Archive for October, 2008

Life Cycle of Stars

The Sun

Some stats about our nearest star:

  • 150 million km from Earth
  • light takes 8½ minutes to travel from Sun to Earth
  • surface temperature about 6000oC
  • core temperature about 15,000,000oC
  • main process is fusion of hydrogen nuclei to helium nuclei
  • estimated age of our sun is 5 billion years
  • estimated lifespan is 10 billion years
  • radiation from the sun includes a range of wavelengths from the entire electromagnet spectrum including cosmic rays

Life cycle slideshow

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A Flash animation of star life cycles can be found here

Hertzsprung-Russell diagram

This is a plot of absolute magnitude (actual brightness) of a star against the surface temperature of the star. When data from a number of known stars is plotted it shows the main sequence clearly as a cluster as well as separate clsuters for dwarf stars and giants.

To find out more on this topic you need to study astrophysics (click here for Astrophysics made simple)

Yr 8 Yearly Revision Guide 2008

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Yr 9 Revision Guide

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Yr 8 Revision Guide 2008

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Yr 7 Yearly Revision Guide

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10 Yearly revision

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See Board of Studies (BOS) for past papers – you can download past papers here

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virus reproduction

Gerroa 08 Excursion

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