20120117

Presentation: redirecting light

Now that we've already been introduced to "light," that is, the electromagnetic spectrum, let's take a look at redirecting (visible) light. Note that like presentations in the previous first semester of this college physics sequence, this presentation will hopefully give you a sense of what Bill Nye ("The Science Guy") likes to describe as "PBJ"--the "passion, beauty, and joy" of reflecting and refracting light. We simply don't have time for an exhaustive, comprehensive discussion of this material in class--that's what your textbook is for!

We refer here, of course, to specular reflection, not diffuse reflection.Reflection is redirecting light by bouncing it off of a surface.

Conventionally we consider reflections off of flat surfaces. (Don't worry about what's about to happen here--it's art!)

This place actually exists in real-life, but curiously enough, real-life Chicago METRA cops sometimes will prevent you from taking pictures of it and escort you off the plaza.  What's up with that?Even with reflections off of curved surfaces, each point on it can be considered a locally flat surface.

Apparently hate is love in the mirror universe.And more "PBJ" for reflections--they have the curious property of reversing front-to-back symmetry (or here in this perspective, left-to-right symmetry).

By convention, angles are only measured between the ray and the normal.  However, if angles between the surface and the ray are used instead, the law of reflection still works.
The law of reflection is simple geometry--for a (visible) ray of light incident on a flat surface, if we measure the angle of incident with respect to the normal (a line drawn perpendicular to the surface), the reflected ray will make the same angle as it leaves the surface. (This law also applies for curved surfaces, provided we look close enough such that it look locally flat.)

Instead of bouncing light off of surfaces, if light can pass into a transparent material, we will have refraction, where it is redirected by being "bent."

Refraction occurs when light starts in one material, and passes into another. (This art installation only gives the illusion of seeing light from people underwater; instead there is only a thin layer of water supported by sheet of glass between these two levels.)

No ducks were harmed in the taking of this photograph.When light does start in one medium, and pass into another medium, it will refract, or bend, which can produce curious results.

Look at the exhaust plume from this jet: heat warms the air and changes its density, making light travel at a different speed through it, and it will be bent in interesting directions. Also note the shockwaves from leading edges on the jet--here air is compressed, and again light traveling through it will be bend it in interesting directions.

Now take a look at this transparent block. Light will travel with a different speed through it than through air, and so the light will be bend in interesting directions. Why can't we see the block when we pour water around it? (Video link: "100108-1140566.")

Again by convention, angles are only measured between the ray and the normal.  However, if angles between the surface and the ray are used instead, would Snell's law still work the same way?  (No--unless the sines were replaced with cosines on both sides of the equations.)
Quantitatively, "Snell's law" describes how light will bend as it passes from one medium into another medium. Note that angles for both the incident ray and refracted ray are measured with respect to the normal (that imaginary line drawn perpendicular to the interface between the two media). The medium with the lower index of refraction will have the larger angle (actually, the larger sine of that angle). (This law of refraction is commonly known as "Snell's law," but in France it is referred to as "Descartes' law," as René Descartes was French, while Willbrord Snellius was Dutch.)

Since the index of refraction is a measure of the "optical slowness" of a material, a faster speed of light corresponds to a lower index of refraction, and a larger angle, as it travels into a material with a slower speed, a higher index of refraction, and a smaller angle. Mnemonic: "Fast-to-slow, bend towards the normal."

Consider starting in a medium with a greater index of refraction. Note that angles for both the incident ray and refracted ray are still measured with respect to the normal (that imaginary line drawn perpendicular to the interface between the two media). The medium with the higher index of refraction will have the smaller angle (actually, the smaller sine of that angle).

The faint reflected ray is not quite visible here, and yes, this picture is flipped left-to-right, but convince yourself that this doesn't change any of the angles and indices of refraction in Snell's law.And since the index of refraction is a measure of the "optical slowness" of a material, a slower speed of light corresponds to a higher index of refraction, and a smaller angle, as it travels into a material with a faster speed, a lower index of refraction, and a larger angle. Mnemonic: "Slow-to-fast, bend away from the normal."

20120116

Presentation: electromagnetic waves

We'll start off the second semester of college physics with light, or more correctly, electromagnetic waves. Since we are covering this topic after rope and string waves, but before electricity and magnetism, this will concentrate on describing their behavior in terms of one-dimensional waves rather than explaining it in terms of three-dimensional electromagnetic fields.

Consider all types of "light."

The electromagnetic spectrum encompasses all types of "light," here listed from low frequency to high frequency. Notice that visible light is only a very small portion of the entire electromagnetic spectrum, which we perceive as colors. The vast majority of the electromagnetic spectrum is invisible to our eyes, but we can detect their presence indirectly with certain instruments, or even different parts of our bodies. (When discussing all types of "light," we'll use "electromagnetic waves," as often "light" refers only to visible light.) Let's introduce these types of light...oops, electromagnetic waves, from lowest to highest frequency.

