For the longest wavelength in the Paschen series:
\[\frac{1}{\lambda} = R \left[ \frac{1}{n_1^2} - \frac{1}{n_2^2} \right]\]
For the longest wavelength, \( n_1 = 3 \) and \( n_2 = 4 \).
\[\frac{1}{\lambda} = R \left[ \frac{1}{3^2} - \frac{1}{4^2} \right]\]
\[\frac{1}{\lambda} = R \left[ \frac{1}{9} - \frac{1}{16} \right]\]
\[\frac{1}{\lambda} = R \cdot \frac{16 - 9}{144} = R \cdot \frac{7}{144}\]
Now, substitute \( R = 1.097 \times 10^7 \):
\[\frac{1}{\lambda} = \frac{7 \times 1.097 \times 10^7}{144}\]
\[\lambda = \frac{144}{7 \times 1.097 \times 10^7} = 1.876 \times 10^{-6} \, \text{m}\]
To determine the longest wavelength associated with the Paschen series, we should first understand the concept of spectral lines in the hydrogen atom. The Paschen series corresponds to transitions where the electron falls to the third energy level (\(n_2 = 3\)) from a higher energy level (\(n_1 \gt 3\)).
The formula to calculate the wavelength (\(\lambda\)) of the emitted photon for a transition from level \(n_1\) to \(n_2\) is given by:
\(\frac{1}{\lambda} = R_H \left( \frac{1}{n_2^2} - \frac{1}{n_1^2} \right)\)
Here, \(R_H\) is the Rydberg constant, approximately equal to \(1.097 \times 10^7\) m-1.
To find the longest wavelength in the Paschen series, we need to consider the transition from the smallest possible value of \(n_1\) to \(n_2 = 3\). The smallest possible integer for \(n_1\) is 4 because \(n_1\) must be greater than 3.
Using \(n_1 = 4\) and \(n_2 = 3\), let's calculate the wavelength:
\(\frac{1}{\lambda} = 1.097 \times 10^7 \left( \frac{1}{3^2} - \frac{1}{4^2} \right)\)
Calculate the expression inside the parentheses:
\(\frac{1}{9} - \frac{1}{16} = \frac{16 - 9}{144} = \frac{7}{144}\)
Thus,
\(\frac{1}{\lambda} = 1.097 \times 10^7 \times \frac{7}{144}\)
Calculate this value to find \(\lambda\):
\(\lambda = \frac{144}{1.097 \times 10^7 \times 7} \approx 1.87568 \times 10^{-6} \text{ meters}\)
Rounding this, we get approximately \(1.876 \times 10^{-6} \text{ m}\), which matches the correct answer.
Therefore, the longest wavelength associated with the Paschen series is 1.876 × 10-6 m.
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)