Lecture 8: Waves and Particle- A Light Motif

"My heart leaps up when I behold A rainbow in the sky."

William Wordsworth-- My Heart Leaps Up



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  • Date: September 27, 1994
    Reading Assignment: pp. 62-73

    Description : introduction to waves and the wavelike nature of the electromagnetic spectrum

    Objectives

  • understand the parts of a wave
  • be able to describe the experiments which show the wave-like nature of light
  • understand the parts of the EM spectrum \\

  • Lecture Outline

    Slide # 1: Waves and Particles

  • Click here for subtitle
  • A Light Motif
  • Slide # 2: Astro 105- the story so far
  • Lecture 1-3
  • Sky, Sun and Moon
  • Lecture 4/5
  • Dead Greeks and the Scientific Method
  • Lecture 6/7
  • Copernican Revolution
  • Slide # 3: Upcoming Topics
  • Lecture 8-10
  • Light, the Spectrum and Atomic Physics
  • Lecture 11-12
  • Telescopes of all kinds
  • Lecture 13-14
  • the Earth
  • Lecture 15
  • the Moon
  • Slide # 4: How do Astronomers know anything?
  • Experiments are not possible
  • No direct contact with Celestial Objects
  • Slide # 5: Light
  • Almost everything we know comes from the analysis of ÒstarlightÓ
  • No information can travel faster than light
  • Slide # 6: The Nature of Light
  • Light is neither a wave or a particle
  • Wave-like properties
  • Particle-like properties
  • Slide # 7: Light
  • A special kind of radiation
  • Only one part of the Electromagnetic Spectrum
  • Slide # 8: Speed of Light
  • All EM radiation travels at the speed of light
  • No information can travel faster than 300,000 km/s
  • Slide # 9: Speed of Light
  • Light travels at a finite speed
  • Slide # 10: Waves
  • a way that energy is moved
  • wave patterns repeat
  • cycles in time
  • cycles in space
  • Slide # 11: Waves - cycles in space
  • Crests
  • Troughs
  • Slide # 12: Waves - cycles in space
  • Wavelength
  • Distance between two crests or troughs
  • Slide # 13: Waves - cycles in space
  • Amplitude
  • Height or depth of the wave
  • Slide # 14: Waves - cycles in time
  • waves and troughs pass the observer
  • Slide # 15: Waves - cycles in time
  • crests and troughs pass at regular time intervals
  • period is the length of time between troughs or crests
  • Slide # 16: Waves - period
  • observer times the time between two crests or two troughs
  • Slide # 17: Waves - frequency
  • observer times the number of cycles per second
  • Slide # 18: Units of Frequency
  • units of inverse time
  • events per unit time
  • normally measured in Hertz
  • one Hertz = one cycle / second
  • Slide # 19: Waves - cycles in time
  • Period and frequency are related
  • Slide # 20: Frequency and Period Slide # 21: Cycles of Space and Time
  • Wavelength, frequency, and velocity are related
  • Slide # 22: Cycles of Space and Time
  • velocities of waves are usually constant
  • frequency and wavelength are inversely proportional
  • Slide # 23: Why do we say light has Òwave-likeÓ properties
  • Diffraction
  • Interference
  • Slide # 24: Diffraction
  • ability of light to bend around corners
  • Slide # 25: Interference
  • ability of waves to reinforce or cancel each other
  • Slide # 26: Interference- reinforcing waves Slide # 27: Interference- cancelling waves Slide # 28: Interference
  • contructive interference- reinforcing
  • destructive interference- cancelling
  • Slide # 29: Interference
  • Waves of the same amplitude and wavelength can exactly cancel
  • Slide # 30: Experiments which demonstrate the wave-like properties of light
