Lesson 5: Environmental Impacts of Energy Production
Lesson 5: Environmental Impacts of Energy ProductionThe links below provide an outline of the material for this lesson. Be sure to carefully read through the entire lesson before returning to Canvas to submit your assignments.
5.1 Lesson 5 Introduction
5.1 Lesson 5 IntroductionWelcome to Lesson 5
As we explored in Lesson 1, energy can be generated from many sources—fossil fuels, nuclear power, hydropower, wind, solar, and more. But here's a critical truth: no energy source is completely impact-free. Every method of producing energy affects the environment in some way, whether through emissions into the atmosphere, water use, land disruption, or waste generation. Understanding these trade-offs is essential for making informed decisions about our energy future.
In this lesson, we will examine the environmental consequences of our energy choices. We'll start by analyzing the major pollutants released when burning fossil fuels—including carbon dioxide, nitrogen oxides, sulfur dioxide, and particulate matter—and how these emissions affect air quality, human health, and climate. Next, we'll highlight historical environmental successes, such as global cooperation to reduce sulfur emissions and heal the ozone layer, demonstrating that science, policy, and innovation can drive meaningful progress. We'll also investigate the challenges of nuclear waste management and the long-term stewardship required for radioactive materials. Finally, we'll explore the water-energy nexus, comparing how much water different technologies consume and why that matters in water-stressed regions.
Learning Objectives
By the end of this lesson, you will be able to:
- Identify the primary environmental impacts associated with major energy sources (fossil fuels, nuclear, hydropower, wind, solar, and biomass).
- Compare the trade-offs between energy technologies across multiple dimensions: greenhouse gas emissions, air pollution, water consumption, land use and change, and waste generation.
- Explain how combustion of fossil fuels releases pollutants that affect human health, ecosystems, and climate—and describe the chemical processes behind key emissions (CO₂, NOₓ, SO₂, PM).
- Analyze the water-energy nexus by evaluating withdrawal vs. consumption across different electricity generation methods and assessing regional implications.
- Evaluate the challenges and strategies for managing high-level nuclear waste, including storage technologies and policy considerations.
- Recognize examples of successful environmental policy—such as the Montreal Protocol and the U.S. Acid Rain Program—and explain how science, technology, and international cooperation enabled positive change.
5.2 Fossil Fuels and Products of Combustion
5.2 Fossil Fuels and Products of CombustionIn Lesson 3 (Energy Supply and Demand), we explored how the United States and the world source their energy. One key takeaway: fossil fuels—petroleum, natural gas, and coal—still dominate the global energy mix.
Want the latest data? Check out the U.S. Energy Information Administration's U.S. Energy Facts Explained for up-to-date statistics. As of 2024, fossil fuels supply more than 80% of total U.S. energy consumption.
How Fossil Fuels Release Energy
When we use fossil fuels for energy, we typically burn (combust) them. This chemical reaction releases stored energy—but also emits substances into the atmosphere.
A simplified representation of hydrocarbon combustion looks like this:
Important note: The "air" in this reaction isn't just oxygen. Earth's atmosphere is ~78% nitrogen (N2), ~21% oxygen (O2), and ~1% argon and other gases. At high combustion temperatures, nitrogen can react to form nitrogen oxides (NOx)—a key pollutant we'll discuss shortly.
What's Actually in Fossil Fuels?
Fossil fuels are primarily made of carbon (C) and hydrogen (H)—the same building blocks found in all living things. That's no coincidence: fossil fuels formed over millions of years from ancient plants and microorganisms that were buried, compressed, and shielded from decay.
In addition to carbon and hydrogen, fossil fuels contain small amounts of:
- Sulfur (S) → can form SO2 (a contributor to acid rain)
- Nitrogen (N) → contributes to NOx formation
- Oxygen (O), trace metals, and mineral matter
Clarification: Not everything in the fuel is emitted unchanged. During combustion, chemical bonds break and reform, producing new compounds—some useful (like energy and water vapor), others harmful (like CO2, NOx, SO2, and particulates).
In this unit, we'll examine the major pollutants released from combustion, how they affect human health and the environment, and what strategies exist to reduce their impact.

Text description of the Fossil Fuel Composition image.
Natural gas is composed of carbon, hydrogen, nitrogen, sulfur, and oxygen.
Petroleum is composed of carbon, hydrogen, nitrogen, sulfur, oxygen, and minerals.
Coal is composed of carbon, hydrogen, nitrogen, sulfur, oxygen, and minerals.
Instructions: Click on the purple hot spot shown above the piece of coal below to determine what products are formed from each during combustion.
The most common products of combustion we will discuss in this module are as follows.
5.2.1 Carbon Dioxide
5.2.1 Carbon DioxideCarbon Dioxide (CO2)
Fossil fuels—coal, oil, and natural gas—are rich in carbon (C) and hydrogen (H). When we burn them for energy, carbon combines with oxygen from the air to form carbon dioxide (CO2). In fact, CO2 is the largest chemical product by mass released from fossil fuel combustion.
Fun connection: Yes, humans also exhale CO2 when we breathe! And plants need CO2 for photosynthesis—the process that powers life on Earth. So CO2 itself isn't "bad". The problem is scale and speed:
- Natural carbon cycle: Plants absorb ~120 billion tons of CO2/year; oceans and soils absorb more.
- Human addition: Burning fossil fuels adds ~38 billion tons of extra CO2 per year (as of 2024)—far more than natural systems can absorb quickly.
Use the “our world in data” interactive below to see which countries emit the most carbon emissions total.
5.2.2 Carbon Monoxide
5.2.2 Carbon MonoxideCarbon Monoxide (CO)
Carbon monoxide is a colorless, odorless, and tasteless gas formed when fossil fuels don't burn completely—a process called incomplete combustion. This happens when there isn't enough oxygen, the temperature is too low, or the fuel-air mixture isn't well mixed.
Carbon dioxide & carbon monoxide (Chemistry) (4:04)
Transcript: Carbon dioxide & carbon monoxide (Chemistry) (4:04)
[Music]
[Applause]
[Music]
[Presenter] Most chemical reactions are pretty predictable. If we know what substances we start with, we know what substances will be formed, and we'll get the same result every time those substances react.
But sometimes the very same reactants can yield different products. There are reactions where the temperature can affect which substances are formed, and there are reactions where it matters whether we use a larger or smaller amount of one of the reactants.
That’s the case with the graphite and oxygen example. Usually, when there is plenty of oxygen, carbon and oxygen will form carbon dioxide when the graphite burns. When there is less available oxygen, like when the reaction takes place in an area with limited air supply, another reaction will occur as well, where another product is formed. In this substance, each carbon atom is attached to one oxygen atom instead of two. Instead of carbon dioxide, carbon monoxide is formed, where “mono” means one. The name of the compound is contracted from mono oxide to monoxide.
Carbon dioxide and carbon monoxide. They sound almost the same, and both are made up of carbon and oxygen, but there is an important difference between them. Carbon dioxide is naturally present in the atmosphere. There’s not much—only four hundredths of one percent—but it’s vital for all plant life. The air you exhale contains about a hundred times that amount, about four percent carbon dioxide. If there is a lot of carbon dioxide in a room, the air feels bad, but it is not dangerous to inhale.
Carbon monoxide, on the other hand, is poisonous for humans and animals. If the air you inhale contains as little as one percent carbon monoxide, that’s enough to kill you within minutes. Carbon monoxide is formed not only when pure graphite burns. Other combustible substances that contain carbon, such as petrol, oil, plastic, or wood, can also form carbon monoxide.
It’s called incomplete combustion and occurs as soon as the oxygen level gets too low. In a house fire, the carbon monoxide produced is particularly dangerous. It can make the people in the house unconscious before they have time to get out, or they can even die in their sleep without even noticing there is a fire. In a fire, there is a greater risk of dying from carbon monoxide poisoning than from the flames.
Good job they had a working smoke detector.
