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Our solar system has been born when, in a spiral arm of the Milky Way galaxy, a giant rotating cloud of dust and gasses began to collapse. Gravity compressed the dust and gasses and the cloud got increasingly hotter and began to spin faster. Throughout the subsequent one hundred thousand decades, the gasses compressed before the center was so hot that nuclear fusion happened giving away tremendous energy, mixing billed atoms of hydrogen to form helium. This process gave birth to a star, our Sun (Our Solar System, n.d.). Scientists have a fantastic deal of data recording the solar system's history for roughly the last 3.9 billion decades, but it had been actually formed approximately 4.6 million decades ago. The first 700 million years have been a bit of a mystery since earthquakes, volcanic eruptions, and erosion have resisted signs from that time. Throughout that initial 700 million years, the planets coalesced and water along with other components necessary for life have been delivered to the interior planets (Cowen, 2009). Our solar system is also a diverse and exceedingly interesting speck in the universe. Earth's solar system is at the Milky Way Galaxy and is a part of a system of eight planets orbiting the Sun, the star which is the center of the solar system. The Sun is continually burning gasoline, which heats and lights Earth and the other planets (Solar System Information, n.d.). The planets in our solar system vary widely in size, composition, distance from sunlight, and atmosphere. Of the Milky Way Galaxy's 100 to 200 billion stars, only about 6,000 of them are able to be observed with the naked eye from Earth and one of these is your Sun. "Planets" means "wanderers" and so were called that because they seemed to travel across the skies. Other objects in the solar syst...