1. Major Concepts of Physics PHY 102 – Lecture #9 1 2015  Syracuse University Lecture #9 How do the colors mix each other up? February 16 th Spring 2015 Prof. Liviu Movileanu lmovilea@syr.edu Room 211, Physics Bldg., 443-8078 Major Concepts of Physics PHY102

2. Major Concepts of Physics PHY 102 – Lecture #9 2 2015  Syracuse University 1. Review/Continuation Blackbody radiation. 2. Comments on Conceptual Examples 3. Color mixing/Dispersion 4. Primary colors/Rules in color mixing 5. Lecture demonstration (Color mixing) 6. Announcements Lecture objectives

3. For increasing temperatures, the black body intensity increases for all wavelengths. The maximum in the energy distribution shifts to shorter (longer f) for higher temperatures. max T = 2.9x10 -3 m K is Wien’s law for the maximum intensity B (T) providing an estimate of the peak emission Wien’s displacement law Major Concepts of Physics PHY 102 – Lecture #9 3 2015  Syracuse University f

4. Major Concepts of Physics PHY 102 – Lecture #9 4 2015  Syracuse University Colors from the Sun Calculate λ p from Wien’s law. T = 6,000K Result: 480 nm. The wavelength 480 nm is in the green (middle) part of the spectrum. Conclude: At 6000K, the radiation produced is a mixture of red, green and blue light, with intensity peaked in the green. But: The eye perceives equal intensities of red, green and blue as white light. This explains why white light is perceived at the highest temperatures.

5. Suppose that we increase the temperature still further. At 8000K, the value of λ p is in the blue part of the visible spectrum. Stars whose surface temperature is more than 8000K are called blue-hot stars. Major Concepts of Physics PHY 102 – Lecture #9 5 2015  Syracuse University Blue-Hot Stars

6. While red and green are produced in prodigious amounts, blue and violet dominate, and the color that appears is blue. Note that the Wien’s law allows us to estimate the surface temperature of a star, by simply observing the dominant colors it emits. Major Concepts of Physics PHY 102 – Lecture #9 6 2015  Syracuse University Wien’s law

7. Major Concepts of Physics PHY102 – Lecture #9 7 2015  Syracuse University Good absorbers are good emitters. Good reflectors are poor emitters. Emissivity of a Solid The emissivity, e, of a solid measures the ability of the solid to emit radiation at a given temperature T. For a perfect black body, e = 1. For a perfect reflector, e = 0. Stefan-Boltzman’s law Recall the law: For a black body, area A, at temperature T: ∆Q/∆t =  AT 4 Its extension for a general solid: Insert the factor e on the right side of the law: ∆Q/∆t = e  AT 4 Emissivity of a solid

8. Major Concepts of Physics PHY 102 – Lecture #9 8 2015  Syracuse University

9. Major Concepts of Physics PHY 102 – Lecture #9 9 2015  Syracuse University

10. Major Concepts of Physics PHY102 – Lecture #8 20 2005  Syracuse University

11. Major Concepts of Physics PHY 102 – Lecture #9 11 2009  Syracuse University What is white light?/Newton’s observation

12. The dispersion of light Major Concepts of Physics PHY 102 – Lecture #9 12 2015  Syracuse University Conclusion: White light is a composite of the primary colors. Prism reveals this by separating them out. The experiment is: the dispersion of light. Later discovery: Each primary color has its own wavelength range. Conversely, light of a single wavelength must be that of a primary color.

13. Major Concepts of Physics PHY102 – Lecture #9 13 2015  Syracuse University Experimental Finding The shortest wavelengths are bent the most. Violet light (shortest wavelength) is bent the most. Red light (longest wavelength) is bent the least. Examine Sunlight The sun’s surface temperature: 6000K. Wien’s Law yields that the intensity of sunlight peaks at the color green. Wavelength is 450 nm. Sunlight Radiation

14. Major Concepts of Physics PHY 102 – Lecture #9 14 2015  Syracuse University Approximate model for sunlight: Assume the intensities for red (R), blue (B) and green (G) are roughly equal. Also: Ignore its emissions in the colors orange, yellow, and violet. We call the colors R, G, and B the primary additives. The primary Additives

15. Rules in Color Mixing Additive Combining You need to know these four facts: R + G = Y (yellow). R + B = M (magenta). G + B = C (cyan). R + G + B = W (white). The color circles demonstration shows these four facts explicitly. Important note: We are combining light sources. That is, each color in the sum is entering our eye, simultaneously. Major Concepts of Physics PHY 102 – Lecture #9 15 2015  Syracuse University

16. Major Concepts of Physics PHY 102 – Lecture #9 16 2015  Syracuse University

17. Major Concepts of Physics PHY 102 – Lecture #9 17 2015  Syracuse University

18. R, G, and B Why are they the primary additives? Because experiment shows: Any perceived color can be matched by an additive combination of R, G and B. Just choose appropriate relative intensities. Reason: The eye has three types of sensors in the retina. They are each sensitive to either R, G, or B light. Major Concepts of Physics PHY102 – Lecture #9 18 2015  Syracuse University Primary Additives

19. Major Concepts of Physics PHY102 – Lecture #9 19 2015  Syracuse University Color TV Example: Color TV Most TV tubes produce color as follows: Use three different phosphors on the screen, arranged in tiny dots. The three phosphors produce red, green or blue light, when struck by the electron beam of the tube. The eye integrates the tiny dots to produce a mixture of the three primaries. The three types produce red, green or blue light when an electron beam impinges.

20. Filters A filter absorbs light of certain colors. It lets through the other colors. Example: An ideal red filter absorbs all colors but red light. It transmits red light. In the model W = R + G + B, the red filter absorbs blue and green light, transmits red. Demonstration: A yellow filter is put on overhead projector above a slit. The light is separated by a diffraction grating. What primary colors are absent? Why? Major Concepts of Physics PHY102 – Lecture #9 20 2015  Syracuse University Filters

21. White light is incident on a pair of overlapping green and red filters. What light emerges? Important note: If we overlap two filters, we are not combining light additively. Each filter subtracts light. Together, no light gets through. We call this subtractive combining. Major Concepts of Physics PHY102 – Lecture #9 21 2015  Syracuse University Question

22. Mixing Paints This is another example of subtractive combining. Example: We make a fine mixture of R and B paints. What color is the mixture? Any color of light that can be absorbed by either pigment is absorbed. This is subtractive combining. Subtractive Mixing Problems Two colors are mixed finely. Or, two filters overlap. What is the resulting color? (Always assume white light is incident.) Major Concepts of Physics PHY 102 – Lecture #9 22 2015  Syracuse University

23. Major Concepts of Physics PHY 102 – Lecture #9 23 2015  Syracuse University 1. Workshop this week: Color mixing; Example of problems and their solutions from previous lectures. 2. The material taught in this lecture cannot be found in the textbook!! Please take a look at print outs and PHY 102 web site. 3. Homework #3 is due on this week. AnnouncementsQuestion: Pigments of cyan and magenta are mixed together finely. What is their resultant color?