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Stellar Evolution

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Nuclear Fusion a nuclear reaction in which to atoms are fused together... DENSITY INCREASES TREMENDOUSLY. D = 1,000,000 g/cm3. 1 sugar cube 1 car ... – PowerPoint PPT presentation

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Title: Stellar Evolution


1
Stellar Evolution
  • The life-cycle of stars

2
Star Energy
  • Nuclear Fusion a nuclear reaction in which to
    atoms are fused together
  • New elements are created and energy is released.
  • This process is responsible for creating ALL
    elements found in the universe
  • in other words, we are all made from star dust.

3
Star Energy (cont)
  • Hydrogen fusion
  • H H ? He
  • Helium fusion
  • He He ? Be
  • As the mass of elements increases, energy
    production increases

Energy
More Energy
4
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5
1. Nebula
  • A cloud of gas and dust
  • Gravity causes the cloud to collapse and condense
  • Temperatures begin to increase Glows
  • Fusion begins at VERY high temps.

(Some of the extra gas and dust may form planets)
6
Main Sequence Stars
  • Core reaches a temp of 15 million K.
  • Hydrogen begins to fuse into Helium in the core.
  • 90 of stars lifetime is spent in the main
    sequence stage.
  • Classified based on temperature and luminosity

7
Giant Stars
  • Core decreases in size as
  • All (or most) H is consumed
  • He fusion is occurring producing more energy
  • Diameter increases x10
  • Surface temp decreases as star expands

8
Super Giants
  • Form from massive stars
  • A chain of reactions take place in the core
    producing He, C, O, Ne, Mg, Si, S, Ar, Ca, Ti,
    Cr, Fe
  • Highest temperature Blue Super Giants
  • Usually explode in a tremendous event called a
    supernova

9
Nova/Super Nova
  • The core of a giant star produces too much energy
    in its core and causes the outside of the star
    to expand.
  • The outer layer of gasses are blown out to space
    (nova, or supernova), leaving behind a small, hot
    core

10
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11
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12
White Dwarf
  • Stars decrease in size same diameter as earth,
    mass stays the same
  • Mass of sun, size of Earth
  • DENSITY INCREASES TREMENDOUSLY
  • D 1,000,000 g/cm3
  • 1 sugar cube gt 1 car
  • Solid, but still hot, so it is glowing
  • Luminosity decreases

13
Neutron stars
  • Form from the remains of extremely massive stars
    after a supernova.
  • Very small 30 km across
  • D 2 x 1014
  • 1 sugar cube mass of humanity

14
The fate of our Sun
15
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