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We Are Stardust

The iron in our blood, oxygen in our breath and calcium in our bones were not made here on Earth. They were formed in the hearts of ancient stars. Those stars forged them and flung them into space. We use the word ‘stardust’ as a poetic metaphor, yet it is also literally true.

A star begins its life in the cold. Vast clouds of gas and dust drift inside a nebula at -250 degrees Celsius. Cold gas is slow and slow gas is easy to pull. So gravity pulls it together. The pull reaches a tipping point called the Jeans instability, where the inward pull of gravity finally beats the gas pushing back. Then the cloud collapses.

A clump like this becomes a protostar. The protostar keeps gathering mass and shrinking as gravity pushes inward. Its core packs tight and traps its own heat, so the temperature climbs. It glows in infrared inside the dust that made it. Astronomers call this restless young star a T Tauri star. The spinning protostar hurls supersonic jets from its poles. The jets slam into nearby dust and light it up. A star screams into existence.

The childhood ends and a star’s adulthood begins at ten million Kelvin. At that temperature, hydrogen nuclei fuse into helium and release energy. Nuclear fusion has begun. The star enters the main sequence and settles in. Our own Sun is in this phase.

The star holds this standoff for billions of years. Gravity pulls in. Pressure generated by fusion pushes out. The two forces cancel. The star looks permanent, but gravity eventually wins when the core runs out of hydrogen. A gentle star like our Sun ends softly as it runs out of fuel. Its outer layers drift off as a glowing shell called a planetary nebula. The core is left behind as a white dwarf, a dense ember of carbon and oxygen. It cannot collapse further because its electrons refuse to be squeezed. This force has a name: electron degeneracy pressure. For small stars, that is the whole story. A quiet retirement.

Massive stars die differently. A star over eight times our Sun’s mass burns through its fuel in a frenzy. As each fuel is exhausted, gravity compresses the core further. This ignites progressively heavier fusion stages. It burns hydrogen, then helium, then carbon, neon, oxygen and silicon. Each stage runs faster than the last. In its final breath, it builds an iron group core. That is a trap! Iron fusion is endothermic, so it absorbs energy. Fusion can no longer support the core against collapse, so the structure destabilizes.

What follows is one of the most cataclysmic events in the known universe. The core collapses at a fraction of the speed of light. Matter is crushed to densities approaching those of an atomic nucleus. The star detonates as a supernova. A neutron star, a city sized core of ultra dense matter, can remain at the center. If the core is heavy enough, a black hole forms instead. Sometimes two neutron stars end up in orbit around each other. Later, when they merge, their collision can forge much of the gold and platinum in the universe.

Gold and platinum came through cosmic violence. Massive stars died and neutron stars collided. Some of that gold and platinum settled into the young Earth. Some of it got dug up. Some of it got shaped into a ring. We take a substance born in extreme events elsewhere in the universe and use it to mark a commitment of love here on Earth. We may have done that without ever knowing. And that is beautiful!

Star trails in the night sky
Star trails centered on Polaris, taken near Fairbanks, Alaska. Photo by author.