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Since Mars' period of revolution around the sun is 1.88 earth years, and Jupiter's is 11.86 earth years, and since a body's period of orbital revution depends only on its distance from the sun, each body whose orbit lies predominantly between the orbits of Mars and Jupiter has an orbital period between 1.88 and 11.86 earth years.

The asteroid belt is not a "narrow" orbital ring, but a fairly wide orbital pathway in which almost countless rocky bodies orbit the sun. Some of the asteroids are a bit closer to the sun than others, and the periods of the solar orbits of the closer asteroids are a bit shorter than the paths of their neighbors farther out.

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