In analyzing the ice-sheet dynamics of Jupiter's moon Europa, astrobiologists originally posited that the outer lithospheric shell remained entirely rigid except when disrupted by high-velocity impacts. However, recent thermal modeling of convective ice plumes suggests that the deep sub-surface ice shell displays a surprisingly plastic response to tidal forces. Far from remaining brittle or undergoing sudden, catastrophic fracturing, the cryogenic ice gradually deforms and flows under low, continuous gravitational stress without losing its solid-phase continuity. Consequently, planetary geologists must revise their rheological models to account for this creeping internal movement, recognizing that the material yields dynamically over vast temporal scales rather than maintaining an unyielding structural monolith.
In the context of the passage, the word "plastic" most nearly means
- Acomposed of synthetic polymeric materials
- capable of continuous deformation without fracturingCevap
- Creturning immediately to an original shape once stress is removed
- Dprone to sudden structural failure under low thermal thresholds
- Efluctuating rapidly over brief temporal intervals