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Published byColleen Smith Modified over 8 years ago
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Origin of the Universe Where did Earth, the solar system, & the stars come from? Where did life come from? Our universe came into existence suddenly as a concentrated single point, containing all known matter & energy. Approximately 13.7 billion years ago this single point began to expand – an event known as the Big Bang. It took about 1 million years for matter in the universe to cool for the first elements to form, mostly hydrogen & helium.
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Matter is not distributed uniformly throughout the universe. A natural property of matter – gravity – began attracting helium & hydrogen atoms together. As the density increased, matter collapsed & compacted under its own weight, causing a warm, dense core called a protostar to form.
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The Theorized “Life-Cycle” of a Star: The nuclear fusion reaction from protostars creates stars. The star burns for millions of years, consuming it’s hydrogen. Heavy elements form as hydrogen atoms fuse during the “life-cycle” of a star. The core becomes denser & eventually collapses under the extreme gravity forces generated. The star may explode causing a supernova. Supernova explosions account for the distribution of heavy elements through-out the universe.
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Origin of the Solar System: The Nebular Theory A shock wave from a supernova caused the cloud to condense, which caused it to spin. As the cloud collapsed & became denser, it flattened in a disk due to the rotation. At the center a protostar developed & began the nuclear fusion process, becoming the sun. Some gas continued to revolve around the sun eventually condensing into masses to small to become stars – they became the planets.
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Origin of the Earth & Moon According to the nebular theory, Earth (& other solar system planets) formed through accretion. Accretion is the process by which small particles clump together because of gravity. As a mass grows the more gravity is has, the more additional mass it attracts. The Earth’s growing mass caused its core to compress causing the core to heat & become molten liquid. The outer core is still molten. With this molten liquid, heavy matter (iron & nickel) sank toward the center, while light matter (oxygen & silicon) moved toward the surface. This process of density stratification formed the layers of the Earth.
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Origin of the Moon The most widely accepted theory for the moon’s origin is the Orpheus Theory. The Orpheus Theory says that a planet – sized body struck Earth during its early development & sent some of its material into orbit, forming the moon.
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Origin of the Atmosphere & the Ocean When the earth cooled enough for the surface to form a crust, gases from volcanic activity escaped accumulating as an early atmosphere. The surface was still so hot that when water vapor formed clouds, then rain, the rain boiled off again when it hit the ground. Finally, the Earth cooled enough to allow the rainwater to accumulate & the ocean formed as water vapor condensed.
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The process that allowed life to form began with the development of the ocean. Carbon dioxide dissolved into the young ocean, leaving a nitrogen-rich atmosphere. Scientists think these were the conditions required for life. Interestingly, there was no oxygen in the atmosphere on early Earth. Although oxygen is essential to almost all life today, according to data recorded in rock, early life didn’t use oxygen. Oxygen entered the atmosphere about 1.5 billion years ago when photosynthesizing organisms (stromatolites) began using carbon dioxide & releasing oxygen.
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