Linked from

The 30 pages that link to Escape velocity, each with the reason it gives.

• Orbital periodCompared with: An unbound trajectory has no repeating orbit and therefore no orbital period.

• Terminal velocityCompared with: It is a threshold speed for escape, not a steady speed set by fluid forces.

• Vis-viva equationCompared with: It is the zero-energy boundary case of the vis-viva relation.

• Orbital decayCompared with: Orbital decay lowers orbital energy toward capture or impact, opposite the energy increase required for escape.

• Specific orbital energyCompared with: At a given distance, it marks the speed at which specific orbital energy reaches zero.

• OrbitCompared with: At the boundary between bound and unbound motion, an object no longer returns on a closed orbit.

• Circular orbitCompared with: Comparing it with circular-orbit speed clarifies the energy needed to leave a bound path.

• Orbital energyCompared with: At the escape threshold, orbital energy changes from negative to zero.

• Orbital spaceflightCompared with: Reaching orbit requires less speed than escaping Earth, though both depend on gravity and motion.

• Equations for a falling bodyCompared with: It concerns gravity over large distances, unlike the near-surface constant-acceleration approximation.

• Potential wellCompared with: It expresses the classical threshold separating a trapped trajectory from escape.