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How the Universe Began: the Secrets of the Big Bang

The Universe 101

By Mariam MelikidzePublished 2 years ago 3 min read

In the quest to understand the origins of the universe, we journey back to a time when there was no space, no time—just everything in the known universe squeezed into a tiny dot, tinier than an atom. Then, suddenly, from this unimaginably small point, our universe burst into existence. Stars lit up, galaxies swirled into shape, and the universe as we know it today began to form.

The story of our universe starts with what we call the Big Bang. But even though the Big Bang is widely accepted as the observed truth, there are still many details to uncover. Science isn't just about being right all the time; it's also about admitting when we might be wrong and continually searching for deeper understanding.

Now, let's talk about the Big Bang itself. When we hear the term "Big Bang," we often picture a loud explosion with fiery flashes and powerful shockwaves. But was it truly an explosion as we usually imagine? Explosions typically involve a sudden release of energy, creating sounds, light, heat, and pressure. However, the Big Bang happened in a place without air, so there was no way for sound waves to travel—it was a silent event.

But for the universe to come into existence, something significant must have occurred. Explosions usually have a central point of ignition, a place where it all begins. So, if we think of the Big Bang as an explosion, we naturally ask: Where is its center? The surprising answer is that there isn't one. The Big Bang isn't limited to a specific spot; it encompasses everything, everywhere. It happened where you are reading this, on the opposite side of the planet, in the farthest reaches of the Andromeda galaxy, and throughout the entire universe, all at the same time.

Explosions typically result in debris being scattered unevenly from a central point. However, when we look at our universe on a grand scale, it appears remarkably uniform—almost the same in all directions. This uniformity, called homogeneity in astronomy, suggests that an equal amount of material was distributed evenly in all directions, challenging the idea of an explosion.

So, if the Big Bang wasn't a conventional explosion, what triggered this colossal event? The answer isn't as simple as we might want it to be. When we talk about the birth of the entire universe, ideas of cause and effect become elusive. There's no external force or entity beyond the universe to set it in motion.

While we might not fully understand the initial chapters of this cosmic story, we've pieced together a narrative that extends far beyond. As cosmologists, we have a unique privilege: telescopes act as time machines for us. By looking deeper into space, we are essentially looking further back in time, gradually revealing the universe's history layer by layer.

The pioneering work of astronomers like Edwin Hubble, who noticed galaxies moving away from us and introduced the term "redshift," played a vital role in uncovering the mystery of the Big Bang. Hubble's groundbreaking discovery supported the idea that our universe is continuously expanding, suggesting that if we trace this expansion backward, everything converges at a single point—an event we've come to know as the Big Bang.

Yet, the beginning of the Big Bang remains a puzzle. It involves a concept known as a singularity—an infinitely small, dense point where the laws of physics no longer apply. The singularity raises profound questions that challenge our understanding of the universe.

As we embark on this cosmic journey, we'll delve deeper into the mysteries of the Big Bang, exploring the remarkable discoveries that have brought us closer to understanding the birth of our universe. In the pages ahead, we'll trace the universe's history back in time, using the cosmos itself as our guide, as we seek to unravel the enigma of the Big Bang and the origins of our existence.

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