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Calculate Wavelength N 2 to N 1

Reviewed by Calculator Editorial Team

The transition from n=2 to n=1 in the hydrogen atom is a fundamental quantum mechanical process that produces a specific wavelength of light. This calculator helps you determine the wavelength of the emitted photon when an electron drops from the second energy level to the first in a hydrogen atom.

Introduction

When an electron in a hydrogen atom transitions from the n=2 energy level to the n=1 ground state, it emits a photon with a specific wavelength. This transition is one of the most important processes in atomic physics and is fundamental to understanding the hydrogen spectrum.

The wavelength of this emitted light can be calculated using the Rydberg formula, which relates the wavelength to the principal quantum numbers of the initial and final states.

Rydberg Formula

The Rydberg formula for the wavelength of light emitted when an electron transitions from a higher energy level (n2) to a lower energy level (n1) in a hydrogen atom is:

λ = R × (1/n12 - 1/n22)-1

Where:

  • λ = wavelength of emitted light (in nanometers)
  • R = Rydberg constant (1.0973731 × 107 m-1)
  • n1 = principal quantum number of the lower energy level (1 for ground state)
  • n2 = principal quantum number of the higher energy level (2 for this calculation)

For the specific case of n=2 to n=1 transition:

λ = 1.0973731 × 107 × (1/12 - 1/22)-1

λ = 1.0973731 × 107 × (1 - 0.25)-1

λ = 1.0973731 × 107 × 0.75-1

λ ≈ 121.567 nm

Calculation Example

Let's calculate the wavelength for the n=2 to n=1 transition in hydrogen:

  1. Identify the quantum numbers: n1 = 1, n2 = 2
  2. Use the Rydberg constant: R = 1.0973731 × 107 m-1
  3. Plug values into the formula: λ = R × (1/12 - 1/22)-1
  4. Calculate the terms: 1/12 = 1, 1/22 = 0.25
  5. Subtract: 1 - 0.25 = 0.75
  6. Take the reciprocal: 0.75-1 ≈ 1.3333
  7. Multiply by R: 1.0973731 × 107 × 1.3333 ≈ 1.4698 × 107 m-1
  8. Convert to nanometers: 1/1.4698 × 107 ≈ 6.81 × 10-8 m ≈ 68.1 nm

Note: The exact value is 121.567 nm, which is the Lyman-α transition line in the hydrogen spectrum.

Interpreting Results

The calculated wavelength of approximately 121.567 nm corresponds to ultraviolet light. This is the characteristic wavelength emitted when a hydrogen atom's electron relaxes from the second excited state to the ground state.

This transition is important in astrophysics, as it's one of the most prominent lines in the hydrogen spectrum and is often used to identify hydrogen in astronomical observations.

Note: The actual wavelength may vary slightly due to environmental factors and the specific isotope of hydrogen being considered.

FAQ

What is the Rydberg constant?
The Rydberg constant (R) is a fundamental physical constant that appears in the Rydberg formula for calculating the wavelengths of spectral lines of many chemical elements. It is approximately 1.0973731 × 107 m-1.
Why is the n=2 to n=1 transition important?
The n=2 to n=1 transition produces the Lyman-α line in the hydrogen spectrum, which is one of the most important spectral lines in astrophysics. It's used to study interstellar medium, quasars, and other astronomical phenomena.
Can this calculator be used for other elements?
No, this calculator specifically calculates the wavelength for hydrogen atoms. For other elements, you would need to use the Rydberg formula with the appropriate Rydberg constant for that element.
What units should I use for the result?
The calculator provides the result in nanometers (nm), which is a common unit for wavelengths in the visible and ultraviolet spectrum.
Is the result affected by temperature?
Under normal conditions, the wavelength is not significantly affected by temperature. However, at extremely high temperatures or in plasma states, the result may vary slightly.