JN

Energy in Earth Processes

  • The thermosphere, the outermost part of Earth's atmosphere, has extremely high temperatures (thousands of degrees).

  • Despite the high temperatures, a person would freeze to death if exposed to the thermosphere without a protective suit.

  • This is because the density of atoms/molecules is very low, resulting in little thermal energy and available heat.

  • An unprotected body would lose its thermal energy to the thermosphere.

Vocabulary

  • condensation

  • conduction

  • convection

  • crystallization

  • electromagnetic energy

  • electromagnetic spectrum

  • energy

  • heat energy

  • joules

  • mechanical energy

  • nuclear decay

  • radiation

  • solidification

  • specific heat

  • temperature

  • texture

  • vaporization

  • wavelength

Topic Overview

  • Energy is the ability to do work and is a fundamental attribute of the universe.

  • Earth operates as a machine driven by two major heat engines.

    • External Engine: Powered mainly by solar energy and drives most Earth surface processes.

    • Internal Engine: Powered by heat from Earth's interior, resulting in mechanical energy.

Electromagnetic Energy

  • Electromagnetic energy is radiated in transverse waves from all matter not at absolute zero.

  • Absolute zero is 0 Kelvin or -273° Celsius, the theoretically lowest possible temperature where particles have no motion.

  • Visible light is a type of electromagnetic energy that is radiated by the sun and can be observed by the human eye.

  • Transverse waves vibrate at right angles to their direction of movement.

Electromagnetic Spectrum

  • Different types of electromagnetic energy are distinguished by their wavelengths.

  • Wavelength: The distance from one crest of a wave to the next crest.

  • Electromagnetic Spectrum: A model showing the various types of electromagnetic energy in order of increasing wavelength.

  • Visible light is the only part of the electromagnetic spectrum that can be seen by the human eye.

  • Infrared energy is often felt due to its heating effects.

  • Instruments are needed to observe most forms of electromagnetic energy, such as ultraviolet energy.

  • Long-wave electromagnetic energy has a wavelength longer than visible light.

  • Short-wave electromagnetic energy has a wavelength shorter than visible light.

Interactions Between Electromagnetic Energy and an Environment

  • When electromagnetic energy interacts with a material, the waves can be:

    • Refracted: Bent in their passage through materials of varying density, changing their direction.

    • Reflected: Bounced off the material.

    • Scattered: Refracted and/or reflected in various directions.

    • Transmitted: Passed through the material.

    • Absorbed: Taken into the material.

Surface Properties and Absorption

  • Absorption characteristics of a surface determine how much electromagnetic energy is absorbed.

  • Darker surfaces absorb more visible light, which is why dark asphalt feels hotter than light concrete on a sunny day.

  • Color is the way the human eye distinguishes different wavelengths of visible light.

  • Rougher surfaces absorb more energy and reflect less, while smoother surfaces (like mirrors) reflect more light.

  • Materials that are effective at absorbing electromagnetic energy are also better at radiating it.

  • Dark-colored objects heat up and cool down quickly, while light-colored objects heat up and cool down more slowly.

Transfer of Energy

  • Energy moves from a region of high concentration (source) to a region of low concentration (sink).

  • Heat energy: Energy transfer from a region of higher temperature to a region of lower temperature.

  • Heat transfers thermal energy: The energy of the motions of atoms and molecules.

Achieving Dynamic Equilibrium

  • Heat continues to move from source to sink until their energies are equal, establishing dynamic equilibrium.

  • Dynamic Equilibrium: A state where a region loses and gains equal amounts of energy.

  • If dynamic equilibrium is between all forms of energy, the temperature of the region or system will remain constant.

Methods of Energy Transfer

  • Heat is transferred from an area of high concentration to an area of low concentration by one of three methods:

    • Conduction

    • Convection

    • Radiation

Conduction
  • Conduction: The transfer of heat energy from atom to atom or molecule to molecule when vibrating atoms or molecules collide.

  • Most effective in solids (especially metals) because atoms/molecules are closer together.

  • Can also occur in liquids and gases.

Convection
  • Convection: The transfer of heat by movement in fluids (gases and liquids) caused by differences in density.

  • Warmer portions of the fluid usually have lower density and rise above cooler portions.

  • Higher-density portions of a fluid are pulled down and displace less dense objects, pushing them upward.

  • Convection Current: A circulatory motion that transfers heat energy from one place to another.

  • Convection currents transfer heat throughout Earth's atmosphere, hydrosphere, and likely below the lithosphere.

Radiation
  • Radiation: The method by which heat is transferred via electromagnetic waves.

  • No medium is needed to transfer electromagnetic energy, allowing it to radiate across empty space.

  • Radiation can also occur in liquids, solids, and gases.

  • The higher an object's temperature, the more electromagnetic energy it gives off.

Transformation of Energy

  • Transformation of energy: The changing of one type of energy into another type of energy.

Heat Production
  • Transformations of energy often occur when there is friction.

  • Example: Kinetic energy of a glacier transforms into heat energy due to friction between the glacier and valley walls.

  • Another example: Wind blowing over the ocean creates waves and ocean currents, forming heat at the interface of the atmosphere and hydrosphere.

Transformations of Mechanical Energy
  • Mechanical energy: All the energy of an object or system not related to the individual motions of atoms and molecules; the total of potential and kinetic energy.

  • Kinetic energy: Energy of