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Dark matter and dark energy: the 95% of the universe we can't see

Space & the universe

Dark matter and dark energy: the 95% of the universe we can't see

11 min

How astronomers discovered that everything we can observe is a tiny fraction of what's out there, the evidence for the invisible majority, and why its true nature remains one of physics' deepest open problems.

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Show notes

Fritz Zwicky discovered that galaxies in the Coma Cluster moved faster than visible gravity should allow.

Vera Rubin proved that outer stars orbit spiral galaxies as fast as inner stars, suggesting invisible halos.

The Bullet Cluster collision shows dark matter passing through obstacles like a ghost through a wall.

Visible matter accounts for less than five percent of the total composition of the universe.

Supernovae observations in nineteen ninety-eight revealed that the expansion of the universe is actually accelerating.

Dark energy acts as a repulsive pressure inherent to space, making up sixty-eight percent of the cosmos.

In this episode

  1. 1Intro1 min
  2. 2The Swiss Anomaly and the German Name2 min
  3. 3Vera Rubin and the Spinning Spirals2 min
  4. 4The Bullet Cluster and Gravitational Lensing2 min
  5. 5The 1998 Shock: Dark Energy3 min
  6. 6Outro1 min

Sources

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Dark matter and dark energy: the 95% of the universe we can't see — Fylom