What Do We Mean When We Say the Universe Is Expanding?

The concept of an expanding universe is one of the most profound discoveries of modern science, fundamentally reshaping our understanding of the cosmos. It suggests that the vastness we observe is not a static stage but a dynamic entity that has been growing ever since its beginning in the Big Bang. This expansion is not merely the movement of objects through space, but a transformation of space itself. Understanding this cosmic growth requires a shift in perspective.

Understanding the Stretching of Space

The universe’s expansion is not like an explosion where galaxies are flying outward from a central point into a pre-existing void. Instead, the space between galaxies is stretching, similar to the surface of an inflating balloon with dots drawn on it. As the balloon inflates, the dots move farther apart, not because they are traveling across the rubber, but because the rubber itself is growing. This analogy helps illustrate that every distant galaxy is moving away from every other distant galaxy, meaning there is no single center to the expansion.

Galaxies are not moving in space, but are being carried along with the expansion of space. If a galaxy is twice as far away, the amount of new space created between us is also doubled, meaning it appears to recede at twice the speed. This mechanism of cosmic stretching is the core of the universe’s expansion.

The Key Evidence: Redshift and Hubble’s Law

Scientists first discovered this expansion by observing a phenomenon called cosmological redshift. As light travels from a distant galaxy toward us, the stretching of space causes the light waves themselves to stretch out over time. This stretching increases the light’s wavelength, shifting its color toward the red end of the electromagnetic spectrum, which is how the effect gets its name.

This redshift is fundamentally different from the Doppler effect, which describes a change in wavelength due to an object’s motion through space. Cosmological redshift is a direct result of the expansion of the intervening space between the light source and the observer. The greater the distance the light has traveled, the more the space has expanded, and consequently, the greater the observed redshift.

In 1929, astronomer Edwin Hubble quantified this observation, establishing what is now known as Hubble’s Law. His foundational work showed a linear relationship between a galaxy’s distance from Earth and the speed at which it appears to be moving away. The farther away a galaxy is, the faster its apparent recessional velocity, a relationship derived from measuring its redshift.

Hubble’s Law provided the first observational proof that the universe is not static but is expanding, overturning the long-held belief of a fixed cosmos. This relationship between distance and recessional speed is expressed by the Hubble constant, which describes the rate of expansion. The discovery provided the necessary evidence to support the theory that the universe originated from a hot, dense state, now known as the Big Bang.

Clarifying What is Not Expanding

A common point of confusion is whether the expansion of space affects everything within the universe. Cosmic expansion only operates on the largest, unbound scales. On smaller scales, the forces of nature are strong enough to overcome the stretching of space and hold matter together.

Local structures, such as planets, stars, and solar systems, are not expanding internally. For example, the Earth and the Sun remain at a fixed distance, and the atoms that compose them do not grow larger. This is because the electromagnetic and nuclear forces binding them are immensely stronger than the expansion force.

Even entire galaxies, like our own Milky Way, are gravitationally bound and are not expanding. The gravitational pull between all the stars, gas, and dark matter within a galaxy is sufficient to keep the structure intact against the background expansion of the universe. Similarly, the galaxies within our Local Group, including the Milky Way and the Andromeda Galaxy, are gravitationally bound and are actually moving toward each other, destined to merge in the distant future.

The expansion of space becomes noticeable only on scales larger than galaxy clusters. In these regions, the average density of matter is too low for gravity to successfully counteract the stretching of space. While space is expanding everywhere, its effect is only evident when looking at the vast, empty regions between galaxy clusters.

What Expansion Means for the Universe’s Future

The expansion of the universe has profound implications for its long-term future, especially since scientists discovered in 1998 that the expansion is accelerating. This acceleration is attributed to a mysterious force called Dark Energy, which is thought to act as a kind of anti-gravity, pushing space apart. Dark energy is believed to be a property of space itself, making up an estimated 68% of the total mass-energy content of the cosmos.

As the universe expands, more space is created, and if the density of dark energy remains constant, this means the total amount of dark energy increases, driving an ever-faster expansion. The continuous, accelerating expansion means that distant galaxies will eventually recede so quickly that their light will never be able to reach us. These galaxies will effectively move beyond our cosmic horizon, making them permanently invisible and unreachable.

The leading scenario for the ultimate fate of the universe is the “Big Freeze,” or heat death. In this future, the accelerating expansion will dilute all matter and radiation to such an extent that the universe becomes cold, dark, and empty. With all stars eventually burning out and new ones unable to form, the cosmos will become a vast, lifeless expanse where processes cease due to a lack of energy density.

While the Big Freeze is the most widely accepted fate based on current data, some models suggest that if dark energy weakens over time, the expansion could slow down. This might potentially lead to a “Big Crunch,” where gravity eventually reverses the expansion. However, the current evidence strongly favors the idea that the acceleration, driven by dark energy, will continue indefinitely.