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The wavelength of emission for the H-atom is 656.3 nanometers (nm).
The wavelength of emission for the H-atom is calculated using the Rydberg formula, which is λ = R(1/n12 - 1/n22), where R is the Rydberg constant (1.097 x 107 m-1) and n1 and n2 are the initial and final energy levels of the electron.
The energy and wavelength of emission for the H-atom are inversely proportional. This means that as the energy level of the electron increases, the wavelength of emission decreases.
The wavelength of emission for the H-atom is unique and cannot be compared to other elements. Each element has its own unique set of energy levels and therefore its own unique wavelength of emission.
The wavelength of emission for the H-atom is significant because it provides valuable information about the energy levels and structure of the atom. It also allows us to identify and study the element in various forms, such as in emission spectra.