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Light and Temperature

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Orion by IRAS. Io from IRTF. 5. The Moon in eclipse. The IR Universe ... Orion by IRAS. R. Gendler. 5. The Greenhouse Effect. Why is my car hot on a summer day? ... – PowerPoint PPT presentation

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Title: Light and Temperature


1
Light and Temperature
  • Astronomy The Science of Seeing

2
Goals
  • What is light?
  • What are the types of light?
  • Where does the light we see come from?
  • Understanding the light of heat.
  • On a sunny day
  • Why does it seem hotter wearing a black T-shirt
    versus a white one?
  • Why are they different?

3
How do you do Astronomy?
  • How do Chemists do Chemistry?
  • Make solutions, mix chemicals
  • How do Biologists do Biology?
  • Breed fruit flies, (and whatever else biologists
    do).
  • Devise and conduct experiments in their labs.
  • But how do you do that for astronomy?

4
What you see is all you get!
  • So you need to squeeze EVERY last drop of
    information out of the light we get.
  • This semester well see how we can use light to
  • Weigh a planet.
  • Take a stars temperature.
  • Tell whats in the center of a star a thousand
    light-years away.
  • Tell what our Galaxy look like from the outside.

5
The Visible Spectrum
  • When you think of light, what do you think of?

6
What is Light?
  • Light is a wave of energy.
  • Moves through a vacuum.
  • Travels at the speed of light (a CONSTANT)
  • c 3 x 1010 cm/s
  • The wavelength (l) and frequency (n) are related
  • c ln

7
(No Transcript)
8
To Sum Up
  • Radio waves, microwaves, rainbows, UV waves,
    x-rays, etc are ALL forms of light
    (electromagnetic waves).
  • They ALL travel through space at the speed of
    light. c
  • The higher the frequency, the shorter the
    wavelength. c ln
  • What does light look like?

9
A Spectrum
  • A spectrum the amount of light given off by an
    object at a range of wavelengths.

10
Three Reasons
  • All objects do one or more
  • Reflect light because of color or smoothness
    (same as scatter)
  • Emit light because of their temperature
  • (thermal radiation)
  • Emit or absorb light because of their composition
  • (spectral lines)
  • A person, house, or the Moon reflects visible
    light, and because each is warm, emits infrared
    light.

11
Temperature and Light
  • Warm objects emit light.
  • Thermal radiation

12
Kelvin Temperature
  • Kelvin an absolute scale.
  • Kelvin is Celsius 273 degrees.
  • Water freezes 0 C ? 273 K
  • Water Boils 100 C ? 373 K
  • Room Temp 80 F ? 27 C ? 300 K
  • Surface Sun 5800 K

13
Thermal Radiation Laws
  • Hotter is bluer.
  • (peak at shorter wavelength)
  • Hotter is brighter.
  • (More intense at all wavelengths)

14
Concept Test
  • Which of the two stars (A or B) is at a higher
    temperature?
  • a. Star A
  • b. Star B
  • c. The two stars have the same temperature.
  • d. It is not possible to infer this relationship.

15
Concept Test
  • Which of the following best describes how Star A
    would appear compared to Star B?
  • a. Star A would appear more red than Star B.
  • b. Both stars would appear more red than blue.
  • c. Both stars would appear more blue than red.
  • d. Star A would appear more blue than Star B.
  • e. None of the above.

16
Concept Test
  • Which of the following best describes the light
    from Star A compared to Star B?
  • a. More ultraviolet light but less visible
    light.
  • b. More infrared light but less visible light.
  • c. More visible light but less infrared light.
  • d. Less infrared light and less ultraviolet
    light.
  • e. More ultraviolet light and more visible
    light.

17
Concept Test
  • Imagine the Suns surface suddenly became much
    cooler (while the Suns size remains the same).
    Compared to the light it now emits, the Sun would
    emit
  • More ultraviolet light but less visible light.
  • More infrared light but less visible light.
  • More visible light but less infrared light.
  • Less infrared light and less ultraviolet light.
  • More ultraviolet light and more visible light.

18
Atoms in Motion
  • Everything is composed of atoms which are
    constantly in motion.

19
Temperature
  • The hotter the object, the faster the average
    motion of the atoms.

COOLER
HOTTER
20
Atoms and Light
  • As atoms move they collide (interact,
    accelerate).
  • Collisions give off energy.
  • But light IS energy.

E hc/l
21
Light and Temperature
  • The hotter the object the faster the average atom
    and the more energetic the average collision.
  • The faster the atoms the more collisions there
    are.

HOT
COLD
22
Energy and Intensity
  • The more energetic the average collision the
    bluer the average light that is given off.
  • Since E hc/l
  • The more collisions that occur the more light
    that is given off per surface area.

1. Hotter is bluer. (peak at shorter wavelength)
  • 2. Hotter is brighter.
  • (more intense at all wavelengths)

23
Graphically
  • lpeak a 1/T F a T4

24
Result
  • HOT toasters are BRIGHTER than cool toasters.
  • HOT toasters are BLUER than cool toasters.
  • What is the peak wavelength for something at room
    temperature (a cool toaster or a cool person)?
  • lpeak a 1/T
  • lpeak k 1/T
  • lpeak (3 x 10-3 m/K) 1/ 300 K
  • lpeak 10-5 m

25
Thermal versus Reflection
  • Thermal radiation is light given off because of
    an objects temperature.
  • Dont confuse with reflected light
  • Buses are yellow not because they are hot enough
    to emit visible radiation but rather they reflect
    the yellow light given off by the Sun.
  • What kinds of thermal radiation do we see in our
    everyday life?

26
The IR World
  • Everyday objects (at everyday temperatures) emit
    thermal radiation in the IR, this is why we
    equate IR with HEAT.

http//www.x20.org/library/thermal/blackbody.htm
27
The IR Universe
  • Everyday things that are hot radiate in the IR
  • Dust There are interstellar clouds of dust.

28
The IR Universe
  • Molten Rock There are lava flows on a moon of
    Jupiter.

Io from IRTF.
Orion by IRAS
29
The IR Universe
  • In eclipse, there is no reflected light.
  • Only thermal radiation.
  • Differences in composition lead to differences in
    temperature.

Orion by IRAS
30
The Greenhouse Effect
  • Why is my car hot on a summer day?
  • At T 6000 K, the Sun radiates mostly visible
    light.
  • Windshield is transparent to visible light.
  • Car seat absorbs this visible light and warms up
    to 400 K.
  • At T 400 K, my seat radiates mostly at longer
    wavelengths in the IR.
  • Windshield is opaque in the IR.
  • Result Energy is TRAPPED inside the car!

31
Venus and Earth
  • Certain gases act the same way as your
    windshield Carbon Dioxide (CO2).
  • Venus Runaway greenhouse effect.
  • Earth Could that happen here?

32
Color Whys
  • Why is that shirt blue?
  • Why is the Sun yellow?
  • Why is this paper white?
  • Why is the light filament orange?
  • Why is Mars red?
  • On a sunny day
  • Why does it seem hotter wearing a black T-shirt
    versus a white one?

33
Homework 5
  • For Monday 20 Sept Read B6.4 6.5
  • Do B6 Problems 4, 14, 24
  • Consider the four stars (A,B,C,D) of Problem 17
    in Chapter B6. Arrange them by speed relative to
    us (starting with the fastest moving towards us
    and ending with fastest away).
  • A, B, C, D
  • B, A, D, C
  • D, C, B, A
  • C, D, A, B
  • None of the above
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