Red giants and angular momentum question

AI Thread Summary
The discussion centers on the fate of Mercury as the Sun expands into its Red Giant phase. It explores the idea that while Mercury may evaporate due to extreme temperatures, it could retain its angular momentum and continue to orbit the Sun's center of gravity. The participants suggest that the gas molecules from the evaporated planet would maintain similar orbital speeds, preventing a spiral into the core. The consensus indicates that angular momentum will remain part of the total angular momentum of the expanding star. Overall, the conversation highlights the intriguing dynamics of planetary evaporation and angular momentum during stellar evolution.
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I was watching a Discovery channel program about the future of our Sun (and any similar star). They were describing the expansion of the star as it goes to Red Giant stage, and how it would eventually expand to include Mercury. At first I thought that the molten planet would slow due to friction within the perimeter of the star and spiral down into the core, but then it occurred to me that the expanded star would still retain the angular momentum, and the gas molecules might be orbiting the center of gravity at the same speed, so the blob of ex-Mercury would just continue as it evaporated away. Correct? Incorrect?

Just one of the weird things I ponder. I'd love to hear some evaluations of what would happen. Thanks in advance.
 
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5000K (red giant surface) is enough to evaporate everything. My guess is that planets will evaporate and diffuse. Angular momentum will be there, just as a part of total angular momentum of the star.
 
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