It’s a simplification to say that when carbon compounds burn, we get either carbon dioxide or carbon monoxide. In reality, both reactions take place at the same time. Less oxygen results in more carbon monoxide. Chemical reactions can give different products even though we start with the same reactants, and in this case, where carbon reacts with oxygen, this difference can mean life or death.
[Music]
Common sources include:
- Vehicles (cars, trucks, buses) — especially in idling or poorly tuned engines
- Home appliances: gas stoves, kerosene heaters, fireplaces, and portable generators
- Industrial processes: boilers, furnaces, and certain manufacturing operations
Why Is CO So Dangerous?
CO is extremely hazardous because it binds to hemoglobin in your blood ~200 times more tightly than oxygen does. When you inhale CO:
- It displaces oxygen in your bloodstream
- Your heart, brain, and other vital organs are starved of oxygen
- Symptoms progress rapidly:
→ Mild exposure: headache, dizziness, nausea, fatigue
→ Moderate exposure: confusion, blurred vision, difficulty breathing
→ Severe exposure: loss of consciousness, organ damage, death
Critical fact: Because CO has no smell or color, you can't detect it without a monitor. Poisoning can happen quickly—and silently.
How to Stay Safe: Prevention Saves Lives
Never run a vehicle inside a closed garage—even with the door open, fumes can accumulate dangerously.
Never use portable generators, grills, or camp stoves indoors (including garages, basements, or near windows).
Ensure proper ventilation for all fuel-burning appliances (heaters, fireplaces, water heaters).
Install battery-backed CO detectors on every level of your home and near sleeping areas. Test them monthly!
Schedule annual maintenance for furnaces, chimneys, and gas appliances to ensure clean, complete combustion.
While CO is primarily a local air quality and safety issue (unlike CO2, which affects global climate), it highlights an important principle in energy engineering: complete, efficient combustion isn't just about performance—it's about protecting human health. Modern engines, power plants, and appliances use advanced controls, catalytic converters, and sensors specifically to minimize CO emissions.
5.2.3 Sulfur Dioxide
5.2.3 Sulfur DioxideSulfur Dioxide (SO2)
Sulfur dioxide is a colorless gas with a sharp, irritating odor. It forms when sulfur (S) present in fossil fuels reacts with oxygen during combustion:
Why do coal and petroleum contain sulfur?
Fossil fuels formed from ancient organic matter that absorbed sulfur from seawater, sediments, and volcanic activity over millions of years. As a result:
- Coal: Often contains 0.5–5% sulfur by weight (varies by mine location)
- Petroleum: Contains sulfur compounds that are partially removed during refining ("sweet" vs. "sour" crude)
- Natural gas: Typically very low in sulfur (mostly removed before distribution)
The Chemistry of Acid Formation
SO₂ is highly soluble in water. When it mixes with atmospheric moisture, a cascade of reactions occurs:
- SO2 + H2O → H2SO3 (sulfurous acid — weak, but irritating)
- H2SO3 + ½O2 → H2SO4 (sulfuric acid — strong acid, major component of acid rain)
- SO2 also reacts with ammonia, metals, and other pollutants to form sulfate particles (aerosols)
These fine particles can:
- Remain suspended in air for days to weeks
- Travel hundreds of miles from the original source
- Scatter light → reduced visibility ("haze")
- Penetrate deep into lungs when inhaled
Global Context & Progress
- Historical peak: U.S. SO₂ emissions peaked in the 1970s (~26 million tons/year), largely from coal-fired power plants.
- Policy success: The 1990 Clean Air Act Amendments created a cap-and-trade program for SO2. Result? U.S. SO2 emissions dropped ~94% since 1990—one of environmental policy's biggest wins.
- Current challenges: SO2 remains a major issue in regions with heavy coal use and fewer emissions controls (e.g., parts of Asia, Eastern Europe). Satellite data now helps track global SO2 hotspots in near real-time.
How Do We Reduce SO2 Emissions?
| Strategy | How It Works | Example |
|---|---|---|
| Flue Gas Desulfurization (FGD) | "Scrubbers" spray limestone slurry into exhaust; SO2 reacts to form gypsum (usable in drywall) | >90% of U.S. coal plants now use scrubbers |
| Fuel Switching | Use low-sulfur coal, natural gas, or renewables instead of high-sulfur coal | U.S. shift from coal → gas cut SO2 dramatically |
| Fuel Desulfurization | Remove sulfur from petroleum during refining (hydrodesulfurization) | Ultra-low-sulfur diesel (ULSD) now standard in vehicles |
| Policy & Monitoring | Emissions caps, continuous monitoring, international agreements | Acid Rain Program; WHO air quality guidelines |
5.2.4 Nitrogen Oxides
5.2.4 Nitrogen OxidesNitrogen Oxides (NOx)
Nitrogen oxides is a generic term for a group of highly reactive gases containing nitrogen and oxygen. The two most important for air quality are:
- Nitric oxide (NO): Colorless, odorless, formed first during combustion
- Nitrogen dioxide (NO2): Reddish-brown gas with a sharp, biting odor; forms when NO reacts with oxygen in the air
How Is NOx Formed?
NOx forms primarily through high-temperature combustion—when nitrogen (N2) and oxygen (O2) from the air react under intense heat. This is called thermal NOx formation:
Key insight: Even if a fuel contains no nitrogen, NOx can still form because air itself is 78% nitrogen. The hotter the flame and the longer gases stay at high temperature, the more NOx is produced.
| Source Category | Examples | Why It Matters |
|---|---|---|
| Transportation | Cars, trucks, buses, ships, aircraft | High-temperature engines; major source in urban areas |
| Electric Power Generation | Coal, oil, and natural gas power plants | Large, continuous combustion sources |
| Industrial/Commercial | Boilers, furnaces, cement kilns, refineries | Often located near communities |
| Residential | Gas stoves, water heaters, fireplaces | Indoor air quality concern; cumulative urban impact |
Why You Can Sometimes See NOx
While NO and many NOx compounds are invisible, nitrogen dioxide (NO2) has a distinctive reddish-brown color. When mixed with other pollutants (like volatile organic compounds and fine particles), it contributes to:
- Photochemical smog: The hazy, brownish layer over cities on sunny days
- Urban haze: Reduced visibility in metropolitan areas and national parks

Text description of the Sunrise towards a smog ridden Los Angeles downtown image.
The image showcases a panoramic view of Los Angeles, dominated by skyscrapers in the background. The skyline is shrouded in a hazy smog. The foreground features a major highway filled with vehicles, curving through the city landscape.
| Strategy | How It Works | Real-World Example |
|---|---|---|
| Catalytic Converters | Use platinum/palladium to convert NOx→ N2 + O2 in vehicle exhaust | Required on all U.S. gasoline vehicles since 1975 |
| Low-NOx Burners | Stage fuel/air injection to lower flame temperature and limit NOx formation | Standard in modern power plants and industrial boilers |
| Selective Catalytic Reduction (SCR) | Inject ammonia/urea into flue gas; catalyst converts NOx to harmless N2 + H2O | Used in >80% of U.S. coal plants and many diesel trucks |
| Electrification & Efficiency | Reduce combustion overall by switching to electric vehicles, heat pumps, renewables | Transportation electrification is the fastest-growing NOx reduction strategy |
| Policy Tools | Emissions standards, cap-and-trade programs, urban low-emission zones | California's Advanced Clean Cars program; EU Euro emissions standards |
5.2.5 Particulate Matter
5.2.5 Particulate MatterParticulate Matter (PM)
Particulate matter (PM) is a mixture of tiny solid particles and liquid droplets suspended in the air. Think of it as a "soup" of microscopic materials—from dust and soot to sulfates, nitrates, and organic compounds.
| Particle Type | Diameter | Visual Comparison | Can Reach... |
|---|---|---|---|
| Coarse PM (PM2.5-10) | 2.5–10 µm | Pollen, mold spores | Nose, throat, upper airways |
| Fine PM (PM2.5) | ≤ 2.5 µm | Smoke, bacteria | Deep lungs (alveoli), bloodstream |
| Ultrafine PM (PM0.1) | ≤ 0.1 µm | Viruses, combustion nanoparticles | Alveoli, potentially cross into blood |
Scale check: A human hair is ~70 µm wide. PM2.5 is 30× smaller—small enough to bypass your body's natural defenses.

