Solveeit Logo

Question

Question: Calculate the wave number for the shortest wavelength transition in the Balmer series of atomic hydr...

Calculate the wave number for the shortest wavelength transition in the Balmer series of atomic hydrogen.

Explanation

Solution

Substitute the values of highest and lowest principal quantum number possible in the Rydberg formula to find the wave number.
Formula: 1λ=Z2R(1n121n22)\dfrac{1}{\lambda }={{Z}^{2}}{{R}_{\infty }}\left( \dfrac{1}{{{n}_{1}}^{2}}-\dfrac{1}{{{n}_{2}}^{2}} \right)
where,
1λ\dfrac{1}{\lambda } is the wavenumber,
Z is the atomic number,
R{{R}_{\infty }} is the Rydberg constant whose value is 1.09677107m11.09677*{{10}^{7}}{{m}^{-1}},
n1{{n}_{1}} is the principal quantum number of lower energy level,
n2{{n}_{2}} is the principal quantum number of upper energy level

Complete step by step answer:
We will now try to understand the emission spectrum of Hydrogen.
-When a hydrogen atom absorbs a photon, it causes the electron to experience a transition to a higher energy level, for example, n = 1 to n = 2.
-When a photon is emitted through a hydrogen atom, the electron undergoes a transition from a higher energy level to a lower, for example, n = 3 to n = 2.
-During this transition from a higher level to a lower level, there is the transmission of light.
The series of hydrogen emission spectrums have unique names based on the transition from higher energy to lower energy.
-Lyman Series: Transition of an electron from outer orbit having n>1 to n=1.
-Balmer Series: Transition of an electron from outer orbit having n>1 to n=2.
-Paschen Series: Transition of an electron from outer orbit having n>1 to n=3.
-Brackett Series: Transition of an electron from outer orbit having n>1 to n=4.
-Pfund Series: Transition of an electron from outer orbit having n>1 to n=5.
-Humphrey Series: Transition of an electron from outer orbit having n>1 to n=6.
It is important to remember that the wavelength emitted in the Balmer series alone lies in the visible range of the light spectrum.
The shortest wavelength transition in Balmer series is n=n=2n=\infty \to n=2
Substituting the above values in the Rydberg formula,
1λ=11.09677107(140)\dfrac{1}{\lambda }=1*1.09677*{{10}^{7}}*\left( \dfrac{1}{4}-0 \right)
1λ=2741925m1\dfrac{1}{\lambda }=2741925{{m}^{-1}}

Therefore, the wavenumber with the shortest wavelength transition is 2741925m12741925{{m}^{-1}}.

Note: Do not get confused between the meaning of n1{{n}_{1}}and n2{{n}_{2}}.n2{{n}_{2}} must always have a larger value than n1{{n}_{1}}for the transition to exist and wavelength to be transmitted.