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The n4-n2 transition of hydrogen is in the cyan, with wavelength of 486.1 nm. blue = als
There are 4 Balmer lines with wavelengths in the visible region. They are red, aqua and two shades of violet. Other Balmer lines are in the ultraviolet. The red line corresponds to the transition from n = 3 to n = 2, the subsequent ones are from the 4, 5 and 6 levels to n = 2.
The wavelength of the hydrogen atom in the 2nd line of the Balmer series is approximately 486 nm. This corresponds to the transition of an electron from the third energy level to the second energy level in the hydrogen atom.
The shortest wavelength radiation in the Balmer series is the transition from the n=3 energy level to the n=2 energy level, which corresponds to the Balmer alpha line at 656.3 nm in the visible spectrum of hydrogen.
The Balmer series is a series of spectral lines in the hydrogen spectrum that corresponds to transitions from energy levels n > 2 to the n=2 level. The longest wavelength in the Balmer series corresponds to the transition from n = ∞ to n = 2, known as the Balmer limit, which is approximately 656.3 nm.
The electron transition from n=5 to n=1 in a hydrogen atom corresponds to the Balmer series, specifically the Balmer-alpha line which is in the visible part of the spectrum.
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The longest wavelength in the Lyman series is the transition to n=2, which corresponds to the Lyman-alpha line at 121.6 nm. The shortest wavelength in the Balmer series is the transition to n=2, which corresponds to the Balmer-α line at 656.3 nm. Since the Lyman-alpha line has a longer wavelength than the Balmer-α line, they do not overlap.
The line spectrum of the hydrogen atom consists of discrete lines at specific wavelengths corresponding to different electron transitions within the atom. These lines are a result of the energy differences between electron orbitals in the atom. Each line represents a specific electron transition, such as the Lyman, Balmer, and Paschen series.
The Balmer series is a section of the hydrogen atomic emission line spectrum. They show the wavelengths of light emitted when electrons transition back to the n = 2 quantum level.
The Balmer series corresponds to the spectral lines produced by hydrogen when electrons transition to the second energy level. The formula to calculate the wavelength for each line in the Balmer series is 1/λ = R(1/2^2 - 1/n^2), where n is the energy level and R is the Rydberg constant. For the fifth line (n=6), the wavelength would be approximately 434 nm.
The Balmer series is a set of spectral lines in the visible region of the electromagnetic spectrum of hydrogen. It consists of four lines in the visible light spectrum resulting from transitions in hydrogen's electron shell to the second energy level. The Balmer series is significant in understanding atomic structure and spectroscopy.