Linked from
The 20 pages that link to Vis-viva equation, each with the reason it gives.
Orbital periodRelated: It explains how orbital speed varies during a period.
Escape velocityRelated: Its zero-binding-energy limit gives the local escape speed.
Semimajor axisRelated: The equation shows how semimajor axis sets orbital speed at a given distance.
PeriapsisRelated: It gives the body's speed when its distance equals periapsis distance.
Gravitational parameterRelated: It uses μ to calculate speed at any point along a two-body orbit.
Orbital maneuverRelated: It connects a burn's velocity change with the resulting orbital energy.
Planetary orbitRelated: It calculates how a planet speeds up near its star and slows farther away.
Kepler orbitRelated: It gives the speed at any point along a Kepler orbit.