Which electronic transition in a hydrogen atom, starting from the orbit n=7, will produce infrared light of wavelength 2170 nm?
`(Given: R_(H)=1.09677xx10^(7)M^(-1))`
Which electronic transition in a hydrogen atom, starting from the orbit n=7, will produce infrared light of wavelength 2170 nm?
`(Given: R_(H)=1.09677xx10^(7)M^(-1))`
`(Given: R_(H)=1.09677xx10^(7)M^(-1))`
A
`n=7 " to " n=4`
B
from `n=2` to `n=4`
C
from `n=5` to `n=1`
D
from `n=3` to `n=5`
Text Solution
AI Generated Solution
The correct Answer is:
To determine which electronic transition in a hydrogen atom starting from the orbit \( n = 7 \) will produce infrared light of wavelength \( 2170 \, \text{nm} \), we can use the Rydberg formula for hydrogen:
\[
\frac{1}{\lambda} = R_H \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right)
\]
where:
- \( \lambda \) is the wavelength of the emitted light,
- \( R_H \) is the Rydberg constant for hydrogen, \( R_H = 1.09677 \times 10^7 \, \text{m}^{-1} \),
- \( n_1 \) is the lower energy level,
- \( n_2 \) is the higher energy level (in this case, \( n_2 = 7 \)).
### Step-by-step Solution:
1. **Convert Wavelength to Meters**:
The given wavelength is \( 2170 \, \text{nm} \). We need to convert this to meters:
\[
\lambda = 2170 \, \text{nm} = 2170 \times 10^{-9} \, \text{m}
\]
2. **Substitute Values into the Rydberg Formula**:
We know \( n_2 = 7 \) and \( R_H = 1.09677 \times 10^7 \, \text{m}^{-1} \). Substitute these values into the Rydberg formula:
\[
\frac{1}{2170 \times 10^{-9}} = 1.09677 \times 10^7 \left( \frac{1}{n_1^2} - \frac{1}{7^2} \right)
\]
3. **Calculate \( \frac{1}{\lambda} \)**:
Calculate \( \frac{1}{2170 \times 10^{-9}} \):
\[
\frac{1}{2170 \times 10^{-9}} \approx 4.608 \times 10^6 \, \text{m}^{-1}
\]
4. **Set Up the Equation**:
Now we can set up the equation:
\[
4.608 \times 10^6 = 1.09677 \times 10^7 \left( \frac{1}{n_1^2} - \frac{1}{49} \right)
\]
5. **Isolate \( \frac{1}{n_1^2} \)**:
Rearranging gives:
\[
\frac{1}{n_1^2} - \frac{1}{49} = \frac{4.608 \times 10^6}{1.09677 \times 10^7}
\]
Calculate the right side:
\[
\frac{4.608 \times 10^6}{1.09677 \times 10^7} \approx 0.420
\]
Therefore:
\[
\frac{1}{n_1^2} = 0.420 + \frac{1}{49}
\]
6. **Calculate \( \frac{1}{49} \)**:
\[
\frac{1}{49} \approx 0.0204
\]
So:
\[
\frac{1}{n_1^2} = 0.420 + 0.0204 \approx 0.4404
\]
7. **Find \( n_1^2 \)**:
Taking the reciprocal:
\[
n_1^2 \approx \frac{1}{0.4404} \approx 2.27
\]
8. **Calculate \( n_1 \)**:
Taking the square root:
\[
n_1 \approx \sqrt{2.27} \approx 1.5
\]
Since \( n_1 \) must be an integer, we round it to \( n_1 = 4 \).
9. **Conclusion**:
The electronic transition occurs from \( n_2 = 7 \) to \( n_1 = 4 \).
### Final Answer:
The electronic transition in a hydrogen atom that produces infrared light of wavelength \( 2170 \, \text{nm} \) is from \( n = 7 \) to \( n = 4 \).
Topper's Solved these Questions
Similar Questions
Explore conceptually related problems
An electron in C^(5+) ion during the transition from n = 3 to n = 1 emits light of wavelength
The shortest wavelength in the balmer series is (R=1.097xx10^7m^-1)
Find the quantum of the excited state of electrons in He^(+) ion which on transition to first excited state emit photons of wavelengths 108.5 nm . (R_(H)=1.09678xx10^(7) m^(-1))
What is the energy difference and the frequency of light emitted when the electron in a hydrogen atom undergoes transition from the energy level n = 4 to the energy n = 3 given that the value of Rydberg constant is 1.0974 xx 10^(7)m^(-1) ?
If an electron transits from n = 7 to n = 1 in a hydrogen atom then the maximum number of spectral lines that can form will be?
calculate the longest wavelength in Balmer series and the series limit . (Given R=1.097xx10^(7)m^(-1) )
The wavelength of the radiation emitted , when in a hydrogen atom electron falls from infinity to stationary state 1 , would be : (Rydberg constant = 1.097 xx 10^(7) m^(-1) )
In what region of the electromagnetic spectrum would you look the spectral line resulting from the electronic transition from the tenth to the fifth electronic level in the hydrogen atoms ? (R_(H)=1.10xx10^(5) cm^(-1))
the wavelength limit present in the pfund series is (R=1. 097xx10^7m^-1)
If an electron in hydrogen atom jumps from third orbit to second orbit, the Wavelength of the emitted radiation is given by (c is speed of light )