Ch. 27.2 Stellar Evolution. Nebula—a cloud of dust and gas. 70% Hydrogen, 28% Helium, 2% heavier...
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Transcript of Ch. 27.2 Stellar Evolution. Nebula—a cloud of dust and gas. 70% Hydrogen, 28% Helium, 2% heavier...
![Page 1: Ch. 27.2 Stellar Evolution. Nebula—a cloud of dust and gas. 70% Hydrogen, 28% Helium, 2% heavier elements. Gravity pulls the nebula together; it spins.](https://reader033.fdocuments.net/reader033/viewer/2022051401/5697bf711a28abf838c7e09e/html5/thumbnails/1.jpg)
Ch. 27.2 Stellar Evolution
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• Nebula—a cloud of dust and gas. 70% Hydrogen, 28% Helium, 2% heavier elements.
• Gravity pulls the nebula together; it spins and flattens into a disk of matter with a central concentration called a protostar.
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• Pressure and temperature increases in the protostar, until the core reaches about 10,000,000 degrees C, and then nuclear fusion starts, releasing energy, and a star is born.
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Main-Sequence Stars
• Main-sequence stage is the longest stage in a star’s life.
• Hydrogen is converted to helium by nuclear fusion, and energy is released.
• The star is in balance. The inward pull of gravity is balanced by the energy from fusion.
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Giants and Supergiants
• 3rd stage, when hydrogen in the star’s core is exhausted. Hydrogen fusion continues in the star’s outer layers.
• Core contracts due to gravity, and its temperature increases.
• Helium in the core fuses into carbon.
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• Combined helium and hydrogen fusion causes outer shell of star to greatly expand.
• Star is now a red giant (10 times bigger than sun) or a red supergiant (100 times bigger than sun)
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White Dwarf Stars
• For medium-sized stars, after helium fusion, the giant stage is over.
• Outer gasses are lost, and a core is revealed, which heats and illuminates the expanding gasses, forming a planetary nebula.
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• The last inner matter collapses inward due to gravity, forming a hot, dense white dwarf star.
• It shines for billions of years, but eventually becomes cooler and fainter, until energy emmission stops, and it becomes a black dwarf.
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Novas
• Explosions on the surface of some white dwarfs, causing brightness to increase by thousands of times for a few days.
• Believed to be caused by gas (from a companion star) buildup on the white dwarf’s surface.
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Supernovas
• Occur when high-mass stars (10 to 100 times mass of the sun) finish the supergiant stage.
• Gravitational collapse causes fusion to restart…carbon is converted into iron…then gravity causes the iron core to collapse and fuse into all heavier elements, in a gigantic explosion.
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Neutron Stars
• What may be left after supernovae explosions…super dense rotating balls of pure neutrons, with a diameter of about 30 km.
• Pulsars are neutron stars that emit beams of radiation.
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Black Holes
• In the most massive stars, gravity crushes the matter down into zero volume.
• Detected by x-rays given off as surrounding matter falls into a black hole.
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