Convert Cosmic Velocity - First (v₁) to Running Speed (run) instantly.
About these units
Cosmic Velocity - First (v₁)
The first cosmic velocity is the minimum horizontal speed an object must achieve to enter a stable orbit around a planetary body without additional propulsion. For Earth, this value is about 7.9 km/s. At this speed, an object's forward motion precisely balances with the gravitational pull downward, creating continuous free-fall—the essence of orbital motion. This velocity is foundational in orbital mechanics. Spacecraft reaching Low Earth Orbit (LEO) must achieve at least this horizontal speed, even if their vertical ascent profile varies. Understanding v₁ was essential in the early space age: it represented the threshold between atmospheric flight and true spaceflight, marking human entry into the orbital era.
Running Speed (run)
Human running speeds range widely: Average jogging (2.5–3.3 m/s or 9–12 km/h), Sprint speeds (8–12 m/s or 29–43 km/h). Elite sprinters can exceed 12 m/s, with Usain Bolt's peak reaching approximately 12.4 m/s. Running is biomechanically complex, involving elastic energy return, stride mechanics, ground-reaction forces, and cardiovascular performance. Sports science uses running speed to evaluate training outcomes, optimize gait, prevent injuries, and enhance athletic performance. Running speed provides a window into human physical capability and evolutionary adaptations.