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supernova's energy is often compared to the total energy output of the Sun over its lifetime. sing the Sun's current luminosity, calculate the total solar energy output, assuming a 1010 ear main-sequence lifetime. sing Einstein's formula E=mc² calculate the equivalent amount of mass, expressed in arth masses. [Hint: The total energy output of the Sun over its lifetime is given by its current aminosity times the number of seconds in a year times its ten billion-year lifetime; Week 5 ide 4; mass of earth = 6x1024kg; c = 3x10®m/s. Your answer should be 200-300 Earth nasses.] %3D

supernova's energy is often compared to the total energy output of the Sun over its lifetime. sing the Sun's current luminosity, calculate the total solar energy output, assuming a 1010 ear main-sequence lifetime. sing Einstein's formula E=mc² calculate the equivalent amount of mass, expressed in arth masses. [Hint: The total energy output of the Sun over its lifetime is given by its current aminosity times the number of seconds in a year times its ten billion-year lifetime; Week 5 ide 4; mass of earth = 6x1024kg; c = 3x10®m/s. Your answer should be 200-300 Earth nasses.] %3D

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A supernova's energy is often compared to the total energy output of the Sun over its lifetime. Using the Sun's current luminosity, calculate the total solar energy output, assuming a 1010 year main-sequence lifetime. Using Einstein's formula E = mc? calculate the equivalent amount of mass, expressed in Earth masses. [Hint: The total energy output of the Sun over its lifetime is given by its current luminosity times the number of seconds in a year times its ten billion-year lifetime; Week 5 slide 4; mass of earth = 6x1024kg; c = 3x10®m/s. Your answer should be 200-300 Earth masses.]
Transcribed Image Text:A supernova's energy is often compared to the total energy output of the Sun over its lifetime. Using the Sun's current luminosity, calculate the total solar energy output, assuming a 1010 year main-sequence lifetime. Using Einstein's formula E = mc? calculate the equivalent amount of mass, expressed in Earth masses. [Hint: The total energy output of the Sun over its lifetime is given by its current luminosity times the number of seconds in a year times its ten billion-year lifetime; Week 5 slide 4; mass of earth = 6x1024kg; c = 3x10®m/s. Your answer should be 200-300 Earth masses.]
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