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 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.
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 Balmer series for hydrogen consists of four spectral lines in the visible region. If there were a fifth line, its wavelength could be calculated using the formula 1/λ = RH(1/4^2 - 1/n^2), where RH is the Rydberg constant and n is the energy level. Plugging in the values, the fifth line wavelength would be smaller than the existing lines in the series.
The ratio of the wavelengths of the last line in the Balmer series to the last line in the Lyman series is 1:5. The Balmer series is associated with transitions to the n=2 energy level, while the Lyman series is associated with transitions to the n=1 energy level in the hydrogen atom.
To find the wavelength associated with the fifth line in the Balmer series, we would use the formula: ( \lambda = \frac{{n^2}}{{n^2 - 4}} \times 656.3 ) nm, where n is the principal quantum number. Substituting n = 6, we get ( \lambda = \frac{{6^2}}{{6^2 - 4}} \times 656.3 = 410.3 ) nm.
5:9 ,i am not sure (;
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 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 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 light in the Balmer series resulting from the transition of an electron from n=3 to n=2 corresponds to a color in the visible spectrum. Specifically, this transition emits light at a wavelength of approximately 656 nanometers, which falls within the red part of the spectrum. This transition is often referred to as the H-alpha line.
Well, the different series represent different electronic transitions. But there is an important equation, the Rydberg formula which describes all of them.. I think you've learned of it since you mention the n values. This lead to the Bohr model of the hydrogen atom, which explained _why_ you had these levels.Or, almost. See, it turned out that those lines were not actually single lines, but several lines very close together.. And so they had to add more variables to describe how these levels-within-levels fit together.. and the answer to that eventually came from quantum mechanics.
The Balmer series for hydrogen consists of four spectral lines in the visible region. If there were a fifth line, its wavelength could be calculated using the formula 1/λ = RH(1/4^2 - 1/n^2), where RH is the Rydberg constant and n is the energy level. Plugging in the values, the fifth line wavelength would be smaller than the existing lines in the series.
The Lyman series corresponds to electronic transitions in hydrogen where the electron falls to the n=1 energy level. The maximum wavelength occurs when the transition is from n=2 (the first level above n=1), yielding a wavelength of approximately 121.6 nm. The minimum wavelength occurs when the transition is from n approaching infinity, resulting in a wavelength of 0.1 nm (or less). Therefore, the ratio of maximum to minimum wavelength for the Lyman series is about 1216:0.1 or 12160:1.
I believe it to be 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.
Use the rydberg equation 1/wavelength = 109677[ 1/n one square - 1/n two square ] 109677 is in cm inverse for balmer series n one = 2 and for the fifth line n two = 7 putting them in the equation we get = 397 nm lies in the violet region of light