Launching an object at escape velocity from Earth's surface leads to complex calculations for the time taken to reach a specific height. While near the surface, gravity can be treated as constant, escape velocity requires consideration of gravitational force diminishing with distance, described by the equation F = -GMm/r^2. This necessitates using quadrature and integrating the resulting expressions, which relate kinetic and potential energy. The integration results in an elliptic integral, known to be non-integrable in elementary terms but tabulated for practical use. Ultimately, starting at escape velocity simplifies the integral, allowing for easier computation of the time to reach the desired height.