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ScienceGrade 9· U.S. National — Common Core & NGSS
Aligned to:Next Generation Science Standards (NGSS)

Earth’s Energy Budget and the Greenhouse Effect

Students use diagrams and data to explain how incoming solar radiation, reflected energy, and greenhouse gases influence Earth’s temperature.

Earth’s Energy Budget and the Greenhouse Effect

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Tracing Incoming Solar Energy

Nearly all energy that drives Earth’s climate begins as radiation from the Sun. This energy travels through space mainly as shortwave radiation, including visible light. At the top of the atmosphere, Earth receives an average of about 340 watts per square meter when sunlight is averaged over the entire planet. However, solar energy is not distributed evenly. Near the equator, sunlight strikes the surface more directly and concentrates energy over a smaller area. Near the poles, sunlight arrives at a lower angle and spreads the same amount of energy over a larger area. For example, a flashlight aimed straight at paper makes a bright, concentrated spot, while the same flashlight tilted sideways makes a wider, dimmer spot. Earth’s rotation, seasons, and curved surface therefore cause variations in incoming energy.

A Sun shines shortwave radiation on a curved Earth, with direct rays at the equator and angled rays at the poles.
A Sun shines shortwave radiation on a curved Earth, with direct rays at the equator and angled rays at the poles.Source: Illustrated for this lesson

Reflection, Absorption, and Radiation

Incoming solar energy can be reflected or absorbed by Earth’s atmosphere, clouds, land, and oceans. About 30 percent is reflected back to space, mainly by clouds, ice, snow, and other bright surfaces. This reflectivity is called albedo. The remaining roughly 70 percent is absorbed by the atmosphere and surface, increasing their thermal energy. Earth then releases energy as longwave infrared radiation because the planet is much cooler than the Sun. In a simple balanced model, 100 units of solar energy arrive, 30 units are reflected, 70 units are absorbed, and 70 units of infrared energy eventually leave for space. For example, fresh snow reflects much more sunlight than dark ocean water. As a result, snow usually absorbs less solar energy and warms more slowly than the ocean under similar sunlight.

An Earth energy diagram shows sunlight being reflected by bright snow and absorbed by dark ocean before leaving as infrared radiation.
An Earth energy diagram shows sunlight being reflected by bright snow and absorbed by dark ocean before leaving as infrared radiation.Source: Illustrated for this lesson

How Greenhouse Gases Retain Heat

Earth’s surface absorbs solar energy and emits infrared radiation upward. Greenhouse gases, including water vapor, carbon dioxide, methane, and nitrous oxide, absorb specific wavelengths of this outgoing infrared energy. The gas molecules then emit infrared radiation in all directions. Some energy continues toward space, while some returns toward the surface and lower atmosphere. This process slows the transfer of energy from Earth to space and keeps the surface warmer than it would be without greenhouse gases. Greenhouse gases do not create energy or simply form a solid blanket. They change how infrared energy moves through the atmosphere. For example, adding carbon dioxide increases infrared absorption at certain wavelengths. The surface and lower atmosphere then warm until outgoing energy once again balances the energy Earth absorbs from the Sun.

Infrared arrows rise from Earth’s surface, interact with greenhouse gases, and travel both toward space and back downward.
Infrared arrows rise from Earth’s surface, interact with greenhouse gases, and travel both toward space and back downward.Source: Illustrated for this lesson

Interpreting an Energy-Budget Model

An energy-budget model uses arrows and numbers to represent energy flowing into and out of Earth’s systems. Arrow direction shows where energy moves, while arrow width or a numerical value shows the amount. Suppose a model shows 340 watts per square meter of incoming solar energy, 100 watts per square meter reflected to space, and 240 watts per square meter absorbed. If 240 watts per square meter also leaves as infrared radiation, the budget is balanced and average temperature is expected to remain relatively stable. To translate the diagram into words, state each flow and compare the totals: 340 enters, 100 is reflected, 240 is absorbed, and 240 leaves. Models simplify reality because energy exchanges also occur among the surface, clouds, oceans, and atmosphere. Even so, they help scientists identify whether Earth is gaining or losing energy.

A numbered Earth energy-budget model shows incoming, reflected, absorbed, and outgoing arrows with balanced totals.
A numbered Earth energy-budget model shows incoming, reflected, absorbed, and outgoing arrows with balanced totals.Source: Illustrated for this lesson

Explaining Changes in Earth’s Temperature

Earth’s average temperature changes when energy entering and leaving the climate system becomes unbalanced. If Earth absorbs more energy than it sends to space, the oceans, land, atmosphere, and ice gain thermal energy and warm. For example, if 240 watts per square meter is absorbed but only 239 watts per square meter initially escapes, the positive difference of 1 watt per square meter produces warming. Increasing greenhouse gas concentrations can create this imbalance by reducing outgoing infrared energy until the climate warms enough to restore balance. Human activities such as burning fossil fuels and clearing forests raise carbon dioxide levels and alter physical systems. Warming can also melt reflective ice, exposing darker water or land that absorbs more sunlight. This ice-albedo feedback strengthens the initial warming and shows how human and physical Earth systems can influence one another.

A climate diagram shows a one-watt energy imbalance warming Earth and melting reflective ice to expose darker ocean.
A climate diagram shows a one-watt energy imbalance warming Earth and melting reflective ice to expose darker ocean.Source: Illustrated for this lesson