I. The Air is Made of Life
II. What the Air Is Now
III. The Ocean of Air, and Its Weight
IV. The Great Heat Engine
V. The Air and You
VI. Cross-Links
Temperature, weather, air currents, and pressure, and how the atmosphere itself was made by life.
Of all the aspects of the biosphere, the air is the most intimate. You are immersed in it now, exchanging it with the world every few seconds, and you cannot stop for more than a couple of minutes without dying. The boundary between the atmosphere and your bloodstream is a film of moist tissue in your lungs thinner than a page, across which the outside world becomes, breath by breath, the inside of you. There is no better illustration of the open-system idea than this: the air is not around you; it is passing through you, continuously, your whole life. This page is about what that air is, where it came from, and how it moves, because all three turn out to be stranger and more alive than they first appear.
Start with the fact that overturns the intuition that the atmosphere is just an inert backdrop: the air you breathe is largely a product of living things, and for most of Earth’s history, it would have killed you.
When the Earth formed, its early atmosphere had essentially no free oxygen. It was a mixture of volcanic gases (carbon dioxide, nitrogen, water vapour, methane, and others), and any organism breathing today’s air dropped into that world would suffocate at once. For the first roughly two billion years of life, the planet’s organisms were adapted to that oxygen-free world, drawing energy from chemical reactions and, eventually, from sunlight, without releasing oxygen.
Then came one of the most consequential events in the planet’s history, introduced in Life Origins: some bacteria evolved a new trick, photosynthesis of the kind that splits water and releases oxygen as waste. Oxygen is chemically aggressive; it reacts with and damages the machinery of cells not adapted to it. As these photosynthesising organisms multiplied, they began pumping out oxygen, and around 2.4 billion years ago its concentration in the atmosphere rose sharply, an episode called the Great Oxygenation Event. For the existing life of the time, this was not a gift. It was a catastrophe, very possibly the largest mass poisoning in the history of the planet, as a waste product flooded the world and killed off vast swathes of organisms that had no defence against it. We sometimes call it the Oxygen Catastrophe: the breathable air that now sustains nearly all complex life began as lethal pollution, produced by organisms as a waste product.
But that oxygen also opened a door. Oxygen-based metabolism yields far more energy than the alternatives, and the organisms that learned to use it rather than be destroyed by it gained access to a powerful new energy supply, which (as Energy Factories described) helped make complex, large, energy-hungry life possible. Every breath you take is drawing on that ancient bargain: the same molecule that poisoned the early world is the one your mitochondria use to extract the energy that keeps you alive. The atmosphere, in other words, is not a fixed stage that life happens to perform on. It is something life built, catastrophically and over billions of years, and is still maintaining. The oxygen would vanish from the air in a geological eye-blink if photosynthesis stopped. You are breathing the exhalation of the planet’s plants and algae, kept topped up moment by moment by living things.
Today’s air settled into a relatively stable mixture: roughly 78 percent nitrogen, 21 percent oxygen, just under 1 percent argon, and a small but enormously important remainder of trace gases, including carbon dioxide, water vapour (which varies a great deal), and others. The proportions matter more than their smallness suggests.
The oxygen is the obvious one, the fraction your metabolism runs on. The nitrogen, though you breathe it in and straight back out, is the vast reservoir from which living things (with the help of specialised bacteria) draw the nitrogen for proteins and DNA, a cycle as essential to you as the oxygen one. And the trace gases, carbon dioxide chief among them, punch far above their concentration: carbon dioxide is the raw material that plants build food from, and it is also, with water vapour, one of the gases that trap heat and keep the planet warm enough for liquid water. That last function is the basis of the climate concern that runs through this section: a gas present in a fraction of a percent of the atmosphere regulates the temperature of the entire planet, which is exactly why changing its concentration, even slightly, has outsized effects. The greenhouse effect itself is not controversial and not new; it is basic, well-established physics, and without it the Earth would be frozen. What is at issue, taken up where it belongs in Our Technological History, is the consequence of raising that concentration rapidly. However, to make things even more complicated, we also need to acknowledge when the concept of climate change is being weaponised by power-hungry psychopaths for global control.
We rarely notice that air has substance, but it does. You are living at the bottom of an ocean of it, kilometres deep, and its weight presses on you from all sides at roughly a kilogram of force on every square centimetre of your body. You do not feel crushed because the same pressure exists inside you, pushing out, in balance. This is atmospheric pressure, and it is not a constant backdrop; it shifts with weather and, more dramatically, with altitude.
As you climb, there is less air above you, so the pressure drops and the air thins. The proportion of oxygen stays the same, but each breath contains fewer molecules of it, which is why high altitude leaves you breathless and why mountaineers near the highest peaks need bottled oxygen. The body can adapt to moderate altitude over weeks (making more red blood cells to carry oxygen more efficiently, among other changes), and populations who have lived at high altitude for many generations, in the Andes, the Ethiopian highlands, and especially the Tibetan plateau, carry genetic adaptations that let them thrive where lowlanders struggle. The Tibetan adaptations in particular are one of the more clearly documented cases of recent, rapid human evolution in response to the environment, which ties back to the point made in The Sapiens Rabbit Hole that we are still very much an evolving animal. Pressure changes are also part of why some people feel weather in their bodies; shifts in barometric pressure can genuinely affect joints, sinuses, and headaches in some individuals, though the size and reliability of the effect vary.