Text description of the Size comparisons for PM particles image.
The image visually compares the size of different particles relative to a human hair. It features a large, detailed depiction of a human hair, shown horizontally in a gray hue with visible texture. Below the hair, there are three irregularly shaped particles labeled as "Fine Beach Sand" in various shades of green, orange, and yellow, with a diameter marked as 90 microns. Above and to the right of the hair, there are smaller, round particles in two groups. One group consists of pink spheres labeled "PM2.5," representing combustion particles, organic compounds, and metals, each less than 2.5 microns in diameter. The second group consists of blue spheres labeled "PM10," representing dust, pollen, mold, and other substances, each less than 10 microns in diameter. Arrows point from these groups to indicate their respective sizes relative to the human hair.
Where Does Particulate Matter Come From?
PM forms through two main pathways:
| Type | How It Forms | Common Energy-Related Sources |
|---|---|---|
| Primary PM | Emitted directly during combustion or physical processes | • Soot from diesel engines • Fly ash from coal plants • Dust from mining, construction, unpaved roads |
| Secondary PM | Forms in the atmosphere when gases react | • SO2 → sulfate particles • NOx + VOCs → nitrate particles + organic aerosols • Ammonia (from agriculture) + acids → ammonium salts |
Key insight: Even if a power plant installs filters to catch primary PM, it may still contribute to secondary PM downwind through gas emissions. This is why controlling SO2 and NOx also reduces particulate pollution.
How PM Affects Your Body: It's All About Size
Your respiratory system has natural filters—but PM can bypass them:
| Particle Size | Where It Deposits | Why It Matters |
|---|---|---|
| > 10 µm | Nasal passages, throat | Usually trapped and cleared by mucus/cilia |
| 2.5–10 µm | Upper airways, bronchi | Can irritate airways; trigger coughing, asthma |
| 0.1–2.5 µm | Deep lungs (alveoli) | Most dangerous: can cause inflammation, enter bloodstream |
| < 0.1 µm | Alveoli; may cross into blood | Emerging research links to cardiovascular effects |
| Strategy | How It Works | Real-World Example |
|---|---|---|
| Electrostatic Precipitators (ESPs) | Charge particles electrically; collect them on plates | Used in >90% of U.S. coal plants; >99% efficient for fly ash |
| Fabric Filters (Baghouses) | Force exhaust through fine fabric that traps particles | Common in cement plants, biomass facilities |
| Diesel Particulate Filters (DPFs) | Trap soot in vehicle exhaust; periodically burn it off | Required on modern diesel cars/trucks in U.S., EU |
| Fuel Switching & Efficiency | Reduce combustion overall: renewables, electrification, efficiency | Replacing coal with wind/solar cuts PM at the source |
| Policy & Monitoring | Air quality standards, emissions limits, public alerts | EPA's National Ambient Air Quality Standards (NAAQS) for PM2.5/PM10 |
Particulate matter (PM) is the general term used to describe a mixture of solid particles and liquid droplets found in the air. Some particles are large enough to be seen as dust or dirt. Others are so small they can be detected only with an electron microscope.
5.3 Green House Effect
5.3 Green House EffectThe greenhouse effect is the natural process in which gases in the atmosphere trap heat from the sun. This process was first identified by scientists in the 1800s. This process is what makes earth habitable for life.
How it works (simplified):
- Sunlight passes through the atmosphere and warms Earth's surface
- Earth radiates that heat back toward space as infrared radiation (invisible heat energy)
- Greenhouse gases (GHGs) absorb and re-emit some of that infrared radiation
- This trapped heat warms the lower atmosphere—like a blanket around the planet
What is the Greenhouse Effect? (2:29)
Transcript: What is the Greenhouse Effect? (2:29)
[Presenter]
What is the Greenhouse Effect?
Earth is a comfortable place for living things. It’s just the right temperatures for plants and animals – including humans – to thrive. Why is Earth so special? Well, one reason is: the greenhouse effect!
A greenhouse is a building with glass walls and a glass roof. The clear glass allows sunlight to shine into the greenhouse, while also trapping the Sun’s heat inside. This is how a greenhouse keeps plants warm, even at night and in the winter. The greenhouse effect keeps Earth warm in pretty much the same way.
Earth isn’t surrounded by glass, but it is surrounded by a jacket of gases called the atmosphere. In the daytime, the Sun shines through the atmosphere warming Earth’s surface. After the Sun goes down, Earth’s surface cools. This releases heat back into the air. But, some of that heat is trapped by the gases in the atmosphere. These heat-trapping gases are called greenhouse gases. Carbon dioxide, water vapor and methane are all examples of greenhouse gases.
Earth needs a balance of greenhouse gases to maintain just the right temperature for living things. But, some human activities are changing Earth’s natural greenhouse effect. For example, burning fossil fuels – like coal and oil – releases more carbon dioxide into our atmosphere. These extra greenhouse gases can cause the atmosphere to trap more and more heat, leading to a warmer Earth.
NASA satellites are constantly measuring the gases in our atmosphere from space. They have observed increases in the amount of carbon dioxide and other greenhouse gases. The information from NASA satellites can help scientists figure out where greenhouse gases are coming from and how they are ending up in our atmosphere. This information will help us better understand the impact that greenhouse gases have on our climate. And help us better understand this very special greenhouse that we call home. Find out more about our Earth at NASA Climate Kids!
5.3.1 Greenhouse Gases
5.3.1 Greenhouse GasesCarbon Dioxide (CO2): Carbon dioxide enters the atmosphere through burning fossil fuels, solid waste, trees, volcanos, and also as a result of certain chemical reactions (e.g., cement production). Carbon dioxide is removed from the atmosphere when it is absorbed by plants as part of the biological carbon cycle. Nearly 80% of all greenhouse gas emissions in the US is from carbon dioxide.
Methane (CH4): Methane is emitted during the production and transport of coal, natural gas, and oil. Methane emissions also result from livestock and other agricultural practices, land use, and by the decay of organic waste in municipal solid waste landfills. While methane emissions only account for about 11% of GHG emissions in the US, methane is more efficient at trapping radiation than carbon dioxide. Methane’s global warming potential is 28 times greater than carbon dioxide.
Nitrous Oxide (N2O): Nitrous oxide is emitted during agricultural, land use, and industrial activities; combustion of fossil fuels and solid waste; as well as during treatment of wastewater. Nitrous oxide oxide accounts for only 6% of GHG emissions in the US, but has a large impact because its global warming potential is 265 times that of carbon dioxide.
Water (H2O): Water is a naturally occurring greenhouse gas and most abundant. Water vapor amplifies global warming cause by other greenhouse gases. Water vapor has a very short lifespan in the atmosphere due to precipitation.
Fluorinated gases: Hydrofluorocarbons, perfluorocarbons, sulfur hexafluoride, and nitrogen trifluoride are synthetic, powerful greenhouse gases that are emitted from a variety of household, commercial, and industrial applications and processes. Fluorinated gases do have a natural cause, unlike the previous GHG discussed above. They are produced entirely from human related manufacturing and industrial processes.
The greenhouse effect is a natural process essential to life on Earth, maintaining a stable and hospitable climate for millions of years. However, human activities have significantly increased atmospheric greenhouse gas concentrations, disrupting this long-standing balance and driving a rapid rise in global temperatures. In the next page, we’ll explore how this warming translates into climate change—examining its real-world impacts, the science behind future projections, and the energy solutions that can help stabilize our planet’s climate.

Text description of the Greenhouse Effect image.
