The Primeval Atom: An Essay on Cosmogony

angular antinomy antipodal points astronomical atomic nucleus billion Buffon clusters of nebulae collisions comet condensations considered coordinates cosmic rays cosmic repulsion cosmogonic cosmological constant cubic centimeter density of matter disintegration distance distributed Earth Einstein elliptic geometry elliptic plane elliptical nebulae elliptical space equal equilibrium evolution exist expansion of space extra-galactic nebulae fact finite force formation Friedmann's equation galaxy gaseous clouds geometry Georges Lemaître giant stars gram per cubic gravitation homogeneity hypothesis idea imagination infinite initial Kant Laplace light light-years manner mass metric tensor mogonic motion natural Nevertheless number of stars observed obtain parsecs particles photons physical possible present pressure primeval atom proper velocity properties proportional R₁ radiation radius of space region represented result rotation space-time spherical symmetry stellar stellar evolution straight line surface tensor test sphere theory of relativity tion tour of space universal attraction uranium volume