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Johann Elert Bode (German:; 19 January 1747 – 23 November 1826) was a German astronomer known for his reformulation and popularisation of the Titius–Bode law. Bode determined the orbit of Uranus and suggested the planet's name.
- German
- Titius–Bode law
Johann Elert Bode (born Jan. 19, 1747, Hamburg [Germany]—died Nov. 23, 1826, Berlin) was a German astronomer best known for his popularization of Bode’s law, or the Titius-Bode rule, an empirical mathematical expression for the relative mean distances between the Sun and its planets.
- The Editors of Encyclopaedia Britannica
Jun 11, 2018 · views 2,066,400 updated May 08 2018. Bode, Johann Elert (1747–1826) A German astronomer who popularized the theory, known later as Bode's law, that there is a simple arithmetical relationship between the distances from the Sun to the planets of the solar system.
Johann Elert Bode. 1749-1826. German Astronomer and Mathematician. German mathematician and astronomer Johann Elert Bode was seemingly born to teach the world about the wonders of astronomy. The child of well-educated parents, Bode early on developed a passion for astronomy and higher mathematics, and only slightly later began publishing ...
Whereas the Titius–Bode law predicts Saturn, Uranus, Neptune, and Pluto at about 10, 20, 39, and 77 AU, the actual values are closer to 10, 19, 30, 40 AU. Origin and history Johann Daniel Titius (1729–1796) Johann Elert Bode (1747–1826) The first mention of a series approximating Bode's law is found in a textbook by D. Gregory (1715):
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Overview. Johann Elert Bode. (1747—1826) Quick Reference. (1747–1826) A German astronomer who popularized the theory, known later as Bode's law, that there is a simple arithmetical relationship between the distances from the Sun to the planets of the solar system.
Nov 23, 2022 · On November 23, 1826, German astronomer Johann Elert Bode passed away. Bode is best known for his popularization of the Titius-Bode ‘s law, a hypothesis that the bodies in some orbital systems, including the Sun ‘s, orbit at semi-major axes in a function of planetary sequence.
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