Latent Heat

1. Latent Heat When a solid melts or a liquid boils, energy must be added but the temperature remains constant! (This can be explained by considering that it takes energy to break the bonds holding the material together.) The amount of energy it takes to melt or boil a certain amount of material is called a latent heat.

2. Latent Heat For water, the latent heat of fusion (heat needed to melt ice to water) is 79.7 cal/gm. For water, the latent heat of vaporization (heat needed to boil water) is 540 cal/gm. For alcohol, the latent heat of vaporization is less at 204 cal/gm.

3. Latent Heat - Example Example: how much energy does it take to vaporize 1 liter of water if the water is initially at a temperature of 98oF ?

4. Latent Heat - Example cont. First we need to find the energy to raise the temperature of the water up to boiling: this involves the heat capacity (which for water is 1 cal/gm*oC) (density of water is 1 gm/cc, 1 liter = 1000 cc): C = Q/(m*T) , with T = (212-98)*5/9=63oC Q= (1 cal/gm*oC)*(1 gm/1cc)*1000 cc*63oC = 63,333 cal * (4.186 J/cal) = 265,000 J .

5. Latent Heat - Example cont. Now we add in the latent heat: (for water, this is 540 cal/gm) Q = L*m = (540 cal/gm)*(1 gm/cc)*(1000 cc) = 540,000 cal * (4.186 J/cal) = 2,260,000 J Total energy required is: 265,000 J + 2,260,000 J = 2,525,000 J .

6. Latent Heat - Example #2 Question: how much water would be needed to keep cool for 4 hours by evaporation if the outside temperature is 100 oF (essentially same as body’s) and a power output of 200 Watts (doing some work) is desired?

7. Latent Heat - Example cont. Since the body generates 200 Watts, or 200 Joules a second, the body must evaporate water to carry this energy away. Q =(200 J/sec)*(4 hs)*(3600 sec/hr)= 2,880,000 J. From the previous considerations, evaporating 1 liter of water carries away 2,525,000 J. Thus we need 2.88MJ / (2.525MJ/liter) = 1.14 liters of water.

8. Latent Heat - Example cont. Would more or less alcohol be needed to keep cool for the same energy output? (The heat capacity of alcohol is 2.4 J/gm*oC; the density of [ethanol] .791 gm/cc; the boiling point is 78oC; latent heat of vaporization is 854 J/gm). From this you should be able to decide whether water or alcohol is better for heat regulation.

9. Heat Transfer There are four ways of moving heat: • Evaporation(using latent heat - we’ve already looked at this) • Convection(moving heat with a material) • Conduction(moving heat through a material) • Radiation We’ll develop equations for conduction and radiation and talk about convection.

10. Heat Transfer: Convection Heat Transfer by Convection is when you heat some material and then move that material containing the heat. The amount of heat energy moved depends on the heat in the material (heat capacity times amount of material times the temperature difference) and how much material you move per time. The blood and hot air furnaces use this method.

11. Heat Transfer: Conduction Heat will flow through a solid material from the hot end to the cold end. What is flowing? No matter is flowing! We can think of energy as flowing in this case! We measure the flow of energy as power: 1 Watt = 1 Joule/sec .

12. Heat Transfer: Conduction Power = Q/t = k*A*T/L where k is a constant that depends on the material, called the thermal conductivity; where A is the cross sectional area; where L is the distance from the hot end to the cold end; and T is the temperature difference between the hot and cold ends. L A k Thi Tlow

13. Conduction - R values Units of thermal conductivity: from Power = Q/t = k*A*T/L k has units of W*m/(m2K) or J/(sec*m*K), and k depends only on the material. Often a material is given an R value, where R includes both the material and the thickness of the material: R = L/k, and R has the units of m2*sec*K/J (or ft2*oF*hr/BTU, where 1 ft2*oF*hr/BTU = 0.176 m2*sec*K/J)

14. Conduction - R values P = Q/t = k*A*T/L = A*T / R where we define R = L / k . where if we have several different materials and thicknesses, we can simply add the individual R’s to get the total R: Rtotal = Ri .

