1. Light: The Cosmic Messenger

2. What is light?

3. WHAT DO YOU THINK? What is “visible” light? What is “visible” light? A wave? A particle? Energy? A wave? A particle? Energy? What is electromagnetic radiation? What is electromagnetic radiation? What are the main functions of telescopes? What are the main functions of telescopes? Why do all research telescopes use mirrors, rather than lenses, to collect light? Why do all research telescopes use mirrors, rather than lenses, to collect light? How can we know anything about stars’ temperatures, sizes, ages, & lives? How can we know anything about stars’ temperatures, sizes, ages, & lives?

4. In this chapter you will discover… Connection between visible light, X-rays, radio waves, & other electromagnetic radiation Connection between visible light, X-rays, radio waves, & other electromagnetic radiation Debate over what light is & how Einstein resolved it Debate over what light is & how Einstein resolved it How telescopes collect and focus light How telescopes collect and focus light Why different types of telescopes are used for different types of research Why different types of telescopes are used for different types of research

5. In this chapter you will discover… Limitations of telescopes, especially those that use lenses to collect light Limitations of telescopes, especially those that use lenses to collect light New generations of land-based and space-based high-technology telescopes New generations of land-based and space-based high-technology telescopes How astronomers use entire spectrum of electromagnetic radiation to observe stars & other astronomical objects and events How astronomers use entire spectrum of electromagnetic radiation to observe stars & other astronomical objects and events

6. White light is composed of different colors when shone through glass…. …but the glass is not creating those colors! Observation: Color is property of light!

7. More Observations: Speed of Light?

8. Roemer’s observations of Jupiter’s Moon’s Eclipses demonstrated light moves at a finite speed More Observations: Speed of Light is not infinite!

9. Non-visible light (beyond the red end of the spectrum) has energy, too! Even More Observations: Light has “energy”

10. Observation: Water Waves naturally interfere & create noticeable patterns

11. Observation: Light has a wavelike property, too! Young’s Experiment (1801)

12. Wavelength and Frequency wavelength  frequency = speed of a wave

13. Observations of Nature Electricity acts through space over a distance Electricity acts through space over a distance Lightening, sparks on a doorknob Lightening, sparks on a doorknob Magnetism acts through space over a distance Magnetism acts through space over a distance Two magnets attract or repel one another without touching Two magnets attract or repel one another without touching

14. More Observations If you spin a conductor in a magnetic field, you get electricity! If you spin a conductor in a magnetic field, you get electricity! Electric Generators @ dams & windmills Electric Generators @ dams & windmills Portable gas generators Portable gas generators If you run electricity into a coil, you get a magnet! If you run electricity into a coil, you get a magnet! “Electromagnetic” cranes “Electromagnetic” cranes Auto solenoids Auto solenoids Electric Motors Electric Motors

15. Maxwell’s Observations Change Electricity => create magnetism Change Electricity => create magnetism Change Magnetism => create electricity Change Magnetism => create electricity Continuously change both, continuously create radiation! Continuously change both, continuously create radiation! Radiation created moves at “c” – the speed of light! Radiation created moves at “c” – the speed of light!

16. Electro-magnetic radiation! The Wave Model of Light

17. Light is an wave. Light is an electromagnetic wave.

18. The Electromagnetic Spectrum

20. Still More Observations of Nature Einstein’s Photo-electric Effect showed light can eject individual electrons Einstein’s Photo-electric Effect showed light can eject individual electrons Energy depended upon light’s color! Energy depended upon light’s color! Metal plate Single electrons emerge Light shining onto metal

21. Still More Observations of Nature Planck’s Energy Curve showed light can be modeled with specific “quanta” of energy Planck’s Energy Curve showed light can be modeled with specific “quanta” of energy Peak depended upon light’s color! Peak depended upon light’s color! Metal plate

22. The Particle Model of Light Particles of light are called photons. Particles of light are called photons. Each photon has a wavelength and a frequency. Each photon has a wavelength and a frequency. The energy of a photon depends on its frequency. The energy of a photon depends on its frequency.

