Sprinting battery pack
A 70 kg sprinter at 10 m/s carries 3,500 J of kinetic energy—roughly the same as a fully charged phone battery. Blink and it becomes heat in the track.
Tip: Press Ctrl/Cmd + Enter to calculate. The URL updates so you can bookmark or share your inputs.
This calculator helps you explore one of the most useful ideas in physics: energy can change form while the total stays the same. It lets you find kinetic energy (energy of motion) and gravitational potential energy (energy stored by height), then compare them to see how an object speeds up, slows down, or rises and falls. Whether you are studying a rolling ball, a thrown object, or a moving vehicle, the tool makes the math quick and clear.
In simple terms, kinetic energy depends on mass and speed: KE = ½ m v². Double the speed and the kinetic energy grows by a factor of four. Gravitational potential energy depends on mass, gravity, and height: PE = m g h. The height is measured relative to any reference level you choose. The sum, E = KE + PE, is called mechanical energy. If air resistance and friction are small, that total stays nearly constant, which is the idea behind the conservation of mechanical energy.
To use the calculator, enter the object’s mass, its speed, the height, and the local value of gravity. The tool will compute kinetic energy, potential energy, and the total. If you are working a conservation problem, enter the known values and let the calculator show how energy converts between forms. For example, an object dropped from rest at height h₀ has v = √(2 g (h₀ − h)) when it falls to height h. A launch straight up with speed v₀ reaches a maximum height hmax = v₀²/(2 g) + h₀ (ignoring drag).
Step by step: choose a reference height, then enter mass in kilograms, speed in meters per second, and height in meters. If you are on Earth, you can leave gravity at 9.81 m/s², or adjust it for other planets or elevations. Click calculate to see energy in joules. If you only know some values, use the conservation idea to solve for a missing speed or height by comparing the energy before and after.
Real-world uses include estimating the energy of a skateboarder on a ramp, the speed of a roller coaster at different points, or the potential energy stored in a lifted load. Students use these formulas in physics homework, and engineers use the same concepts when analyzing motion, safety, and energy efficiency in systems like elevators, cranes, or regenerative braking.
Disclaimer: Educational tool only. Ignores air resistance, rotation, and real-world losses.
A 70 kg sprinter at 10 m/s carries 3,500 J of kinetic energy—roughly the same as a fully charged phone battery. Blink and it becomes heat in the track.
Hoist a 10 kg backpack onto a 2 m shelf and you’ve banked 196 J of gravitational energy—enough to lift a small drone for a second if you could reclaim it perfectly.
A peregrine stooping at 90 m/s (0.9 kg mass) packs about 3,645 J. That’s the energy of a 1 kg rock dropped from a 372 m cliff—no wonder prey rarely walks away.
Dropping 1 litre of water (≈1 kg) through a 100 m dam releases 981 J. A typical 1 GW hydro plant chews through about a billion litres every 100 s.
The ISS orbits at 7.66 km/s. If you froze its 419,000 kg mass and dumped all kinetic energy into height, it could climb another ~3,000 km before stalling. Orbit is just fancy KE↔PE juggling.