In hydrogen spectrum, the shortest wavelength in the Balmer series is λ. The shortest wavelength in the bracket series is :
16λ
2λ
4λ
9λ
To determine the shortest wavelength in the Brackett series compared to the Balmer series, we refer to the Rydberg formula for wavelength of emitted light:
\[\frac{1}{\lambda} = R \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)\]
where \( R \) is the Rydberg constant, \( n_1 \) and \( n_2 \) are integers with \( n_2 > n_1 \). For the Balmer series, the transitions end at \( n_1 = 2 \), and for the Brackett series, transitions end at \( n_1 = 4 \).
For the Balmer series shortest wavelength (transition from infinity to n=2), we have:
\[\frac{1}{\lambda_{Balmer}} = R \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) = \frac{R}{4}\]
For the Brackett series shortest wavelength (transition from infinity to n=4), we have:
\[\frac{1}{\lambda_{Brackett}} = R \left( \frac{1}{4^2} - \frac{1}{\infty^2} \right) = \frac{R}{16}\]
Comparing these:
\[\frac{\lambda_{Balmer}}{\lambda_{Brackett}} = \frac{R/4}{R/16} = \frac{16}{4} = 4\]
Thus, the shortest wavelength in the Brackett series is \( 4\lambda \).
The shortest wavelength in the Balmer series occurs when an electron transitions from \(\infin\ \text{to}\ n = 2.\)
\(\because\frac{1}{λ}=Rz^2[\frac{1}{2^2}-\frac{1}{\infin^2}]\)
\(\frac{1}{λ}=\frac{R}{4}\ \ ....(i)\)
The shortest wavelength in the Brackett series occurs when an electron transitions from \(\infty\ \text{to}\ n = 4\).
\(\frac{1}{\lambda}=R(1)^2[\frac{1}{4^2}-\frac{1}{∞^2}]\)
\(⇒\frac{1}{λ'}=\frac{R}{16}\ \ ...(ii)\)
Now, By dividing Equation (i) and Equation (ii)
\(\frac{λ'}{λ}=\frac{R}{4}\times\frac{16}{R}⇒λ'=4λ\)
So, the correct option is (C) : 4λ.
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.