Angular momenta in the solar system. II

Details Angular momenta in the solar system. II Angular momenta in the solar system. II

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984em%26p...31..157q&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 31, Oct. 1984, p. 157-174. Research supported by the Conselho Nacional de Pesqui

Physics

3

Angular Momentum, Orbital Elements, Solar Orbits, Solar System, Celestial Bodies, Planetary Mass, Solar Rotation, Statistical Analysis

Scientific paper

A statistical analysis of the orbital parameters of the meteors, comets, and isolated asteroids outside the asteroid belt indicates that they are associated with discrete levels n(i) in the solar potential well. These levels are multiples of a fundamental unit of action/unit mass of 9.2275 x 10 to the 18th cgs units. The level transitions in comets perturbed by close approaches to Jupiter are analysed, and comparisons with previous results about the spatial orientation of the angular momentum vectors suggest quantizations in all the necessary variables for the description of the angular momenta of these objects. A method for determining the constant H(0) is postulated, and a discussion is conducted concerning the possible physical implications of this in relation with the planets.

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