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Physics, 28.05.2020 19:00 Jacobolobo7

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P=4pi r ^2 oT^4
where P is the energy rate output of the object, T is it’s temperature, r is it’s radius, and is the Stefan Boltzman constant (5.670 x 10^-8W m ^2K ^-4 . If the temperature and radius of the Sun are approximately 5800 K (hot!!) and 6.995 x 10^8 , respectively, calculate the rate of energy output of the Sun in Watts.

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P=4pi r ^2 oT^4
where P is the energy rate output of the object, T is it’s...
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