Balmer Rydberg Equation:
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The Balmer Rydberg equation calculates the wavelengths of spectral lines in the Balmer series of the hydrogen atom. It describes the electromagnetic radiation emitted when an electron transitions from a higher energy level to the n=2 level.
The calculator uses the Balmer Rydberg equation:
Where:
Explanation: The equation calculates the inverse wavelength of light emitted when an electron drops from quantum level n to level 2 in a hydrogen atom.
Details: The Balmer series is particularly important because its spectral lines are in the visible range, making them the first atomic spectral lines to be observed and studied in detail.
Tips: Enter the quantum number n (must be an integer greater than 2) and the Rydberg constant (default value is 1.097 × 10⁷ m⁻¹). The calculator will output the wavelength in meters.
Q1: What are typical values for n in the Balmer series?
A: n can be any integer from 3 up, but the most prominent lines are n=3 (H-alpha, red), n=4 (H-beta, blue-green), n=5 (H-gamma, violet), and n=6 (H-delta, ultraviolet).
Q2: Why is the Rydberg constant important?
A: The Rydberg constant is a fundamental physical constant relating to atomic spectra and appears in the equations describing the hydrogen spectrum.
Q3: Can this equation be used for other elements?
A: The simple form shown here applies only to hydrogen. Other elements have modified versions of the Rydberg equation.
Q4: What are the practical applications of this calculation?
A: It's used in spectroscopy, astronomy (to analyze stellar composition), and quantum physics education.
Q5: Why does the equation use 1/4 (1/2²)?
A: The 1/4 represents the lower energy level (n=2) in the Balmer series transitions. Other series (like Lyman) use different denominators.