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How The Origins Of Galaxies And Stars

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To explain how the origins of galaxies and stars, we must go back to the previous threshold: the big bang. Gravity was one of the four fundamental forces that came from the big bang, and as a result, plays a central role in the formation of stars and galaxies as it has the ability to change something else. Gravity holds the ability to garner more mass when there is more mass involved and vice versa, this leads to a different effect of different areas depending on mass. Like stars, stars begin very small, just particles in vast clouds of dust and gas. These ‘nebulae’ remain cold for ages until an external force come through and causes a disturbance. As the force moves through the cloud, particles collide and clump together. These clumps then gain more mass, and as I mentioned above, a stronger gravitational pull, attracting, even more, particles. as these clumps grow, the center grows denser and hotter. This is a long process, it takes a few million years before it moves onto the next stage: the protostar. This process will continue as the protostar grows until the center becomes too hot, then its hydrogen atoms begin to fuse which produce an influx of helium and energy. This reaction is called nuclear fusions, and while it may sound as the changing factor, but this outflux of energy is still weaker than the inward pull of gravity. The turning point of a protostar into a star is when there is too much material being fed into the protostar. Is enough mass increases into the

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