Bohr Atomic Model. A Danish physicist named Neil Bohr in proposed the Bohr atomic model. According to Bohr Atomic model, a small positively charged nucleus is surrounded by revolving negatively charged electrons in fixed orbits. The objections of Rutherford atomic model was contested by Niels Bohr atomic model in Niels Bohr proposed the The value of h is x J-s. In Bohr proposed his quantized shell model of the atom (see Bohr atomic model) In the Bohr model of the atom, electrons travel in defined circular orbits around the nucleus. The orbits are labeled by an integer, the quantum number n. Electrons can jump from one orbit to another by emitting or absorbing energy.


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Bohr model - Wikipedia

Balmer series is found in visible region of spectrum. Pashen series is found in infrared region of spectrum. Brackett series is found in infrared region of spectrum. By limiting the orbiting electrons to a series of circular orbits having discrete radii, Bohr could account for the series bohr s model of atom discrete wavelengths in the emission spectrum of hydrogen.

Light, he proposed, radiated from hydrogen atoms only when an electron made a transition from an outer orbit to one closer to the nucleus.

What Is Bohr's Atomic Model? - Universe Today

These orbits were associated with definite energies, which he referred to as energy shells or energy levels. Influence of the Bohr Model: For starters, it assumed that electrons have both a known radius and orbit, something bohr s model of atom Werner Heisenberg would disprove a decade later with his Uncertainty Principle.

In these cases, where atoms have multiple electrons, the energy levels were not consistent with what Bohr predicted. The Bohr model also could not account for the Zeeman Effecta phenomenon noted by Dutch physicists Pieter Zeeman inwhere spectral lines are split into two or more in the presence of an external, static magnetic field.

Bohr model

The energy quantum is related to the frequency of the light by a new fundamental constant, h. When a body is heated, its radiant energy in a particular frequency range is, according to classical theory, proportional to bohr s model of atom temperature of the body.

With Planck's hypothesis, however, the radiation can occur only in quantum amounts of energy. If the radiant energy is less than the quantum of energy, the amount of light in that frequency range will be reduced.

Planck's formula correctly describes radiation from heated bodies. The energy levels of the orbitals are shown to the right.

Hydrogen Spectrum The movement of electrons between these energy levels produces a spectrum. These wavelengths are at,and nm. The Rydberg formula, below, generalizes the Balmer series for all energy level transitions.

Bohr's Hydrogen Atom

To get the Balmer lines, the Rydberg formula is used with an nf of 2. Because the electrons strongly repel each other, the effective charge description is very approximate; the effective charge Z doesn't usually come out to be an integer.


The shell model was able to qualitatively explain many of the mysterious properties of atoms which became codified in the late 19th century in the periodic table of the elements.

One property was the size of atoms, which could be determined approximately by bohr s model of atom the viscosity of gases and density of pure crystalline solids.

Atoms tend to get smaller toward the right in the periodic table, and become much larger at the next line of the table. Atoms to the right of the table tend to gain electrons, while atoms bohr s model of atom the left tend to lose them.