1. A photon checks into a hotel. The desk clerk asks, “Do you need help with your luggage?” The photon replies, “I don’t have any. I’m travelling light.” (get it?)

2. The Electromagnetic Spectrum AKA--- LIGHT!

3. Big Questions: What is light? Why do scientists study light?

4. Image from My NASA Data website

5. Properties of EM Waves: Wavelength  The distance between peaks or troughs of a wave  Measured in nanometers (nm) or angstrom (Å)  Each type of EM radiation (and each color of visible light) has a different wavelength

6. Properties of EM Waves: Frequency  The is measured by the number of waves (or cycles) that pass a given point in one second.  The frequency is measured by the number of waves (or cycles) that pass a given point in one second.  Measured in Hertz -- Hz 0 1 sec 15 Hz 3 Hz

7. Energy and Wave Properties  All EM Waves travel at the speed of light- 300,000 km/s  Frequency and Wavelength are inversely proportional

8. Electromagnetic Radiation EMR has properties of both a wave and a particle – Photons are the elementary particles of electromagnetic radiation of all wavelengths – Photons can travel through the vacuum of space All types of EMR carry energy

9. Studying light By studying light energy at different wavelengths along the electromagnetic spectrum, astronomers can learn about: – An object’s size – An object’s temperature – The amount of energy an object is producing – The elements found in that object – An objects speed and direction relative to Earth – The interstellar matter between that object and Earth

10. Doppler Effect A change in wavelength as a result of a shift in the frequency of sound waves or electromagnetic radiation. Can show the direction a celestial object is traveling in relation to Earth

11. Doppler Effect video explanation https://www.youtube.com/watch?v=h4OnBYrbCjY

12. Red Shift Radiation emitted by objects moving away from earth is stretched or shifted to the RED end of the spectrum- RED SHIFT EARTH

13. Blue Shift Objects such as stars and galaxies moving toward Earth seem to have their wavelengths of radiation squeezed and the frequency increased- Blue Shift EARTH

15. Doppler Effect Simulation http://astro.unl.edu/classaction/animations/light/dopplershift.html

16. Spectroscopy

18. Spectroscope- a tool that disperses a ray of light into its constituent colors Astronomers can learn about a celestial object by studying the wavelengths, intensities, and patterns of its spectrum

19. Spectroscopy When looked at through a spectroscope, every gas gives off a different spectrum of colors, just like every person has a different fingerprint. When astronomers use a spectroscope to look at stars, they can determine what type of gases the stars are made of by the color of the lines in the spectrum they see. Astronomers can tell the temperature of a star by studying the intensities of the lines in the spectrum. The thickness of the lines tell astronomers about the rotation speed, density, magnetic field and gas turbulence of the star

20. Continuous Spectrum An unbroken band of colors, such as a Rainbow Shows the size, temperature, and life expectancy of a star

21. Emission or Bright Line Spectrum: An unevenly spaced series of lines of different colors and different brightness Determined by the chemical make up of an object

22. Dark line or absorption spectrum A series of dark or absorption lines that appear on the continuous spectrum Show the make up of cooler gases in the universe

23. Big Questions: What is light? Why do scientists study light?