Titius–Bode law | Wikipedia audio article
Channel: wikipedia tts
Date: 17/06/2019

This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Titius%E2%80%93Bode_law


00:00:39 1 Formulation
00:03:18 2 Origin and history
00:10:13 3 A potentially earlier explanation
00:11:21 4 Data
00:11:31 5 Theoretical explanations
00:12:23 5.1 Lunar systems and other planetary systems
00:12:37 6 See also
00:12:50 7 Footnotes
00:14:46 8 References
00:16:26 9 Further reading
00:17:37 0.0142 e 0.9975 n, and controversially predicts for n
00:20:12 See also



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SUMMARY
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The Titius–Bode law (sometimes termed just Bode's law) is a hypothesis that the bodies in some orbital systems, including the Sun's, orbit at semi-major axes in a function of planetary sequence. The formula suggests that, extending outward, each planet would be approximately twice as far from the Sun as the one before. The hypothesis correctly anticipated the orbits of Ceres (in the asteroid belt) and Uranus, but failed as a predictor of Neptune's orbit and was eventually superseded as a theory of Solar System formation. It is named for Johann Daniel Titius and Johann Elert Bode.