The lowest frequency form of electromagnetic waves are collectively known as radio waves, which are subdivided into microwave, TV, FM and AM bands depending on the type of device used to send and receive these forms of electromagnetic waves.

Those aren't necessarily sunglasses--most plastic and glass lenses are opaque to infrared light, while remaining transparent to visible light.Slightly higher in frequency along the electromagnetic spectrum is infrared, also known as "heat waves," which our eyes cannot directly see (but we can indirectly feel), but certain devices allow us to "see" in the infrared. (Video link: "infrared heat cam.")

Then slightly higher in frequency on the electromagnetic spectrum is visible light, the only type of "light" we can directly see with our eyes. (What is this person looking at?)

Higher in frequency on the electromagnetic spectrum, we're back again to types of "light" we cannot directly see with our eyes, but we can indirectly "see" with special devices, or in this case, materials that react in certain ways to being exposed to ultraviolet, such as our skin, or this Milky WayTM candy bar.

Don't even think of saying Emperor Palpatine."Who was Count Dooku's Jedi Mentor?"

So either children are supposed be Star Wars trivia experts, or have to go to a nightclub with "blacklights" in order to answer this correctly... (Video link: "090529-1090772.")

Higher in frequency is x-rays, which again cannot be seen by our eyes (well, maybe for Superman), but can be made visible with special devices or certain materials. Note that tissue is relatively transparent to x-rays, while bone, and especially metals are opaque. (What is that thing in this person's nose?)

And highest in frequency are gamma rays, which have higher penetration than x-rays, allowing inspection inside metal shipping containers.

Now let's look at the parameters used to describe these forms of "light," and the connections between them. (From here on, since we'll be discussing the transmission of visible light through different types of transparent media, we'll drop the quotation marks around "light.")

(This is a review of a previous discussion of one-dimensional rope and string waves from last semester.) Note the hierarchy of these wave parameters. Since the wave speed is determined by properties of the material it travels through (independent of the source), and the frequency is determined by the source (independent of the medium), these are said to be independent wave parameters. In contrast, the wavelength of the wave is dependent on both the independent speed and frequency parameters. Algebraically there is nothing wrong with expressing this relation as v = λf and f = v/λ, as long as you recognize that the dependency of λ doesn't change.

To convince yourself that the frequency of the wave remains constant, count how many crests appear from the left edge of the screen over 10 seconds, then count how many crests disappear at the right edge of the screen over 10 seconds.
This is a very simple but adequate model of how the independent and dependent parameters remain constant, or change. Consider light passing from a medium where it has a fast speed, into a different medium where it has a slow speed. The frequency of this light does not change (which depends on its source), so ideally it is still visible light, and hasn't changed frequency to become some other type of electromagnetic waves such as radio or gamma rays! Since the frequency (and type of light) is unchanged, but the speed does change (due to the change in medium), then the wavelength changes, here decreasing ("scrunching") due to the decrease in speed in the new medium.

(N.b.: we are ignoring dispersion for the purposes of this discussion.)

Light changes speed (and wavelength) as it travels through different materials. Commonly used instead of the speed of light through different materials is the "index of refraction."

The index of refraction is defined as the ratio of speed of light in vacuum (c = 3.00x108 m/s) to the actual speed of light in that material. Thus for vacuum, n = 1, while for all other materials, light will travel slower, such that n > 1, and the index of refraction can be considered a measure of "optical slowness" of a material.

Light will travel quickest through vacuum, and the index of refraction is 1.

Through air, light will travel very slightly slower than it does through vacuum, so the index of refraction for air is slightly greater than 1, but to three or fewer significant figures, n can be approximated as 1.

Light will travel noticeably slower through ice, so the index of refraction for ice is noticeably greater than 1.

Light travels a bit slower through water, and so the index of refraction for water is slightly greater than for ice.
Light typically travels slower through glass than through water, so again, a greater index of refraction for glass than water. (Note that different types of glass will have slightly different indices of refraction.)

At the extreme is light traveling through diamond, which for our purposes has the greatest "optical slowness," and the greatest possible index of refraction.

20111230

Astronomy haiku: dark matter

Astronomy 210 Haiku review, fall semester 2011
Cuesta College, San Luis Obispo, CA

Students find their assigned groups of three to four students, and work cooperatively on an worksheet to review for a midterm.

