On the relationship between the total mass of a celestial body and the averaged mass of its constituent particles

Details On the relationship between the total mass of a celestial body and the averaged mass of its constituent particles On the relationship between the total mass of a celestial body and the averaged mass of its constituent particles

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phla...84..223f&link_type=abstract

Physics Letters A, Volume 84, Issue 4, p. 223-225.

Physics

2

Scientific paper

In the framework of the bifurcational theory of the formation of
celestial bodies (galaxies, stars, planets and their satellites) the
relationship between the total mass of a body and the averaged mass of
its constituent particles, responsible for the hydrodynamical
equilibrium at the moment of separation of a body, is derived.

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