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What Are the Key Differences Between Conduction, Convection, and Radiation?

Key Differences Between Conduction, Convection, and Radiation

  1. Conduction:

    • This is when heat moves through direct contact.
    • It usually happens in solids.
    • For example, if you put a metal spoon in hot soup, the spoon will get hot and reach the same temperature as the soup.
    • Metals, like aluminum, are good at conducting heat. Aluminum conducts heat much better than wood.
  2. Convection:

    • This is how heat moves through liquids and gases.
    • In convection, the fluid itself is moving.
    • For example, warm air goes up while cooler air sinks. This movement creates what we call convection currents.
    • In most homes, the air moves at around 0.1 meters per second.
  3. Radiation:

    • This is when heat travels through electromagnetic waves.
    • It doesn’t need anything to travel through.
    • A good example is the heat we get from the sun; it reaches Earth through space.
    • There’s a rule called the Stefan-Boltzmann Law, which says that the amount of power radiated changes with the temperature of the object.

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What Are the Key Differences Between Conduction, Convection, and Radiation?

Key Differences Between Conduction, Convection, and Radiation

  1. Conduction:

    • This is when heat moves through direct contact.
    • It usually happens in solids.
    • For example, if you put a metal spoon in hot soup, the spoon will get hot and reach the same temperature as the soup.
    • Metals, like aluminum, are good at conducting heat. Aluminum conducts heat much better than wood.
  2. Convection:

    • This is how heat moves through liquids and gases.
    • In convection, the fluid itself is moving.
    • For example, warm air goes up while cooler air sinks. This movement creates what we call convection currents.
    • In most homes, the air moves at around 0.1 meters per second.
  3. Radiation:

    • This is when heat travels through electromagnetic waves.
    • It doesn’t need anything to travel through.
    • A good example is the heat we get from the sun; it reaches Earth through space.
    • There’s a rule called the Stefan-Boltzmann Law, which says that the amount of power radiated changes with the temperature of the object.

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