Stars can appear to be brighter at their poles in this phenomenon's namesake darkening. The Eötvös experiment concerned this force, whose balancing point with outward radiation is the Eddington limit. Its namesake waves were reported by Hulse and Taylor, and its namesake constant was first measured using a torsion balance by Cavendish. General relativity has supplanted Newton's model of this force, which treated it as an inverse-square phenomenon. With its namesake acceleration on earth about equal to 9.81 meters per se
Stars can appear to be brighter at their poles in this phenomenon's namesake darkening. The Eötvös experiment concerned this force, whose balancing point with outward radiation is the Eddington limit. Its namesake waves were reported by Hulse and Taylor, and its namesake constant was first measured using a torsion balance by Cavendish. General relativity has supplanted Newton's model of this force, which treated it as an inverse-square phenomenon. With its namesake acceleration on earth about equal to 9.81 meters per second squared, name this weakest fundamen- tal force, which is exclusively attractive and acts between objects with mass.
Stars can appear to be brighter at their poles in this phenomenon's namesake darkening.
{gravity} [or {gravitation}, etc.; accept {gravity brightening} or {gravity darkening}]