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1. The solar energy spectral density is shown in the right figure. By assuming that the sun is a blackbody, use the Plancks

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emperaturu abore the absolute Zer adliali em energy as function t Tenmber varve The amount s AkT ower per unit anea adbated t2 2. b Planek diutnbutin ook 4000 wavelength (m) 2max Can be detev mine thwaugh cseing alis placamant lows maxTo 0282.mk7ene dx 1- 2. 2hc hc eho/AKTh c K T n ax 9965k weinh clisplacement lao As夹omb uno reas e peakot spectrum Anttes tmated valiue 3 Theora Hal vauduue =| TheDva HCV - Estimated valw Value X100- 2 892.5 X100 2,898 13-7 ,/。 =​​​​​​

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