Identify the relevant astronomy concept/answer for this haiku. Briefly explain your choice. Partial credit possible.
Surrounding halo,
invisible gravity.
Holds Milky Way tight.
http://twitter.com/#!/Patrick_M_Len/status/72024267604234240
Concept: __________
Explanation: __________

Section 70160
"Dark matter--Evidence that extra mass lies in extended halo sometimes called dark halo. Not luminous matter detected by its gravitational force."

"Dark matter--No one has seen dark matter because it doesn't give off light, but it creates gravity, so we know it exists."

"Dark matter--Proves Kepler's third law wrong because stars farther out do not move slower because there is no center of gravity."

"Dark matter--Dark matter is gravity that holds the Milky Way together and is unable to be seen."

"Dark matter--The Milky Way doesn't follow Kepler's third law."

"Dark matter--Dark matter is invisible and it holds everything inside the Milky Way."

"Dark matter--Dark matter holds the Milky Way together."
Section 70158
"Dark matter--That's what holds the Milky Way together."

"Monolithic collapse--flattens out over time with halo making disk left."

"Dark matter--Dark matter is the unseen gravity force which fills the universe around galaxies, surrounding the Milky Way."

"Black hole! You know black holes are present when there is a gravity alteration like an entire galaxy clumped together."

"Dark matter--Dark matter is the stuff that surrounds the Milky Way and keeps everything tight."

"Black hole--Black holes are at the center of spiral galaxies and have infinite gravity due to their immense density."

"Dark matter--Dark matter surrounds galaxies, holding them together as they rotate with lots of mass."

"Antimatter/dark matter--is found all around the Milky Way and is unexplained but we know it's there."

Dark matter--Dark matter is invisible but still creates a gravitational pull."

20111228

Astronomy in-class activity: planet-hunting

Astronomy 210 In-class activity 6 v.11.12.22, spring semester 2012
Cuesta College, San Luis Obispo, CA

Students find their assigned groups of three to four students, and work cooperatively on an in-class activity worksheet to determine where in the sky each naked-eye planet will be observed on a given date (here, February 2, 2012).



Previous posts:

20111214

Physics quiz archive: temperature, thermal equilibrium, heat transfer

Physics 205A Quiz 7, fall semester 2011
Cuesta College, San Luis Obispo, CA

Sections 70854, 70855, version 1
Exam code: quiz07n0N3
Sections 70854, 70855 results
Quiz 7 results (max score = 30):
0- 6 : * [low = 6]
7-12 : ********
13-18 : *******************
19-24 : *************** [mean = 19.2 +/- 5.7]
25-30 : ********* [high = 30]

20111211

Astronomy quiz archive: solar system

Astronomy 210 Quiz 7, fall semester 2011
Cuesta College, San Luis Obispo, CA

Section 70160, version 1
Exam code: quiz07n0N3
Section 70160
Quiz 7 results (max score = 40):
0- 8.0 :
8.5-16.0 : ***** [low = 11.5]
16.5-24.0 : **********
24.5-32.0 : ******** [mean = 24.5 +/- 8.1]
32.5-40.0 : ***** [high = 40.0]

Astronomy quiz archive: solar system

Astronomy 210 Quiz 7, fall semester 2011
Cuesta College, San Luis Obispo, CA

Section 70158, version 1
Exam code: quiz07s3tI
Section 70158
Quiz 7 results (max score = 40):
0- 8.0 : ** [low = 4.0]
8.5-16.0 : *******
16.5-24.0 : ***************** [mean = 18.8 +/- 7.2]
24.5-32.0 : ****
32.5-40.0 : * [high = 40.0]

20111210

Total lunar eclipse, December 10, 2011

111210-1280484-1
http://www.flickr.com/photos/waiferx/6486545953/
Originally uploaded by Waifer X

Wifey X and Briquetta (puppy) watching the total lunar eclipse, December 10, 2011.

20111205

Overheard: all that glitters

Astronomy 210L, fall semester 2011
Cuesta College, San Luis Obispo, CA

(Overheard while students set up their research posters for the last astronomy lab meeting.)

Student: "Do you like how I did the galaxies [at the top of the poster]?"

Instructor: "Are those [elliptical galaxy and spiral galaxy] just glitter and glue?"

Student: "Yeah. I had some space to fill in so I went with that."

Instructor: "Seriously, when was the last time you got to use glitter and glue?"

Student: (Beat.) "I'll have to get back to you on that."

20111204

Overheard: fabulous graph

Astronomy 210L, fall semester 2011
Cuesta College, San Luis Obispo, CA

(Overheard while students set up their research posters for the last astronomy lab meeting.)

Instructor: "Are these data points on your graph...sequins?"

Student: "No, they're just drawn in with purple ink."

Instructor: "That's too bad." (Beat.) "Because if they were sequins, your graph would be...fabulous!"