What is the approximate mass loss rate for a Sun-like star during the Red Giant/AGB phase, according to the provided table?
Answer
$\sim 10^{-6}$ to $10^{-5} M_{\odot}/\text{yr}$
The table specifies that during the Red Giant/AGB phase, the approximate mass loss rate is in the range of $10^{-6}$ to $10^{-5}$ solar masses per year, which is significantly higher than the main sequence rate of $10^{-14} M_{\odot}/\text{yr}$.
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