Caption: A conceptual animation of both (3-dimensional physical) space distortions and time distortions (i.e., the spacetime) near a general spherically symmetric mass distribution (e.g., star or black hole outside of the event horizon).
The spacetime geometry is that of the Schwarzschild solution (1916) to general relativity (1915) for a spherically symmetric mass distribution. Karl Schwarzschild (1873--1916) discovered his eponymous solution while serving in the Imperial German Army at the Russian front in 1915: he was soon invalided home to die. The Schwarzschild solution was the first exact analytic solution to general relativity. Albert Einstein (1879--1955) himself only ever found one exact analytic solution and it was NOT a top-level solution. For more information on exact analytic solutions to general relativity, see Relativity file: general_relativity_exact_solutions.html.
Features:
The animation can only show certain aspects of 3-dimensional curved space of the Schwarzschild solution.
Friedmann was the
discoverer of the
Friedmann equation (1922), another
exact
analytic solution
to general relativity
and the key equation of
modern general relativistic cosmology.
For more on Friedmann, see
Astronomer file:
alexander_friedmann.html.