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Electrons in a certain energy level n=n(...

Electrons in a certain energy level `n=n_(1)` can emit 3 spectral lines. When they are in another energy level, `n=n_(2)`, they can emit 6 spectral lines. The orbital speed of the electrons in the two orbits are in the ratio

A

`4 :3 `

B

`3:4`

C

`2:1`

D

`1:2`

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To solve the problem, we need to determine the energy levels \( n_1 \) and \( n_2 \) based on the number of spectral lines emitted and then find the ratio of the orbital speeds of the electrons in these energy levels. ### Step 1: Determine \( n_1 \) The number of spectral lines emitted by electrons in a given energy level \( n \) can be calculated using the formula: \[ \text{Number of spectral lines} = \frac{n(n-1)}{2} \] Given that for \( n = n_1 \), the number of spectral lines is 3, we can set up the equation: \[ \frac{n_1(n_1 - 1)}{2} = 3 \] Multiplying both sides by 2 gives: \[ n_1(n_1 - 1) = 6 \] Now, we can solve for \( n_1 \): \[ n_1^2 - n_1 - 6 = 0 \] Factoring the quadratic equation: \[ (n_1 - 3)(n_1 + 2) = 0 \] This gives us \( n_1 = 3 \) (since \( n \) cannot be negative). ### Step 2: Determine \( n_2 \) For \( n = n_2 \), the number of spectral lines is 6. Using the same formula: \[ \frac{n_2(n_2 - 1)}{2} = 6 \] Multiplying both sides by 2 gives: \[ n_2(n_2 - 1) = 12 \] Now, we can solve for \( n_2 \): \[ n_2^2 - n_2 - 12 = 0 \] Factoring the quadratic equation: \[ (n_2 - 4)(n_2 + 3) = 0 \] This gives us \( n_2 = 4 \) (again, \( n \) cannot be negative). ### Step 3: Find the ratio of orbital speeds The orbital speed \( v \) of electrons in a hydrogen-like atom is given by the formula: \[ v \propto \frac{Z}{n} \] where \( Z \) is the atomic number (for hydrogen, \( Z = 1 \)). The ratio of the speeds in the two orbits is: \[ \frac{v_{n_1}}{v_{n_2}} = \frac{n_2}{n_1} \] Substituting the values we found: \[ \frac{v_{n_1}}{v_{n_2}} = \frac{4}{3} \] ### Final Answer The ratio of the orbital speeds of the electrons in the two orbits is: \[ \frac{v_{n_1}}{v_{n_2}} = \frac{4}{3} \]

To solve the problem, we need to determine the energy levels \( n_1 \) and \( n_2 \) based on the number of spectral lines emitted and then find the ratio of the orbital speeds of the electrons in these energy levels. ### Step 1: Determine \( n_1 \) The number of spectral lines emitted by electrons in a given energy level \( n \) can be calculated using the formula: \[ \text{Number of spectral lines} = \frac{n(n-1)}{2} \] Given that for \( n = n_1 \), the number of spectral lines is 3, we can set up the equation: ...
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CP SINGH-BOHR THEORY-Exercises
  1. Hydrogen (H), deuterium (D), singly ionized helium (He^(+)) and doubly...

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  2. Energy levels A, B, C of a certain atom corresponding to increasing va...

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  3. Electrons in a certain energy level n=n(1) can emit 3 spectral lines. ...

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  4. The figure indicates the enegry level diagram of an atom and the origi...

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  5. The ionisation potential of hydrogen atom is -13.6 eV. An electron in...

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  6. Hydrogen atom in ground state is excited by a monochromatic radiation ...

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  7. A hydrogen sample is prepared in a particular state A photon of energy...

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  8. A hydrogen atom in a state having a binding energy of 0.85 eV makes tr...

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  9. Imagine an atom made of a proton and a hypothetical particle of double...

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  10. In an excited state of hydrogen like atom an electron has total energy...

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  11. Light form a dicharge tube containing hydrogen atoms falls on the surf...

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  12. The electron in the hydrogen atom jumps from excited state (n=3) to it...

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  13. Three photons coming from excited atoms hydrogen sample are picked up ...

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  14. In a laboratory experiment on emission from atomic hydrogen in a disch...

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  15. The de-Broglie wavelength of an electron in the first Bohr orbit is

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  16. Consider an eelctron in the nth orbit of a hydrogen atom in the Bohr m...

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  17. The ratio of the longest and shortest wavelengths of the Lyman series ...

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  18. The ratio of longest wavelength and the shortest wavelength observed i...

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  19. In terms of Rydberg's constant R, the wave number of the first Balman ...

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  20. The wavelength of the first line of the Balmer series of hydrogen atom...

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