15. Conduction - Conductivity approximate k values for some materials: • metals: k = 1 cal/(sec*cm*oC) • glass: k = 2 x 10-3 cal/(sec*cm*oC) • wood, brick, fiberglass: k = 1 x 10-4 cal/(sec*cm*oC) • air: k = 5 x 10-5 cal/(sec*cm*oC)

16. Conduction - Example Let’s calculate the R valueof brick 4 inches in thickness: L = 4 in * (.0254 m/in) = .10 m k = 1.5 x 10-4 cal/(sec*cm*oC) * (4.186 J/cal)*(100 cm/m) = .063 J/(sec*m*oC) R = L/k = .10 m / .063 J/(sec*m*oC) = 1.6 m2*K/Watt * (1 ft2*oF*hr/BTU) /( .176 m2*K/Watt) = 9 (1 ft2*oF*hr/BTU)

17. Conduction - Example What is the heat loss through the brick walls (assume no other insulation) of a house that is 50 ft x 30 ft (floor area: 1500 ft2) x 8 ft when the temperature inside is 72oF and the temperature outside is 20oF ?

18. Conduction - Example P = Q/t = k*A*T/L = A*T / R A = 50ft * 8ft + 30ft * 8ft + 50ft * 8ft + 30ft*8ft = 1280 ft2 * (1 m2/10.76 ft2) = 120 m2 . T = (72-20)oF * (5K/9oF) = 29 K R = 1.6 m2*K/Watt P = 120 m2 * 29 K / 1.6 m2*K/Watt = 2175 Watts = 2.175 kW.

19. Blackbody Radiation: What is a blackbody? A BLACK object absorbs all the light incident on it. A WHITE object reflects all the light incident on it, usually in a diffuse way rather than in a specular (mirror-like) way.

20. Blackbody Radiation: The light from a blackbody then is light that comes solely from the object itself rather than being reflected from some other source. A good way of making a blackbody is to force reflected light to make lots of reflections: inside a bottle with a small opening.

21. Blackbody Radiation: If very hot objects glow (such as the filaments of light bulbs and electric burners), do all warm objects glow? Do we glow? (Are we warm? Are you HOT?)

22. Blackbody Radiation: What are the parameters associated with the making of light from warm objects?

23. Blackbody Radiation: What are the parameters associated with the making of light from warm objects? • Temperature of the object. • Surface area of the object. • Color of the object ? (If black objects absorb better than white objects, will black objects emit better than white objects?)

24. Blackbody Radiation:Color Experiment Consider the following way of making your stove hot and your freezer cold:

25. Color Experiment Put a white object in an insulated and evacuated box with a black object. The black object will absorb the radiation from the white object and become hot, while the white object will reflect the radiation from the black object and become cool. Put the white object in the freezer, and the black object in the stove.

26. Color Experiment Does this violate Conservation of Energy?

27. Color Experiment Does this violate Conservation of Energy? NO Does this violate the Second Law of Thermodynamics (entropy tends to increase) ?

28. Color Experiment Does this violate Conservation of Energy?NO Does this violate the Second Law of Thermodynamics (entropy tends to increase) ? YES This means that a good absorber is also a good emitter, and a poor absorber is a poor emitter. Use the symbol  to indicate the blackness (=1) or the whiteness (=0) of an object.

29. Blackbody Radiation: What are the parameters associated with the making of light from warm objects? • Temperature of the object, T. • Surface area of the object, A. • Color of the object, 

30. Blackbody Radiation: Is the  for us close to 0 or 1? (i.e., are we white or black?) We emit light in the IR, not the visible. So what is our  for the IR?

31. Blackbody Radiation: So what is our  for the IR? Have you ever been near a fire on a cold night? Have you noticed that your front can get hot at the same time your back can get cold? Can your hand block this heat from the fire? Is this due to convection or radiation?

32. Blackbody radiation: For humans in the IR, we are all fairly good absorbers (black). An estimated value for  for us then is about .97 .

