1. Using the Electromagnetic Spectrum
Objective: Students will explain the need for observing the universe using different wavelengths and will be able to relate wavelength, frequency, and energy

2. The Electromagnetic Spectrum

3. Why look at the Universe through different wavelengths?
We get different information depending on how we observe it. Think of what different things you learn by using different senses when exploring something.
Smell
touch
Taste
Sound
Sight

4. Wavelength, Frequency, and Energy
Notice how small is the visible light section of the entire EM spectrum.

5. Why does this slide look orange?
Brainpop Video
Why does this slide look orange?
Absorbs all of the other wavelengths and reflects the wavelength of orange

6. Crab Nebula as seen from different wavelengths
Optical is the only real color. We can’t see the other wavelengths… they color them to show intensity. IR- red= hotter.
The new Chandra X-Ray Telescope has recorded detailed pictures of the heart of the Crab Nebula, first seen on Earth in the year Here are pictures of the Crab at x- ray (Chandra), optical (Palomar), infrared (Keck), and radio (VLA) wavelengths.

7. Arecibo Observatory - Radio
Puerto Rico- The observatory's 1,000 ft (305 m) radio telescope is the world's largest single-aperture telescope.
Takes data in radio waves… really long (miles long) to catch them we need huge dish or lots of satalites

8. The Very Large Array - Radio
New Mexico - The observatory consists of 27 independent antennas, each of which has a dish diameter of 25 meters (82 feet) and weighs 209 metric tons. The antennas are arrayed along the three arms of a Y-shape (each of which measures 13 miles long)

9. South Pole Telescope - Microwave
Antarctica – A 10 meter diameter designed for observations in the microwave region, with the particular design goal of measuring the faint, diffuse emission from the cosmic microwave background.
The South Pole is the premier observing site in the world for millimeter-wavelength observations. The Pole's high altitude (2.8 km/1.7 mi above sea level) means the atmosphere is thin, and the extreme cold keeps the amount of water vapor in the air low
At south pole because the atmosphere… they are picked up best. Our atm blocks most of it

10. W.M. Keck Observatory – Vis, IR
Hawaii –at the summit of Hawaii’s dormant Mauna Kea volcano It has twin telescopes -optical & infrared. The telescopes operate together to form a single image
On top of volcano

11. Images from Keck
On left: Mosaic false-color image of thermal heat emission from Saturn and its rings. The black square at 4 o'clock represents missing data.

12. Spitzer Space Telescope - IR
Space - The Spitzer Space Telescope is an infrared space observatory launched in 2003

13. Images from Spitzer- IR
The Helix Nebula, often photographed for its colors and resemblance to a giant eye.

14. Image from Spitzer
Images of the stormy atmosphere of a brown dwarf, creating a detailed "weather map“ for this class of cool, star-like orbs. (This image is a composite of Spitzer and Hubble data.)

15. Palomar Observatory - Visible
California - this observatory operates several telescopes, including the famous 200-inch Hale Telescope (5.1 m)

16. Images from Palomar
On right: IC 410, IC 405 (Flaming Star Nebula), and environs. This image is a composite from B&W images. The images were recorded on 2 types of photographic plates, one sensitive to red light and the other to blue, and then digitized. Credit: David De Martin

17. Hubble Space Telescope – Visible, UV
Space- This telescope was carried into a low earth orbit by the space shuttle in Hubble's four main instruments observe in the near UV, Visible, and Near IR.
Hubble's orbit outside the distortion of Earth's atmosphere allows it to take extremely sharp images with almost no background light. Hubble's Deep Field have been some of the most detailed visible-light images ever, allowing a deep view into space and time. Many Hubble observations have led to breakthroughs in astrophysics, such as accurately determining the rate of expansion of the universe.

18. Images from Hubble
image of the nearby spiral galaxy Messier 74. Bright knots of glowing gas light up the spiral arms; regions of new star birth shining in pink.
On right- this is commonly known as the Sombrero galaxy because in visible light, it resembles the broad-brimmed Mexican hat. However, in Spitzer's IR view, the galaxy looks more like a "bull's eye.“ This image is a composite of both telescopes.

19. Chandra X-ray Observatory
Space - The Chandra X-ray Observatory is the world's most powerful X-ray telescope. Since the earth’s atmosphere absorbs the vast majority of X-rays, they are not detectable from Earth-based telescopes.

20. Images from Chandra
“Chandra has allowed astronomers to watch a young neutron star cool steadily over time. By giving us a snapshot of the temperature roughly every two years for the past decade.

21. Compton Gamma Ray Observator
Space – operated in Earth’s orbit from 1991 to It featured four telescopes in one spacecraft covering x-rays and gamma-rays

22. Images from Compton
This computer processed image represents a map of the entire sky. These gamma-ray photons are more than 40 million times more energetic than visible light photons and are blocked from the Earth's surface by the atmosphere. A diffuse gamma-ray glow from the plane of our Milky Way Galaxy is clearly seen across the middle.

23. Why are all these telescopes in space, or remote places on Earth?
Because astronomers are anti social.
Because astronomers like to go to exotic places to do their work.
To reduce the interference from the atmosphere and the electromagnetic signals from human activity.

24. The Electromagnetic Spectrum
You need to memorize these in order!
Let’s learn some details!

26. Speed of Light
All light travels at the speed of light (c) which is: C= 3.0 X 108 meter/sec or 186,000 miles/sec

27. Wavelength, Frequency, and Energy
Wavelength – The distance from one point on a wave to the same point on the next wave. (Symbol = λ )
The units are in meters.
Frequency – The number of waves that pass by in a given time period .(Symbol = ν or f )
The units are 1/sec or hertz (Hz)
As the wavelength increases, the frequency decreases (& vice versa).
They are INVERSELY related through the equation: c=

28. Check for Understanding!
What happens to the frequency as wavelength increases?
It remains the same.
It also increases.
It decreases by the same amount.
It decreases by double that amount.
c =  x λ

29. Answer: 3
c = f x λ
show mathematically AND draw two wavelengths (one short and one long)  which one would take longer to pass in a second?

30. The equation that relates energy to frequency is E = h
Light with the highest energy has the highest frequency, but the smallest wavelength.
The equation that relates energy to frequency is E = h
where h= X Jsec

31. Which color light has the longest wavelength?
Red
Green
C) Blue
Which color light has the highest frequency?
3. Which color light has the highest energy?
Blue
4. Which color light has the greatest speed?

32.
NASA Tour of the EMS Video