Since we need to consider the photon with the longest wavelength that ends the electron transition in the state with the quantum number "n=2" , this will be transition "3-2" since the photon energy formula "E=h\\times \\frac{c}{\\lambda}" , (where "h" is the Planck constant, "c" is the speed of light, and "\\lambda" is the wavelength) shows that the photon energy is inversely proportional to the wavelength, and since a larger transition corresponds to a large absorption/release of energy, we choose the smallest transition (transition "1-2>" transitions "2-3" ). By the formula "\\frac{1}{\\lambda}=R\\times(\\frac{1}{m^2}-\\frac{1}{n^2})" (where "R" is the Rydberg constant, and "n" and "m" are the quantum numbers of the photon state) "\\frac{1}{\\lambda}=3.29\\times10^{15}\\times(\\frac{1}{2^2}-\\frac{1}{3^2})" "=\\frac{5\\times 3.29\\times10^{15}}{36}" therefore "\\lambda=\\frac{36}{5\\times 3.29\\times10^{15}}=2.19\\times 10^{-15}" m.
"E=6.63\\times 10^{-34}\\times \\frac{3\\times 10^8}{2.19\\times 10^{-15} }=9.08\\times 10^{-11}" J.
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