BLACK HOLES AND BEYOND

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At the heart of general relativity—the theory that best describes the structure and evolution of our universe—lurks a tiny problem. A very tiny problem. For in the intricacies of the theory lies the possibility of a region of space-time so unimaginably small and so incredibly bizarre that the theory ceases to work. Yet this region, known as a singularity, apparently describes the state of the universe when it was born.
 

Black hole

       Singularities and their big brothers, black holes, play important roles in cosmologists’ attempts to understand the workings of the universe. Not only does a singularity appear to describe the state of the universe at its inception, but black holes and their associated singularities seem to power quasars, the most energetic objects in the universe, and may even offer potential passageways into entirely different universes.
 

       Although general relativity breaks down at a singularity, it’s the only theory that can describe the exotic region of space-time surrounding it—the black hole. It’s surprising, then, that the idea of a black hole dates back to well before Einstein. In the late 1700s, British professor John Michell and French astronomer and mathematician Pierre Simon, Marquis de Laplace, advanced the idea of what Laplace called “dark bodies.” Using Newton’s concepts of gravity and light, they reasoned that the gravitational pull of a very massive star could be large enough to prevent even light, traveling at a speed of 186,000 miles per second, from escaping.
 

Learn  more about:

Singularity

Black Holes

Quasars

Albert Einstein

Isaac Newton

 

       Unfortunately, Newton’s theory couldn’t describe what happens when the force of gravity grows so intense. That understanding wouldn’t come until Einstein developed general relativity in the 1910s, but even then it took decades before many scientists thought of black holes as more than a theoretical curiosity.
 

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