how to calculate the wavelength of second line of balmer series
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For the first line of any series (For Balmer, n = 2), wavenumber (1/λ) is represented as: 1/λ = R [1/n² - 1/(n+1)²], R is the Rydberg constant. The second line is represented as: 1/λ = R [1/n² - 1/(n+2)²], R is the Rydberg constant.
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=> The wavelengths of these lines are given by 1/λ = RH (1/4 − 1/n2), where λ is the wavelength, RH is the Rydberg constant, and n is the level of the original orbital.
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