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The Bohr Model of the Atom

The Bohr model of the atom is often called the planetary model. As shown in Figure 1 for a hydrogen atom, the Bohr model envisions the nucleus of the atom occupying a fixed position at the center of an atomic system with the electron revolving around the nucleus in the same way that a planet revolves around the sun.

Figure 1

The Bohr Model of a Hydrogen Atom


Exercise 1 What is the approximate ratio of the mass of a proton to the mass of an electron?

18/1 180/1 1,800/1 18,000/1

Exercise 2 We describe the motion of the planets around the fixed position of the sun. Is the sun's position really fixed?

yes no

Exercise 3 What fact allows us to assume that the position of the nucleus is fixed in a hydrogen atom?

gravity attracts the nucleus more than it does the electron the mass of the electron is much smaller than that of the protonthe nucleus is positively charged the electron is too small to locate


In fact, the planetary model pre-dates Bohr. The model bears his name because of his interpretation of the emission spectrum of hydrogen: If a small amount of hydrogen gas is confined within a glass tube and subjected to a high voltage, it emits light, some of which falls in the visible region of the electromagnetic spectrum. When this light is passed through a prism, it becomes apparent that its pink-violet hue is a composite of four discrete colors-red, green, blue, and purple. Figure 2 illustrates the basic experiment involved in measuring an atomic emission spectrum.

Figure 2

Measuring the Emission Spectrum of Hydrogen

Bohr knew that the emission of light was the way the atoms released the energy they had absorbed when the high voltage was applied. He made a connection between the discrete colors emitted and the discrete energy levels that were available to the electron. He postulated that each color corresponded to the transition of an electron from one energy state to another, lower energy state. He indexed the energy states of the electron with the letter n, the value of n being 1 for the state where the electron had the lowest energy (the ground state), 2 for the next higher energy state, 3 for the third electronic energy state, etc. Bohr's index n became what we now refer to as the principal quantum number.

Figure 3 animates the changes that occur during the measurement of the emission spectrum of hydrogen.

Figure 3

Electronic Excitation in a Sample of Hyrdogen Atoms

Bohr's success in rationalizing the emission spectrum of hydrogen led to the general acceptance of the planetary model of the atom. It has since been shown that this model is overly simplistic. Despite its shortcomings, the simplicity of the Bohr model appeals to organic chemists because it lends itself to a simple pictorial description of molecular structure.

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