The sun is about 864000 miles wide and filled with sweltering hot gases. Hydrogen is the most abundant element present in the Sun, composition of the Sun by its constituent mass is 71% hydrogen (H), 27% helium (He) and 2% other heavier elements. Inside the Sun the gravitational pull compresses the gases, and increase the temperature and pressure at the core. (CAIN, F., 2009) The temperature is about 10000°F on the surface and more than 28 million degrees Fahrenheit at the core of the sun. The pressure at the core of the sun is 250 billion times the ...
Nuclear Fusion College Essays Samples For Students
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MEM 695
Abstract
The purpose of this research paper is to introduce the different types of energy resources utilized worldwide. This paper discusses the history of the different resources used, starting with the utilization of conventional fossil fuel based technologies, the emergence of nuclear power and finally, the commercialization of renewable energy resources. The main objective of this research paper is to provide an insight on how these energy sources are accessed, utilized, distributed and developed. The paper also seeks to impact of the utilization of these various energy resources on the environment, especially the effect of continued utilization of ...
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The Sun has been with us for 4 billion years, and is the nearest star to the Earth. The Sun is comprised of about 74% of hydrogen, 25% of helium, and 1% of other elements. The surface of the Sun has a temperature of about 5800 K. The core of the Sun has a temperature ranging from 10 – 15 million Kelvin. This temperature range is high enough to activate nuclear fusion within the Sun. Here, four protons will fuse together to obtain a helium nucleus containing two protons and two neutrons via a proton-proton chain. The core of the ...
Nuclear energy is a clean source of energy because it does not emit green house gas. Nuclear power plant produces energy like any other steam-electric power plant; but in nuclear power plant, source of heat to boil water is chain reaction due to nuclear fission of Uranium rather than using coal, oil or fossil fuel. Nuclear reaction is of two types- Nuclear Fission and Nuclear Fusion. Nuclear Fusion produces more heat than Nuclear Fission. So, there are possibilities of using Nuclear Fusion for the eventual generation of electrical power. But Fusion cannot be controlled and a perfected nuclear reactor has not ...
Future Energy
Introduction
The increasing quest for renewable sources of energy has greatly influence perception and appreciation of the benefits that could be derived from solar energy. Although the use of solar power as a form of energy to generate electrical energy is not a new technology, majority are yet to be aware of the benefits of using such forms of energy to both health and environment. It uses date back to ancient times where people make use of the energy to achieve their daily task i.e. drying purposes. The issue with the energy from sun could be associated with the challenges ...
Gravitational, electromagnetic, strong and weak nuclear forces. Gravitational force is an attraction between any two pieces of matter in the universe. Electromagnetic force is present in pieces of matter, which are able to carry electrical charge. Strong force is holding the nuclei of atoms together. Weak force is responsible for radioactive decay.
Molecules are built from the atoms and atoms consist of protons, neutrons and electrons. Protons and neutrons are built of smaller particles called quarks.
Electromagnetic spectrum is the range of all the light in the universe. Depending on the wavelength and frequency there are radio, micro, infrared, ...
Blue supergiant stars are staller evolutions that have resulted over millions of years. Stars during the main sequence phase spend a majority of their lives. During the main sequence stage, the star converts hydrogen to helium by nuclear fusion in the cores of stars the process also known as proton-proton chain. After spending of hydrogen fuel, the star will collapse and heat up rapidly causing the outer layers to expand inwards. When the core is very hot, the energy spreads through the interior of the star’s large surface area. The different fusion rates of different elements vary wildly to ...