| | Orbits in Strongly Curved Spacetime |
 | | Kepler's laws of planetary motion, grounded in Newton's theory of gravity, state that the orbit of a test particle around a massive object is an ellipse with one focus at the centre of the massive object. |
 | | The summit on the left side of the curve is unique to General Relativity--in Newtonian gravitation the curve rises without bound as the radius decreases, approaching infinity at zero. |
 | | That tiny discrepancy in the orbit of Mercury was actually the first evidence for what lay beyond Newtonian gravitation, the first step down a road that would lead to understanding fl holes, gravitational radiation, and the source of inertia, which remains a fertile ground for theoretical and experimental physics almost a century thereafter. |
| www.fourmilab.ch /gravitation/orbits (2354 words) |