Showing posts with label Light Spectra. Show all posts
Showing posts with label Light Spectra. Show all posts

Thursday, January 12, 2012

Curiosities of the Color Wheel

Reading about Goethe's experimentations with the origins of light and color this week got me interested about other curiosities of the color wheel. In my journey though many an internet page led me to find a very interesting phenomenon about the color magenta. While this color may seem just as uninteresting as the rest of them, there are actually some very interesting aspects to magenta. To understand what is so interesting about magenta, one must first understand the basic properties of the visible light spectrum. Anyone with two brain cells to rub together knows that the visible light spectrum is made up of red, orange, yellow, green, blue, and violet. Now you may be thinking, "Wait Joey, how could there possibly be a color wheel? Wouldn't violet and red have to be connected somehow?" If these were your thoughts then you are indeed correct! It turns out that our brains have invented this color so that it can "bridge the gap" between red and violet on the light spectrum. When our brains interpret color, they detect the wavelength of light emitted or reflected from an object. When we detect light of multiple wavelengths our brains produce compounds of these colors (e.g. yellow light + red light = orange light.) Your brain does this by averaging the two wavelengths of light that the eye receives. The one case where your brain fails at this is with the case of adding red light to violet light. The average of these two wavelengths would be green (that seems wrong doesn't it?) Instead of producing green, your brain invents this new color magenta! Isn't that interesting? I'm sure that if you have read this you will never look at the color magenta the same way ever again!

-Joey Gurrentz
http://www.biotele.com/magenta.html

Wednesday, March 23, 2011

LIGHT


Hello fellow bloggers, my first post!

Light Diffraction Experiment:


The aim of our past experiment was to compare the spectrum of an energy-saving light bulb with that of a normal tungsten light bulb.The first time we attempted this experiment we came across some difficulty when trying to actually see the different orders, or groups of diffraction patterns that were visible to our eyes.
However, after some useful instructions from classmates, we tried it again. This time we got much clearer results. After setting up our “lab,” we first tested out the tungsten light bulb. With this light bulb we were able to see two distinct orders of diffraction pattern. The observed rectangular areas of visible light behind the diffraction grating had three distinct colors—blue on the far right, green in the middle, and red on the left. In this case, the colors all blended together in a continuous fashion.

Order, n

Angle of diffraction

Uncertainty

Sin On

Uncertainty in sin On

Blue Spectral Line





1

53

1

0.799

0.017

2

57

1

0.839

0.017

Green Spectral Line





1

50

1

0.766

0.017

2

55

1

0.819

0.017

Red Spectral Line





1

47

1

0.731

0.017

2

53

1

0.799

0.017

Using the equation: wavelength=d x gradient we got the following values for wavelengths using the tungsten light bulb: blue= 400 nm, green=530 nm, and red=680 nm.

We then exchanged the normal tungsten light bulb out for the energy-saving light bulb. Using this light bulb we again only observed two different orders. However, in contrast to the normal light bulb, in these orders of lights the colors did not blend together continuously, rather they were discrete. This could possibly have something to do with how it saves energy, with the spectral lines representing that it only emits certain energies, whereas the normal lightbulb emitted wavelengths of all energies. We recorded and calculated the following values:

Order, n

Angle of diffraction

Uncertainty

Sin On

Uncertainty in sin On

Blue Spectral Line





1

32

1

0.530

0.017

2

35

1

0.574

0.017

Green Spectral Line





1

34

1

0.599

0.017

2

38

1

0.616

0.017

Red Spectral Line





1

36

1

0.588

0.017

2

41

1

0.656

0.017

Calculating the wavelengths, we got measurements of 440 nm for blue, 570 for green, and 680 for red. These were similar to the numbers we got when using the normal bulb, which makes sense because wavelengths of light for each color should not differ. These values are also relatively close to the actual values for the wavelengths of light for red, blue, and green.

When performing this experiment, a number of uncertainties arose. To take the measurements of the angles, the numbers were also a result from which angle we looked at the diffraction grating, so it was important to take measurements from the same viewing angle. Also, a very small error in measurements could result in a much larger difference in sin values and therefore wavelength measurements.


Monday, February 21, 2011

Comparing Spectra of Tungsten and Energy- Saving Light Bulbs

Comparing Spectra of Tungsten and Energy- Saving Light Bulbs

Purpose

Compare the spectrum of an energy-saving light bulb with that of a tungsten-filament light bulb by meanings of wavelength measurements and observational techniques.

Equipment and Materials

Shoe Box

Lamp

Tungsten-filament light bulb

Mercury vapor; energy saving light bulb

300 and/or 1000 diffraction grating

Scissors

Modeling Clay

Dark thread

Sewing pin

Drawing pin

Electrical tape

Protractor

Flashlight

Procedure

1. A fairly dark location was obtained for the conduction of the experiment. This was a room without windows (hallway and bathroom).

