Give the equation of wavelengths in balmer series of hydrogen atom
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Explanation:
The Rydberg Formula and Balmer's Formula
The λ symbol represents the wavelength, and RH is the Rydberg constant for hydrogen, with RH = 1.0968 × 107 m−1. You can use this formula for any transitions, not just the ones involving the second energy level.
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Give the equation of wavelengths in balmer series of hydrogen atom
- The wavelength of visible radiation in the H spectrum is given by Balmer as n24kn2, with the Balmer series in the visible region being the best-known example. The wavelengths of the visible hydrogen lines can be stated using a straightforward formula, which was discovered by Swiss mathematician Johann Balmer in 1885: the reciprocal wavelength (1/) is equal to a constant (R) times the difference between two terms, 1/4.
- When an electron transitions from a higher level to the energy level with the primary quantum number 2, it produces a series of spectral emission lines known as the Balmer series.
- The Balmer series refers to a group of visible lines in the spectrum of hydrogen atoms. When an electron moves from a high energy level (n=3,4,5,6,...) to the lower energy level n=2, this happens.
- The electromagnetic spectrum's visible portion of light is released by the Balmer series. The longer arrows in the Lyman series necessitate the UV region's higher energy. With shorter arrows, the Paschen and Brackett series requires less IR energy. The visual emission spectrum of hydrogen is shown below.
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