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Earth's Early History

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Submitted By DareWolf
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Milky Way Galaxy, the Sol System, 4.2 billion years ago, rock and ice particles swirling around a very young sun collide and merge, producing large planetoids. One of them, an infant planet we have come to call home, is born. This planet will later be named Earth. At this point the baby Earth is nothing more than a scorching inferno of magma and vaporized rock, spitting up nothing more than magma volcanoes. This infant planet is very different from the one we know today. Its atmosphere is comprised of deadly gasses and probably had a sky the color of a pinkish-orange. Its oceans containing large quantities of dissolved iron were most likely a kind of brown color. Life on early Earth began with very little amounts of oxygen compared to the quantities we have today, it was comprised of primitive elements and very slowly evolved into the Earth we know today. Had you been on Earth all that time ago, when it was just beginning to evolve, you would have died with just a few deep breaths! Earth’s early atmosphere contained little or no oxygen. It was primarily comprised of carbon dioxide, water vapor, and nitrogen, with smaller amounts of carbon monoxide, hydrogen sulfide, and hydrogen cyanide. Over time a controversial question emerged, could organic molecules assemble under the conditions on early Earth? In 1953, biochemists Stanley L. Miller and Harold C. Urey conducted an experiment to find these answers; they tested for what kind of environment would be needed to allow life to begin. To start they used water, methane, ammonia and hydrogen, component believed to represent major elements in early Earth’s atmosphere. These chemicals were all sealed and circulated inside a sterile array of glass tubes connected together in a loop, with one sterile flask with, and another flask containing electrodes. The liquid water was heated to add water vapor to the chemical mixture

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