1. Light and the Electro- magnetic Spectrum

2. Light and the Electromagnetic Spectrum Almost all of our information on the heavens is derived from the light we see We have returned samples from the Moon and a comet –Also obtained meteor samples We have landed (with unmanned probes) on only a handful of planets and moons

3. EM Spectrum in Astronomy If we could only observe in visible light, our knowledge of the universe would be greatly limited By looking at objects at different wavelengths, we get a different view and lots more information Some objects are only visible at certain wavelengths

4. Objects in space that emit different frequencies on the EM Spectrum

5. The Electromagnetic Spectrum Human eyes are only able to process information from the visible part of the spectrum Toward longer wavelengths, the spectrum includes infrared light, microwaves, and radio Toward shorter wavelengths, the spectrum includes ultraviolet light, X- rays, and gamma rays All of these are forms of electromagnetic radiation

6. Wavelength The distance from one wave crest to the next Radio waves have longest wavelength and Gamma rays have shortest!

7. What do we mean by wavelength? Light as a Wave One way to think about light is as a traveling wave A wave is just a disturbance in some medium (water, air, space) A wave travels through a medium but does not transport material A wave can carry both energy and information

8. Wave Terminology Wavelength - distance between two like points on the wave Amplitude - the height of the wave compared to undisturbed state Period - the amount of time required for one wavelength to pass Frequency - the number of waves passing in a given amount of time

9. Wave Relationships Note that light is always traveling at the same speed (c ~ 3 x 10 8 m/s, or 300,000 m/s, or 186,000 miles/sec, or 7 times around the earth in 1 second!) –Remember: velocity = wavelength x frequency If frequency increases, wavelength decreases If frequency decreases, wavelength increases

10. Wavelength Units Meters: More commonly in nanometers (1 nm = 10 -9 meters) Angstroms still used –Named for Swedish Astronomer who first named these wavelengths –1 nanometer = 10 A o

11. Wavelengths of Light - Visible What we see as white light is actually made up of a continuum of components Traditionally, we break white light into red, orange, yellow, green, blue, indigo, and violet (ROY G BIV) There is actually a continuous transition of color, each with its own wavelength and frequency

14. Bright Line Spectra

15. Doppler Effect The motion of an object can be measured through a change in the frequency of the waves emitted by the object The increase in pitch of an approaching police car is caused by the compression of the sound wave –The pitch decreases as the police car moves away

17. Doppler Shift In astronomy, the same effect happens to light waves A source that is moving away will appear redder (redshift) A source that is moving toward us will appear bluer (blueshift) Note: Only objects moving toward or away from us (radial motion) will show this effect

18. Which spectrum (spectra) indicates an object is moving towards earth? Which spectrum (spectra) indicates an object is moving away from earth?