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DC of a collapsing star?

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As the title suggests, what is initially DC of the gravitational force of a collapsing star?
 
GBE is used to measure the minimal energy needed to disrup the gravitional field of a celestial body. Gradualing destroying an star should yield less than that, but in an unknown amount.
 
After looking up the GBE, I found for the sun is 6.87e41j, would be in the Yottatons right?
 
Since the question has been answered, I will close this thread.
 
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