The Universe expands within itself, then what is it expanding into?

The observable Universe will more than double in volume over time as light from unseen regions continues to reach us.

Key Takeaways

  1. The Universe expands into itself, not into any external space or medium.
  2. This counterintuitive idea is rooted in the framework of General Relativity and the concept of spacetime.
  3. Early 20th-century discoveries by Vesto Slipher and Edwin Hubble showed that galaxies farther away move faster, supporting the theory of expansion.
  4. Analogies like balloons and raisin bread dough help visualize expansion, but they have limitations.
  5. The observable Universe is just a fraction of what might be an infinite cosmos, potentially part of a multiverse.

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For nearly a century, the Big Bang theory has provided the most comprehensive explanation of our Universe’s origins. Born from a hot, dense state 13.8 billion years ago, the Universe has been expanding and cooling, eventually giving rise to stars, galaxies, and life as we know it. However, a common question lingers: what is the Universe expanding into? Surprisingly, the answer is “itself.”

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This idea stems from General Relativity, which shows that space and time are not fixed but dynamic and interwoven. Two key discoveries in the early 20th century solidified this understanding. First, Vesto Slipher observed that light from many nebulae was redshifted, indicating they were moving away. Second, Edwin Hubble measured distances to these galaxies and found that the farther they were, the faster they receded. This correlation, now known as Hubble’s Law, confirmed that the Universe is expanding.

Hubble discovery cepheid andromeda
Hubble’s discovery of a Cepheid variable in the Andromeda galaxy, M31, opened up the Universe to us, giving us the observational evidence we needed for galaxies beyond the Milky Way and leading us, in short order, to the discovery of the expanding Universe. Credits: NASA, ESA and the Hubble Heritage Team (STScI/AURA); Illustration via NASA, ESA, and Z. Levay (STScI)

Analogies and Challenges in Understanding

Scientists often use analogies to explain this phenomenon. The “balloon analogy” imagines galaxies as coins on a balloon’s surface, moving apart as the balloon inflates. Another analogy is a loaf of raisin bread dough, where the raisins (galaxies) move apart as the dough (space) expands. However, these analogies fall short in some respects. Unlike the dough or balloon, the Universe doesn’t expand into anything; it’s all there is.

Observations suggest the observable Universe is only a fraction of a potentially infinite cosmos. While light from unseen regions will eventually reach us, expanding spacetime itself ensures galaxies continue moving farther apart. The theory of cosmic inflation suggests that our Universe is one “bubble” in a vast multiverse, though these regions remain isolated from one another.

hubble plot expanding universe
Edwin Hubble’s original plot of galaxy distances, from 1929, versus redshift (left), establishing the expanding Universe, versus a more modern counterpart from approximately 70 years later (right). Many different classes of objects and measurements are used to determine the relationship between distance to an object and its apparent speed of recession that we infer from its light’s relative redshift with respect to us. As you can see, from the very nearby Universe (lower left) to distant locations over a billion light-years away (upper right), this very consistent redshift-distance relation continues to hold. Earlier versions of Hubble’s graph were composed by Georges Lemaître (1927) and Howard Robertson (1928), using Hubble’s preliminary data. Credit: E. Hubble; R. Kirshner, PNAS, 2004

Understanding expansion also challenges our intuition. Space isn’t a thing moving through something larger—it’s the very fabric of reality, stretching and evolving. Even in an infinite Universe, expansion is a natural property of spacetime, governed by physical laws.

A Fascinating Reality

The expanding Universe doesn’t require an external medium. Instead, it demonstrates the beauty of physics and mathematics, where concepts like infinity and spacetime help us comprehend a reality far beyond everyday experience. While intriguing theories like extra dimensions or a multiverse are possibilities, they remain speculative. What’s certain is that the Universe’s expansion defines not just its past but its future—offering endless opportunities for discovery.

regions of the universe
In a Universe that comes to be dominated by dark energy, there are four regions: one where everything within it is reachable, communicable and observable, one where everything is observable but unreachable and incommunicable, one where things will someday be observable but aren’t today, and one where things will never be observable. The labeled numbers correspond to our consensus cosmology as of 2024, with boundaries of 18 billion light-years, 46 billion light-years, and 61 billion light-years separating the four regions. On scales of ~10 billion light-years and larger, the Universe is almost perfectly uniform. Credit: Andrew Z. Colvin/Wikimedia Commons; annotations: E. Siegel
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