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PLEASE HELP, WITH JUST #2. I understand number 1 with answers being 2.15x10^-22 kJ and longest wavelength being 1.88x10^3 nm.

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1) Use the Balmer-Rydberg equation to calculate the wavelength (in nm) and energy (in kJ/mol) emitted due to the transition of electrons from the 9th to the 3 orbital (Paschen series). Calculate the wavelength (in nm) and energy (in kJ/mol) for the longest wavelength in this series. 2) For the problem above, the wavelength differences between lines in the Balmer series become smaller as n” becomes larger. In other words, the wavelengths converge toward a minimum value as n” becomes very large. At what wavelength (in nm) do the lines converge?

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Answer #1

nマ= oemes 2 ว่า E 3-G 21 佇- 8211 3 A US aNejen

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