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Vsauce·
5 min read

Based on Vsauce's video on YouTube. If you like this content, support the original creators by watching, liking and subscribing to their content.

TL;DR

Ultra-high vacuum still contains residual matter—about 100 particles per cubic centimeter—so it isn’t literal nothingness.

Briefing

“Nothing” can’t exist in any literal, physics-grade sense because space never becomes free of fields and quantum fluctuations. Even when engineers strip air out of a chamber, the best they can reach is an ultra-high vacuum—around 100 particles per cubic centimeter—far from the absolute emptiness implied by the word “vacuum.” The gap between “very empty” and “literally nothing” is where the real science lives.

In everyday terms, air is so dense that even a “not empty” glass is packed with molecules: one cubic centimeter of air contains nearly 30 quintillion molecules. Removing air can create a vacuum, but the practical challenge is removing every last gas molecule. Ultra-high vacuum systems get close by reducing the particle count dramatically, yet they still leave enough residual matter that the chamber isn’t truly empty. A vacuum cleaner illustrates the scale: at sea level, the vacuum inside the machine only reaches the thinness of air found in Denver, Colorado—meaning it barely changes the number of particles you’re breathing.

Altitude shows another limit: nature won’t wait for human comfort. Commercial aircraft keep cabin pressure so passengers experience conditions no higher than about 8,000 feet, even though the plane cruises around 30,000 feet. At extreme thinness, the body can’t get enough oxygen; within under a minute of breathing the outside air at very high altitude, hypoxia can set in. Push higher—past roughly 60,000 feet—and Armstrong’s Limit arrives: the boiling point of blood drops to about body temperature, so bubbles form inside the bloodstream. The body doesn’t explode because skin and organs are flexible, but the physiological risk becomes immediate.

Even in a lab, emptiness is undermined by outgassing. When air is pumped out, materials in the chamber begin releasing their own trapped gases. Outgassing happens in partial vacuums and is especially noticeable in confined spaces; it’s part of why a new car has “new car smell,” as adhesives and chemicals release volatile compounds that accumulate indoors.

Space does get emptier, but not to zero. Between planets, space contains roughly 10 particles per cubic centimeter; in interstellar space, it drops to about one particle per cubic centimeter; and in intergalactic regions outside the Milky Way, densities can fall to around one or two particles per cubic meter. Still, absolute nothingness remains out of reach.

Quantum mechanics supplies the final barrier. Gravitational and electromagnetic fields extend forever, and the particles responsible for those fields are effectively massless. On top of that, “virtual particles” are thought to constantly appear and vanish even in regions that look vacuum-like. Two observed phenomena motivate this picture: the universe’s continued expansion and the Casimir Force. In the Casimir effect, two very close metal plates in a vacuum attract each other, often explained by virtual particles interacting with the plates—long-wavelength fluctuations can’t fit between them, leaving an imbalance in pressure from outside versus inside. The upshot is simple but unsettling: whenever someone feels like nothing matters, physics insists there’s always something—fields, fluctuations, and residual particles—preventing true emptiness.

Cornell Notes

“Nothing” can’t be achieved literally because physics leaves no region completely free of matter-like effects. Even ultra-high vacuum systems still contain about 100 particles per cubic centimeter, and real materials outgas when exposed to partial vacuum. In the atmosphere, thin air at high altitude quickly causes hypoxia, and at Armstrong’s Limit the boiling point of blood drops to body temperature, leading to bubble formation. In space, particle densities fall dramatically—from interplanetary to intergalactic scales—but never reach zero. Quantum mechanics adds the decisive constraint: fields persist and virtual particles fluctuate even in what looks like a vacuum, with the Casimir Force offering evidence of such effects.

Why does “ultra-high vacuum” still fail to produce literal nothingness?

Ultra-high vacuum reduces particle density to about 100 particles per cubic centimeter, but it doesn’t remove every molecule. Residual gases remain, and materials in the chamber begin releasing trapped gases through outgassing. That means the chamber’s walls and components contribute particles even after pumping removes air.

How does outgassing explain why vacuum chambers and enclosed products never feel truly “empty”?

Outgassing occurs when materials release gases they held onto, and it can happen even in partial vacuums. The transcript links this to everyday experience: adhesives and chemicals in a car release volatile compounds that collect inside, creating the “new car smell.” In vacuum systems, the same mechanism prevents reaching absolute emptiness.

What does high-altitude physiology reveal about the limits of “thin air”?

At around 30,000 feet, outside air is too thin and dangerous, so aircraft pressurize cabins so passengers feel like they’re no higher than about 8,000 feet. Breathing the thinner outside air can cause hypoxia within less than a minute—people may look alert but still lack sufficient oxygen. The transcript also notes that above about 60,000 feet, Armstrong’s Limit is reached.

What is Armstrong’s Limit, and why does it threaten the body?

Armstrong’s Limit is the altitude where the boiling point of blood drops to the temperature of the body. Without a special suit, bubbles form inside the bloodstream because the liquid can boil at those conditions. The body doesn’t explode because skin and internal organs are flexible, but the physiological consequences are severe.

How do particle densities change across space, and what do those numbers still leave unresolved?

Particle density decreases from roughly 10 particles per cubic centimeter between planets to about 1 particle per cubic centimeter in interstellar space. Leaving the Milky Way can reduce densities further to around 1–2 particles per cubic meter in intergalactic regions. Yet these are still nonzero values, so they don’t answer the question of whether absolute emptiness is possible.

Why does quantum mechanics rule out a region with absolutely nothing in it?

Quantum mechanics implies persistent fields and fluctuations. Gravitational and electromagnetic fields extend forever, and the particles associated with those fields are effectively massless. The transcript also points to “virtual particles” that appear and disappear even around us. The Casimir Force supports this picture: two very close metal plates attract because virtual-particle effects differ inside versus outside the gap, where long wavelengths can’t fit between the plates.

Review Questions

  1. What two mechanisms prevent a vacuum chamber from reaching absolute emptiness even after pumping out air?
  2. How do the Casimir Force and virtual particles connect to the idea that “vacuum” still contains physical effects?
  3. At what altitude does Armstrong’s Limit occur in the transcript, and what happens to the boiling point of blood there?

Key Points

  1. 1

    Ultra-high vacuum still contains residual matter—about 100 particles per cubic centimeter—so it isn’t literal nothingness.

  2. 2

    Outgassing blocks perfect emptiness because chamber materials release trapped gases even after air is removed.

  3. 3

    Aircraft pressurize cabins because thin air at high altitude can cause hypoxia within minutes or less.

  4. 4

    Armstrong’s Limit (around 60,000 feet) lowers the boiling point of blood to body temperature, causing bubble formation without protective suits.

  5. 5

    Particle density drops dramatically from interplanetary to intergalactic space, but it remains nonzero.

  6. 6

    Quantum mechanics adds a deeper constraint: fields persist and virtual particles fluctuate even in regions that look like vacuum.

  7. 7

    The Casimir Force provides observational support for quantum vacuum effects, explaining attraction between closely spaced metal plates.

Highlights

A vacuum cleaner at sea level doesn’t create a “near-empty” environment—it only reaches the thinness of air found in Denver, Colorado.
At Armstrong’s Limit, the boiling point of blood falls to body temperature, so bubbles form inside the bloodstream.
Even intergalactic space still contains about one or two particles per cubic meter—never absolute zero.
The Casimir Force is often explained by virtual particles interacting with metal plates, producing an imbalance in quantum pressure inside versus outside the gap.

Topics

  • Vacuum
  • Outgassing
  • Hypoxia
  • Armstrong's Limit
  • Casimir Force

Mentioned