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The Hubble Research Paper

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There have been many theories concerning what the universe looks like, how it became this way, and where it is going. For many years the universe has confused many astronomers and scientist, it is difficult to have a good understand of something that is so far away. Especially, back then where there was a lack of tools to be able to view and see the universe like we do today. However, with the collaboration of many great scientists and astronomers we have established a more concrete understanding on our universe. It is still hard today to understand the complexity of our universe because to many see it as irrelevant or to foreign to their knowledge. However, our universe should not be overlooked; it is the beginning to life and all that exists. …show more content…
The law is usually stated as v = H0D, where v is the velocity of recession, D is the distance of the galaxy from the observer and H0 is the Hubble constant which links them. The exact value of the Hubble constant itself has long been the subject of much controversy: Hubble's initial estimates were of the order of approximately 500 kilometers per second per mega parsec (equivalent to about 160 km/sec/million light years); the most recent best estimates, with the benefit of the Hubble Telescope and the WMAP probe, is around 72 kilometers per second per mega …show more content…
The constant expansion makes it impossible to accurately determine a certain edge or center to our universe. Even thought the universe is infinite does it have a shape? This leads to three possibilities a flat universe, closed universe, or an open universe. (Look at the figure below). The photo below shows the multiple ways the universe could go in the future. While most of them show how the universe could just expand forever, I find that the future of the closed universe to be the most interesting. The shape is dependent on the mass, energy, and gravity there is in the universe. According to Einstein's theory of General Relativity, space itself can be curved by mass. As a result, the density of the universe determines its shape, as well as its future. Calculating the Critical Density, which decides its shape and fate, helped scientist discover that our universe is flat due to

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