Unverified50% confidenceFactExact time
The outer atmospheres of red supergiants are extremely tenuous and dynamically changing, and stellar pulsation, convection, and mass ejection make it impossible to clearly define a boundary between the stellar surface and the stellar wind, so there is no precise upper limit on the maximum radius.
1
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50%
Confidence
Long-term
Relevance
10/13/2026
First Seen
Sources
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