1. 1 Fingerprints in Sunlight Understanding Spectroscopy Stanford University Solar Center

2. 2 How can we study the stars & Sun? We can ’ t get there from here We can ’ t get there from here Only/primary way of learning about distant objects is through their light (electromagnetic spectrum) Only/primary way of learning about distant objects is through their light (electromagnetic spectrum) Light has ‘ fingerprints ” which provide information about it Light has ‘ fingerprints ” which provide information about it How can we “ read ” these fingerprints and what do they tell us about the star? How can we “ read ” these fingerprints and what do they tell us about the star? No matter how good your telescope, a star is only a point of light No matter how good your telescope, a star is only a point of light

3. 3 What is the spectrum of light? Anything hotter than absolute zero radiates/emits energy, i.e. light Anything hotter than absolute zero radiates/emits energy, i.e. light Sun & stars emit a continuous spectrum ( “ black body ” ) of EM radiation Sun & stars emit a continuous spectrum ( “ black body ” ) of EM radiation Our eyes see “ white ” light, which is made of the spectrum of colors visible in a rainbow Our eyes see “ white ” light, which is made of the spectrum of colors visible in a rainbow Spectrum = “ The distribution of energy emitted by a radiant source, e.g. the Sun, arranged in order of wavelengths ” Spectrum = “ The distribution of energy emitted by a radiant source, e.g. the Sun, arranged in order of wavelengths ”

4. 4 What is a spectrograph? A relatively simple-to- understand scientific instrument to look at a spectrum A relatively simple-to- understand scientific instrument to look at a spectrum Like a prism – breaks light into its colors Like a prism – breaks light into its colors Thin, rectangular slit produces a rectangle of light Thin, rectangular slit produces a rectangle of light Example output from a spectrograph

5. 5 Your Simple Spectrograph Diffraction grating Diffraction grating (similar effect to prism (similar effect to prism or CD) or CD) Slit & light source Slit & light source Scale (optional) Scale (optional) Eye or instrument Eye or instrument for viewing for viewing

6. 6 Most astronomy is done with spectrographs! Your spectrograph Stanford Solar Center Home-made spectrograph attached to telescope NASA ’ s SOHO Spacecraft Hubble ’ s new Cosmic Origins Spectrograph Student spectrograph & gas lamp

7. 7 What can we learn with a spectrograph? Sometimes there are extra bright colors Sometimes there are missing colors To infraredTo ultraviolet

8. 8 Fingerprints in Light The extra or missing colors indicate certain chemical elements (e.g. hydrogen, helium, gold, etc.) have affected the light The extra or missing colors indicate certain chemical elements (e.g. hydrogen, helium, gold, etc.) have affected the light Each chemical element changes the spectrum either by making certain colors brighter or removing certain colors Each chemical element changes the spectrum either by making certain colors brighter or removing certain colors Each chemical element has a different and unique pattern of colors, hence the “ fingerprints ” Each chemical element has a different and unique pattern of colors, hence the “ fingerprints ”

9. 9 Example fingerprints Hydrogen Hydrogen Helium Helium Sodium Sodium

10. 1010 Absorption vs. Emission? Absorption lines – produced when a chemical element has absorbed energy Absorption lines – produced when a chemical element has absorbed energy Emission lines – produced when a chemical element has emitted energy Emission lines – produced when a chemical element has emitted energy Whether something produces an absorption or emission spectrum depends upon its temperature, the temperature of any gas between it and the observer, and the observer’s line of site.

11. 11 Some Elements on the Sun Hydrogen (H) Hydrogen (H) Helium (He) Helium (He) Sodium (Na) Sodium (Na) Oxygen (O 2) Oxygen (O 2) Iron (Fe) Iron (Fe) Sun

12. 12 Build your spectroscope Point your spectrograph to an incandescent light or sunlight Point your spectrograph to an incandescent light or sunlight Next, point your spectrograph to a fluorescent light bulb Next, point your spectrograph to a fluorescent light bulb What do you see? Especially notice the bright green line What do you see? Especially notice the bright green line

13. 13 You should have seen a continuous spectrum with some extra bright colored lines Fluorescent bulb, old style Fluorescent bulb, old style Fluorescent bulb, new style Fluorescent bulb, new style Mercury Mercury What do you conclude? What do you conclude?

