A gravitational approach to the Titius-Bode law

Details A gravitational approach to the Titius-Bode law A gravitational approach to the Titius-Bode law

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93.1272l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 93, May 1987, p. 1272-1279.

Astronomy and Astrophysics

Astronomy

4

Center Of Mass, Gravitational Effects, Orbital Mechanics, Solar Orbits, Equations Of Motion, Four Body Problem, Kepler Laws, Stellar Motions

Scientific paper

The Titius-Bode law tells us that the distances of the planets
sufficiently far from the Sun roughly follow a geometric progression of
ratio equal to 2. The authors give a gravitational explanation of this
fact taking into account the motion of the solar system around the
center of mass of the galaxy.

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