0
so when an electron moves from an excited state to a ground state and photon with a discrete wavelength is emitted. this photon has a specific energy according to the energy between the excited and ground state.
E = (1/nf2 - 1/ni2)A = hv
where is A is a constant, but in this question is unimportant.
h= planks constant
v=frequency (should be a greek symbol)
nf and ni are the electronic states.
now to answer your question the lyman series is when nf is the ground state or nf =1
balmer series is when nf =2
when nf is 1 the value in the quantity above can range from ni from 2 to infinity giving values between 1 and 1/2
for the balmer series ni goes from 3 to infinity and values range between 1/4 and 5/36
these intervals dont overlap therefore the energies dont overlap therefore the lines in the series cant overlap
What else can I help you with?
Spectral lines of the Lyman and Balmer series do not overlap Verify this statement by calculating the longest wavelength associated with the Lyman series and shortest wavelength associated with the B?
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.
What is the name of the third series in the spectrum of hydrogen?
In ascending order of the lower energy state involved in the transition, the first six families of lines in the hydrogen spectrum are: Lyman series Balmer series Paschen series Brackett series Pfund series Humphreys series
How did balmer contribute to atomic theory?
Dalton's atomic postulations stated that:Elements are made of tiny particles called atoms.All atoms of a given element are identical.The atoms of a given element are different from those of any other element; the atoms of different elements can be distinguished from one another by their respective relative weights.Atoms of one element can combine with atoms of other elements to form chemical compounds; a given compound always has the same relative numbers of types of atoms.Atoms cannot be created, divided into smaller particles, nor destroyed in the chemical process; a chemical reaction simply changes the way atoms are grouped together.
If your eyes could see a slightly wider region of the electromagntic spectrum we would see a fifth line in the balmer series emissions spectrum what is the wavelenght associted with the fifth line?
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
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 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.
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 Spectral Class does Medium-strength Balmer lines strong helium lines belong to?
a balmer line is the ghostly remnants of a poltergeist. They float around your house and murder your pet kitten.
Spectral lines of the Lyman and Balmer series do not overlap Verify this statement by calculating the longest wavelength associated with the Lyman series and shortest wavelength associated with the B?
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.
Is Balmer series only present in hydrogen atom?
No, the Balmer series is observed in hydrogen-like atoms, which have one electron orbiting a nucleus. It consists of the spectral lines produced when the electron transitions from higher energy levels to the second energy level. Other atoms with similar electron configurations can also exhibit Balmer-like series in their spectra.
What was the effects of Neils Bohr's contribution to the atomic theory?
That led to know about the size of the atom and the reason of getting five different series of spectral lines in case of hydrogen such Lymann, Balmer, Pashcen, Bracket and Pfund.
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.
What is the name of the third series in the spectrum of hydrogen?
In ascending order of the lower energy state involved in the transition, the first six families of lines in the hydrogen spectrum are: Lyman series Balmer series Paschen series Brackett series Pfund series Humphreys series
What are the wavelengths of the first lines in the Balmer series?
The first lines in the Balmer series of hydrogen correspond to transitions to the n=2 energy level. The wavelengths of these lines are 656.3 nm (Hα), 486.1 nm (Hβ), 434.0 nm (Hγ), and 410.2 nm (Hδ).
The three laws dealing with the creation of various spectra are due to?
The three laws dealing with the creation of various spectra are due to Johann Balmer for Balmer series in the visible region of hydrogen spectrum, and Johann Rydberg who extended the concept for series in other regions of the spectrum. These laws led to the development of the Rydberg formula which accurately describes the spectral lines of hydrogen and other elements.
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.