14. 14 Another experiment Work in teams Work in teams Take your candle Take your candle Burn a hollow around your wick Burn a hollow around your wick Put salt in the hollow, or pour salt onto the flame Put salt in the hollow, or pour salt onto the flame Look for a brief flash Look for a brief flash What do you see? What do you see?

15. 15 What did you see? The candle The candle Sodium spectrum Sodium spectrum What is salt? What is salt? Sodium chloride

16. 16 What secrets do spectra tell us? Chemical Composition Chemical Composition Temperature Temperature Movement Movement Magnetic fields Magnetic fields

17. 1717 Spectra tell us about composition Am emission or absorption line means a specific chemical element has been involved with the light you are seeing Am emission or absorption line means a specific chemical element has been involved with the light you are seeing Careful, though. The element could be from the source, or from an intervening plasma or gas cloud Careful, though. The element could be from the source, or from an intervening plasma or gas cloud

18. 1818 Reading a spectrum A spectrum can be graphed as wavelength vs. intensity Measure Here Location and shape changes of the line give us a lot of additional information

19. 1919 Spectra tell us temperatures If you look at the strongest colors or wavelength of light emitted by a star, then you can calculate its temperature If you look at the strongest colors or wavelength of light emitted by a star, then you can calculate its temperature

20. 2020 How do spectra tell us about movement? A Doppler shift happens when an object is moving towards or away from us, as in a siren coming towards us A Doppler shift happens when an object is moving towards or away from us, as in a siren coming towards us Wavelength is influenced by the movement Wavelength is influenced by the movement It works with sound, with light, with any wave It works with sound, with light, with any wave

21. 2121 Doppler, continued Motion away from us results in a “ red shift ” Motion away from us results in a “ red shift ” Motion towards us results in a “ blue shift Motion towards us results in a “ blue shift Why don ’ t they call it a violet shift?

22. 2222 Spectra tell us about magnetism Sunspots are magnetic storms on the Sun Magnetic fields cause spectral lines to split into thirds

23. 2323 The Sun “ in H alpha ” Hydrogen alpha filters allow only light in the 656nm wavelength to pass through. This is the line that appears in the red part of the spectrum when an electron moves from Level 3 to Level 2. This allows us to see light produced at a particular temperature in the photosphere (surface) of the Sun.

24. 24 NASA ’ s Solar Dynamics Observatory (SDO) Launched February 2011 to study the Sun Launched February 2011 to study the Sun 3 instruments, AIA, EVE, HMI 3 instruments, AIA, EVE, HMI HMI is from the Solar Observatories team at Stanford – my group! HMI is from the Solar Observatories team at Stanford – my group! HMI works similarly to a spectroscope HMI works similarly to a spectroscope

25. Each SDO image of the Sun is taken in a different spectral line (of extreme ultraviolet light) 25

26. 26 IRIS (Interface Region Imaging Spectrograph) Launching sometime after December 2012 Launching sometime after December 2012 Goal is to understand the interface between the Sun ’ s photosphere (visible surface) and corona (atmosphere) Goal is to understand the interface between the Sun ’ s photosphere (visible surface) and corona (atmosphere) IRIS is a spectrograph! IRIS is a spectrograph!

27. 27 What are your questions? Have your students make simple spectrographs out of CDs Have your students make simple spectrographs out of CDs Use your spectrographs to look at moonlight, reflected sunlight, fluorescent lights, neon signs, mercury vapor and sodium streetlights, candles, their TV set, etc. Use your spectrographs to look at moonlight, reflected sunlight, fluorescent lights, neon signs, mercury vapor and sodium streetlights, candles, their TV set, etc. Show them how science is done by teaching about the Sun and spectroscopy! Show them how science is done by teaching about the Sun and spectroscopy! Thank you! Sun Dragon Art image © by Henry Roll. Used with permission.