The image illustrates the greenhouse effect, divided into two sections: "Natural" and "Human-Enhanced." On the left, under "Natural," the atmosphere is shown as a curved line with "Greenhouse Gases" labeled. A large sun in the upper left corner emits an arrow labeled "Sun Energy" pointing towards Earth. Some of this energy is reflected as "Heat" back into space. The landscape includes small, subtle green shapes resembling hills and grass. The gases CH₄ and CO₂ are labeled above the line. On the right side, under "Human-Enhanced," the same concept is depicted, but with a denser layer of gases, labeled "More Greenhouse Gases." Additional visuals include industrial icons like factories. The arrows indicating heat reflection are more prominent, suggesting increased heat retention. The background is a gradient of blue, with text boxes providing explanations under each heading.
5.4 Climate Change
5.4 Climate ChangeClimate change refers to long-term shifts in global temperatures and weather patterns, typically measured over decades or longer. It's important to distinguish between weather the short-term conditions outside today, like rain, sunshine, or a cold snap and climate, which is the average of weather patterns over 30 years or more. Just because a particular day is cold or a region experiences a severe snowstorm does not mean climate change isn't happening or that the Earth isn't warming overall; climate is defined by long-term trends, not single events
Natural vs. Human-Caused Change
- Climate can change naturally (volcanic eruptions, solar activity)
- Since the 1800s, human activities have been the MAIN driver of recent climate change
- The primary cause? Burning fossil fuels: coal, oil, and natural gas
Humans are responsible for global warming
Climate scientists have showed that humans are responsible for virtually all global warming over the last 200 years. Human activities like the ones mentioned above are causing greenhouse gases that are warming the world faster than at any time in at least the last two thousand years.
The average temperature of the Earth’s surface is now about 1.42°C warmer than it was in the late 1800s-prior to the industrial revolution-and warmer than at any time in the last 100,000 years. Scientists can gather information on the environment going back hundreds of thousands of years through ice cores. Ice core samples trap small amounts of air bubbles which allow scientists to gather information on the environment at that time, including the amount of carbon dioxide in the atmosphere.
The last decade (2015-2024) was the warmest on record, and each of the last four decades has been warmer than any previous decade since 1850.
How Ancient Ice Proves Climate Change Is Real (12:25)
Transcript: How Ancient Ice Proves Climate Change Is Real (12:25)
[Dr. Jeffrey Severinghaus] You can see the tiny air bubbles in there? Those are what we study. This is a piece of ice – about 20,000 years old – from Antarctica. And bubbles trap air from 20,000 years ago, so we can find out what air was like back then. Can figure out if carbon dioxide has gone up or down. And what we’ve learned from that is carbon dioxide is higher now than it’s been for at least the last million years, probably the last 20 million years, but that’s less certain. So it’s really quite a dramatic thing that we humans have done to the carbon dioxide.
[♩ music ♩]
[Dr. Joe Hanson] Hey smart people. Joe here. Earth’s atmosphere and climate have changed in a big way, and they are continuing to change. There’s no doubt about that, and we’ve known it for decades. But Earth’s climate has always changed throughout its history. So how do we know this time is different? We know because at places like the Scripps Institution of Oceanography in southern California, we have freezers full of ancient ice that let us look into the past, thousands–even millions of years, and measure exactly what Earth’s atmosphere, and its climate, were like throughout deep history.
I recently stopped by to visit Dr. Jeffrey Severinghaus, who studies ice cores. He’s part of a team working to find the oldest ice on Earth. Each of these little blocks of frozen water can tell us something about our planet’s past, long before we existed – and where it’s heading, now that we do.
And inside these tiny bubbles in this ice, is old bubbles of air that existed on this planet as old as that ice is.
[Severinghaus] Yeah.
[Hanson] That’s the atmosphere of the planet, trapped in those little bubbles.
[Severinghaus] What happens in the polar regions is it’s too cold to melt. So when snow falls it doesn’t melt, it just piles up and piles up, and eventually turns into ice under its own weight. But if you think about what snow is like, if you have a snowflake you have air in between the snowflake. As snow becomes more and more dense, it tends to squeeze out the air between snowflakes, but it turns out it doesn’t squeeze out all the air.
[Hanson] As more layers of snow fall and condense, those tiny voids are literally frozen in time, layer upon layer. And, there are a lot of layers.
[Severinghaus] Some ice cores have annual layers just like trees do, you know how you can count tree rings? So some graduate student sits there and counts 50,000 annual layers. Of course it has to be a graduate student! What a lot of work.
[Hanson] But to study ancient ice, first you have to find ancient ice. Where are you doing this research? Where are you collecting these ice cores?
[Severinghaus] This is from a place called Taylor Glacier in Antarctica.
[Hanson] Taylor Glacier is a 54 kilometer stretch of ice and rock. People like Dr. Severinghaus can read it like a book–full of stories about our ancient climate. Taylor Glacier is special because it’s one of the few places on Earth where the ancient ice has risen to the surface.
[Severinghaus] So, you only have to drill 5-10 meters to get the ice. Which is much easier than drilling a deep ice core which is 3,000 meters and costs 50 million dollars.
[Hanson] It’s basically a cylinder that has little tiny teeth on the bottom. And when you rotate the barrel it carves out the ice, but only a little bit in a ring, and it leaves behind an ice core in the middle. Once the core is pulled up, it’s packed up and sent off, carrying a slice of history inside it.
[Severinghaus] It’s a slow process, it takes like a month for the ship to get here.
[Hanson] Whether you’re standing in the middle of the Amazon rainforest or at the North Pole, you’re breathing roughly the same air. Our atmosphere is pretty much the same everywhere. Which means that a tiny air bubble from that one spot is enough to paint a picture of what the entire planet’s atmosphere looked like so many years ago.
[Severinghaus] This is the freezer. We won’t be in there long, so don’t worry about the cold. So this is what a typical ice core sample looks like. Now you’ll notice that there’s no bubbles. That’s because when you get down below 600-700 meters, the pressure is so high that the air turns into something called a clathrate which is an ice-like substance.
[Hanson] Clathrates are crystals, where instead of bubbles, the molecules are trapped in a cage made by the bonds between frozen water molecules. There’s still gas in there.
[Severinghaus] There’s still gas molecules but they’re not in a gas phase.
[Hanson] Man the patterns are so cool, you must randomly see such cool ice phenomena. It’s cold in here! This cold!
[Severinghaus] Funny how that works.
[Hanson] Okay, but how do you get the ancient air out of the ice to measure it? I mean, without contaminating it with… all this air around us?
[Severinghaus] So this is how we actually extract the ancient air, if you will. We take a piece of ice and put it in a vacuum flask, and pump out all of the modern air, the air we’re breathing right now, using a vacuum line. This is a vacuum pump here. So we make a seal, and close this valve, and then you only have an ice cube and a little bit of water vapor, but no air. Then we melt the ice, and the melting of the ice releases those little air bubbles of ancient air.
[Hanson] So because you already let out the “now air,” the only gasses that are coming out are the ones that are trapped inside the ice.
[Severinghaus] Right, and then we can purify the gas a little bit by freezing the water.
[Hanson] So they pump out all the modern air, melt the ice to let the ancient atmosphere vaporize, re-freeze the water, and pump that ancient atmosphere out so it can be measured. This is a liquid helium tank?
[Severinghaus] It’s cold enough - it’s at 4 kelvin, 4 degrees about absolute zero. It’s cold enough that all the air actually condenses and turns into ice - air ice.
[Hanson] Every gas, will freeze.
[Severinghaus] Every gas except helium.
So then we take it over here. This is the analysis part of it. This tube is actually a bottle, a long skinny bottle that’s capable of dipping itself into the liquid helium.
[Hanson] You wouldn’t want to be getting your own hands too close to 4 kelvin.
[Severinghaus] No.
[Hanson] The frozen air gets put into this, a mass spectrometer, which basically measures the masses of really tiny things.
We measure the chemical composition of the atmosphere using isotopes: they’re like different flavors of atomic elements. Isotopes, those flavors of elements, have unique masses, and the mixture of them in the air bubbles can tell us all kinds of things about ancient earth.
