Taking the wavelength of first Balmer line in hydrogen spectrum (n = 3 to n = 2) as 660 nm, the wavelength of the `2^(nd)` Balmer line (n = 4 to n = 2) will be :
Taking the wavelength of first Balmer line in hydrogen spectrum (n = 3 to n = 2) as 660 nm, the wavelength of the `2^(nd)` Balmer line (n = 4 to n = 2) will be :
A
`889.2 nm`
B
`488.9 nm`
C
`642.7 nm`
D
`388.9 nm`
Text Solution
AI Generated Solution
The correct Answer is:
To find the wavelength of the second Balmer line (from n = 4 to n = 2) given the wavelength of the first Balmer line (from n = 3 to n = 2) as 660 nm, we can use the Rydberg formula for hydrogen:
### Step-by-Step Solution:
1. **Understand the Rydberg Formula**: The Rydberg formula for the wavelength of light emitted during electron transitions in hydrogen is given by:
\[
\frac{1}{\lambda} = R \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right)
\]
where \( R \) is the Rydberg constant, \( n_f \) is the final energy level, and \( n_i \) is the initial energy level.
2. **Calculate for the First Balmer Line**: For the first Balmer line (n = 3 to n = 2):
- Here, \( n_f = 2 \) and \( n_i = 3 \).
- The wavelength \( \lambda_1 \) is given as 660 nm.
- Plugging into the formula:
\[
\frac{1}{660} = R \left( \frac{1}{2^2} - \frac{1}{3^2} \right)
\]
- Calculating the right-hand side:
\[
\frac{1}{2^2} = \frac{1}{4}, \quad \frac{1}{3^2} = \frac{1}{9}
\]
- Therefore,
\[
\frac{1}{4} - \frac{1}{9} = \frac{9 - 4}{36} = \frac{5}{36}
\]
- Thus, we have:
\[
\frac{1}{660} = R \cdot \frac{5}{36}
\]
3. **Calculate for the Second Balmer Line**: For the second Balmer line (n = 4 to n = 2):
- Here, \( n_f = 2 \) and \( n_i = 4 \).
- Using the Rydberg formula again:
\[
\frac{1}{\lambda_2} = R \left( \frac{1}{2^2} - \frac{1}{4^2} \right)
\]
- Calculating the right-hand side:
\[
\frac{1}{2^2} = \frac{1}{4}, \quad \frac{1}{4^2} = \frac{1}{16}
\]
- Therefore,
\[
\frac{1}{4} - \frac{1}{16} = \frac{4 - 1}{16} = \frac{3}{16}
\]
- Thus, we have:
\[
\frac{1}{\lambda_2} = R \cdot \frac{3}{16}
\]
4. **Relating the Two Equations**: Now we have two equations:
\[
\frac{1}{660} = R \cdot \frac{5}{36} \quad \text{(1)}
\]
\[
\frac{1}{\lambda_2} = R \cdot \frac{3}{16} \quad \text{(2)}
\]
- From (1), we can express \( R \):
\[
R = \frac{1}{660} \cdot \frac{36}{5}
\]
- Substitute \( R \) into (2):
\[
\frac{1}{\lambda_2} = \left( \frac{1}{660} \cdot \frac{36}{5} \right) \cdot \frac{3}{16}
\]
5. **Calculate \( \lambda_2 \)**:
- Simplifying the right-hand side:
\[
\frac{1}{\lambda_2} = \frac{36 \cdot 3}{5 \cdot 16 \cdot 660}
\]
- Calculate \( \lambda_2 \):
\[
\lambda_2 = \frac{5 \cdot 16 \cdot 660}{36 \cdot 3}
\]
- Performing the calculations:
\[
\lambda_2 = \frac{5 \cdot 16 \cdot 660}{108} = \frac{52800}{108} \approx 489.44 \text{ nm}
\]
### Final Answer:
The wavelength of the second Balmer line (n = 4 to n = 2) is approximately **489.44 nm**.
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