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![]() Photo courtesy NASA White light passing through a prism. |
![]() Photo courtesy NASA Continuous spectrum of white light. |
Now, when you pass sunlight through a prism, you get a continuous spectrum of colors like a rainbow. However, when light from these various sources was passed through a prism, they found a dark background with discrete lines.
![]() Photo courtesy NASA Hydrogen spectrum |
![]() Photo courtesy NASA Helium spectrum |
Each element had a unique spectrum and the wavelength of each line within a spectrum had a specific energy (see How Light Works for details on the relationship between wavelength and energy).
In 1913, a Danish physicist named Niels Bohr put Rutherford's findings together with the observed spectra to come up with a new model of the atom in a real leap of intuition. Bohr suggested that the electrons orbiting an atom could only exist at certain energy levels (i.e., distances) from the nucleus, not at continuous levels as might be expected from Rutherford's model. When atoms in the gas tubes absorbed the energy from the electric current, the electrons became excited and jumped from low energy levels (close to the nucleus) to high energy levels (farther out from the nucleus). The excited electrons would fall back to their original levels and emit energy as light. Because there were specific differences between the energy levels, only specific wavelengths of light were seen in the spectrum (i.e., lines).
![]() Bohr models of various atoms. |
The major advantage of the Bohr model was that it worked. It explained several things:
Bohr's model was the predominant model until new discoveries in quantum mechanics were made.
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