23. Wavelength, Frequency, and Energy  f = c  f = c  = wavelength, f = frequency c = 3.00  10 8 m/s = speed of light E = h  f = photon energy h = 6.626  10 −34 joule  s Planck’s constant

24. Thought Question The higher the photon energy, the longer its wavelength. the longer its wavelength. the shorter its wavelength. the shorter its wavelength. Energy is independent of wavelength. Energy is independent of wavelength.

25. Thought Question The higher the photon energy, the longer its wavelength. the longer its wavelength. the shorter its wavelength. the shorter its wavelength. Energy is independent of wavelength. Energy is independent of wavelength. X-rays can kill you! X-rays can kill you! Country-western music on the radio can’t Country-western music on the radio can’t

26. What we “see” is only a small part of what there is! The entire EM Spectrum

27. EM Spectrum Varies by… Size (wavelength, color) Energy How the waves are detected But not…. How fast they move through space!

28. What is matter?

29. Atomic Terminology Atomic Number = # of protons in nucleus Atomic Number = # of protons in nucleus Atomic Mass Number = # of protons + neutrons Atomic Mass Number = # of protons + neutrons

30. Atomic Terminology Isotope: same # of protons but different # of neutrons ( 4 He, 3 He) Isotope: same # of protons but different # of neutrons ( 4 He, 3 He) Molecules: consist of two or more atoms (H 2 O, CO 2 )

31. Interactions of Light with Matter Interactions between light and matter determine the appearance of everything around us.

32. How do light and matter interact? Emission Emission Absorption Absorption Transmission: Transmission: — Transparent objects transmit light. — Opaque objects block (absorb) light. Reflection or scattering Reflection or scattering

33. Reflection and Scattering Mirror reflects light in a particular direction. Movie screen scatters light in all directions.

34. Thought Question Why is a rose ? Why is a rose red? The rose absorbs red light. The rose absorbs red light. The rose transmits red light. The rose transmits red light. The rose emits red light. The rose emits red light. The rose reflects red light. The rose reflects red light.

35. Thought Question Why is a rose red? The rose absorbs red light. The rose absorbs red light. The rose transmits red light. The rose transmits red light. The rose emits red light. The rose emits red light. The rose reflects red light.

36. Learning from Light What are the three basic types of spectra? What are the three basic types of spectra? How does light tell us composition - what things are made of? How does light tell us composition - what things are made of? How does light tell us the temperatures of planets and stars? How does light tell us the temperatures of planets and stars? How does light tell us the speed of a distant object towards or away from us? How does light tell us the speed of a distant object towards or away from us?

37. Learning from Light Spread light out with prism or grating: Spread light out with prism or grating: Hot solids give off rainbows Hot solids give off rainbows Hot gases give off bright lines of particular color Hot gases give off bright lines of particular color Cool gases show dark shadows over particular colors (only) Cool gases in front of a hot solid show dark shadows over particular colors (only)

38. Continuous Spectrum The spectrum of a common (incandescent) light bulb spans all visible wavelengths, without interruption. The spectrum of a common (incandescent) light bulb spans all visible wavelengths, without interruption.

39. Emission Line Spectrum A thin or low-density cloud of gas emits light only at specific wavelengths that depend on its composition and temperature, producing a spectrum with bright emission lines. A thin or low-density cloud of gas emits light only at specific wavelengths that depend on its composition and temperature, producing a spectrum with bright emission lines.

40. Absorption Line Spectrum A cloud of gas between us and a light bulb can absorb light of specific wavelengths, leaving dark absorption lines in the spectrum. A cloud of gas between us and a light bulb can absorb light of specific wavelengths, leaving dark absorption lines in the spectrum.

41. Three basic types of spectra Continuous Spectrum Emission Line Spectrum Absorption Line Spectrum Spectra of astrophysical objects are usually combinations of these three basic types.

42. How does light tell us what things are made of? Spectrum of the Sun

43. Chemical Fingerprints Each type of atom has a unique set of energy levels. Each type of atom has a unique set of energy levels. Each transition corresponds to a unique photon energy, frequency, and wavelength. Each transition corresponds to a unique photon energy, frequency, and wavelength. Energy levels of hydrogen

44. Chemical Fingerprints Downward transitions produce a unique pattern of emission lines. Downward transitions produce a unique pattern of emission lines.

