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Lecture 11 ASTR 111 – Section 002

Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

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Page 1: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Lecture 11

ASTR 111 – Section 002

Page 2: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Outline

• Short review on interpreting equations

• Light– Suggested reading: Chapter 5.1-5.2 and 5.6-

5.8 of textbook

Page 3: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Volume

2 meters

1 m

eter

Side view of sphere

Increase r by a factor of 2. What happens to volume?

Page 4: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Related questions

• What happens to answer if measurements were 1 yard and 2 yards instead of 1 meter and 2 meters?

• What happens if diameter increases by a factor of two?

• How much more paint is required to cover the larger sphere?

Page 5: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Outline

• Short review on interpreting equations

• Light– Suggested reading: Chapter 5.1-5.2 and 5.6-

5.8 of textbook

Page 6: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Particle versus Wave

• Light is composed of photons.

• To fully understand light, we need to think of it in terms of both a particle and a wave.

Page 7: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Particle

• When thinking about the speed of light, we think of a photon as a wave.

Page 8: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Lecture Experiment

X Y

X Launches a photon every 5 seconds.How often does Y get hit by a photon?

photon

Page 9: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook
Page 10: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Light travels through empty space at a speed of 300,000 km/s

• In 1676, Danish astronomer Olaus Rømer discovered that the exact time of eclipses of Jupiter’s moons depended on the distance of Jupiter to Earth

Page 11: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

http://en.wikipedia.org/wiki/File:Roemer.jpg

Page 12: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Light travels at 300,000 km/sec

• About how fast does your car travel in km/hour when you are on the freeway?

• About how fast does your car travel in km/second when you are on the freeway?

• If it takes light 8 minutes to travel from the sun to Earth, how long would it take you to drive?

Page 13: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook
Page 14: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Determining the Speed of Light

• Galileo tried unsuccessfully to determine the speed of light using an assistant with a lantern on a distant hilltop

Page 15: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• In 1850 Fizeau and Foucalt also experimented with light by bouncing it off a rotating mirror and measuring time

• The light returned to its source at a slightly different position because the mirror has moved during the time light was traveling

• d=rate x time again gave c

Page 16: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• What would happen if the stationary mirror was actually moving towards the rotating mirror?

Page 17: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Waves

• A review of waves

Page 18: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Light is electromagnetic radiationand is characterized by its wavelength ()

Page 19: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Frequency and Wavelength

f or unit time

1unit length

The Greek letter “nu” and not the letter “v”

Page 20: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook
Page 21: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Cars are traveling at 100 km/hr to the right• What would you need to know in order to

be able to tell how often (frequently) a car will pass the finish line?

Finish line

velocity = 100 km/hr

Page 22: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Finish line

v = 100 km/hr

Replace cars with lines

Page 23: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Cars are traveling at 100 km/hr to the right• What would you need to know in order to

be able to tell how often a peak will pass the finish line?

Finish line

v = 100 km/hr

Page 24: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Finish line

cDistance between peaks

How often peakpasses finish line

How fast wave moves to right

Frequency and wavelength are intimately related for a wave.

Page 25: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Demo with snapping rope

Page 26: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Interference - destructive

t=1

t=2

Page 27: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Interference - destructive

t=3

t=4

Page 28: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Interference

?

t=1

t=2

Page 29: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Interference

?

?t=3

t=4

Page 30: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Video

http://phys23p.sl.psu.edu/CWIS/SPT--BrowseResources.php?ParentId=189

Page 32: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

x

x

x x

x x

x x

x xx

x

Page 33: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

The electromagnetic spectrum

Page 34: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Because of its electric and magnetic properties, light is also called electromagnetic radiation

• Visible light falls in the 400 to 700 nm range

• Stars, galaxies and other objects emit light in all wavelengths

Page 35: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook
Page 36: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Which of the following has the highest frequency?– Visible light– Radio waves– Microwaves– X-Rays– Infrared light– Ultraviolet light– Gamma rays

Page 37: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Which of the following has the highest wavelength?– Visible light– Radio waves– Microwaves– X-Rays– Infrared light– Ultraviolet light– Gamma rays

Page 38: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Which of the following has the highest speed?– Visible light– Radio waves– Microwaves– X-Rays– Infrared light– Ultraviolet light– Gamma rays

Page 39: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• Which of the following has the highest energy E (h is a constant)?– Visible light– Radio waves– Microwaves– X-Rays– Infrared light– Ultraviolet light– Gamma rays

hc

E

Page 40: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• How is the energy of a photon related to its frequency?

Page 41: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

The dual nature of light

• Particle

• Wave

Page 42: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Particle

Page 43: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

What would you expect if instead of a laser beam you used yellow spray paint beam?

Draw it!

Page 44: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Wave

Page 45: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

x

x

x x

x x

x x

x xx

x

Page 46: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

x

x

x x

x x

x x

x xx

xThe amplitude of the wave in the middle is the highest

“Projection screen”

Page 47: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

The atom and light

Page 48: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

• An atom has a small dense nucleus composed of protons (and neutrons)

• Rutherford’s experiments with alpha particles shot at gold foil helped determine the structure

Probing the atom

Page 49: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook
Page 50: Lecture 11 ASTR 111 – Section 002. Outline Short review on interpreting equations Light –Suggested reading: Chapter 5.1-5.2 and 5.6- 5.8 of textbook

Spectral lines are produced when an electron jumps from one energy level to another within an atom

• The nucleus of an atom is surrounded by electrons that occupy only certain orbits or energy levels

• When an electron jumps from one energy level to another, it emits or absorbs a photon of appropriate energy (and hence of a specific wavelength).

• The spectral lines of a particular element correspond to the various electron transitions between energy levels in atoms of that element.

• Bohr’s model of the atom correctly predicts the wavelengths of hydrogen’s spectral lines.