The document discusses spectroscopy and spectral lines. It explains that spectra can be observed using a spectroscope, which contains a discharge tube, diffraction grating, and eyepiece. Gases like neon and helium emit distinct spectral lines that can be observed through the spectroscope and related to the energies of electron transitions in the gases. The wavelengths of the prominent red and blue lines in neon and helium spectra are measured and converted to frequencies and energies using physics equations.
18. Line Red Blue
656 nm
= 656 x 10-9 m
434 nm
= 434 x 10-9 m
f
=
=
3108
656109
= 4,57 x 1014 Hz
19. Line Red Blue
656 nm
= 656 x 10-9 m
434 nm
= 434 x 10-9 m
f
=
=
3108
656109
= 4,57 x 1014 Hz
=
=
3108
434109
= 6,91 x 1014 Hz
20. Line Red Blue
656 nm
= 656 x 10-9 m
434 nm
= 434 x 10-9 m
f
=
=
3108
656109
= 4,57 x 1014 Hz
=
=
3108
434109
= 6,91 x 1014 Hz
21. Line Red Blue
656 nm
= 656 x 10-9 m
434 nm
= 434 x 10-9 m
f
=
=
3108
656109
= 4,57 x 1014 Hz
=
=
3108
434109
= 6,91 x 1014 Hz
E = hf
= h f
= 6,63 10-34 4,57 x 1014
= h f
= 6,63 10-34 6,91 x 1014
22. Line Red Blue
656 nm
= 656 x 10-9 m
434 nm
= 434 x 10-9 m
f
=
=
3108
656109
= 4,57 x 1014 Hz
=
=
3108
434109
= 6,91 x 1014 Hz
E = hf
= h f
= 6,63 10-34 4,57 x 1014
= 3,03 x 10-19 J
= h f
= 6,63 10-34 6,91 x 1014
= 4,68 x 10-19 J