45. Chemical Fingerprints Because those atoms can absorb photons with those same energies, upward transitions produce a pattern of absorption lines at the same wavelengths. Because those atoms can absorb photons with those same energies, upward transitions produce a pattern of absorption lines at the same wavelengths.

46. Chemical Fingerprints Each type of atom has a unique spectral fingerprint. Each type of atom has a unique spectral fingerprint.

47. Chemical Fingerprints Observing the fingerprints in a spectrum tells us which kinds of atoms are present. Observing the fingerprints in a spectrum tells us which kinds of atoms are present.

48. Example: Solar Spectrum

49. Thought Question Which letter(s) labels absorption lines? ABCDE

50. ABCDE

51. Thought Question ABCDE Which letter(s) labels the peak (greatest intensity) of infrared light?

52. ABCDE Thought Question Which letter(s) labels the peak (greatest intensity) of infrared light?

53. Thought Question Which letter(s) labels emission lines? ABCDE

54. ABCDE

55. Gathering Light Where must telescopes be placed to observe the universe in different wavelengths? What are the basic types of telescopes? What 3 functions do ALL telescopes do? How can we combine observations to get even more detail?

56. Gather Radio waves & Visible Light on the Ground

57. Infra-red, UV, X-ray, & Gamma Rays can’t reach the ground

58. Atmospheric “Windows” to the stars & universe: Visible & Radio light Optical & Radio Telescope observatories on Earth Other wavelength telescopes launched ABOVE atmosphere

60. Refracting Telescopes bend light through lenses Heavy glass lenses, bending different colors to different points (“Chromatic aberration”) & imperfections in glass, limit practical size

61. Reflecting Telescopes bounce light off mirrors

62. Different types of Reflecting Telescopes

64. Functions of ALL Telescopes! 1. Gather Light 2. Resolve Sharp Details 3. Magnify Resulting Images Regardless of Wavelength range & size

66. #1 Function: Gathering Light Depends upon the size of the objective mirror or lens. Depends upon the size of the objective mirror or lens. Light gathering area increases with SQUARE of the diameter Light gathering area increases with SQUARE of the diameter 10 m telescope gather 4x more light than 5m 10 m telescope gather 4x more light than 5m Subject to interference from other sources! Subject to interference from other sources!

67. Tucson, 1959 Tucson, 1989

68. Small Telescope image of Andromeda Galaxy

69. Larger Telescope image of Andromeda Galaxy

70. #2 Function: Resolution Depends upon the size of the objective mirror or lens. Depends upon the size of the objective mirror or lens. Better resolution with more light Better resolution with more light Depends upon wavelength of light, too! Depends upon wavelength of light, too! Smaller wavelengths provide smaller details Smaller wavelengths provide smaller details UV images have more detail than Radio UV images have more detail than Radio Also subject to interference Also subject to interference

71. Resolution is the ability to see small details Affected by: Imperfections in optics (shapes of lenses/mirrors) Atmospheric motion, density, temperature, moisture Improved by: Adaptive optics “subtracting out” the atmospheric effects Getting above atmosphere!

72. Radio Telescopes gather long-wave, low-energy light Poor resolution unless made LARGE!

73. Improve resolution by getting above the atmosphere (and gather more types of light, too!)

74. 1.Ground-based image of Neptune 2.Ground-based image with adaptive optics 3.Hubble Space Telescope image 123

75. #3 Function: Magnification Least important Least important Without a bright, sharp image, no use! Without a bright, sharp image, no use! Bigger, Dimmer, Fuzzier! Bigger, Dimmer, Fuzzier! Depends upon EYEPIECE used Depends upon EYEPIECE used Small scopes: $50-500 each Small scopes: $50-500 each Easily swapped to magnify images Easily swapped to magnify images Depends upon telescope geometry, too Depends upon telescope geometry, too

