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9.3 Conservation of Energy

9.3 Conservation of Energy

Written by the Fiveable Content Team • Last updated August 2025
Written by the Fiveable Content Team • Last updated August 2025
🫴Physical Science
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Conservation of Energy

Energy conservation is a fundamental principle in physics: energy can't be created or destroyed, only transformed from one form to another. This concept applies to every physical process, from a swinging pendulum to a hydroelectric dam, and it gives you a powerful tool for predicting how systems behave. Understanding energy conservation also helps explain why real-world machines are never perfectly efficient, since some energy always spreads into less useful forms like heat.

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Fundamental Principles

The Law of Conservation of Energy states that the total energy in a closed system remains constant over time. A closed system is one where no energy or matter enters or leaves. Energy can change forms within that system, but the total amount stays the same.

This is expressed mathematically as:

Einitial=EfinalE_{initial} = E_{final}

If you track all the energy at the start of a process and all the energy at the end, those two numbers must be equal. Energy isn't appearing from nowhere or vanishing. It's just shifting between forms, like kinetic energy converting to potential energy and back again.

This law applies universally. It holds for mechanical systems, chemical reactions, electrical circuits, and nuclear processes.

Forms of Energy

Fundamental Principles of Energy Conservation, Thermodynamics | Biology for Majors I

Mechanical Energy

Mechanical energy is the sum of an object's kinetic energy and potential energy.

  • Kinetic energy (KE) is the energy of motion: KE=12mv2KE = \frac{1}{2}mv^2
    • mm = mass (kg), vv = velocity (m/s)
    • A 2 kg ball moving at 3 m/s has KE=12(2)(32)=9 JKE = \frac{1}{2}(2)(3^2) = 9 \text{ J}
  • Gravitational potential energy (PE) is energy stored due to an object's height above a reference point: PE=mghPE = mgh
    • mm = mass (kg), gg = acceleration due to gravity (9.8 m/s²), hh = height (m)
    • A 2 kg ball held 5 m above the ground has PE=(2)(9.8)(5)=98 JPE = (2)(9.8)(5) = 98 \text{ J}
  • Elastic potential energy is energy stored in stretched or compressed objects, like springs or rubber bands. For a spring, it depends on how far the spring is deformed and how stiff it is.

In an ideal system with no friction, the total mechanical energy stays constant:

KEi+PEi=KEf+PEfKE_i + PE_i = KE_f + PE_f

This means that as an object loses potential energy (falls), it gains an equal amount of kinetic energy (speeds up), and vice versa.

Thermal Energy and Heat Transfer

Thermal energy is the total kinetic energy of all the particles in a substance. The faster the particles move, the more thermal energy the substance has. Temperature measures the average kinetic energy of those particles, which is a slightly different thing. Two objects can have the same temperature but different amounts of thermal energy if one has more mass.

Heat is the transfer of thermal energy from a warmer object to a cooler one. This transfer happens in three ways:

  • Conduction: energy passes through direct particle-to-particle contact (a metal spoon getting hot in soup)
  • Convection: energy moves through the bulk flow of a fluid, as warmer fluid rises and cooler fluid sinks (warm air rising from a heater)
  • Radiation: energy travels as electromagnetic waves, requiring no medium at all (sunlight warming your face)
Fundamental Principles of Energy Conservation, Conservation of Energy | Physics

Applications of Energy Conservation

A pendulum is one of the clearest demonstrations. At the top of its swing, the pendulum has maximum potential energy and zero kinetic energy (it momentarily stops). At the bottom, that potential energy has fully converted to kinetic energy, and the pendulum moves at its greatest speed. Then it swings back up, converting kinetic back to potential. The total stays the same throughout.

Here are other examples of energy transformation:

  • Roller coasters convert gravitational PE at the top of a hill into KE as the car descends, then back to PE on the next climb. Each successive hill must be shorter than the first because some energy is lost to friction.
  • Hydroelectric dams convert the gravitational PE of elevated water into KE of flowing water, which spins turbines to generate electrical energy.
  • Solar panels transform light energy from the sun into electrical energy.
  • Nuclear power plants convert nuclear energy into thermal energy (heating water to steam), which then drives turbines to produce electrical energy.
  • Photosynthesis converts light energy into chemical energy stored in glucose molecules.

In every case, you can trace where the energy starts and where it ends up. The total is always conserved.

Energy Loss and Dissipation

Friction

In real systems, friction converts mechanical energy into thermal energy. This is why a sliding book on a table slows down and stops, and why your hands warm up when you rub them together. The kinetic energy doesn't disappear; it becomes heat spread into the surfaces and surrounding air.

The main types of friction are:

  • Static friction: resists the start of motion between surfaces in contact
  • Kinetic friction: acts on surfaces already sliding against each other
  • Rolling friction: acts on rolling objects (typically much less than sliding friction)
  • Fluid friction (drag): resistance from moving through air or liquid

The energy removed by friction over a distance can be calculated as:

Wfriction=fdW_{friction} = f \cdot d

where ff is the friction force and dd is the distance over which it acts. For surfaces sliding against each other, the friction force equals μN\mu N, where μ\mu is the coefficient of friction (a number that depends on the two surfaces) and NN is the normal force. Friction isn't always a problem, though. Without it, you couldn't walk or drive.

Lubricants like oil reduce friction between surfaces by keeping them from making direct contact, which is why engines need regular oil changes.

Energy Dissipation and Efficiency

Energy dissipation is the spread of energy into less useful forms, primarily heat. Because of dissipation, no real-world process is 100% efficient. A car engine, for example, converts only about 20–25% of the chemical energy in gasoline into useful motion. The rest becomes waste heat.

Energy efficiency is calculated as:

Efficiency=useful energy outputtotal energy input×100%\text{Efficiency} = \frac{\text{useful energy output}}{\text{total energy input}} \times 100\%

For example, if you put 100 J of electrical energy into a light bulb and it produces 10 J of light energy, its efficiency is 10%. The other 90 J became heat.

This connects to the Second Law of Thermodynamics, which states that in any energy transfer, some energy becomes less organized and harder to use. Entropy (a measure of disorder) in a system tends to increase over time. This is why energy transformations always go in the direction of more spread-out, less concentrated energy.

Strategies to reduce energy dissipation include:

  • Insulation to reduce heat loss (in buildings, pipes, and engines)
  • Streamlined designs to reduce air resistance (in cars and aircraft)
  • Energy-efficient technologies like LED lights (which convert more electrical energy to light and less to heat than incandescent bulbs) and hybrid cars (which recapture braking energy through regenerative braking)

The energy isn't truly "lost" in any of these cases. It still exists, just in a form that's no longer useful for doing work. Conservation of energy always holds.

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