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Many planetary scientists argue that the chaotic terrain on Jupiter's moon Europa, characterized by disrupted blocks of ice, suggests a thin ice shell (under 5 kilometers thick) that regularly breaches. This thin-shell model implies that Europa's subsurface ocean frequently interacts with the surface, allowing photosynthetic organisms to potentially thrive near fractures where sunlight penetrates, and facilitating the detection of oceanic biosignatures by passing spacecraft.
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Conversely, planetary geophysicist Dr. Clara Sterling and her team utilize thermal modeling to argue that Europa's ice shell is likely over 20 kilometers thick. Sterling contends that the heat generated by tidal flexing is dissipated primarily through solid-state convection within the ice, rather than melting it thin. According to Sterling, any chaotic terrain is the result of warm, buoyant ice plumes rising slowly through the thick shell, never actually exposing the ocean directly to the surface.
Based on the passages, is the following statement true or false?
Dr. Clara Sterling would argue that the chaotic terrain on Europa can be explained by geological processes that do not involve the subsurface ocean breaching the ice shell.
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