76. Magnify this… To THIS

77. Photographs vs. CCD chips vs. Multi-color filtered CCD composite images

78. Orion in UV, Infrared, & Optical Wavelengths

79. Active & Adaptive Optics! Active optics (1980’s) Active optics (1980’s) Put actuators on segmented mirrors to “bend” them to the right shape Put actuators on segmented mirrors to “bend” them to the right shape Keck, NTT, VLT Telescopes Keck, NTT, VLT Telescopes Adaptive optics (1990’s to present) Adaptive optics (1990’s to present) “Deform” mirror in real time to compensate for atmospheric motion “Deform” mirror in real time to compensate for atmospheric motion Laser Guide Stars Laser Guide Stars

80. VLT in Chile (4) combined 8.2 m telescopes (4) combined 8.2 m telescopes Tracking motions of stars at Milky Way Center Tracking motions of stars at Milky Way Center Tracking motions of stars at Milky Way Center Tracking motions of stars at Milky Way Center

81. SALT in Africa Largest current “single” surface scope Largest current “single” surface scope Largest current “single” surface scope Largest current “single” surface scope

82. Next Generation Space Telescope NASA’s next great observatory NASA’s next great observatory Bigger than Hubble Bigger than Hubble Bigger than Hubble Bigger than Hubble

83. Seeing in Stereo!

84. Interferometry – Combining signals simultaneously from 2 or more scopes

85. Visible & Radio wave views of Saturn

90. Why build telescopes at all? We already have enough! Why do we need a more detailed picture of Mars? Who cares? This cost $100 Million dollars? You’ve got to be kidding me…

91. Summary: The Nature Of Light Photons, units of vibrating electric and magnetic fields, all carry energy through space at the same speed, the speed of light (300,000 km/s in a vacuum, slower in any medium). Photons, units of vibrating electric and magnetic fields, all carry energy through space at the same speed, the speed of light (300,000 km/s in a vacuum, slower in any medium). Radio waves, microwaves, infrared radiation, visible light, ultraviolet radiation, X rays, and gamma rays are the forms of electromagnetic radiation. They travel as photons, sometimes behaving as particles, sometimes as waves. Radio waves, microwaves, infrared radiation, visible light, ultraviolet radiation, X rays, and gamma rays are the forms of electromagnetic radiation. They travel as photons, sometimes behaving as particles, sometimes as waves.

92. The Nature Of Light Visible light occupies only a small portion of the electromagnetic spectrum. Visible light occupies only a small portion of the electromagnetic spectrum. The wavelength of a visible light photon is associated with its color. Wavelengths of visible light range from about 400 nm for violet light to 700 nm for red light. The wavelength of a visible light photon is associated with its color. Wavelengths of visible light range from about 400 nm for violet light to 700 nm for red light. Infrared radiation and radio waves have wavelengths longer than those of visible light. Ultraviolet radiation, X rays, and gamma rays have wavelengths that are shorter. Infrared radiation and radio waves have wavelengths longer than those of visible light. Ultraviolet radiation, X rays, and gamma rays have wavelengths that are shorter.

93. Optics and Telescopes A telescope’s most important function is to gather as much light as possible. Its second function is to reveal the observed object in as much detail as possible. Often the least important function of a telescope is to magnify objects. A telescope’s most important function is to gather as much light as possible. Its second function is to reveal the observed object in as much detail as possible. Often the least important function of a telescope is to magnify objects. Reflecting telescopes, or reflectors, produce images by reflecting light rays from concave mirrors to a focal point or focal plane. Reflecting telescopes, or reflectors, produce images by reflecting light rays from concave mirrors to a focal point or focal plane.

94. Optics and Telescopes Refracting telescopes, or refractors, produce images by bending light rays as they pass through glass lenses. Glass impurity, opacity to certain wavelengths, and structural difficulties make it inadvisable to build extremely large refractors. Refracting telescopes, or refractors, produce images by bending light rays as they pass through glass lenses. Glass impurity, opacity to certain wavelengths, and structural difficulties make it inadvisable to build extremely large refractors. Reflectors are not subject to the problems that limit the usefulness of refractors. Reflectors are not subject to the problems that limit the usefulness of refractors. Earth-based telescopes are being built with active and adaptive optics. These advanced technologies yield resolving power comparable to the Hubble Space Telescope. Earth-based telescopes are being built with active and adaptive optics. These advanced technologies yield resolving power comparable to the Hubble Space Telescope.

