2. Photoelectron Spectrometers

4. Survey of the Universe Harry Kroto 2004

5. Interstellar Matter Harry Kroto 2004

8. http://www.ugcs.caltech.edu/~yukimoon/BigBang/

10. Gamow

12. Big Bang Hydrogen

15. Milky Way Fog

16. We can only see about 1/6 (ca 6000ly) of the way to the Galctic Centre due to scattering by gas and dust in the disk

17. Harry Kroto 2004 H...H 3 Body Collision

18. Total energy must be conserved and in a plant at snooker or billiards the blue ball takes away the energy and the white and red can thus remain in contact after collision

19. Reaction Coordinate - Energy Harry Kroto 2004 A + B Products C

21. Radioastronomy History

22. Harry Kroto 2004 3 Degree Background

24. Harry Kroto 2004 M e  n ’  n ”  Franck Condon

25. Harry Kroto 2004 Ro-vib-ronic Spectra

26. Harry Kroto 2004 [H o + V(t)]  = iħ  /  t Time Dependent Theory

27. Fermi Golden Rule I

28. Harry Kroto 2004. CN CN Spectrum

30. H 2 Dissociation Energy GH&M K&W