The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 86
Síða 96
... velocity . The formula may be looked upon as showing how to calculate the coordinate - velocity from an observed spectral shift when the radial coordinate is known , and clearly there was no justification for a straight acceptance of ...
... velocity . The formula may be looked upon as showing how to calculate the coordinate - velocity from an observed spectral shift when the radial coordinate is known , and clearly there was no justification for a straight acceptance of ...
Síða 143
A History of Modern Cosmology John David North. constant velocity to be subtracted from the apparent nebular velocity before evaluation of the solar motion . ( The name ' K - term ' had already been used in the evaluation of the solar ...
A History of Modern Cosmology John David North. constant velocity to be subtracted from the apparent nebular velocity before evaluation of the solar motion . ( The name ' K - term ' had already been used in the evaluation of the solar ...
Síða 155
... velocity of his signal , is constant and equal to c . The same result is found for the mean return velocity , and if B is an equivalent observer it is easily shown that B arrives at exactly the same results . This quantity the observers ...
... velocity of his signal , is constant and equal to c . The same result is found for the mean return velocity , and if B is an equivalent observer it is easily shown that B arrives at exactly the same results . This quantity the observers ...
Efni
COSMOLOGICAL DIFFICULTIES WITH | 16 |
FIELD THEORIES AND THE WISH TO | 24 |
The Le SageThomson explanation of gravitation | 38 |
Höfundarréttur | |
19 aðrir hlutar ekki sýndir
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The Measure of the Universe: A History of Modern Cosmology John David North Engin sýnishorn í boði - 1965 |
Common terms and phrases
absolute apparent magnitude appear argument assumption astronomical Bondi chapter clusters concept constant coordinates corresponding Cosmological Principle cosmological theories cosmologists covariant creation curvature density derived distance Eddington Einstein energy equivalent Euclidean Euclidean geometry example expanding universe expansion explained fact field equations finite formula function galactic galaxies geodesics geometry given gravitational field homogeneous Hubble Hubble's Hubble's Law hypothesis ibid idea infinite infinity interpretation isotropy Leibniz Lemaître light line-element Mach's Principle mass Math mathematical matter McCrea McVittie mean metric Milne Milne's motion nebulae Newton's Newtonian non-Euclidean geometry objects observer P. G. Tait parallax particles Phys physical possible problem radial reason regarded relation relativistic cosmology result Riemannian scientific seems sense simple Sitter solution space space-time spatial spectral spherical stars steady-state theories supposed tensor theoretical theory of gravitation Theory of Relativity tion Tolman universe velocity Weyl's Principle Whitehead Whitrow