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Hertzsprung-Russell Diagram. Astrophysics Lesson 11. Learning Objectives. To recap:- Analysis of absorption spectra gives clues as to the make up and surface temperature of stars. To know:- How to draw a Hertzsprung-Russell Diagram The range on each axis.
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Hertzsprung-Russell Diagram Astrophysics Lesson 11
Learning Objectives To recap:- Analysis of absorption spectra gives clues as to the make up and surface temperature of stars. To know:- How to draw a Hertzsprung-Russell Diagram The range on each axis. The position of white dwarfs, the main sequence and red giants
Homework Open book exam to do over the next week. Real mock exam the first week after half term (will be in Mr. Moore’s lesson).
Main Classes Oh Be A Fine Girl, Kiss Me!
For Example • Therefore in the Sun, the spectral lines would be seen for iron and calcium, indicating a surface temperature of about 6000 K. • Very hot stars show spectral lines for light elements while cool stars will show up heavy elements, and spectra for molecules as well.
Sub-divisions • The classifications of stars according to spectra are also subdivided further with numbers (e.g A5) to allow the surface temperature to be determined within about 5 %.
Question • What would you not see when looking at the spectrum of the red giant Betelgeuse? What elements would you expect to see?
Answer • You would see little evidence of Balmer Lines. • You would see spectral lines for iron and calcium. • You would also see evidence for molecules of titanium dioxide.
Classification • In the last topic we saw how we can classify stars according to their apparent and absolute magnitude, and their temperature and spectral analysis. • However these classifications do not tell us a great deal about the age of the star or how it has evolved.
HR Diagram • Hertzsprung and Russell noticed that a plot of absolute magnitude against temperature (or spectral class) showed certain patterns. • This is referred to as a Hertzsprung-Russell diagram.
HR Diagram Notes • Notice that:- • the temperature scale is decreasing (50,000 K to 2,500 K). • the classes of star are placed alongside the temperature scale; • the luminosity scale is logarithmic to compress it; • But AQA seem to prefer the absolute magnitude scale going from -15 to 10.
Main Sequence • The long, diagonal band is called the main sequence. • This is the long stable phase of a star’s life where they are fusing hydrogen into helium. • The Sun is a main sequence star.
Red Giants • Objects that have a high luminosity and a low surface temperature must have a large surface area. (Stefan’s Law) • These stars are called red giants and are found in the top right corner of the HR diagram. • These are stars that have moved off the main sequence and fusion reactions other than H He are taking place.
White Dwarfs • Objects that have a low luminosity and a high surface temperature must have a low surface area. (Stefan’s Law). • These stars are called white dwarfs and lie in the bottom right hand corner of the HR diagram. • White dwarfs are stars at the end of their lives, where all of their fusion reactions have stopped and are they are just cooling down.
Luminosity (Sun = 1) Surface Temp (K)Group • Sun1.05800Main sequence • Betelgeuse20 000 Red Supergiant • Aldebaran2004700 • Regulus 14000 Main Sequence • Rigel 20000 Main Sequence • Sirius B 0.00 220000