  • single slit
  • demonstration of diffraction
  • double slit
  • YoungÕs demonstration of interference
  • Slide # 31: Waves in what?
  • electromagnetic waves do not travel through a medium
  • oscillations of the electrical field
  • Slide # 32: Electrical Fields
  • All charged particles have electrical fields
  • electrical fields are Òinverse square lawsÓ like gravity
  • charged particles ÒcommunicateÓ through their electrical fields
  • Slide # 33: Electromagnetism
  • changing electrical fields produce magnetic fields
  • electricity and magnetism are two aspects of one phenomenon
  • Slide # 34: Electromagnetism
  • oscillating electrical fields produce electromagnetic waves
  • Slide # 35: Light is one form of electromagnetic energy
  • light is produced by oscillating electromagnetic fields
  • Slide # 36: Visible Light
  • white light is mixture of colors
  • red
  • orange
  • yellow
  • green
  • blue
  • violet
  • Slide # 37: Visible Light Slide # 38: Wavelengths of Visible Light
  • Red light = 7 x 10-5 cm
  • 0.00007 cm
  • Blue light = 4 x 10-5 cm
  • 0.00004 cm
  • Slide # 39: Red Light vs Blue Light
  • Red has a longer wavelength
  • Red has a lower frequency
  • Remember: Longer wavelengths = lower frequencies
  • Slide # 40: Electromagnetic Waves
  • wavelengths > 7 x 10-5 cm are invisible to humans
  • wavelengths < 4 x 10-5 cm are invisible to humans
  • longer and shorter wavelengths are also electromagnetic radiation
  • Slide # 41: The Electromagnetic Spectrum
  • Radio
  • Infrared
  • Visible
  • Ultraviolet
  • X-ray
  • Gamma-ray
  • Slide # 42: Radio
  • Wavelengths > 1 mm
  • Frequencies 0 to 300 Giga-Hz (3x1011Hz)
  • Typical Examples
  • AM/FM Radios
  • TV signals
  • Slide # 43: Infrared
  • Wavelengths between 1mm and 7 x 10-5 cm
  • Frequencies between 3 x 1011 Hz and 4 x 1014 Hz
  • Typical Examples
  • Heating devices
  • stove burners
  • space heaters
  • TV remote controls
  • Slide # 44: Visible
  • Wavelengths between 7 x 10-5 cm and 3 x 10-5 cm
  • Frequencies between 4 x 1014 Hz and 1 x 1015 Hz
  • Typical Examples
  • All that you see
  • Slide # 45: Ultraviolet
  • Wavelengths between 3 x 10-5 cm and 3 x 10-7 cm
  • Frequencies between 1 x 1015 Hz and 1 x 1017 Hz
  • Typical Examples
  • Sunlight which causes sunburn and suntan
  • Slide # 46: X-rays
  • Wavelength between 3 x 10-7 cm and 3 x 10-10 cm
  • Frequencies between 1 x 1017 Hz and 1 x 1020 Hz
  • Typical Example
  • Medical X-ray Machines
  • Slide # 47: Gamma-Rays
  • Wavelengths < than 3 x 10-10 cm
  • Frequencies > 1 x 1020 Hz
  • Typical Examples
  • Nuclear reactions
  • Nuclear bombs
  • Slide # 48: Atmospheric Blockage
  • some wavelengths are blocked by the atmosphere
  • Slide # 49: Opacity
  • the extent which a wavelength is blocked
  • opaque is the opposite of transparent
  • Slide # 50: Atmospheric Opacity- Why does it happen?
  • gases absorb and scatter light
  • the amount of absorption depends on
  • the type of molecule
  • the wavelength of light
  • Slide # 51: Atmospheric Opacity - Some Examples
  • Water and Oxygen absorb some radio frequencies
  • Carbon Dioxide absorbs some infrared frequencies
  • the Ozone layer blocks most Ultraviolet, X-ray and Gamma-rays
  • Slide # 52: Summary of Lecture 8
  • Waves are oscillations in space and time
  • Light has wavelike properties
  • Frequency and wavelength are mathematically related
  • Light is just one part of the EM spectrum
  • The atmosphere absorbs most of the other parts of the EM Spectrum