Introduction to Physical Science Monday, Wednesday, Thursday Tom Burbine tomburbine@astro.umass.edu - PowerPoint PPT Presentation

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Introduction to Physical Science Monday, Wednesday, Thursday Tom Burbine tomburbine@astro.umass.edu

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Title: Linking Asteroids and Meteorites through Reflectance Spectroscopy Author: Smithsonian Institution Last modified by: Tom Created Date: 5/23/2001 8:09:58 PM – PowerPoint PPT presentation

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Title: Introduction to Physical Science Monday, Wednesday, Thursday Tom Burbine tomburbine@astro.umass.edu


1
Introduction to Physical ScienceMonday,
Wednesday, ThursdayTom Burbinetomburbine_at_astr
o.umass.edu
2
Quiz on Thursday
  • Magnetism
  • Waves
  • Light
  • c ?f
  • E hf
  • Electromagnetic spctrum
  • Doppler shift

3
Wave
  • Something that vibrates in space and time
  • Light acts as a wave
  • Sound acts as a wave

4
(No Transcript)
5
Frequency
  • The number of vibrations per unit time

6
Light
  • Light is a form of energy

7
Light
  • These are all forms of light
  • Gamma rays
  • X-rays
  • Ultraviolet light
  • Visible light
  • Infrared light
  • Radio waves

8
Light
  • Can act as a particle
  • Can also act as a wave

9
Particle aspect
  • Particles called photons stream from the Sun and
    can be blocked by your body

10
Photons
  • Light is quantized
  • Comes in discrete packets called photons

11
Wave aspect
12
Thomas Young Experiment
  • http//micro.magnet.fsu.edu/primer/java/interferen
    ce/doubleslit/

13
Characteristics of waves
  • velocity wavelength x frequency
  • Wavelength distance
  • Frequency cycles per second hertz

3 x 108 m/s
14
Speed of sound
  • Speed of sound 340 m / s

15
For light
  • c wavelength x frequency
  • In vacuum, speed of light stays the same
  • So if wavelength goes up
  • Frequency does down
  • f frequency
  • ? wavelength
  • c ? x f

16
Calculations
  • c ? x f
  • So if the wavelength is 1 x 10-12 m
  • 3 x 108 m/s 1 x 10-12 m f
  • f 3 x 108 m/s/1 x 10-12 m
  • f 3 x 1020 s-1 3 x 1020 Hz

17
Calculations
  • c ? x f
  • So if the frequency is 1 x 1015 Hz
  • 3 x 108 m/s ? 1 x 1015 Hz
  • ? 3 x 108 m/s/1 x 1015 Hz
  • ? 3 x 10-7 m

18
Energy of light
  • Energy is directly proportional to the frequency
  • E h f
  • h Plancks constant 6.626 x 10-34 J/s
  • since f c/?
  • Energy is inversely proportional to the
    wavelength
  • E hc/?

19
Higher the frequency, Higher the energy of the
photon Higher the wavelength, Lower the energy of
the photon
20
Calculations
  • What is the energy of a radio wave with a
    frequency of 1 x 107 Hz?
  • E h f
  • h Plancks constant 6.626 x 10-34 J/s
  • E 6.626 x 10-34 J/s 1 x 107
  • E 6.626 x 10-27 J

21
Calculations
  • What is the energy of a gamma ray photon with
    wavelength of 1 x 10-15 m
  • E hc/?
  • h Plancks constant 6.626 x 10-34 J/s
  • E 6.626 x 10-34 J/s 3 x 108 m/s / 1 x 10-15 m
  • E 1.99 x 10-10 J

22
So why are some types of radiation dangerous?
  • Higher the energy, the farther the photons can
    penetrate
  • So gamma and X-rays can pass much more easily
    into your the body
  • These high-energy photons can ionize atoms in
    cells
  • Ionization means removes electrons from an atom

23
More dangerous
24
http//www.arpansa.gov.au/images/basics/emr.jpg
25
ROYGBIV
  • ROYGBIV
  • Red long wavelength
  • Violet short wavelength

26
Doppler Shift
  • If a light or sound source moves towards you, the
    wavelength you measure (hear) from the source
    decreases
  • Frequency increases
  • If a light or sound source moves away from you,
    the wavelength you measure (hear) from the source
    increases
  • Frequency decreases

27
  • http//www.youtube.com/watch?v-t63xYSgmKEfeature
    related

28
Doppler Shift
http//www.psi.edu/esquerdo/asp/shifts.jpg
29
(No Transcript)
30
  • http//www.youtube.com/watch?va3RfULw7aAY

31
Wavelength
http//www.psi.edu/esquerdo/asp/method.html
32
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