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What transition in the hydrogen spectrum would have the same wavelenght as the balmer transition n4 to n2 of he spectrum?
The Balmer transition from ( n=4 ) to ( n=2 ) in the hydrogen spectrum corresponds to a wavelength of approximately 486 nm. The transition in the hydrogen spectrum that would have the same wavelength is the transition from ( n=5 ) to ( n=3 ), which also produces a spectral line at around the same wavelength. Both transitions can be calculated using the Rydberg formula for hydrogen spectral lines.
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Who created the hydrogen line emission spectrum?
The hydrogen line emission spectrum was discovered by physicists Johann Balmer, Johannes Rydberg, and Niels Bohr. They observed that hydrogen gas emitted specific wavelengths of light, which formed a distinct spectrum now known as the Balmer series.
Why it is not possible to observe the n7 to n2 transition in the Balmer Series?
The Balmer Series describes the transitions of electrons in a hydrogen atom from higher energy levels (n ≥ 3) down to the n = 2 level, resulting in visible light emissions. The n = 7 to n = 2 transition falls within the ultraviolet range, which is not part of the visible spectrum typically associated with the Balmer Series. Consequently, while such transitions can occur, they cannot be observed as part of the Balmer Series since they emit wavelengths that are outside the visible range. Thus, the n = 7 to n = 2 transition is not considered part of the series.
What are the absorption lines in the infrared portion of the spectrum of a star that are produced by hyrdrogen are from?
The absorption lines in the infrared portion of the spectrum of a star produced by hydrogen are primarily the Paschen series. These lines are transitions of electrons in hydrogen atoms from higher energy levels to the third energy level (n=3). Typical Paschen series lines in the infrared include Paschen-alpha at 1.875 μm and Paschen-beta at 1.282 μm.
What color is the wavelength of light in the balmer series that results from the transition of an electron from n4 to n2?
The n4-n2 transition of hydrogen is in the cyan, with wavelength of 486.1 nm. blue = als
Which one of the following series of lines in the hydrogen spectrum arises from transitions down to n2?
The series of lines in the hydrogen spectrum that arises from transitions down to n=2 is known as the Balmer series. This series includes visible light emissions when electrons fall from higher energy levels (n≥3) to the n=2 level. The Balmer lines are characterized by wavelengths that fall within the visible range, producing colors such as red, green, and blue in the spectrum.
What is the Balmer 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.
What is the shortest wavelength radiation in balmer series?
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.
To which series would the emitted light belong if an electron in a hydrogen atom underwent a transition from level n 5 to level n 1?
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.
What is the balmer spectrum?
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.
What is the maximum wavelength of balmer series?
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.
What is the name of the visible series in the hydrogen spectrum?
I believe it to be the Balmer Series.
What color is the wavelength of light in the Balmer series that results from the transition of an electron from n 4 to n 2?
The transition of an electron from n=4 to n=2 in the Balmer series produces light with a wavelength of approximately 486 nm, which falls within the blue-green region of the visible spectrum. This transition corresponds to the H-beta line, one of the prominent spectral lines in the Balmer series for hydrogen.
Which spectrum of hydrogen consists of the Lyman Balmer and Paschen series?
The Lyman series consists of transitions to the n=1 state, the Balmer series to the n=2 state, and the Paschen series to the n=3 state in the hydrogen atom. Each series represents a specific range of wavelengths or frequencies of electromagnetic radiation emitted by hydrogen when electrons transition between these energy levels.
Who created the hydrogen line emission spectrum?
The hydrogen line emission spectrum was discovered by physicists Johann Balmer, Johannes Rydberg, and Niels Bohr. They observed that hydrogen gas emitted specific wavelengths of light, which formed a distinct spectrum now known as the Balmer series.
In hydrogen spectrumwhat is the ratio of first line of Lyman series to the first line of balmer series?
The ratio of the first line of the Lyman series to the first line of the Balmer series in the hydrogen spectrum is 1:5.
What has the author Percy Lowe written?
Percy Lowe has written: 'Structure of the Balmer series lines in the spectrum of hydrogen'
Why it is not possible to observe the n7 to n2 transition in the Balmer Series?
The Balmer Series describes the transitions of electrons in a hydrogen atom from higher energy levels (n ≥ 3) down to the n = 2 level, resulting in visible light emissions. The n = 7 to n = 2 transition falls within the ultraviolet range, which is not part of the visible spectrum typically associated with the Balmer Series. Consequently, while such transitions can occur, they cannot be observed as part of the Balmer Series since they emit wavelengths that are outside the visible range. Thus, the n = 7 to n = 2 transition is not considered part of the series.
