Recall that the solar constant—the flux of solar energy reaching Earth’s vicinity—is about 1,400 W/m2. If the Sun’s energy originates in the proton-proton cycle, at what rate (kg/s) does the Sun lose mass? Compare the yearly mass loss with the Sun’s total mass. Mass rate = 4.404 x 10^9 kg/s
Recall that the solar constant—the flux of solar energy reaching Earth’s vicinity—is about 1,400 W/m2. If the Sun’s energy originates in the proton-proton cycle, at what rate (kg/s) does the Sun lose mass? Compare the yearly mass loss with the Sun’s total mass. Mass rate = 4.404 x 10^9 kg/s
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Recall that the solar constant—the flux of solar energy reaching Earth’s vicinity—is about 1,400 W/m2. If the Sun’s energy originates in the proton-proton cycle, at what rate (kg/s) does the Sun lose mass? Compare the yearly mass loss with the Sun’s total mass.
Mass rate = 4.404 x 10^9 kg/s
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