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The intense Lyman-a hydrogen solar emission line at 121.58 nm is strongly absorbed by O_2 in the stratosphere. This results in O_2's dissociation and the ultimate formation of ozone, O_3, to form the ozone layer. a. Calculate the energy of one photon with a wavelength of 121.58 nm. b. Calculate the energy for a mole of photons of wavelength 121.58 nm. (Remember that 1 mole = 6.022 times 10^23)
The intense Lyman-a hydrogen solar emission line at 121.58 nm is strongly absorbed by O_2 in the stratosphere. This results in O_2's dissociation and the ultimate formation of ozone, O_3, to form the ozone layer. a. Calculate the energy of one photon with a wavelength of 121.58 nm. b. Calculate the energy for a mole of photons of wavelength 121.58 nm. (Remember that 1 mole = 6.022 times 10^23)
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Keith LeannonLv2
18 May 2019
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