[Severinghaus] We use the isotopes of nitrogen to tell ancient temperature at the time the snow was falling. Ordinary nitrogen has a mass of 14, but the rare isotope nitrogen 15 has a mass of 15. It turns out that relative proportions of N15 and N14 are sensitive to temperature.
[Hanson] So, whatever the temperature is at a particular time, it’s creating different mixes of different flavors of gasses in the atmosphere, like a fingerprint for temperature.
[Severinghaus] That’s right, and that’s trapped in air bubbles for posterity. So the sample here starts out waiting its turn and when its turn comes the sample opens and goes into this little tiny tube, which leads into the mass spectrometer, here, and it gets accelerated by a 3,000 volt electrical gradient, which makes the ions go really fast. And then they hit this magnet and they’re forced to make a 90-degree right turn, and in doing so, heavy things like N15 try to go straight, and lighter things like N14 get bent more.
[Hanson] It’s like being in a car. You can’t turn as fast in a big heavy car. So they swing out, and then the detector is seeing what swung out farther.
So, you’re getting resolution of things that differ by a single neutron when they’re flying through that curve? That’s pretty cool.
The same idea can be used to find out more than just temperature. Labs all over the world use elements trapped in air, trapped in ice cores, to paint a map from our distant past to today. Oxygen isotopes can tell us how oceans changed, mineral dust tells us about how the atmosphere moved around, there are chemical clues about early volcanoes. But maybe most importantly, we can trace changing levels of carbon dioxide.
So the climate has changed before, how do we know that this time it’s us?
[Severinghaus] The way we know, is just like we talked about with nitrogen, the carbon in carbon dioxide also has two flavors. There’s carbon 12, which is ordinary carbon, and then a very rare form of carbon, carbon 13. So, that’s how we know it’s human caused. The atmosphere, as it goes up in CO2 concentration, the carbon 13 of the atmosphere is taking a nosedive. And that’s not what would happen if it was natural CO2. Because fossil fuel CO2 is very depleted in carbon 13.
[Hanson] This comes from the fact that plants prefer to eat CO2 made of carbon-12, and when we burn fossil fuels made from those ancient plants, the fraction of carbon-12 in the atmosphere goes up while carbon-13 goes down. We’ve only been measuring carbon dioxide in the atmosphere since 1957, but using the data from ice cores, we can trace levels back way farther. And this is what we see:
[Severinghaus] CO2 was pretty flat for most of the past 1,000 years. All around 280 ppm. Now we’re going to add in the carbon 13 abundance, this gold line. And you can see that was also pretty constant for most of the last thousand years.
But then around 1850, right when carbon dioxide concentration started to rise, the carbon 13 abundance started taking a nosedive. And this kind of unambiguously tells you that humans did it. That’s why I call it the smoking gun of human causation. There are lots of other ways we know, but this is the simplest.
[Hanson] We’re moving into uncharted territory. The last time something like this shows up in the ice record is around 55 million years ago, when a volcano popped up under an oil field and cooked basically everything.
[Severinghaus] It sent all the carbon dioxide into the atmosphere. So, the carbon dioxide shot up, we think it nearly quadrupled, and the climate warmed by 6 degrees.
The most important thing is right away to solve this global warming problem. We don’t have much time left. We have to put aside all of our political differences, The health and wellbeing of the planet is so much more important than everything else. We can do this, I know we can.
[Hanson] We can. But will we? I hope so. Stay curious.
Many people think that climate change means warmer temperatures. But increasing temperatures are only the beginning of the story. Because the Earth is a system where everything is connected, changes in one area can influence changes in all others.
The consequences of climate change include, among others, intense droughts, water scarcity, severe fires, rising sea levels, flooding, melting polar ice, catastrophic storms and declining biodiversity.
People are experiencing climate change in diverse ways
Climate change can affect our health, ability to grow food, housing, safety and work. Some of us are already more vulnerable to climate impacts, such as people living in small island nations and other developing countries. Conditions like sea-level rise and saltwater intrusion have advanced to the point where entire communities have had to relocate, while protracted droughts are putting people at risk of famine. In the future, the number of people displaced by weather-related events is expected to rise.
Read more about climate change on the United Nations What is Climate Change page.
Crash Course What is Climate Change
What is Climate Change? (13:57)
Transcript: What is Climate Change? (13:57)
Our planet has been draped in ice sheets, filled with boiling-hot oceans, and dimmed by volcanic ash – all before anything more complicated than a single-celled organism showed up. So climate change is nothing new around here… when it happens gradually, over millions of years.
But something new has happened in the last few centuries. People like us…except, wearing hats like this… began burning fossil fuels like coal, oil, and natural gas to make energy. Most of us aren’t wearing hats like those anymore. But we’re still powering our daily lives and industries with those fuels, releasing billions of tons of carbon dioxide every year. And that’s caused Earth’s climate to change in the span of just a few human lifetimes, the geological blink of an eye.
Hi! I'm Dr. Sammy, your friendly neighborhood entomologist, and this is Crash Course Biology! Hey, do you guys smell that? …smells like... theme music?
[THEME MUSIC]
Now, I know what you’re thinking. “Wait, isn’t this Crash Course Biology?” And yeah, this episode is heavy on the gases, low on the golgi bodies. And that might leave you wondering, what does climate change have to do with the science of life?
Here’s the thing: life and climate are tied together, like that tangled pair of headphones at the bottom of your backpack. You know, like you tug one end and then a knot tightens, which is looped around a paperclip, somehow snagged on that tiny notebook where you drew hearts around your crush’s name, which after several tugs is now lying open on the floor and…I’m breaking into a cold sweat just thinking about it.
But back to the point, we can’t talk about life without talking about climate —which doesn’t mean last week’s thunderstorm or a one-day temperature swing – that’s weather. Climate is long-term weather conditions averaged over many years. To understand the difference between them, just remember that knowing the weather will help you decide if you should grab an umbrella before you head out, but knowing the climate will help you decide if you should invest in a good air conditioner.
While the weather might impact your choice of clothing for the day, the climate directly impacts where and when different kinds of life can survive.
The Greenhouse Effect
We owe today’s climate to the fact that our little green-and-blue marble of a home isn’t just floating in space unprotected. It’s wrapped up in an atmosphere; a big, invisible, gassy jacket. Which, granted, sounds pretty weird when you put it that way. But without it, we wouldn’t exist.
This jacket is made of different kinds of gases. And a small fraction of them, known as greenhouse gases, absorb solar energy like, super well. We’re talking about gases like methane, water vapor, and most importantly carbon dioxide – also known as CO2. They account for less than half of one percent of our atmospheric jacket. But they’re a part of what makes it so good at trapping heat, sort of like all the little white feathers in your puffy coat.
When sunlight beams down from space, most of it travels through those gases with no problem. The energy from that sunlight gets absorbed as it strikes the
Earth, warming the surface. That type of warming is normal and seasonal. The Earth naturally bounces some of that solar energy back toward space. Where some of it exits the atmosphere and heads right back out into the inky ether.
But the rest of that energy gets trapped by the Earth’s gassy jacket. Specifically by those super absorbent greenhouse gases, which suck up heat and bounce itback down to us again. This warming process is called the greenhouse effect. Unsurprisingly, It works the same way as a greenhouse – using layers of glass to trap heat inside. And it keeps Earth at a nice, cozy, insulated average of 14 degrees Celsius.
Without it, our Earth would be a chilly average of -18 degrees Celsius. Great for storing ice cream! Not so good for rainforests, swimsuits, or us for that matter. So, the greenhouse effect is a natural, helpful process that makes Earth habitable for all of life!
But you can have too much of a good thing. When our atmospheric jacket contains more carbon dioxide, for example, it gets really good at trapping heat. Like, too good. And the hotter things get, the more water evaporates and joins the atmosphere—and remember, water vapor itself is a greenhouse gas, so that in turn absorbs even more heat, creating a looping system of cause-and-effect that just keeps reinforcing itself.
