Kinetic, elastic and gravitational energy explained
Principles of energy • Energy stores and changes
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Key concepts
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Kinetic energy (Ek)
Kinetic energy is the energy held by an object because of its motion. The kinetic energy equation is E_k = 0.5 × m × v^2 where m is mass in kilograms and v is speed in metres per second. Doubling mass doubles kinetic energy; doubling speed increases kinetic energy by a factor of four because speed is squared. Kinetic energy calculations use the SI unit joule (J). Practical calculations link kinetic energy change to work done by forces, for example when brakes convert kinetic energy to thermal energy in stopping a car .
Elastic potential energy (Ee)
Elastic potential energy is the energy stored in an elastic object when it is stretched or compressed, provided the deformation stays within the elastic limit. The equation on the physics equation sheet is E_e = 0.5 × k × e^2 where k is the spring constant (N/m) and e is extension (m). Energy stored is proportional to the square of extension, so small increases in extension produce larger increases in stored energy. If deformation passes the limit of proportionality, the formula no longer applies and permanent deformation occurs .
Gravitational potential energy (Ep)
Gravitational potential energy is the energy associated with an object’s position in a gravitational field. The equation is E_p = m × g × h where m is mass (kg), g is gravitational field strength (N/kg, typically 9.8 N/kg near Earth's surface) and h is height above a chosen reference point (m). Raising an object against gravity requires work; the work done equals the increase in gravitational potential energy. The equation applies for uniform g and for height changes small enough that g is effectively constant .
Key notes
Important points to keep in mind