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How can SSM be utilized to predict the radius of the Sun when it becomes a red giant?
The discussion revolves around the utilization of the Standard Solar Model (SSM) to predict the radius of the Sun when it transitions into a red giant phase. The scope includes theoretical aspects of stellar evolution and modeling.
Participants have not reached a consensus on how SSM specifically applies to predicting the Sun's radius as a red giant, and multiple interpretations of SSM exist within the discussion.
The discussion includes a variety of definitions for SSM, which may lead to misunderstandings regarding its application in the context of the Sun's evolution.