Measuring the Greenhouse Effect
And while dressing in layers is great if you’re hiking in the Alps, it’s really hard for our planet to shed its extra coats. So all of that heat gets stuck going from the ground to the atmosphere like the worst game of hot potato ever played.
When I learned about this, I was like, "Wow, what a revelation! I can’t believe we’ve only recently figured this out!" But it turns out that this isn’t new knowledge; we’ve known how, and why, this could happen for nearly 170 years.
Let’s pay a visit to the Theater of Life… [Inquisitive music] Back in 1856, Eunice Foote, an American scientist and suffragette, was thinking about how the Sun’s warmth affected different gases. In those days, the scientific community was a bit like a fort with a handmade “no girls allowed” sign out front. But Foote wasn’t deterred, and ran her experiments anyway.
She filled tubes with different combinations of gases, including carbon dioxide. After putting some tubes in the Sun and some in the shade, she compared their temperatures, trying to find the hottest gas. All the tubes in direct sunlight warmed up. But none as intensely as the tube that contained carbon dioxide. The temperature had soared to 51.7 degrees Celsius, hot enough to burn your fingers.
From that insight, Foote theorized that if our atmosphere ever contained more carbon dioxide, the whole planet would warm up as a result, which would mean a lot more than a few scalded fingers. And sure enough, today, that’s exactly the situation we’re in.
Foote was one of the first scientists to recognize carbon dioxide’s potential to affect Earth’s climate. But she wasn’t the only one to connect the dots. For example, just a few decades later, another scientist named Dr. Svante Arrhenius observed that burning coal releases carbon dioxide. As a fossil fuel, coal forms from the decomposed, carbon-based bodies of plants and animals that lived and died a long time ago. And I’m talking before the dinosaurs. So no, I’m afraid that means you aren’t gassing up your car with the remains of a T-Rex.
When we burn those fossil fuels—whether it’s in the form of coal, oil, or natural gas—carbon dioxide gets released into the atmosphere. When Arrhenius ran the numbers, he predicted that carbon dioxide released by burning fossil fuels could warm our climate within a few thousand years if we kept burning them at their current rate. But we’ve far outpaced his estimates.
Our emissions of carbon dioxide have grown and grown and grown — and so has the mountain of evidence that those emissions are warming our planet. Some oil and gas companies have worked to promote uncertainty around the existence of climate change and what’s causing it. While they have only very recently acknowledged its existence, as of 2023, they're still trying to deflect from what's causing it. But the scientific consensus on this is overwhelming. You can learn much more about that in our Climate & Energy series.
We’ve only been reliably taking direct measurements of Earth’s global temperature since the 19th century. But that measly slice of time shows a steady rise in temperature of about 1.1 degree Celsius since 1880. And we know that that’s unusual because we’ve learned to read Earth’s much longer climate diary, in the form of ice cores.
See, when snow hardens into ice, tiny bubbles of air remain trapped in the gaps between snowflakes. These gases and water molecules stay frozen, like entries in a frosty journal. So by drilling deep down into polar ice, we can snoop on what the atmosphere was like hundreds of thousands of years ago.
Carbon Sinks
Ice cores show us that carbon dioxide levels have fluctuated over the past 800,000 years. And temperatures have fallen and risen alongside them, too. But when people started burning fossil fuels, carbon dioxide levels began to spike quickly, like really, really quickly. And they haven’t stopped rising.
Before the Industrial Revolution, for every million molecules of air in our atmosphere, around 280 were carbon dioxide molecules. But by 2022, that number had increased to 422 —the highest concentration of CO2 our planet has seen in 4 million years.
And that surge in carbon dioxide affects more than just the temperature. As the amount of carbon dioxide in our atmosphere rises, it impacts all of Earth’s systems. Just like yanking on the end of that tangled mess of headphones impacted all of the other items in my bag (and eventually, everybody around us when stuff started falling out). It’s all connected, is what I’m saying.
For example, the ocean is our planet’s largest carbon sink. It’s sort of like a big storage container for carbon. In fact, the ocean holds 50 times more carbon than the air or soil do. But a chemical reaction happens when carbon dioxide meets water, it creates an acid. So that influx of carbon has already turned the ocean 30% more acidic since the 19th century.
As carbon dioxide and other greenhouse gases trap more heat, there’s more energy pouring into our planet than going out. That means more energy is pumped into the ocean, fueling hurricanes and typhoons to become more frequent and more intense.
Environmental Justice
As the whole planet gets hotter, that triggers all kinds of changes. Spring arrives earlier, leading to shorter winters and longer summers. Rising temperatures lead to double-whammy droughts and heatwaves. And that leaves forest floors full of dried-up plants that serve as fuel for wildfires to ignite—spreading faster, farther, and more often.
Plus, Earth’s polar ice caps are melting, transforming solid ice to slush and seawater. And that’s causing ocean levels to rise and encroach on land. So while some communities are already facing a problem of not enough water, others are facing a problem of too much.
And because these adverse changes layer on top of existing social inequalities, they disproportionately affect lower-income communities and people of color, making climate change not only a scientific issue, but a matter of environmental justice that has spurred some researchers to political action.
For example, climate scientist Nicole Hernandez Hammer witnessed first-hand, through her field research, the sea-level rise alongside Miami Beach’s Latino communities. But these communities were not included in conversations about climate change or the dangers of rising sea levels. So, Hammer took action, moving into environmental outreach and education.
And, while the threat is still there, these communities are now in conversation about climate change, and able to plan and advocate for the future of their environment. And the good news more broadly is we know exactly why these tangled, complex effects are happening.
The more we burn those fossil fuels, the more greenhouse gases we release —and that’s driving sweeping changes all over our planet. And these changes are impacting life at all levels from the tiniest bacterium, to the elephants of Botswana, to you and me.
We can slow these impacts by breaking up with fossil fuels. But we also have to invest in nature’s carbon sinks —such as soils and forests— which pull carbon out of the atmosphere and back into the land, where it can’t keep heating things up.
Review & Credits
It won’t be the easiest breakup. We’ve designed whole societies and global systems around fossil fuels. We should fully expect to be listening to Jazmine Sullivan on repeat with a gallon of Rocky Road. But this is one relationship we can't afford to stay in.
So, in order to halt emissions, we have to both invent new systems and work more efficiently within old ones, and to do that, we’ve got to get a whole planet’s worth of people on board. And if you’ve ever been part of a group project, you know that last part isn’t easy.
Thankfully, when faced with global crises, humans have one great thing going for us: we are creative. I mean, we’ve been to space, we’ve got electric cars, we made furbies for some reason. So yes, It’s going to take all of our creativity and cooperation to tackle. But the only way out is through, and the only way through is together.
In our next episode, we’ll tune back into the world of living things— and see how our rapidly changing climate involves much more than the atmosphere. It affects every living, breathing, organism on this planet— including you and me.
This series was produced in collaboration with HHMI BioInteractive. If you’re an educator, visit BioInteractive.org/CrashCourse for classroom resources and professional development related to the topics covered in this course.
Thanks for watching this episode of Crash Course Biology, which was filmed at our studio in Indianapolis, Indiana, and was made with the help of all these nice people. If you want to help keep Crash Course free for everyone, forever, you can join our community on Patreon.
Climate Change Solutions
Since climate change is a worldwide problem that requires international cooperation. It will affect everyone, although the impacts of climate change are more readily seen in island populations as sea levels rise.
Paris Agreement is an agreement signed in 2015 at the UN Climate Change Conference (COP 21) in Paris. This agreement set long term goals to guide all nations to
- Reduce Global Greenhouse Emissions to hold global temperatures to well below 2°C above pre-industrial levels.
- Periodically assess the collective progress towards meeting long term goals
- Provide financing to developing countries to mitigate climate change, strengthen resiliency and adapt to climate impacts
What is the Paris Agreement (1:39)
Transcript: What is the Paris Agreement (1:39)
[Presenter] What is the Paris Agreement?
