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Calculate The Wavelength of Light From N 2 N 1

Reviewed by Calculator Editorial Team

Calculating the wavelength of light emitted or absorbed during electronic transitions in atoms is fundamental to atomic physics and spectroscopy. This guide explains how to use the Rydberg formula to determine the wavelength of light when an electron transitions from quantum state n2 to n1.

Introduction

The wavelength of light emitted or absorbed during electronic transitions in atoms can be calculated using the Rydberg formula. This formula is named after the Swedish physicist Johannes Rydberg, who developed it in 1888. The Rydberg formula provides a relationship between the wavelength of light and the quantum numbers of the initial and final states of the electron.

Understanding how to calculate the wavelength of light from n2 to n1 is essential for various applications in physics, chemistry, and engineering. It helps in analyzing atomic spectra, designing lasers, and understanding the behavior of electrons in different energy levels.

Rydberg Formula

The Rydberg formula for calculating the wavelength of light emitted or absorbed during a transition from quantum state n2 to n1 is given by:

λ = R × (1/n12 - 1/n22)-1

Where:

  • λ is the wavelength of light in nanometers (nm)
  • R is the Rydberg constant (1.0973731568508 × 10-2 nm-1)
  • n1 is the principal quantum number of the initial state
  • n2 is the principal quantum number of the final state

The Rydberg formula is derived from the Bohr model of the atom, which assumes that electrons orbit the nucleus in quantized energy levels. The formula shows that the wavelength of light emitted or absorbed during a transition depends on the difference in energy between the initial and final states of the electron.

Online Calculator

Use the calculator below to calculate the wavelength of light emitted or absorbed during a transition from quantum state n2 to n1. Simply enter the values for n1 and n2, then click the "Calculate" button to get the result.

Worked Examples

Let's look at a few examples to understand how to use the Rydberg formula to calculate the wavelength of light emitted or absorbed during electronic transitions in atoms.

Example 1: Transition from n2 = 3 to n1 = 2

Using the Rydberg formula:

λ = 1.0973731568508 × 10-2 × (1/22 - 1/32)-1

λ = 1.0973731568508 × 10-2 × (0.25 - 0.1111) × 102

λ = 1.0973731568508 × 10-2 × 0.1389 × 102

λ = 1.0973731568508 × 13.89

λ ≈ 152.2 nm

The wavelength of light emitted or absorbed during a transition from n2 = 3 to n1 = 2 is approximately 152.2 nm.

Example 2: Transition from n2 = 4 to n1 = 2

Using the Rydberg formula:

λ = 1.0973731568508 × 10-2 × (1/22 - 1/42)-1

λ = 1.0973731568508 × 10-2 × (0.25 - 0.0625) × 102

λ = 1.0973731568508 × 10-2 × 0.1875 × 102

λ = 1.0973731568508 × 18.75

λ ≈ 204.5 nm

The wavelength of light emitted or absorbed during a transition from n2 = 4 to n1 = 2 is approximately 204.5 nm.

Frequently Asked Questions

What is the Rydberg formula used for?
The Rydberg formula is used to calculate the wavelength of light emitted or absorbed during electronic transitions in atoms. It provides a relationship between the wavelength of light and the quantum numbers of the initial and final states of the electron.
How do I use the Rydberg formula to calculate the wavelength of light?
To use the Rydberg formula, you need to know the principal quantum numbers of the initial and final states of the electron. Plug these values into the formula along with the Rydberg constant, and then solve for the wavelength of light.
What are the units for the Rydberg constant?
The Rydberg constant is typically given in units of nanometers to the power of -1 (nm-1). The value of the Rydberg constant is approximately 1.0973731568508 × 10-2 nm-1.
Can the Rydberg formula be used for any type of electronic transition?
The Rydberg formula is specifically designed for electronic transitions in hydrogen-like atoms, where the electron moves between quantized energy levels. It may not be applicable to more complex systems or different types of transitions.