lecture 8 astr 111 – section 002. outline quiz discussion light –suggested reading: chapter...
TRANSCRIPT
Lecture 8
ASTR 111 – Section 002
Outline
• Quiz Discussion
• Light– Suggested reading: Chapter 5.3-5.4 and 5.9
of textbook
• Optics and Telescopes– Suggested reading: Chapter 6.1-6.4
The wavelength of a spectral line is affected by therelative motion between the source and the observer
Doppler Shifts• Red Shift: The object is moving away from the
observer• Blue Shift: The object is moving towards the
observer
/o = v/c
= wavelength shift
o = wavelength if source is not movingv = velocity of sourcec = speed of light
Blackbody Definition• Does not reflect incoming radiation, only
absorbs• Emits radiation, depending on temperature• Temperature and emitted radiation
intensity follow a special relationship
Photon enters
If hole is very small, what is probability that it exits?
One way of creating a blackbody
• Blackbodies do not always appear black!
–The sun is close to being a “perfect” blackbody
–Blackbodies appear black only if their temperature very low
Special Relationship
Wavelength
Inte
nsity
For Intensity, think photons/second on a small area
Question
• Why is photon/second similar to energy/second? How are they related?
Watt? Energy Flux?
Flux
Flux is a measure of how much “stuff” crosses a small patch in a given amount of time. Can have flux of green photons, red photons, etc.
Blackbodies and Astronomy
Blackbody Laws• Stefan-Boltzmann Law – relates
energy output of a blackbody to its temperature
• Wein’s law – relates peak wavelength output by a blackbody to its temperature
Wien’s law and the Stefan-Boltzmann law are useful tools for
analyzing glowing objects like stars
• A blackbody is a hypothetical object that is a perfect absorber of electromagnetic radiation at all wavelengths
• Stars closely approximate the behavior of blackbodies, as do other hot, dense objects
• The intensities of radiation emitted at various wavelengths by a blackbody at a given temperature are shown by a blackbody curve
Special Relationship
Wavelength
Ene
rgy
Flu
x In
tens
ity For Intensity, think photons/second on a small area
Stefan-Boltzmann Law
• A blackbody radiates electromagnetic waves with a total energy flux F directly proportional to the fourth power of the Kelvin temperature T of the object:
4~ TF
Special Relationship
Wavelength
Stefan-Boltzmann Law tells us that if we add up the energy from all wavelengths, then the total energy Flux
4~ TF
Ene
rgy
Flu
x In
tens
ity
Special Relationship
Wavelengthmax
Wien’s law tells us that max depends on temperature
Max intensity at max
T
1~max
Ene
rgy
Flu
x In
tens
ity
Special Relationship
Wavelength
Sketch this curve for larger and smaller T
Ene
rgy
Flu
x In
tens
ity
Overall amplitude increases with Temperature
At high wavelengths, intensity goes to zero
As wavelength goes to zero, intensity goes to zero
Wavelength of peak decreases as temperature increases
Color and Temperature
What would this object look like at these three temperatures?
• Why does it glow white before blue
• Can this figure help us explain?
• Can this figure help us explain?
Near this temperature, this special combination of intensities is what we call white. Also, the realcurve is a little flatter near the peak
The Sun does not emit radiation with intensities that exactly follow the blackbody curve
• If “white” was actually defined by the ideal blackbody curve, we could add a little green to white
So, what color is the sun in space?
Solid green square
So, what color is the sun in space?
Add a little green to white background by makingsolid green square mostly transparent
• If “white” was actually defined by the ideal blackbody curve, this would (sort of) make sense.
• What we call white is actually not the ideal blackbody curve. See http://casa.colorado.edu/~ajsh/colour/Tspectrum.html
So, what color is the sun in space?
• http://casa.colorado.edu/~ajsh/colour/Tspectrum.html
Right side is (should be) alittle “pinker”
Left side is white
If blue light has higher energy, and energy is proportional to temperature, why are my cold spots blue?
AB
C
Ene
rgy
Flu
x
1
2
3
4
5
0
• Which curve represents an ideal blackbody?– Curve A– Curve B– Curve C
• If the object in Figure 1 were increased in temperature, what would happen to curves A, B, and C?