The Paris Agreement is a legally binding international treaty on climate change, to limit global warming to well below 2, preferably to 1.5 degrees Celsius compared to pre-industrial levels. This requires economic and social transformation to face the climate challenges now and moving into the future, based on the best available science.
The Paris Agreement works on a 5 year cycle of increasingly ambitious climate action. By 2020, countries communicate their plans, known as "nationally determined contributions". Countries communicate actions they will take to reduce the greenhouse gas emissions in order to reach the goals of the Paris Agreement. Countries also communicate actions they will take to build resilience to adapt to the impact of rising temperatures. This may include information on adaptation and finance flows.
The Paris Agreement also provides a framework for financial, technical, and capacity-building support to those countries who need it. Starting in 2024, Countries report transparently on actions taken. Collective progress under the Paris Agreement will be assessed through a global stocktake. This will lead to recommendations for countries to set more ambitious plans in the next round.
5.5 Past Pollutant Problems and Solutions
5.5 Past Pollutant Problems and SolutionsIt’s easy to feel overwhelmed by the environmental impacts of energy production, but history shows that meaningful progress is possible. Throughout the 20th century, scientists and policymakers collaborated to solve several major environmental crises; issues that once dominated the headlines but are rarely discussed today. These success stories demonstrate how science and policy, when working together, can drive real, lasting change.
5.5.1 Acid Rain
5.5.1 Acid RainAcid rain is a serious environmental problem around the world, particularly affecting Asia, Europe, and large parts of the U.S. and Canada. The acidic pollutants such as SO2 and NOx are emitted into the environment by combusting fossil fuels.
Most of the sulfur in any fuel combines with oxygen and forms SO2 in the combustion chamber. This SO2, when emitted into the atmosphere, slowly oxidizes to SO3. SO3 is readily soluble in water in the clouds and forms H2SO4 (sulfuric acid).
Most of the NOx that is emitted is in the form of NO. This NO is oxidized in the atmosphere to NO2. NO2 is soluble in water and forms HNO3 (nitric acid).
Pure water has a pH of 7.0. Normal rain is slightly acidic because carbon dioxide dissolves into it, so it has a pH of about 5.5. As of the year 2000, the most acidic rain falling in the US has a pH of about 4.3. By the 2020's most locations of the US have precipitation with pH of 5.0-5.5.
Below is a video demonstration that replicates the effect of acid rain on plant life. In this video, beans are placed in: a) water, b) slightly acidic water and c) acidic water, and their growth is observed over a period of three days. Please watch the following 5:35 video:
Acid rain looks, feels, and tastes just like clean rain. The harm to people from acid rain is not direct. Walking in acid rain, or even swimming in an acid lake, is no more dangerous than walking or swimming in clean water. However, the pollutants that cause acid rain also damage human health.
- Effects of Sulfur Dioxide (SO2): These gases interact in the atmosphere to form fine sulfate and nitrate particles that can be transported long distances by winds and inhaled deep into people's lungs. Fine particles can also penetrate indoors. Many scientific studies have identified a relationship between elevated levels of fine particles and increased illness and premature death from heart and lung disorders, such as asthma and bronchitis.
- Effects of Nitrogen Oxide (NOx): Decrease in nitrogen oxide emissions are also expected to have a beneficial impact on human health by reducing the nitrogen oxides available to react with volatile organic compounds and form ozone. Ozone impacts on human health include a number of morbidity and mortality risks associated with lung inflammation, including asthma and emphysema.

Text description of the Annual Wet Sulfate Deposition image.
The image is a comparison of two maps of the United States showing annual wet sulfate (SO₄²⁻) deposition over two different time periods, 1989-1991 and 2020-2022. Each map displays the continental U.S. with color gradients representing the levels of sulfate deposition.
On the left, the map from 1989-1991 shows high levels of sulfate deposition concentrated mostly in the eastern and central regions, especially pronounced in the Ohio Valley and surrounding areas, depicted in dark red and orange, indicating higher levels. The western regions are shown in lighter greens and yellows, indicating lower levels of deposition.
On the right, the map from 2020-2022 has a more uniform teal color across the entire country, suggesting significantly reduced sulfate deposition levels compared to the earlier period. This illustrates a substantial improvement in air quality over time.

Text description of the Annual Sulfur Dioxide Emissions image.
The image is a bar and line graph titled "Annual Sulfur Dioxide Emissions, 1990–2020." It displays data on sulfur dioxide emissions and gross electricity generation in the United States over the period of 1990 to 2020. The vertical axis on the left measures sulfur dioxide emissions in million short tons, ranging from 0 to 17.5, while the right vertical axis measures gross generation in billion megawatt-hours (MWh), ranging from 0 to 3.5. The bars in blue represent the sulfur dioxide emissions for each year, starting at 15.73 million short tons in 1990 and decreasing to 0.79 million short tons in 2020. The green line indicates gross generation, which shows a generally increasing trend from 1990 until around 2008, then slightly decreasing towards 2020. The graph includes a note that data for sulfur dioxide emissions from 1991 to 1994 are not available.
| Year | Sulfur Dioxide (million short tons) | Gross Generation (Billion MWh) |
|---|---|---|
| 1990 | 15.73 | |
| 1991 | ||
| 1992 | ||
| 1993 | ||
| 1994 | ||
| 1995 | 11.83 | |
| 1996 | 12.51 | |
| 1997 | 12.94 | 2.25 |
| 1998 | 13.09 | 2.34 |
| 1999 | 12.45 | 2.39 |
| 2000 | 11.20 | 2.49 |
| 2001 | 10.64 | 2.46 |
| 2002 | 10.20 | 2.48 |
| 2003 | 10.59 | 2.53 |
| 2004 | 10.26 | 2.58 |
| 2005 | 10.22 | 2.74 |
| 2006 | 9.39 | 2.72 |
| 2007 | 8.93 | 2.83 |
| 2008 | 7.62 | 2.78 |
| 2009 | 5.82 | 2.65 |
| 2010 | 5.17 | 2.80 |
| 2011 | 4.55 | 2.73 |
| 2012 | 3.32 | 2.71 |
| 2013 | 3.24 | 2.69 |
| 2014 | 3.16 | 2.70 |
| 2015 | 2.22 | 2.66 |
| 2016 | 1.49 | 2.59 |
| 2017 | 1.34 | 2.49 |
| 2018 | 1.26 | 2.61 |
| 2019 | 0.97 | 2.53 |
| 2020 | 0.79 | 2.38 |
5.5.2 Hole in the Ozone Layer
5.5.2 Hole in the Ozone LayerThe earth’s ozone layer protects life from harmful radiation from the sun. Ozone is comprised of three oxygen molecules bonded together. Without this layer of protection, too much UV light would hit the earth’s surface, resulting in damage to crops and increased skin cancer and cataract rates in humans.
In the 1970’s scientists discovered that some chemicals such as: chlorofluorocarbons (CFCs), hydrochlorofluorocarbons (HCFCs), carbon tetrachloride, and methyl chloroform were depleting the ozone layer. These chemicals were often found in refrigerants, fire suppressants, foam insulation and aerosols.
In 1985 the Vienna Convention on the protection of the ozone layer formalized international cooperation to find a solution. The Montreal Protocol on Substances that Deplete the Ozone Layer was an international agreement signed in 1987 which phased out the use of these ozone depleting chemicals on a global scale. The positive impact of this international agreement is why many of you may have never heard of the hole in the ozone layer. For earlier generations (those born in 1970-1990s) would have grown up learning about this in environmental issue beginning in elementary school. Thanks to the Montreal Protocol and international cooperation, the hole in the ozone layer is on track to be fully recovered by 2040.
2025 Ozone Hole Update (0:48)
Note: The video has music in the background but no spoken words.
Transcript: 2025 Ozone Hole Update (0:48)
[Background music]
[Transcribed Text]
This year, the ozone hole over Antarctica reached its annual maximum extent on September 9th, 2025, with an area of 8.83 million square miles (22.86 million square kilometers.)
