#:In Einstein's equation, <math>T_{\mu\nu}\,</math> is the "stress-energy tensor", and <math>8 \pi T_{\mu\nu}\,</math> gives the density of the Sun, taking the place of <math>\frac{M}{r^2}\,</math>. <math>G_{\mu\nu}\,</math> is the "Einstein curvature tensor", and says how spacetime curves to create an apparent gravitational acceleration. | #:In Einstein's equation, <math>T_{\mu\nu}\,</math> is the "stress-energy tensor", and <math>8 \pi T_{\mu\nu}\,</math> gives the density of the Sun, taking the place of <math>\frac{M}{r^2}\,</math>. <math>G_{\mu\nu}\,</math> is the "Einstein curvature tensor", and says how spacetime curves to create an apparent gravitational acceleration. |