Nick Mark MD on X: "The Stefan–Boltzmann law tells us that the power radiated by an object depends on its A surface area ε emissivity T temperature (σ is a constant) Emissivity (
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![Odia] The emissivity of black body is equal to](https://static.doubtnut.com/ss/web-overlay-thumb/10771975.webp "Odia] The emissivity of black body is equal to")
Odia] The emissivity of black body is equal to
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