Energy (E) of the nth Bohr orbit of an atom is given by,
\(E_n = \frac {-(2.18×10^{-18})Z^2}{n^2}\)
Where,
Z = atomic number of the atom
Ground state energy = - 2.18 × 10-11 ergs
= - 2.18 × 10-11× 10-7 J
= - 2.18 × 10-18 J
Energy required to shift the electron from n = 1 to n = 5 is given as:
\(ΔE = E_5-E_1\)
\(ΔE= \frac {-(2.18×10^{-18}) (1)^2}{(5)^2} - (- 2.18×10^{-18})\)
\(ΔE= (2.18×10^{-18}) [1 - \frac {1}{25}]\)
\(ΔE = (2.18×10^{-18}) (\frac {24}{25})\)
\(ΔE = 2.0928×10^{-18} J\)
Wavelength of emitted light = \(\frac {hc}{E}\)
= \(\frac {(6.626 × 10^{-34}) (3×10^8)}{(2.0928×10^{-18})}\)
= \(9.498×10^{-18} m\)
The emission spectrum of a chemical element or chemical compound is the spectrum of frequencies of electromagnetic radiation emitted due to an electron making a transition from a high energy state to a lower energy state. The photon energy of the emitted photon is equal to the energy difference between the two states.
Read More: Atomic Spectra
The Rydberg formula is the mathematical formula to compute the wavelength of light.
\[\frac{1}{\lambda} = RZ^2(\frac{1}{n_1^2}-\frac{1}{n_2^2})\]Where,
R is the Rydberg constant (1.09737*107 m-1)
Z is the atomic number
n is the upper energy level
n’ is the lower energy level
λ is the wavelength of light
Spectral series of single-electron atoms like hydrogen have Z = 1.