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Radiation and Spectroscopy

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PTYS/ASTR 206. The Nature of Light 2/3/09. Radiation and Spectroscopy. The Nature of Light and Atoms ... Spectroscopy ! Shape of spectrum Temperature. Lines ... – PowerPoint PPT presentation

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Title: Radiation and Spectroscopy


1
Radiation and Spectroscopy
  • The Nature of Light and Atoms

2
Announcements
  • Starry Night Enthusiast Project is due Thursday
  • Thursdays reading assignment
  • Finish all of Chapter 5 (focus particularly on
    sections 5.4, 5.4, and 5.6)
  • Pick up graded assignments
  • grading issues

3
Mission update
4
Todays topics
  • Speed of light
  • Lights wave-like properties
  • Concept of a Spectrum
  • The electromagnetic spectrum
  • Wiens law
  • Stefan-Boltzmann law
  • Lights particle-like properties

5
Activity 1
  • What is spectroscopy? Why is useful? What
    information can it give us?

6
Why is studying Light important to Planetary
Scientists?
  • Spectroscopy !
  • Shape of spectrum Temperature
  • Lines in spectrum Composition
  • Imaging at a variety of wavelengths

7
The speed of light
  • Galileos experiments (early 1600s)
  • Inconclusive
  • Romers observations (1675)
  • Demonstrated that light moves at a finite speed
  • Fizeau-Foucault method (1850)
  • Rotating mirror
  • Very close to the correct answer
  • Speed of light is often denoted with the symbol
    c
  • c 3 x 108 m/s (in a vacuum)

8
Romers Observations
  • Meticulous observations of the eclipses of
    Jupiters moons
  • He found that the observed eclipse times were
    different than those predicted and depended on
    the relative position of Jupiter and the Earth
  • Attributed this to being due to the finite speed
    of light

9
The Speed of Light depends on the medium in which
it is moving
The refractive index of a medium is the speed
of light in a vacuum, divided by the speed of
light in the medium For instance, water has a
refractive index of about 1.3 (depending on the
wavelength)
10
Waves
  • Traveling disturbance
  • Energy moves a long way, but the carrier doesnt
  • Characterized by
  • Wavelength Distance between crests
  • Amplitude Height of crest
  • Frequency Number of crests per second
  • Velocity Speed and direction of the wave

Speed of a wave is the wavelength times the
frequency v ? ? (v
speed, ? wavelength, ? frequency )
11
Changing Waves
Interference
  • Interference
  • Waves add when they collide
  • Can be constructive or destructive
  • Diffraction
  • Waves bend going around corners
  • Doppler Effect
  • Waves compress or expanded due to moving source
  • Useful to determine speed of wave emitters

Diffraction
12
Youngs double-slit experiment
  • This famous experiment convincingly demonstrated
    the wave-like property of light

13
Newtons Experiment
Showed convincingly that Light is a SPECTRUM
14
Electromagnetic Spectrum
  • Light has many frequencies and wavelengths
  • But all move at the same speed in a vacuum
  • Blue light has a shorter wavelength than Red light

15
Activity 2
  • Suppose that a transmitter onboard a
    spacecraft in orbit about Mars sends two
    different signals to Earth. One of the signals
    is a radio wave, and the other a highly
    collimated beam of visible light. Which signal
    will arrive at Earth first?

16
Why is it called the Electromagnetic Spectrum?
  • Because Electric and Magnetic Fields are what is
    waving in light

17
Imaging Solar System Bodies at Different
Wavelengths
Uranus
Sun
? Visible ?
Near IR
Xrays
18
False color images Cassini/VIMS scientists
created these images by mapping 3 separate IR
wavelengths into Red,Green,Blue to get this image
of Titan
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