33. Blackbody Radiation:Experimental Results At 310 Kelvin, only get IR Intensity blue yellow red IR UV wavelength

34. Blackbody Radiation:Experimental Results At much higher temperatures, get visible look at blue/red ratio to get temperature Intensity blue yellow red IR UV wavelength

35. Blackbody Radiation:Experimental Results Ptotal = AT4 where  = 5.67 x 10-8 W/m2 *K4 peak = b/T where b = 2.9 x 10-3 m*K Intensity blue yellow red IR UV wavelength

36. Blackbody Radiation:Example • Given that you eat 2000 Calories/day, your power output is around 100 Watts. • Given that your body temperature is about 90o F , and • Given that your surface area is about 1.5 m2,

37. Blackbody Radiation:Example • Given Ptotal = 100 Watts • Given that Tbody = 90o F • Given that A = 1.5 m2 WHAT IS THE POWER EMITTED VIA RADIATION?

38. Blackbody Radiation:Example Pemitted = AT4 •  = .97 • = 5.67 x 10-8 W/m2 *K4 • T = 273 + (90-32)*5/9 (in K) = 305 K • A = 1.5 m2 Pemitted= 714 Watts (compared to 100 Watts generated!)

39. Blackbody Radiation:Example need to consider power absorbed at room T Pabsorbed = AT4 •  = .97 • = 5.67 x 10-8 W/m2 *K4 • T = 273 + (72-32)*5/9 (in K) = 295 K • A = 1.5 m2 Pabsorbed= 625 Watts (compared to 714 Watts emitted!)

40. Blackbody Radiation:Example Total power lost by radiation = 714 W - 625 W = 89 Watts (Power generated is 100 Watts.) Power also lost by convection (with air) and by evaporation.

41. Blackbody Radiation:Example At colder temperatures, our emitted power stays about the same while our absorbed power gets much lower. This means that we will get cold unless • we generate more power, or • our skin gets colder, or • we reflect the IR back into our bodies. Use metal foil for insulation!

42. Thermodynamics The First Law of Thermodynamics is a fancy name for the Law of Conservation of Energy applied to thermal systems. It says: DU = Q - W where DU indicates the change in the internal energy of the system. This internal energy is related to the temperature and heat capacity of the system; Q is the heat energy added to the system; and W is the work done by the system.

43. Thermodynamics The first law of thermodynamics, like the conservation of energy, does not indicate the direction. It does not explain why, when cold milk is added to hot coffee, the cold milk warms up and the hot coffee cools down. The conservation of energy (first law of thermodynamics) permits the possibility that the milk would get even colder while the coffee gets hotter after they are mixed.

44. Second Law of Thermodynamics It is the Second Law of Thermodynamics that explains why the hot coffee does cool down and the cold milk warms up when they are mixed. To understand the second law, however, we need to first look a little atprobability.

45. Probability Consider flipping four coins. How many heads would you expect to get (assuming they were honest coins)? Why do you expect this? Let’s look at all the possible combinations of flipping four coins:

46. Flipping Four Coins Four heads: (only one way) HHHH Three heads: (four ways) THHH HTHH HHTH HHHT Two heads: (six ways) TTHH THTH THHT HTTH HTHT HHTT One head: (four ways) HTTTTHTTTTHTTTTH Zero heads: (only one way) TTTT

47. Probability We see that there are more ways of getting two heads and two tails than any other combination. The same argument can be made about the distribution of energy among many molecules: the highest probability corresponds to the most ways of having that outcome.

48. Probability In the case of distributing the thermal energy between the hot coffee and the cold milk, there are more ways of distributing the energy equally among the many coffee and milk molecules than there are ways of giving it all to just the coffee or just the milk molecules.

49. Statement of 2nd Law A system will tend to go to its most probable state. To measure the ways of having the same state (like determining the number of ways of having two heads out of four coins), we use the concept of entropy.

50. Another Statement Entropy is a measure of the probability of being in a state. Since things tend to go to their most probable state, we can write the 2nd Law of Thermodynamics as: systems tend to have their entropy increase.