A modified Titius-Bode law for planetary orbits

Details A modified Titius-Bode law for planetary orbits A modified Titius-Bode law for planetary orbits

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ncimc...2..505b&link_type=abstract

Nuovo Cimento C, Serie 1, vol. 2C, Sept.-Oct. 1979, p. 505-510.

Physics

Condensed Matter

Statistical Mechanics

10

Celestial Mechanics, Planetology, Solar Orbits, Solar System, Asteroids, Astronomical Models, Orbit Calculation, Statistical Mechanics

Scientific paper

A modified Titius-Bode law has been derived for planetary orbits in the solar system. Some consequences of this power law are examined: the law introduces two missing planets between Mars and Jupiter (i.e., the asteroid belt) and a missing planet between Saturn and Uranus just where Chiron has been discovered and where a new asteroid belt has been conjectured to exist.

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