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LIFECYCLES OF STARS

LIFECYCLES OF STARS. Option 2601. Stellar Physics. Unit 1 - Observational properties of stars Unit 2 - Stellar Spectra Unit 3 - The Sun Unit 4 - Stellar Structure Unit 5 - Stellar Evolution Unit 6 - Stars of particular interest. Unit 6. Particularly Interesting Stars.

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LIFECYCLES OF STARS

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  1. LIFECYCLES OF STARS Option 2601

  2. Stellar Physics • Unit 1 - Observational properties of stars • Unit 2 - Stellar Spectra • Unit 3 - The Sun • Unit 4 - Stellar Structure • Unit 5 - Stellar Evolution • Unit 6 - Stars of particular interest

  3. Unit 6 Particularly Interesting Stars

  4. Particularly Interesting Stars • Binaries – visual, spectroscopic, eclipsing • Variable stars • Active/interacting binaries (Novae) • Stellar pulsations • Cepheid variables and the distance scale

  5. Types of binary system

  6. Spectroscopic Binaries

  7. Eclipsing Binaries

  8. Eclipsing Binaries

  9. Information from Binary Systems • Masses of components • Dimensions of components (particularly in eclipsing systems) • Physical characteristics of systems

  10. (Other) Variable Stars • Intrinsic variables… i.e. pulsating stars • Geometric (extrinsic) variables… i.e. eclipsing systems • Naming variables… constellation & letters beginning with R • R…. To Z, then RR…. To ZZ (i.e. R CrB) • Then Vijk constellation (i.e. V471 Tau)

  11. Accretion in Binaries

  12. Novae

  13. Novae • Brightness increases by 10 magnitudes during outburst • Rise time 2-3 days • Gradual decline over months (fast novae) or years (slow novae) • Material ejected with velocities up to ~2000km s-1 • Explosions can repeat (recurrent novae)

  14. Nova Cassiopeiae 1993 light curve (first 3 months)

  15. Nova Cassiopeiae 1993 light curve (first 2½ years)

  16. Nova Cassiopeiae 1995 light curve

  17. Pulsating Stars • Pulsating stars are not in hydrostatic equilibrium • Star is partially ionized at some critical depth • Degree of ionization sensitive to small temperature changes • Small perturbation can be “amplified”

  18. MAX. COMPRESSION Pressure driving Max. opacity & ionisation, min. photon flux COMPRESSION EXPANSION Max. compression rate Max. expansion rate Gravity (restoring force) Min. opacity & ionisation, max. photon flux MAX. EXPANSION Cycle of a pulsating star Phase

  19. H-R diagram for pulsating stars

  20. Cepheid Variables Typical Cepheid light curve

  21. Cepheid Variables

  22. Cepheid Variables

  23. The period-luminosity relation for Cepheids

  24. Redshift • Edwin Hubble discovers galaxies are receding from us (c. 1930) • Hubbles Law - speed increases with distance • Expansion of the Universe - Big Bang theory

  25. Cepheids in M100

  26. Beyond M100

  27. Unit 6 Particularly Interesting Stars

  28. Particularly Interesting Stars • Binaries – visual, spectroscopic, eclipsing • Variable stars • Active/interacting binaries • Stellar pulsations • Cepheid variables and the distance scale

  29. Stellar Physics • Unit 1 - Observational properties of stars • Unit 2 - Stellar Spectra • Unit 3 - The Sun • Unit 4 - Stellar Structure • Unit 5 - Stellar Evolution • Unit 6 - Stars of particular interest

  30. LIFECYCLES OF STARS Option 2601

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