HomeThe World We DiscoverWhere Does Everything Come From?

Where Does Everything Come From?

Everything around you came from somewhere - but the trail leads to questions science may never answer

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The World We Discover · Explore this series
December 14, 2025
Key Takeaways
  • Earth formed from the same gas cloud as the Sun about 5 billion years ago.
  • Heavy elements like gold form only during neutron star mergers, not in ordinary stars.
  • Before atoms existed, the early universe was a plasma of quarks and gluons.

Where does everything come from? In this video from Sabine Hossenfelder, this deceptively simple question launches an investigation that travels from Hossenfelder’s desk to the edge of scientific knowledge.

The journey begins with chemistry. Most complexity requires a Goldilocks zone - not too cold like outer space where little happens, not too hot like inside stars where too much happens. Earth sits in that sweet spot where molecules can combine into DNA, cells, and eventually YouTube.

Key figure

5 billion years

Age of Earth – formed from the same gas cloud as the Sun

From Planetary Formation to Nuclear Fusion

Our planet formed from the same gas cloud as the sun about 5 billion years ago. But Earth ended up with more heavy elements because of how the protoplanetary disc cooled.

Close to the sun, only solid materials like iron and silicon could clump together. Farther out, past the snow line where water freezes, planets grew faster and captured hydrogen and helium to become gas giants.

The atoms themselves trace back to stars. Light elements like hydrogen formed in the early universe, then clumped into stars that fused them into heavier elements up to iron. When stars exploded as supernovas, they scattered these elements across the galaxy.

Gold and platinum require even more extreme conditions - they form during neutron star mergers.

The Plasma Era and Beyond

Going deeper, the constituents of atoms emerged from the early universe's extreme heat. When temperatures were so high that electrons couldn't stick to nuclei, everything existed as plasma.

Before that, even protons and neutrons broke apart into their constituent quarks and gluons. This soup of fundamental particles formed during nucleogenesis, which physicists can partially test with particle colliders.

But the trail grows speculative. The leading theory suggests an inflaton field drove exponential expansion, then decayed into all the particles we see today.

What is an inflaton field?

An inflaton field is a hypothetical energy field thought to have driven the universe's rapid expansion in its first fraction of a second – a period called cosmic inflation. According to the theory, this field eventually decayed, releasing its energy as the particles that make up everything we see today. No one knows what the inflaton field itself was made of, or where it came from.

The Ultimate Question Mark

Where did the inflaton field come from? Maybe it existed forever. Maybe it's made of strings from string theory. Maybe our universe bounced from a previous one.

We don’t know.

As Hossenfelder points out, this sequence of “why” questions can’t end with a scientific answer.

Logic is one of the most important - if not the most important - skill one needs in life.

Sabine Hossenfelder, Phycisist and YouTube Host

Science explains observations by making assumptions, but it can never explain why we observe what we observe in the first place.

The insight is elegant. Every answer reveals another question, stretching from your desk to the logically impossible.

Fact Check: Claim-by-Claim Verification Verified

The recap accurately reflects the content and tone of Hossenfelder’s video and current scientific understanding, with only minor simplifications typical of popular science.

1 Verified
The description of Earth forming from the same protoplanetary disk as the Sun, with composition differences linked to disk cooling and distance from the star, is consistent with standard models of planetary formation
2 Verified
The account of element formation—light elements from the early universe, heavier elements up to iron in stellar fusion, and very heavy elements like gold and platinum in neutron star mergers—matches current astrophysical evidence and interpretations

Commentary

  • The statement that gold and platinum “form during neutron star mergers” reflects a leading but still actively researched view; other sites such as certain supernovae may also contribute, so this is slightly more definite than the underlying literature.
  • The term “nucleogenesis” for the quark–gluon plasma era is nonstandard (cosmologists usually distinguish quark–gluon plasma, baryogenesis, and nucleosynthesis), but the physical picture conveyed in the recap aligns with mainstream early-universe cosmology and the way Hossenfelder typically presents it.
  • The recap’s discussion of an inflaton field, its unknown origin, and the idea that ever-deeper “why” questions may exceed the scope of science, faithfully represents how Hossenfelder frames the speculative end of the story and clearly labels it as uncertain or philosophical.

Sources used for verification

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