The Sun: The Importance Of The Sun On Earth

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Hopefully we all know how important the Sun is to us. However, some often forget why that is. The Sun is the star at the center of the solar system and is the most important star for the living and non-living organisms on Earth do to the fact that it provides the light energy and the heat needed to support life. Without the heat and light that it provides, the Earth would be lifeless and a ball of ice. The sun was created in a vast cloud of gas and dust over five billion years ago. . Over a period of many millions of years, this gas and dust began to fall into a common center under the force of its own gravity. At the center, an ever growing body of mass was forming. As the matter fell inward, it generated a tremendous amount of heat and pressure. …show more content…

It is by far the brightest object in the sky and is about 13 billion times brighter than the next brightest star, Sirius. Without it the earth would be dark and cold. The Sun and the light in provides supplies us with many resources. It helps plants produce oxygen through the process of photosynthesis and overtime creates fossil fuels. Photosynthesis is a chemical process which water and carbon dioxide combine together in the presence of sunlight and chlorophyll, which is the chemical that makes the leaves in plants green, to produce glucose and oxygen. Plants absorb sunlight for food and they release oxygen, in which we breathe. If there were no sunlight, the photosynthesis process could not take place. The plants would not be able to produce energy for their survival, leading to the disappearing of people and animals because they depend on food and oxygen to breathe which is supplied by the plants. So in simple terms, if there were no sunlight, there would be no life on earth. Another point is that because the Sun has no defined surface like that of the Earth, it is too hot to be anything but gas. So what we see as the Sun’s atmosphere is a photosphere, a sphere of light. Which in turn emits light because of its high temperature. The energy that comes from the center of the sun, its core, is created by hydrogen-to-helium fusion. With this energy, atoms absorb photons and convert their energy to kinetic energy, maintaining the high temperatures needed for fusion. The frequency of these collisions and the temperature decrease with increasing distance from the core, however, and at the photosphere, which is the sun 's outer layer, some of the photons radiate into space. They are responsible for the light that humans see on

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