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What are the wavelengths of hydrogen?
The hydrogen spectrum consists of several series of spectral lines, each corresponding to a different electron transition. The Lyman series, which corresponds to transitions to the n=1 energy level, has wavelengths in the ultraviolet region. The Balmer series, corresponding to transitions to the n=2 energy level, has wavelengths in the visible region.
What color is the wavelength of light in the Balmer series that results from the transition of an electron to N equals 2?
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.
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 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.
Why do the Balmer lines of hydrogen get closer together?
The Balmer lines of hydrogen get closer together because as electrons move from higher energy levels to lower energy levels, the energy difference between the levels decreases, causing the wavelengths of light emitted to be closer together.
What are the colours in the balmer series?
The Balmer series consists of visible spectral lines emitted by hydrogen atoms when electrons transition from higher to lower energy levels. The colors in the Balmer series include red (656.3 nm), blue-green (486.1 nm), and violet (434.0 nm) wavelengths.
What are the wavelengths of hydrogen?
The hydrogen spectrum consists of several series of spectral lines, each corresponding to a different electron transition. The Lyman series, which corresponds to transitions to the n=1 energy level, has wavelengths in the ultraviolet region. The Balmer series, corresponding to transitions to the n=2 energy level, has wavelengths in the visible region.
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 color is the wavelength of light in the Balmer series that results from the transition of an electron to N equals 2?
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.
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 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.
The Bohr model of the atom was able to explain the Balmer series because?
The Bohr model of the atom was able to explain the Balmer series by proposing that electrons orbit the nucleus in quantized, discrete energy levels. The transition of electrons between these levels corresponds to the emission of light at specific wavelengths, which gives rise to the spectral lines observed in the Balmer series.
Why do the Balmer lines of hydrogen exhibit a phenomenon where they get closer together as you move towards shorter wavelengths?
The Balmer lines of hydrogen exhibit a phenomenon where they get closer together as you move towards shorter wavelengths because of the energy levels of the hydrogen atom. As the electron transitions from higher to lower energy levels, the wavelengths of light emitted become shorter, causing the lines to converge.
Why do the Balmer lines of hydrogen get closer together?
The Balmer lines of hydrogen get closer together because as electrons move from higher energy levels to lower energy levels, the energy difference between the levels decreases, causing the wavelengths of light emitted to be closer together.
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 is the line spectrum of the hydrogen atom?
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.
What has the author Percy Lowe written?
Percy Lowe has written: 'Structure of the Balmer series lines in the spectrum of hydrogen'
