The universe is an endless mystery filled with stars, planets, and galaxies spread across unimaginable distances. Astronomers have studied the night sky for centuries to understand how vast it truly is. With the help of advanced telescopes and modern technology, scientists are now exploring deeper into space, trying to uncover how many galaxies might exist across the vast expanse of the universe.
In the past, people believed that the Milky Way was the only galaxy in the universe. This changed in the 1920s when astronomer Edwin Hubble discovered that what were once thought to be “nebulae” were actually separate galaxies far away from our own. His discovery completely changed how we understand the size and structure of the universe.
Galaxies come in many shapes and sizes.
Each type shows how galaxies form, grow, and interact over time.
With the help of telescopes like NASA’s Hubble Space Telescope, scientists have estimated that there may be 100 to 200 billion galaxies in the observable universe. Each of these galaxies could contain billions of stars and countless planets. As technology improves, astronomers might find even more galaxies that are too faint or distant to see today.
Galaxies are not spread evenly across space. They form groups known as clusters, which join together to create larger superclusters. These clusters are connected by long threads of matter called cosmic filaments, leaving huge empty areas between them known as voids. This web-like pattern helps scientists understand how the universe formed and continues to expand.
Galaxies are always changing. They collide, merge, and create new stars over time. Some galaxies have supermassive black holes at their centers that release enormous energy. Studying galaxies helps scientists learn how the universe began, how it evolves, and what it might become in the future.
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