Continuous ablation during engulfment dissolves Jupiter-like planets completely inside stellar convective envelopes, enabling observable lithium enrichment.
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SPH simulations show that ice can be preferentially stripped from a differentiated moon during close encounters with Saturn to produce rings matching the observed mass and composition, if the closest approach lies between the ice and rock Roche limits.
citing papers explorer
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Continuous mass ablation of planets engulfed in stellar envelopes
Continuous ablation during engulfment dissolves Jupiter-like planets completely inside stellar convective envelopes, enabling observable lithium enrichment.
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Investigating tidal stripping of a pre-existing moon as the origin of Saturn's young icy rings
SPH simulations show that ice can be preferentially stripped from a differentiated moon during close encounters with Saturn to produce rings matching the observed mass and composition, if the closest approach lies between the ice and rock Roche limits.