The observable universe, the portion of the cosmos from which light has had enough time to reach us since the Big Bang, is not a static entity. Due to the continuous expansion of spacetime, the observable universe is constantly growing. As light from increasingly distant regions has had more time to travel, these previously unseen areas come into view, effectively expanding our cosmic horizon. This ongoing expansion reveals more of the universe’s vastness over time.
The current size of the observable universe is estimated to be about 93 billion light-years in diameter. This seemingly paradoxical figure, larger than the age of the universe multiplied by the speed of light, arises from the fact that space itself has been expanding while the light has been traveling. Distant galaxies that emitted light billions of years ago are now much farther away than the distance light has traveled, due to this continuous stretching of spacetime.
As the universe continues to expand, the light from even more distant objects will eventually reach us, causing the observable universe to grow larger. Galaxies that are currently beyond our cosmic horizon will, in the distant future, become visible. This doesn’t mean the entire universe is getting larger, but rather that the sphere of space from which light can reach our location is increasing with time, allowing us to witness previously unseen cosmic structures and events.
However, the expansion of the universe also has a limiting effect on what we will eventually be able to observe. Galaxies that are currently very far away are receding from us at speeds approaching and even exceeding the speed of light due to the expansion of space. Light emitted from these extremely distant objects will be increasingly redshifted, eventually becoming undetectable, and these galaxies will effectively disappear from our observable universe in the very distant future.