economy broke the news in on Thursday, November 6, 2025.
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