Given that the solar spectrum corresponds to a temperature of T- 5800K and peaks at a wavelength of 1- 500 nm, use Wien's law to determine the wavelength (2') corresponding to the peak of the blackbody curve (a) in the core of the Sun, where the temperature is T' - 10'K, (b) in the solar convection zone (10° K), and (c) just below the solar photosphere (10* K). [Hint: AT - AT' (why?)] What form (visible, infrared, X ray, etc.) does the radiation take in each case?

Given that the solar spectrum corresponds to a temperature of T- 5800K and peaks at a wavelength of 1- 500 nm, use Wien's law to determine the wavelength (2') corresponding to the peak of the blackbody curve (a) in the core of the Sun, where the temperature is T' - 10'K, (b) in the solar convection zone (10° K), and (c) just below the solar photosphere (10* K). [Hint: AT - AT' (why?)] What form (visible, infrared, X ray, etc.) does the radiation take in each case?