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How Big is the Universe?

minutephysics·
5 min read

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

TL;DR

The observable universe is about 93 billion light-years across today, while the whole universe is likely much larger—possibly infinite.

Briefing

The universe’s size depends on which “universe” people mean: the observable universe (everything we can see) is about 93 billion light-years across today, while the whole universe is likely far larger—possibly infinite. The key reason the observable universe isn’t the simple 27.5 billion light-years you might expect from the universe’s age is that space itself has been expanding. Light that left distant galaxies roughly 13.8 billion years ago has been traveling through an expanding space-time, so those sources are now more than 46 billion light-years away. Double that distance for opposite directions and the observable diameter comes out to about 93 billion light-years.

That scale also clarifies why “edge” and “center” are different questions for the observable universe versus the whole universe. The observable universe has a center because it’s defined by what can be seen from a given location on Earth. From our vantage point, the visible region forms a sphere centered on us—much like the circular view from a tall tower is centered on the tower. In fact, each person effectively occupies the center of their own observable universe, even though that doesn’t mean everyone shares a single physical center of the whole cosmos. The “whole universe” likely has no special center, just as the tower’s center is only the center of the view up to the horizon, not the center of the entire world.

The observable universe also has an “edge,” but it’s not a wall in space; it’s a horizon set by time. We can only see light that has had enough time to reach us since the universe began. Anything farther than about 46 billion light-years lies beyond our cosmic horizon. Yet that boundary isn’t fixed: as the universe ages, light from slightly farther away has time to arrive. Each second, the furthest reachable light source increases by about one light-second, so the observable universe grows continuously.

As for whether the universe is getting bigger, the answer is yes in two linked ways. Space is expanding, which stretches distances and makes both the observable universe and the whole universe larger. At the same time, the observable universe grows because we can see older light from farther away as time passes. Taken together, these effects mean the “view from the tower” keeps expanding.

In short: the observable universe is about 93 billion light-years across, it has a center at the observer and an edge defined by the cosmic horizon, and it expands over time. The whole universe is probably infinite in size, almost certainly lacks a spatial edge, has a temporal beginning, and likely has no overall center—so the statement “you are the center of the universe” is true only in the limited, observational sense.

Cornell Notes

The universe’s size depends on whether “observable universe” or “whole universe” is meant. The observable universe is currently about 93 billion light-years across, not ~27.5 billion, because space has expanded while light traveled for up to 13.8 billion years. That expansion pushes distant sources to more than 46 billion light-years away today, setting the observable diameter. The observable universe has a center at the observer and an edge defined by the cosmic horizon, but the whole universe likely has no spatial center or edge. As time passes, new light reaches us, so the observable universe grows continuously, and space expansion makes it grow even faster.

Why isn’t the observable universe simply 27.5 billion light-years across given the universe’s age?

A naive estimate uses the age of the universe (~13.8 billion years) and the fact that light travels at one light-year per year, giving ~2 × 13.77 ≈ 27.5 billion light-years across. But that ignores expansion: light emitted 13.8 billion years ago travels through space that has been stretching. As a result, the sources that emitted that light are now a bit more than 46 billion light-years away. Doubling that distance for opposite directions gives a diameter of about 93 billion light-years for the observable universe.

What does it mean to say the observable universe has a center—and why is it “us”?

The observable universe is defined as the region of space visible from a particular location. From Earth, the visible region forms a sphere centered on Earth, analogous to how the view from a tall tower is a circle centered on the tower. Since “observable universe” depends on the observer’s location, each person is at the center of their own observable universe. That doesn’t imply a single physical center for the whole universe.

What counts as an “edge” of the universe?

The observable universe has an edge in the sense of a horizon: about 46 billion light-years away in any direction. It’s not a boundary you can reach; it’s the limit set by how long light has had to travel since the universe’s beginning. Beyond that distance, light hasn’t had enough time to reach us yet.

How does the observable universe grow over time?

The horizon moves outward. Each second, the furthest light we can receive comes from about one light-second farther away. As the universe ages, older light from increasingly distant regions has time to arrive, so the observable universe’s size increases continuously.

How can the universe be both expanding and “getting bigger” in two different ways?

Space expansion stretches distances, making the observable universe and the whole universe larger. Separately, the observable universe grows because time allows light from farther away to reach us. Together, expansion changes physical distances while the passage of time changes what becomes observable.

What’s the difference between a spatial edge and a temporal edge (beginning)?

The observable universe has a spatial limit set by the horizon, while the whole universe has a temporal boundary: a beginning (often described as the start of the universe). The discussion suggests there’s almost certainly no spatial edge for the whole universe, even though there is a time-based beginning.

Review Questions

  1. What numerical steps lead to the observable universe’s ~93 billion light-year diameter, and where does the expansion factor enter?
  2. Why does each observer count as the “center” of their observable universe without implying a center for the whole universe?
  3. What physical mechanism makes the observable universe’s edge move outward as time passes?

Key Points

  1. 1

    The observable universe is about 93 billion light-years across today, while the whole universe is likely much larger—possibly infinite.

  2. 2

    The observable diameter isn’t ~27.5 billion light-years because space has expanded during the ~13.8 billion years light has been traveling.

  3. 3

    The observable universe has a center at the observer because it’s defined by what can be seen from that location.

  4. 4

    The observable universe has an edge defined by the cosmic horizon (~46 billion light-years away), not by a physical boundary.

  5. 5

    The observable universe grows continuously because new light from farther away reaches us over time.

  6. 6

    Space expansion makes the universe bigger, and the passage of time makes more of the universe observable.

  7. 7

    The whole universe likely has no spatial edge and no overall center, but it has a temporal beginning.

Highlights

Light from the universe’s earliest observable era (~13.8 billion years ago) is now coming from sources more than 46 billion light-years away, yielding an observable diameter near 93 billion light-years.
“You are the center of the universe” is true only for the observable universe: each observer has their own observable sphere centered on them.
The observable universe’s “edge” is a horizon set by light-travel time, and it moves outward as the universe ages.
Space expansion and the arrival of older, more distant light both contribute to the observable universe getting larger over time.

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