请输入您要查询的字词:

 

单词 Titius–Bode law
释义
Titius–Bode law

Astronomy
  • See bode’s law.


Geology and Earth Sciences
  • An empirical arithmetical relationship between the distances of the planets from the Sun. If the Sun–Earth distance is taken as 10, then the distances of Mercury, Venus, Earth, Mars, Jupiter, and Saturn are approximately satisfied by the sequence: 4, 4 + 3, 4 + 6, 4 + 12, 4 + 48, and 4 + 96. The more accurate version of the ‘law’ is given by the function rn = ABn, where rn is the distance of the nth planet, A is a constant, and B = 1.73. This version is due to Mary Blagg (1858–1944). It is not clear that the ‘law’ has any fundamental significance, but may be merely a consequence of gravitational and tidal evolution following planetary and satellite formation. The asteroid belt occurs about 4 + 24, corresponding to the former ‘missing planet’ in the sequence, that was believed to exist for many years. Uranus, discovered in 1781, occurs close to the next term, 4 + 192, but the position of Neptune does not fit the ‘law’. The regular satellites of the giant planets fit modifications of the ‘law’. The ‘law’ was discovered in 1766 by J. D. Titius (1729–96) and was popularized by J. E. Bode (1747–1826).


随便看

 

科学参考收录了60776条科技类词条,基本涵盖了常见科技类参考文献及英语词汇的翻译,是科学学习和研究的有利工具。

 

Copyright © 2000-2023 Sciref.net All Rights Reserved
京ICP备2021023879号 更新时间:2024/6/30 18:48:13