Greenhouse Gases
Overview
Greenhouse gases are molecules that absorb thermal radiation emitted by a planet and emit it in all directions, including back to the planet's surface. Unlike the various types of light that a planet can reflect, this emitted planetary radiation is primarily a smaller subset of the electromagnetic spectrum (e.g., infrared). By acting as a blanket that prevents some of this energy from escaping to space, a planet warms in a phenomenon called the greenhouse effect.
In the early 1800s, as scientists began developing the field of thermodynamics to improve the efficiency of steam engines, an analysis of Earth revealed it to be much warmer than expected. Sunlight alone was shown to be insufficient, and the atmosphere was hypothesized to act as an insulator. By mid-century, experiments showed that some atmospheric gases, including water vapor and carbon dioxide, could absorb and emit some infrared radiation—the kind emitted by Earth's surface—significantly altering the planet's climate.
Despite greenhouse gases accounting for less than 0.04% of the Earth's atmosphere, average surface temperatures would be about 33 degrees Celsius (59 degrees Fahrenheit) lower without them. However, atmospheric carbon dioxide concentrations have increased by over 50% since before the Industrial Revolution—primarily driven by the burning of fossil fuels—causing a rise in average surface temperatures during the same period.
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