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In order to continue enjoying our site, we ask that you confirm your identity as a human. Thank you very much for your cooperation. Text Solution Solution : since `n_(1) = 5 and n_(1) = 2 `, this transition gives rise to a spectral line in the visible region of the balmer series. From equation <br> `DeltaE=2.18xx10^(-18)J[1/5^(2)-1/2^(2)]` <br>` 4.58xx 10^(-19)J` <br> it is an emission energy <br> the frequency of the photon ( taking energy in terms of magnitude ) is given by <br> `v=(DeltaE)/h` <br> `( 4.58xx10^(-19)J)/(6.626xx10^(-34) Js)` <br> `6.91xx10^(14)Hz` <br> ` lambda=c/v= (3.0xx10^(8)m s^(-1))/(6.91xx10^(14)Hz)=434 nm` The energy transition will be equal to #1.55 * 10^(-19)"J"#. So, you know your energy levels to be n = 5 and n = 3. Rydberg's equation will allow you calculate the wavelength of the photon emitted by the electron during this transition #1/(lamda) = R * (1/n_("final")^(2) - 1/n_("initial")^(2))#, where #lamda# - the wavelength of the emitted photon; So, you've got all you need to solve for #lamda#, so #1/(lamda) = 1.0974 * 10^(7)"m"^(-1) * (1/3^2 - 1/5^2)# #1/(lamda) = 0.07804 * 10^(7)"m"^(-1) => lamda = 1.28 * 10^(-6)"m"# Since #E = (hc)/(lamda)#, to calculate for the energy of this transition you'll have to multiply Rydberg's equation by #h * c#, where #h# - Planck's constant - #6.626 * 10^(-34)"J" * "s"# So, the transition energy for your particular transition (which is part of the Paschen Series) is #E = (6.626 * 10^(-34)"J" * cancel("s") * "299,792,458" cancel("m/s"))/(1.28 * 10^(-6)cancel("m"))# #E = 1.55 * 10^(-19)"J"# |