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To calculate the temperature of an object using a telescope, you can apply the principles of blackbody radiation and the Stefan-Boltzmann law. By observing the object's emitted infrared radiation through the telescope and measuring its brightness at various wavelengths, you can estimate its temperature. The temperature can then be inferred from the peak wavelength of the emitted radiation using Wien's displacement law or calculated using the total power emitted based on the measured flux. This method is commonly used in astrophysics to study celestial bodies like stars and planets.

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2mo ago

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