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The line with smallest wavelength in the...

The line with smallest wavelength in the Balmer series in the hydrogen spectrum will have the frequency :-

A

`(a)8.22xx10^(14)s^(-1)`

B

(b)`3.29xx10^(15)s^(-1)`

C

`(c)7.22xx10^(16)s^(-1)`

D

(d)`8.05xx10^(13)s^(-1)`

Text Solution

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The correct Answer is:
To find the frequency of the line with the smallest wavelength in the Balmer series of the hydrogen spectrum, we can follow these steps: ### Step 1: Understand the relationship between wavelength and frequency The speed of light (c) is related to wavelength (λ) and frequency (ν) by the equation: \[ c = \lambda \cdot \nu \] From this, we can express frequency as: \[ \nu = \frac{c}{\lambda} \] ### Step 2: Identify the parameters for the Balmer series For the Balmer series in hydrogen, the transition occurs from higher energy levels (n2) to n1 = 2. The smallest wavelength corresponds to the transition from the highest energy level (n2 = ∞) to n1 = 2. ### Step 3: Calculate the wave number (ν̅) The wave number (ν̅) is given by: \[ \nu̅ = \frac{1}{\lambda} = R \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] Where R (Rydberg constant) is approximately \( 1.097 \times 10^7 \, \text{m}^{-1} \). For the smallest wavelength (n2 = ∞): \[ \nu̅ = R \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) \] This simplifies to: \[ \nu̅ = R \left( \frac{1}{4} - 0 \right) = \frac{R}{4} \] ### Step 4: Substitute the value of R Substituting the value of R: \[ \nu̅ = \frac{1.097 \times 10^7}{4} \] Calculating this gives: \[ \nu̅ = 2.7425 \times 10^6 \, \text{m}^{-1} \] ### Step 5: Calculate the frequency (ν) Now, we can find the frequency using the relationship: \[ \nu = \nu̅ \cdot c \] Where \( c = 3 \times 10^8 \, \text{m/s} \): \[ \nu = \left( 2.7425 \times 10^6 \right) \cdot \left( 3 \times 10^8 \right) \] ### Step 6: Perform the calculation Calculating the frequency: \[ \nu = 2.7425 \times 10^6 \times 3 \times 10^8 = 8.2275 \times 10^{14} \, \text{s}^{-1} \] ### Step 7: Final answer The frequency of the line with the smallest wavelength in the Balmer series is approximately: \[ \nu \approx 8.23 \times 10^{14} \, \text{s}^{-1} \]
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