A star has 1040 deuterons. It produces energy via the process: 21H+21H⟶31H+11H 21H+31H⟶42He+10n If the average power radiated by the star is 1016W, then the deuteron supply of the star is exhausted in a time of the order of:
A
106sec
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B
108sec
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C
1012sec
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D
1016sec
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