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3. Fusion Processes At one point in a star's lifetime, it fuses Helium into Carbon. At another stage, it fuses Carbon into Oxygen. Use the

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3. Fusion Processes At one point in a star's lifetime, it fuses Helium into Carbon. At another stage, it fuses Carbon into Oxygen. Use the binding energy plot below to answer the following questions: a. b. Do these processes release energy or take in energy? How much? If the star maintains approximately the same luminosity during each phase, which fusion phase will last longer? Explain your reasoning. Average binding energy per nucleon (MeV) 30 60 90 120 150 180 210 240 270 Number of nucleons in nucleus

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