Stars: The Light of Space. . By Cody Smith, Kyle Taddeo, and Jacob Dulworth. What is a Star? .
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By Cody Smith, Kyle Taddeo, and Jacob Dulworth.
Look up in the night sky and you'll see lots of stars. But what exactly is a star? In a scientific sense, a star is ball of hydrogen and helium with enough mass that it can sustain nuclear fusion at its core. The sun is a star, but there are many stars with all shapes and colors. The sun and most other stars are made of gas and a hot, gassy substance known as plasma. But some stars, called white dwarfs and neutron stars, consist of closely packed atoms or subatomic particles. These stars are therefore much more dense than Earth. The star is mainly composed of plasma. The star’s surface is 99.9% plasma. Plasma is highly sensitive to magnetism making it highly sensitive and unstable.
Stars form in dense molecular clouds within galaxies. These clouds of dust and gas obscure the early stages of stellar formation from optical telescopes. Gravity is the force responsible for stellar formation and the mass of material that forms at star largely determines its life and fate. The most common nuclear process which is the energy force of the star is the proton- proton chain which is what keeps a star “living.” After ten billion years, a main sequence would commonly have converted about 10% of its hydrogen to helium. Outside of the range of pressures there is still mostly hydrogen, but it cannot be used because the pressures are not high enough to initiate fusion. This helium begins to contract and the outer layers begin to expand and cool glowing redder. The star is now a red giant. When a star becomes a red giant the nuclear fusion begins.
The star was previously unable to fuse the helium; however, now that the core has contracted, the added pressure is enough to fuse helium into heavier elements. Simultaneously, hydrogen fusion also occurs at this point in a shell around the helium core, for pressures there have also increased enough for hydrogen to fuse. Life expectancy from here on is about 100,000,000 years. After this process occurs the red giant is know mostly composed of carbon. The outer shell of the Star then expands two times its size because of the lack of helium in the core so the hydrogen expands exponentially. The star then collapses on its self because the balance between gravity and the output and input of energy of the star is off balance. The star then collapses on itself and explodes creating a supernova. Another option is the core then remains of neutrons and collapses on it self creating a black hole.