1. Warm Up – Page 200 What do you know about the universe?

3. Planets do not twinkle because they are closer and not a single point of light.

7. We only see the visible range. But stars give off energy in all the wavelengths!

8. Using light to discover information about the universe. There are two kinds:

9. Uses lens to collect the light.

11. Today’s refracting telescopes!

12. Uses mirrors to collect light Reflecting scope Reflecting telescope

14. Spotting scope - A small refractor to line up the big scope. Eyepiece for viewing Today’s reflector

15. Mount Palomar Observatory Hale Telescope Inside Mt. Palomar Observatory Large telescopes are put in observatories to protect them.

16. Other scopes at Palomar Look across the mountain tops!

17. 1. Mountain tops above atmospheric haze. Reduces the twinkle effect and distortion. 2. Far from city lights ( light pollution). 3. If our atmosphere blocks the wavelength needed to study, then the scope goes into orbit!

18. Notice which wavelengths are blocked!

19. The USA at night – notice the light pollution. Where would you put a telescope? Atlanta Notice the Great Lakes

20. Mauna Kea, Hawaii – elevation 13,796 ft High to “look through” less atmosphere

21. Multi-mirror reflector in Hawaii

23. Infrared scope in Hawaii Infrared scopes “look for” heat and are best at locating new stars just forming.

24. COBE - An Infrared scope that is in orbit. Cosmic Background Explorer It has located very important data about the formation of the universe. Infrared = heat

25. The constellation of Orion in visible light energy and infrared energy. These two views see very different things in the same area of the sky!

26. Radio Telescopes Records radio waves Sees to the edges of the universe

27. VLA New Mexico Very Large Array uses multiple radio telescopes.

28. VLA from above. They work as a unit kind of like a fly’s eye.

29. Largest radio scope in the world in the top of an extinct volcano! Puerto Rico

30. Records UV radiation. Astronomers use this wave length mostly to look at and track what the sun is doing.

31. Solar & Heliospheric Observatory This spacecraft has an ultraviolet scope.

32. The sun in different UV wavelengths.

33. Records x ray emissions from objects in “deep” space Best for “looking” for black holes, dying stars, and other strange objects. Must be above the atmosphere!

34. Chandra X-Ray scope

35. X Rays from two Black holes in one Galaxy.

36. These telescopes are looking for high energy events: black holes, neutron stars and quasars. Due to their high energy content, Gamma rays are able to cause serious damage when absorbed by living cells. Gamma rays are also able to penetrate dense materials. Aren’t we glad our atmosphere blocks them!

37. The Compton Gamma Ray Observatory orbits the Earth, detecting high-energy photons – GAMMA RAYS

38. Takes light from stars and analyzes it.

39. Light from a star or other source goes through the slit.

40. Every element has a different set of spectrum lines. Much like people having different fingerprints.

41. Krypton’s spectrum Neon’s spectrum Emission spectrum

44. Notice that emission and absorption are the same.

45. Warm Up – Page 200 Why are large Earth based telescopes placed on high mountain tops.

47. They seem to form a picture in the sky. People use them to find their way around the sky like someone using objects to get from place to place.

48. The constellation looks flat but all the stars are at different distances from us.

49. Can you see the drawing ?

51. The Zodiac is a special group of constellations that extend out from Earth’s equator.

52. From here on earth, they all look the same distance. In fact, ancient people thought they were all “stuck” on a glass sphere.

53. To measure the distances in space, astronomers use a light year. A light year is the DISTANCE light travels in one year. One light year is equal to a little under 6 trillion miles! (6,000,000,000,000) Proxima Centauri is the closest star to our solar system. It is about 4 light years away. Going the speed of light it would take us 4 years to get there. Traveling as fast as the average spaceship, it would take between 70,000 and 100,000 years to get there! Video clip on a light year

55. Video clip on galaxies

56. Pictures by the Hubble Space Telescope

57. Notice the individual stars in the picture. They are not part of the galaxy in the picture but part of our own Milky Way Galaxy.

58. So why are they in the pictures? If you look out a window with wood trim, it is hard to get a view without them in the way. These stars are in our view as we are looking out of our galaxy!

61. We think! This is not really a picture of our galaxy – just one that looks like what we think our galaxy is like!

62. If you were inside Lanier Middle and had never been out of the building your entire life, would you be able to know what the school looked like from a distance? Of course not. All you could do is look out the windows and get some view of part of the building. If you looked out enough windows you might get a general idea but you could never know for sure if you were right about all its features.

63. Top view Side view Video clip on our location in the galaxy

64. Milky Way using a “fish eye” lens Notice the comet In the night sky, a band of stars can be seen across the sky as a blurry image. When you see this, you are looking into the part of the galaxy with more stars. Our view of the Milky Way

65. Every star we see in the night sky is in our own galaxy. We cannot see stars in other galaxies because they are too far away. The Milky Way is estimated to have 200 billion stars.

66. Witch head nebula Veil nebula Horse head nebula They provide the material for new stars to form.

67. North American nebulaCat’s eye nebula ring nebula ant nebula

68. Current estimate of the age of the universe is 13.7 billion years. The solar system is 4.6 billion years old. The solar system is not the same age as the entire universe.

69. Hubble deep field Click on the picture and watch as the Hubble telescope zooms in to an area just above the Big Dipper!

70. Prove that the following wff is valid by means of resolution:  xp(x)v  xq(x)   x  p(x)vq(x)  Why can’t you do this problem?

71. You cannot do these problems because you do not know the math between what you now know and what you would need to know to do the problem!

72. You will have the same problem with understanding the process that scientists call the big bang. Just because you cannot understand some of what scientists say about the big bang does not mean that scientists do not understand it clearly! They know the science between what you know and what is needed to be known to understand the big bang!

74. Did the detectives see the explosion? No! They have to figure it out from evidence!

75. They take evidence from space to figure out the science!

78. Some sort of “event” occurred to cause the change that formed the universe we have today.

79. This event is what scientists call the

81. Instead, it was the expansion of space and time itself, and therefore occurred everywhere at the same time.

82. Any galaxies farther than ~ 13.7 billion ly away we cannot see! Why: because the light hasn’t had time to get here!!!

83. Are there galaxies beyond what we can see? Astronomers think that answer is yes. We just can’t see them.

85. is the evidence for this expansion. Universal red shift

86. Sound shows Doppler effect too! Clip on this picture to experience the Doppler effect.

87. red shift What you just heard was the Doppler effect with sound. Red shift is the Doppler effect with light.

89. Notice that the line groupings are the same – only shifted red.

91. From our position in the universe, it looks like we are the center because everything appears to be moving away from us.

92. As a balloon gets larger every point moves away from every other point.

93. If your galaxy was a raisin, notice that every raisin is moving away from every other raisin. In fact, a raisin far away from you is moving away faster than those that are closer. Our expanding universe acts the same way.

94. The second evidence is Cosmic Microwave Background Radiation!

95. This is energy “left over” from the Big Bang. -discovered in the early 1960’s.

97. This is like an oven that was used to make cookies. The cookies are not visible but the smell is there (evidence) and when you open the oven door there is just a little bit of heat still there (another piece of evidence).

98. What are the two pieces of evidence that support eh Big Bang Theory that we discussed? Video clip of the big bang