The average size of the ozone hole between September 7 and October 13 this year was the 5th-smallest since 1992— when the Montreal Protocol began to take effect.
NASA and NOAA previously ranked ozone hole severity using a time frame dating back to 1979, when scientists began tracking Antarctic ozone levels with satellites. Using that longer record, this year’s hole area ranked 14th smallest over 46 years of observations.
The annual maximum extent of the ozone hole can vary year to year due to weather, but the multi-decadal record shows that the ozone layer appears to be slowly recovering and is on track to rebound by later this century.
5.5.3 Lead (Pb)
5.5.3 Lead (Pb)Lead was added to gasoline in the 1920’s to reduce “knocking” and improved fuel efficiency. But lead proved to be a toxic pollutant, having a major effect on the cognitive development of children. Many countries began phasing out the use of leaded gasoline in the 1970s, which is why you still find signs indicating “unleaded gasoline” at the gasoline pump today. Japan was the first country to entirely ban leaded gasoline in 1986. The US and Canada banned it in 1996.
For more information on the phase of Lead in gasoline: Please read this article.
Did you know, Algeria was the last country to finally ban leaded gasoline, but it wasn’t until 2021!
Use the slider at the bottom of the Map to see how and when lead was phased out of on road fuels!
5.6 Nuclear Waste
5.6 Nuclear WasteNuclear power plays a significant role in the U.S. energy mix, providing about 18–19% of the US’s electricity in 2024, and roughly 9–10% of global electricity generation
Like coal or natural gas plants, nuclear facilities generate electricity by heating water to create steam that spins a turbine. The key difference is the heat source: nuclear plants use fission—splitting atoms of uranium or plutonium—rather than burning fossil fuels. This process produces no direct carbon emissions during operation, but it does generate radioactive waste, primarily in the form of spent nuclear fuel rods that remain hazardous for thousands of years.
In the United States and most countries, spent nuclear fuel is not recycled. While reprocessing—chemically separating usable materials from waste—is technically feasible and practiced in a few nations like France, the U.S. has maintained a policy against commercial reprocessing since 1977 due to cost, proliferation concerns, and technical challenges
As a result, spent fuel is treated as high-level waste and must be safely stored until its radioactivity decays to safe levels. Radioactive materials are classified by hazard: low-level waste (contaminated tools, clothing) requires minimal shielding, while high-level waste (spent fuel) demands robust, long-term isolation. Because some isotopes have half-lives spanning millennia—meaning it takes that long for half their radioactivity to decay—storage solutions must be secure for geological timescales.
Currently, all commercial nuclear waste in the U.S. is stored on-site at power plants. After removal from reactors, spent fuel rods are first cooled in water-filled pools for several years. Once sufficiently cooled, they are transferred to dry cask storage: sealed steel cylinders encased in concrete or steel structures, designed to withstand earthquakes, floods, and other hazards

These casks are monitored and maintained above ground, with the expectation that a permanent deep geological repository—such as the long-proposed Yucca Mountain site—will eventually provide a final solution. However, political and technical debates have delayed such a facility for decades, leaving interim storage as the de facto national strategy.
Even with secure containment, nuclear waste management raises important questions about intergenerational responsibility, environmental justice, and energy policy trade-offs. While nuclear power offers reliable, low-carbon electricity, its waste legacy requires careful planning, transparent decision-making, and sustained investment. As we evaluate energy options for a sustainable future, understanding both the benefits and challenges of nuclear power—including how we steward its waste—is essential for informed citizenship and engineering innovation.
5.7 Water Use in Energy Production
5.7 Water Use in Energy ProductionWater and energy are deeply interconnected in what scientists call the water-energy nexus. In the twentieth century alone, global energy use grew ten-fold while water use grew six-fold, and both continue to rise with population growth and increasing affluence. Understanding water use in electricity generation requires distinguishing between water withdrawal (water removed from a source) and water consumption (water that is evaporated, transpired, or otherwise not available for immediate reuse). Electricity is the fastest-growing form of energy, making water consumption across different generation methods—typically measured in liters per megawatt-hour (L/MWh)—a critical metric for sustainable energy planning.
The water intensity of electricity generation varies dramatically across different technologies. Wind and solar photovoltaic (PV) systems have the lowest water consumption because they require no cooling; their minimal water use occurs upstream during mining and manufacturing of components, plus occasional panel cleaning. In contrast, thermal power plants (coal, natural gas, nuclear, and biomass) require substantial water for cooling, depending on the cooling technology. Hydropower and biomass show the widest ranges: hydropower averages can appear high due to reservoir evaporation, while biomass water use depends heavily on whether feedstock crops are rain-fed or irrigated.
For thermal power plants, which account for over 70% of utility-scale electricity generation, the cooling system type is the primary determinant of water use. Once-through cooling draws water from rivers or lakes, passes it through the plant once, and returns it—resulting in high withdrawal but relatively low consumption. However, this method creates thermal pollution, returning water at higher temperatures that reduces oxygen levels and severely disrupts aquatic ecosystems. Wet cooling (recirculating) systems use cooling towers where heat dissipates through evaporation, reducing withdrawal but increasing consumption as water is lost to the atmosphere. Dry cooling systems use no water for cooling, relying instead on air conduction and convection, but they are more expensive and less efficient than wet systems.
Hydropower and biomass present unique water challenges. While water flowing through hydroelectric turbines isn't considered consumptive (it remains available downstream), large reservoirs significantly increase surface area and evaporation rates, creating consumptive losses that vary widely by location and climate. Similarly, biomass electricity consumes substantial water through crop irrigation, plant transpiration, and processing—with irrigated crops using dramatically more water than rain-fed alternatives. These site-specific factors make average water consumption estimates for both hydropower and biomass highly variable and context-dependent.
Even when water isn't consumed, energy production still impacts the environment. Thermal power plants using once-through cooling return warmed water to rivers and lakes, creating thermal pollution that degrades aquatic habitats. Nuclear plants are often sited near large water bodies specifically to access cooling water, concentrating environmental impacts in those ecosystems. As climate change intensifies droughts and water scarcity, the water-energy nexus becomes increasingly critical: choosing low-water technologies like wind and solar PV isn't just about reducing emissions—it's about building resilient energy systems that can operate sustainably in a water-constrained future.
5.8 Conclusion
5.8 ConclusionAs we’ve explored in this lesson, every energy source carries environmental trade-offs. Fossil fuel combustion releases pollutants that impact air quality, human health, and global climate. Thermal power plants draw and consume vast quantities of water, with cooling system choices dramatically shaping local ecosystems. Nuclear power offers reliable, low-carbon electricity but requires secure, long-term management of radioactive waste. And while renewables like wind and solar PV minimize operational water use and emissions, their manufacturing, land use, and material supply chains still carry environmental footprints. The key insight isn’t that any single technology is perfect, but rather that informed energy decisions require weighing impacts across multiple dimensions.
Yet this lesson also demonstrates that environmental challenges are not insurmountable. The successful global phaseout of ozone-depleting chemicals and the dramatic reduction of acid rain-causing sulfur emissions prove that science, technology, and coordinated policy can drive real progress. These achievements weren’t built on waiting for flawless solutions—they emerged from iterative innovation, regulatory frameworks, and public engagement. Today, that same collaborative approach is guiding efforts to decarbonize grids, deploy water-smart cooling systems, advance nuclear waste stewardship, and scale renewable integration.
As you move forward in this course, keep the water-energy-emissions-waste nexus in mind. Energy choices ripple through ecosystems, economies, and communities, and understanding those connections is essential for designing resilient, equitable systems. In our next unit, we’ll shift from assessing impacts to exploring energy efficiency and demand-side solutions—because the cleanest, most affordable, and lowest-impact energy is often the energy we never have to generate. Reflect on how the trade-offs we’ve discussed might shape infrastructure planning, policy debates, or your own career path in the evolving energy sector.