Now to why the air moves at all, which is the foundation of weather, climate, and the distribution of life across the planet. The answer is the Sun, and the air is best understood as the working fluid of a vast solar-powered heat engine.
The Sun heats the Earth unevenly. The equator, where sunlight strikes most directly, receives far more energy than the poles, where it arrives at a glancing angle. This uneven heating is the engine’s fuel. Warm air at the equator expands, becomes less dense, and rises; cooler air flows in to replace it; the risen air spreads toward the poles, cools, and sinks. The whole atmosphere is, in essence, a system for moving heat from where there is too much of it (the tropics) toward where there is too little (the poles), and the wind is that redistribution in motion. This is the entropy story from Entropy at planetary scale: concentrated solar energy arrives, drives the churning of the atmosphere as it spreads out, and radiates back to cold space as dispersed heat. Weather is what the dispersal looks like from inside it.
The rotation of the Earth complicates this simple picture because it shapes where everything lives. A spinning planet deflects moving air (an effect called the Coriolis effect), breaking the simple equator-to-pole flow into bands of circulating cells and prevailing winds. These create the planet’s great climate zones: the wet tropics where the rising equatorial air dumps its moisture as rain, the bands of desert around 30 degrees north and south where that air descends dry (the Sahara, the Australian outback, and most of the world’s great deserts sit in these bands), the temperate zones with their shifting weather, and so on. The reason rainforests and deserts sit where they do, and therefore where dense human populations could and could not easily live, traces directly back to this solar heat engine and the planet’s spin. The distribution of human civilisation is, in part, a map of atmospheric circulation.
High in this system run the jet streams, fast rivers of air that steer weather systems, and the slower churning of these patterns is what we experience as the daily and seasonal drama of weather. The fundamental difficulty with weather, and the reason forecasts degrade beyond a week or so, is that the atmosphere is a complex nonlinear system of exactly the kind described in Emergence & Complexity: tiny differences in starting conditions balloon into large differences in outcome. This is a deep property of the system itself, the original “butterfly effect.” It is worth distinguishing this clearly from climate, a confusion that causes endless trouble: weather is the system’s short-term, chaotic, unpredictable behaviour, while climate is its long-term statistical average, which is far more predictable. That a particular forecast is uncertain says nothing about whether the long-run averages are shifting, in the same way that not being able to predict a single coin toss says nothing about your confidence that a weighted coin will trend toward one side over many throws.
The most direct effect of air on the human body is breathing itself, developed practically in Breathing. Every cell you have runs on the oxygen pulled from the air and disposes of carbon dioxide back into it; you are a node in the planet’s gas exchange, the same oxygen-and-carbon cycle that runs through the forests and oceans running through you on a timescale of seconds. The composition and quality of the air you breathe are therefore not a small matter. Air pollution, the introduction of particulates and reactive gases largely from burning fuels, has well-documented effects on respiratory and cardiovascular health.
Temperature and season reach you too. Your body is built to thermoregulate within a fairly narrow range, work taken up in Thermoregulation, and the air is the medium with which it does much of that exchange. Seasonal shifts in light and temperature measurably affect mood, sleep, and energy in many people; the winter dip in mood that some experience is a genuine, if variable, phenomenon tied largely to reduced light, which connects to the circadian biology in Sleep & Circadian Rhythm. The felt sense that you are a different person in high summer than in deep winter is not imagination; you are an organism tuned to a cycling environment, and the cycle runs partly through the air.
There is a temptation, when drawing these connections, to claim that particular weather patterns, ionisation states, or atmospheric subtleties have large and specific effects on health and mood. Some of these ideas have a kernel of evidence and the honest approach is to hold the well-established connections firmly (oxygen, air quality, light, temperature, pressure at altitude) while treating the more exotic claims as interesting and unproven rather than established. These are topics for the Rabbit Hole.
Step back and the air resolves into something remarkable: a thin, restless, life-made shell, churned by the Sun into the patterns we call weather, distributing heat and water across the planet and thereby deciding where life can flourish, and passing through your lungs every few seconds as the most continuous and intimate exchange you have with the rest of the world. We talk about the environment as though it begins at the skin. The air makes a mockery of that. It is outside you and inside you at once, and the difference between the two is only a matter of timing.
Bryson, B. (2003). A short history of nearly everything. Broadway Books.
Lane, N. (2002). Oxygen: The molecule that made the world. Oxford University Press.
Canfield, D.E. (2014). Oxygen: A four billion year history. Princeton University Press.
Walker, G. (2007). An ocean of air: Why the wind blows and other mysteries of the atmosphere. Harcourt.
Dessler, A.E. (2022). Introduction to modern climate change (3rd ed.). Cambridge University Press.