2. The light box was then prepared. This was done by cutting off one end of a shoe box and cutting a 1mm wide slit 5 cm long on the other side. This box was then taped to a table and covered with a light, non-synthetic towel to minimize light pollution.

3. The protractor was placed approximately 55 cm directly in front of the shoe- box; with its zero degree point of the protractor aligned with the slit of the box. A drawing pin was inserting through its apex, with its sharp point exposed.

4. The diffraction plating was placed parallel to the flat edge of the protractor and was secured upright with modeling clay. The diffraction plate was centrally aligned with the slit of the shoe- box and the tip of the drawing pin.

5. Black thread was attached to the drawing pin and a piece of modeling clay, which held a sewing pin. This served as the sighting mechanism.

6. A lamp with an energy-saving bulb was then inserted into the shoe -box and was turned on. Once observations and recordings were taken, the tungsten-filament bulb was inserted to compare qualitatively the differences between the two bulb-type’s spectra.

Data

1000 Gradient

Observation Table

1000 Gradient

Order

Sin(Degrees)

Degrees

Wavelength

Blue Spectral Line

445 nm

1

0.446

26.5

1

0.446

26.5

2

0.876

61.2

2

0.906

64.9

3

4

5

Green Spectral Line

1

0.581

35.5

1

0.566

34.5

2

3

4

5

Red Spectral Line

1

0.67

42.1

1

0.64

39.8

2

3

4

5


Observation Table

300 Gradient

Order

Sin(Degrees)

Degrees

Wavelength

Wavelength with Zeros
for Missing Orders

Blue Spectral Line

533.13 nm

465 nm

1

0.131

7.5

2

0.272

15.8

3

No Blue

4

No Blue

5

0.766

50

Green Spectral Line

533.47 nm

589 nm

1

0.158

9.1

2

0.335

19.6

3

0.483

28.9

4

No Green

5

0.804

53.6

Red Spectral Line

692 nm

692 nm

1

0.206

11.9

2

0.376

22.1

3

0.52

31.3

4

0.728

46.7

5

0.909

65.3


















































Discussion/ Conclusions

Observations and data were taken after the equipment was set up. The first set of data was taken with the 1000 gradient. With the 1000 gradient, the blue spectra line produced two orders (26.5 and 64.9 degrees; 26.5 and 61.5). The green spectral line was only seen with one order (35.5; 34.50 degrees) and the red spectral line was only seen with one order (42.1; 39.8 degrees). The measurements for the 1000 gradient was taken twice; once from each side of the spectra (once from the right, once from the left). It was predicted that the degree measurement for a specific order from a specific color line would be the same from both the right and left side orders. As the data represents, the degree measurements from the left and right sides are very similar, with the largest difference being 3.7 degrees (blue spectral line, second order). This is most likely because the second order was blurry and not distinct.

The second set of data was taken with the 300 gradient. The 300 gradient produced more distinct, clear and bright color orders. The blue spectral line produced five orders, although the third and fourth orders were not distinct enough for measurements. The green spectral line also produced five orders, while the fourth order was not distinct enough to take measurements. The red spectral produced five vivid orders of color lines.

After the data was taken, the sin of the degrees measured were calculated. As implied by the graphs, with the 300 gradient, the sin (degrees) increased as the order number increased. This was true for all of the spectral lines that contained more than one order. In general, the slopes increased from blue, to green, to red; although the slope differences between the blue and green data was minute. This increase correlates to the increases in standard wavelengths from blue, to green, to red.

The second part of this experiment was performed with a tungsten- filament light bulb as compared to the energy-saving bulb that was used previously. With the tungsten-filament light bulb the orders were much different in appearance than the energy-saving light bulb. The tungsten-filament light bulb produced two full orders of diffraction and one partial order up to blue. These orders were very blurry and fuzzy. They were very non-distinct and had a grayish haze over the colors. The colors in the energy-saving light bulb were significantly more distinct and there were more orders observable.

Measurement uncertainties arose for the higher orders. This was due to the degradation of order clarity within the spectrum as the higher orders were reached. These measurements could be improved upon by using a diffraction gradient of a larger size. This would allow the higher orders to be clearer at less tangential viewing angles. Copious amounts of data and measurements would further the validity of this experiment.

Our calculated wavelengths with the 300 gradient deviated approximately 30-60 nm from the accepted wavelength values. This is most likely due to the light bulb or the specific condition that surrounded the experiment. Additionally, the 300 gradient diffraction plate had a slight diagonal crack, which may have slightly altered the results.