(also Titius-Bode law, Titius-Bode rule), an empirical rule (improperly called a law) that states the relation between the distances of the planets from the sun. The rule was proposed by J. D. Titius in 1766 and became well known owing to works by J. E. Bode published in 1772.
Bode’s law gives the distances of Mercury, Venus, the earth, Mars, the central part of the asteroid belt, Jupiter, Saturn, Uranus, and Pluto (Neptune deviates from the relation) from the sun in astronomical units. To obtain the distances, the number 4 is added to each number in the sequence 0, 3, 6,12, 24, 48, 96,192, 384, which forms, starting with 3, a geometric progression. If the resulting sums are then divided by 10, we obtain the new sequence of numbers 0.4, 0.7, 1.0, 1.6, 2.8, 5.2, 10.0, 19.6, and 38.8, which gives the distances of the above-mentioned bodies of the solar system from the sun in astronomical units with an accuracy of about 3 percent. There is no satisfactory theoretical explanation of this empirical relation.