Calculate Wavelength N 2 to N 1
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:
- Identify the quantum numbers: n1 = 1, n2 = 2
- Use the Rydberg constant: R = 1.0973731 × 107 m-1
- Plug values into the formula: λ = R × (1/12 - 1/22)-1
- Calculate the terms: 1/12 = 1, 1/22 = 0.25
- Subtract: 1 - 0.25 = 0.75
- Take the reciprocal: 0.75-1 ≈ 1.3333
- Multiply by R: 1.0973731 × 107 × 1.3333 ≈ 1.4698 × 107 m-1
- 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.