How do we measure a universe 93 billion light-years wide?

Astrophysics Explained Like You Are 5 Years Old | No Fluff Academy · 16:17 · Video: No Fluff Academy · Watch at the source

In short: Humans have never traveled further than the Moon, yet we can map the edges of the observable universe. Without rulers or probes to reach distant stars, astronomers rely on a clever cosmic trick: using light itself as a universal yardstick to bridge the impossible gap between Earth and the deep cosmos.

Measuring distances in space presents a unique problem because traditional tools like radar, GPS, or physical rulers are useless over billions of miles. To solve this, astronomers use a method known as the cosmic distance ladder. This system relies on the fact that the brightness of an object fades at a precise, calculable rate as it moves further away. By identifying objects with a known, consistent brightness—referred to as "standard candles"—scientists can calculate exactly how far away they are based on how dim they appear from Earth.

Another vital tool is spectroscopy, which allows scientists to split light into its component colors to reveal an object's "redshift." A common misconception is that redshift happens because galaxies are flying through space like projectiles. In reality, redshift is caused by the expansion of space itself. As space stretches, the light traveling through it also stretches, shifting toward the red end of the spectrum. By combining the data from standard candles and redshift measurements, astronomers were able to confirm Hubble's Law.

Hubble's Law provides one of the most solid results in astrophysics: it proves that the universe is expanding. This discovery revealed that this expansion is actually accelerating. These principles aren't just for looking at distant galaxies; they have practical applications on Earth, including the technology behind GPS satellites, the detection of exoplanets, and even medical spectroscopy used in healthcare.

The observable universe spans 93 billion light-years across. Because light takes time to travel, looking further into space is functionally equivalent to looking back in time. By mastering these measurements, we can reconstruct the history of the cosmos without ever leaving our own backyard.

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