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Learning from Light: Spectra, Composition, Temperatures, and Speed

Explore how light spectra can inform us about the composition of objects, their temperatures, and their speeds. Learn about absorption and emission lines, thermal radiation, the Doppler effect, and more.

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Learning from Light: Spectra, Composition, Temperatures, and Speed

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  1. Chapter 5Light: The Cosmic Messenger

  2. 5.2 Learning from Light • Our goals for learning • What types of light spectra can we observe? • How does light tell us what things are made of? • How does light tell the temperatures of planets and stars? • How does light tell us the speed of a distant object?

  3. What types of light spectra can we observe?

  4. Example: Solar Spectrum

  5. How does light tell us what things are made of? • Electrons in atoms have distinct energy levels. • Each chemical element, ion, molecule, has a unique set of energy levels.

  6. Distinct energy levels lead to distinct emission or absorption lines. Hydrogen Energy Levels

  7. Chemical Fingerprints • Every atom, ion, and molecule has a unique spectral “fingerprint” • We can identify the chemicals in gas by their fingerprints in the spectrum. • With additional physics, we can figure out abundances of the chemicals, and much more.

  8. Thought QuestionWhich letter(s) labels absorption lines? A B C D E

  9. Which letter(s) labels absorption lines? A B C D E

  10. Thought QuestionWhich letter(s) labels the peak (greatest intensity) of infrared light? A B C D E

  11. Which letter(s) labels the peak (greatest intensity) of infrared light? A B C D E

  12. Thought QuestionWhich letter(s) labels emission lines? A B C D E

  13. Which letter(s) labels emission lines? A B C D E

  14. How does light tell us the temperatures of planets and stars? Thermal Radiation • Nearly all large or dense objects emit thermal radiation, including stars, planets, you… • An object’s thermal radiation spectrum depends on only one property: its temperature

  15. Two Properties of Thermal Radiation: Hotter objects emit more light at all frequencies per unit area. Hotter objects emit photons with a higher average energy.

  16. Spectra

  17. Thought QuestionWhich is hotter? • A blue star. • A red star. • A planet that emits only infrared light.

  18. Which is hotter? • A blue star. • A red star. • A planet that emits only infrared light.

  19. Thought QuestionWhy don’t we glow in the dark? • People do not emit any kind of light. • People only emit light that is invisible to our eyes. • People are too small to emit enough light for us to see. • People do not contain enough radioactive material.

  20. Why don’t we glow in the dark? • People do not emit any kind of light. • People only emit light that is invisible to our eyes. • People are too small to emit enough light for us to see. • People do not contain enough radioactive material.

  21. How does light tell us the speed of a distant object? The Doppler Effect.

  22. The amount of blue or red shift tells us an object’s speed toward or away from us:

  23. Doppler shift tells us ONLY about the part of an object’s motion toward or away from us:

  24. The Doppler Effect

  25. Same for Light

  26. Thought QuestionI measure a line in the lab at 500.7 nm.The same line in a star has wavelength 502.8 nm. What can I say about this star? • It is moving away from me. • It is moving towards me. • It has unusually long spectral lines.

  27. I measure a line in the lab at 500.7 nm.The same line in a star has wavelength 502.8 nm. What can I say about this star? • It is moving away from me. • It is moving towards me. • It has unusually long spectral lines.

  28. Measuring Redshift

  29. Measuring Redshift

  30. Measuring Velocity

  31. Measuring Velocity

  32. Doppler Effect Summary Motion toward or away from an observer causes a shift in the observed wavelength of light: • blueshift (shorter wavelength)  motion toward you • redshift (longer wavelength)  motion toward you • greater shift  greater speed

  33. What types of light spectra can we observe? Thermal radiation spectrum – looks like rainbow of light Absorption line spectrum – specific colors are missing from the rainbow Emission line spectrum– see light only of a specific color What have we learned?

  34. How does light tell us what things are made of? Every kind of atom, ion, and molecule produces a unique set of spectral lines. How does light tell use the temperatures of planets and stars? We can determine temperature from the spectrum of thermal radiation What have we learned?

  35. What have we learned? • How does light tell us the speed of a distant object? • The Doppler effect tells us how fast an object is moving toward or away from us. • Blueshift:objects moving toward us • Redshift: objects moving away from us

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