• Curve C is more jagged. The locations where the curve C is small correspond to– Spectral lines of a blackbody– Spectral lines of atmospheric molecules– Instrumentation error– Diffraction lines– Spectral lines of the lens used to the light into
colors
• What is the intensity of curve B at 550 nm?– Impossible to tell; 550 nm is not shown in this
figure– Nearest 0.2– Nearest 0.1– Nearest 0.05– Nearest 0.0
• Venus has no atmosphere. If you measure the spectrum from its surface, – Curves B and C would not change– Curve C would look more like A– Curve C would look more like B– Curve B would look more like A– Curve B would look more like C
• White light is composed of– Equal intensities of all colors of the rainbow– Unequal intensities of all colors of the rainbow– Equal number of photons of all colors of the
rainbow– Unequal number of photons of all colors of the
rainbow– Equal numbers of red, green, and blue
photons
• Does a blackbody have color?– Yes, and they all appear the color of the sun– No, you cannot see a blackbody– Yes, but its depends on its temperature– Maybe, it depends on if it is an ideal
blackbody
• Why is the best reason for putting a telescope in orbit? – Closer to stars– Better view of celestial sphere– The speed of light is higher in space– Less atmospheric interference– Cost
Optics and Telescopes• Questions about blackbody curves
Key Words
• refraction/reflection
• converging/diverging lens
• focal point
• angular resolution
• magnification
• chromatic aberration
Key Questions• Why are there so many telescopes in Hawaii?• Why is our best most famous telescope orbiting
Earth and not in Hawaii?• What is the difference between optical and digital
magnification (zoom)?• How and when (but not why) does light (and other
forms of electromagnetic radiation) bend?• How does a telescope work?
• What is the difference between magnification and light-gathering power?
side note: What is the difference between optical and digital zoom?
T
side note: What is the difference between optical and digital zoom?
T
Same amount of information
Practical note: What is the difference between optical and digital zoom?
T
Much more information (detail)
• You can create a digital zoom effect by taking a digital picture and expanding it (with photoshop, etc.)
• You can’t squeeze out more detail from the image (that is, increase the optical resolution), contrary to what you see on TV
Therefore
Can explain lots about telescopes and other
devices with only three optics principles
Principle 1• Light rays from distant object are nearly
parallel
Principle 1• Light rays from distant object are nearly
parallel
Collector
Principle 2• Light reflects off a flat mirror in the same
way a basket ball would bounce on the floor (angle of incidence, i = angle of reflection, r)
Principle 3 prep
What happens, a, b, or c?
• As a beam of light passes from one transparent medium into another—say, from air into glass, or from glass back into air—the direction of the light can change
• This phenomenon, called refraction, is caused by the change in the speed of light
Axle and wheel from toy car or wagon
Sidewalk
Grass
Principle 3• Light changes direction when it moves
from one media to another (refraction). Use wheel analogy to remember which direction normal
90o
Low index (e.g., air)
Higher index (e.g. water)
Principle 3a• Light changes direction when it moves
from one media to another (refraction). Use wheel analogy to remember which direction normal
90o
Low index (e.g., air)
Higher index (e.g. water)
Principle 3b• Same principle applies when going in
opposite direction
normal
90o
Low index (e.g., air)
Higher index (e.g. water)
Principle 3c• At interface light diffracts and reflects
(you can see your reflection
in a lake and someone in lake
can see you)
Low index (e.g., air)
Higher index (e.g. water)
These angles are equal
i r
What happens to each beam?A
B
C
A
B
C
A
B
C
What happens?
?
?
?
zoom box
zoom box contents nearly flat whenzoomed in
norm
al
90o
zoom box contents
To figure out path, draw normal and un-bent path.
What happens?
?
?
?zoom box
zoom box contents
F
What happens to the beams here?
But you said different colors bend different amount!?
But you said different colors bend different amount!?
This is chromatic aberration
How I remember red bends less
How my optometrist remembers
Red light bends only a little
Red light has little energy (compared to blue)
What happens?
?
?
Now we can explain
… rainbow color ordering
Observer sees red higher in sky than blue
Sunlight
Sunlight diffractionreflection
diffraction
Water droplet
Now we can explain
… how an eye works
… how an eye works
Retina
Info from distant object is concentrated on small area on retina
Eye lens
… how an eye works
RetinaEye lens
Light from Sun
Light from a distant lighthouse
Sunlight lower than lighthouse light
… how an eye works
RetinaEye lens
Light from a distant lighthouseSun appears lower than lighthouse light
Now we can explain
… how telescopes work
• Magnification is ratio of how big object looks to naked eye (angular diameter) to how big it looks through telescope
Telescope principles
½ o
10 o
Magnification is 10/0.5 = 20x
• Although telescopes magnify, their primary purpose is to gather light
Telescope principles
Collector
• How much more energy does a 1 cm radius circular collector absorb than a 4 cm radius collector?– Same– 2x– 4x– 16x– Need more info
Question
Collector
Reflecting telescope
• Previously I described a refracting telescope. The principles of reflection can be used to build a telescope too.
Solutions