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But, with great simulations come great, intricate, daunting catalogues of information to formulate and keep track of.
Inside the simulation's hypothetical section of the universe are all of the ingredients that go into creating a star, such as the fundamental chemical properties of the gases present, the expansion of the universe, and gravity. The code also calculates the rate at which molecular hydrogen cools the cloud as it forms. Finally, it takes into consideration Cold Dark Matter, a cosmic material that researchers know exists but haven't been able to observe. They have, however, been able to figure out the amount that exists, how it behaves, and what impact it has on other, observable cosmic material. | |||
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