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THE UNIVERSE ESSAY · PERSONAL VIEW

Night Is Just Earth’s Shadow, and We Are Stardust

Two ordinary truths—the turning of Earth and the atoms inside our bodies—can make the sky feel much closer than it did before.

“Day and night do not really exist,” I once said.

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View from the International Space Station of Earth's curved surface, split between light and dark. A bright blue horizon and sunlit clouds at the upper right fade into deep shadow at the lower left, with golden solar panels along the right edge.
About this picture

Earth’s day–night line, photographed from the International Space Station.

NASA/Christina Koch, via Wikimedia Commons · Public domain · Image source ↗

My daughter would probably answer, “What? What? What?”

Of course day and night exist as human experiences, timekeeping words, and powerful parts of culture. My point is physical: the Sun does not turn off, rise, or set. Earth turns.

What we call night is the period when our part of the planet has rotated into Earth’s own shadow.

That may sound obvious. Sometimes the obvious becomes new again when we change the angle from which we see it.

The Sun does not stop shining on Earth

Sunlight reaches one half of Earth at every moment. The other half faces away.

So instead of picturing the Sun “going down,” picture the ground beneath you rotating until your part of the planet turns its back to the Sun.

Stand outside facing the sunlight. Then turn around.

You did not make the Sun disappear. You changed your orientation to it.

Earth does the same thing on a planetary scale.

The Sun will continue shining for billions of years. What changes every twenty-four hours is which part of our rotating world receives its light directly.

Language preserves older appearances. We still say sunrise and sunset even though the Sun is not circling us each day. There is nothing wrong with those words. They are beautiful and useful. But remembering the motion behind them can make an ordinary evening feel like astronomy.

What space makes easier to see

At the poles, the everyday meaning of day and night becomes less familiar. Near the North Pole, the Sun can remain above the horizon for months during the warmer part of the year and below it for months during the colder part.

Astronauts on the International Space Station orbit Earth roughly every ninety minutes. They can see about sixteen sunrises and sixteen sunsets during one Earth day.

From orbit, the boundary is visible: a moving line between the illuminated half of Earth and the half inside its shadow.

At every moment, billions of us are riding on one side or the other.

Pink Floyd called an album The Dark Side of the Moon, though the Moon has no permanently dark side. Its far side receives sunlight too. Likewise, Earth’s night side is not a separate world. It is simply the side currently facing away.

What if our language followed the motion?

Imagine speaking with the mechanics exposed:

Kids, bedtime. Our side of Earth is turning into shadow.

How long until we face the Sun again?

Let’s finish while our part of the planet is still in direct light.

We are not likely to replace day and night, and I am not seriously asking anyone to try. I like the words too.

The point is to notice how language can freeze an appearance long after science reveals the motion underneath it.

And Earth is not the only familiar thing whose deeper story is hidden by ordinary words.

So are we.

Why scientists say we are stardust

“Stardust” can sound poetic, but it is also a summary of chemistry and cosmic history.

A star begins when a cold cloud of gas and dust collapses under gravity. As matter gathers, the center becomes hotter and denser. Eventually, nuclear fusion begins.

Fusion is not ordinary fire. It is the joining of atomic nuclei under extreme pressure and temperature. In stars like the Sun, hydrogen fuses into helium. In later stages and in more massive stars, fusion builds heavier elements, including carbon and oxygen.

When stars die, they return material to space. Some shed their outer layers gradually. Massive stars can explode. Colliding neutron stars and other extreme events also help create and distribute heavy elements.

Those atoms become part of new clouds, new stars, new planets—and eventually living bodies.

The atoms inside you have different birthdays

An adult human body is mostly oxygen, carbon, hydrogen, and nitrogen.

The hydrogen in the water inside you is ancient. Most of it traces back to the early universe.

The oxygen you breathe and carry in your body was forged in stars.

The carbon central to life was made through stellar processes and spread into space as stars aged and died.

Calcium in your bones, iron in your blood, phosphorus in your cells—their histories are older than Earth.

For you to exist, generations of stars had to form, transform matter, and return those elements to space. A solar system had to assemble. Earth had to cool. Chemistry had to become biology. Life had to survive long enough to become capable of asking where its atoms came from.

That took billions of years.

Two shifts in perspective

So the next time darkness arrives, remember what is physically happening.

The Sun did not leave.

Your side of Earth turned away.

And when you look up at the stars, remember that you are not looking at something completely separate from yourself. You are looking toward the kinds of places where most of the material inside you was made.

Night is Earth’s shadow.

And we are the universe’s recycled light and matter, briefly awake enough to notice.

Sources & further reading

(13)
  1. International Space Station Facts and Figures ↗In 24 hours the station makes 16 orbits of Earth, traveling through 16 sunrises and sunsets; orbits about every 90 minutes.
  2. Arctic Zone: Daylight, Darkness and Changing of the Seasons at the North Pole ↗The Sun rises at the North Pole around the March equinox and sets around the September equinox; the Pole stays in sunlight all summer.
  3. The Dark Side of the Moon ↗The side of the Moon we do not see gets just as much sunlight as the side we do see.
  4. Sun: Facts ↗The Sun is about 4.5 billion years old and will last another 5 billion years or so.
  5. UN projects world population to peak within this century ↗World population of 8.2 billion in 2024 (World Population Prospects 2024).
  6. Universe: Overview ↗About 13.8 billion years ago; protons and neutrons produced the earliest elements, hydrogen, helium and traces of lithium and beryllium.
  7. Protostar ↗“Collapse into a star like our Sun takes about 50 million years.”
  8. Origin of the Elements in the Solar System ↗Six sources of elements; where the r-process (which makes most gold) happens “is currently in dispute,” with merging neutron stars a leading candidate.
  9. The Water in You: Water and the Human Body ↗Up to 60 percent of the adult human body is water; about 60 percent in adult men and 55 percent in adult women.
  10. Composition of the human body ↗Oxygen 65, carbon 18.5, hydrogen 9.5 percent by mass; nitrogen given as 2.6 percent (other references give 3.2-3.3); about 99 percent of mass from six elements. Hydrogen is 62 percent of all atoms in the body by number.
  11. The Origin of Elements from Carbon to Uranium ↗Half of carbon in the Universe is produced by massive stars (>10 solar masses), the rest mainly by low-mass AGB stars (1-4 solar masses); nitrogen is produced mainly by intermediate-mass AGB stars (4-7 solar masses); neutron-star mergers make r-process elements but may not be the only source.
  12. Elements of surprise: neutron stars contribute little, but something's making gold ↗“Half of carbon is produced from dying low-mass stars, but the other half comes from supernovae”; smaller stars make carbon and nitrogen; the source of most gold is still unresolved.
  13. Composition of the Human Body (NIGMS Biomedical Beat) ↗Oxygen 65, carbon 18.5, hydrogen 9.5, nitrogen 3.3 percent; these four make about 96 percent of body mass.

#day and night#Earth's rotation#perspective#stardust#stars

Portrait of Ricardo Maldonado

Ricardo Maldonado, founder and editor of God Plays Dice.
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