95. Nonoptical Astronomy Radio telescopes have large, reflecting antennas (dishes) that are used to focus radio waves. Radio telescopes have large, reflecting antennas (dishes) that are used to focus radio waves. Very sharp radio images are produced with arrays of radio telescopes linked together in a technique called interferometry. Very sharp radio images are produced with arrays of radio telescopes linked together in a technique called interferometry. Earth’s atmosphere is fairly transparent to most visible light and radio waves, along with some infrared and ultraviolet radiation arriving from space, but it absorbs much of the electromagnetic radiation at other wavelengths. Earth’s atmosphere is fairly transparent to most visible light and radio waves, along with some infrared and ultraviolet radiation arriving from space, but it absorbs much of the electromagnetic radiation at other wavelengths.

96. Nonoptical Astronomy For observations at other wavelengths, astronomers mostly depend upon telescopes carried above the atmosphere by rockets. Satellite-based observatories are giving us a wealth of new information about the universe and permitting coordinated observation of the sky at all wavelengths. For observations at other wavelengths, astronomers mostly depend upon telescopes carried above the atmosphere by rockets. Satellite-based observatories are giving us a wealth of new information about the universe and permitting coordinated observation of the sky at all wavelengths. Charge-coupled devices (CCDs) record images on many telescopes used between infrared and X-ray wavelengths. Charge-coupled devices (CCDs) record images on many telescopes used between infrared and X-ray wavelengths.

97. Key Terms active optics adaptive optics angular resolution Cassegrain focus charge-coupled device coudé focus electromagnetic radiation electromagnetic spectrum eyepiece lens focal length focal plane focal point frequency gamma ray infrared radiation interferometry light-gathering power magnification Newtonian reflector objective lens photon pixel primary mirror prime focus radio telescope radio wave reflecting telescope reflection refracting telescope Schmidt corrector plate secondary mirror seeing disk spectrum spherical aberration twinkling ultraviolet (UV) radiation very-long-baseline interferometry (VLBI) wavelength X ray

98. WHAT DID YOU THINK? What is light? What is light? Light—more properly “visible light,” is one form of electromagnetic radiation. All electromagnetic radiation (radio waves, microwaves, infrared radiation, visible light, ultraviolet radiation, X rays, and gamma rays) has both wave and particle properties. Light—more properly “visible light,” is one form of electromagnetic radiation. All electromagnetic radiation (radio waves, microwaves, infrared radiation, visible light, ultraviolet radiation, X rays, and gamma rays) has both wave and particle properties.

99. WHAT DID YOU THINK? What type of electromagnetic radiation is most dangerous to life? What type of electromagnetic radiation is most dangerous to life? Gamma rays have the highest energies of all photons, so they are the most dangerous to life. However, ultraviolet radiation from the Sun is the most common everyday form of dangerous electromagnetic radiation that we encounter. Gamma rays have the highest energies of all photons, so they are the most dangerous to life. However, ultraviolet radiation from the Sun is the most common everyday form of dangerous electromagnetic radiation that we encounter.

100. WHAT DID YOU THINK? What is the main purpose of a telescope? What is the main purpose of a telescope? A telescope is designed primarily to collect as much light as possible. A telescope is designed primarily to collect as much light as possible.

101. WHAT DID YOU THINK? Why do all research telescopes use mirrors, rather than lenses, to collect light? Why do all research telescopes use mirrors, rather than lenses, to collect light? Telescopes that use lenses have more problems, such as chromatic aberration, internal defects, complex shapes, and distortion from sagging, than do telescopes that use mirrors. Telescopes that use lenses have more problems, such as chromatic aberration, internal defects, complex shapes, and distortion from sagging, than do telescopes that use mirrors.

102. WHAT DID YOU THINK? Why do stars twinkle? Why do stars twinkle? Rapid changes in the density of Earth’s atmosphere cause passing starlight to change direction, making stars appear to twinkle. Rapid changes in the density of Earth’s atmosphere cause passing starlight to change direction, making stars appear to twinkle.