Download presentation
Presentation is loading. Please wait.
1
WilliamThompson (Lord Kelvin)
Thermodynamics Understanding the words Temperature Heat Heat capacity The 0, 1, 2 laws of thermodynamics (one of) Kelvin’s legacy’s WilliamThompson (Lord Kelvin)
2
What is Heat? I feel hot Perception as to hot and cold defined relative to our own body temperature, i.e. object is hotter or colder than oneself Objective measurement of temperature Macroscopic, display of temperature gauge Microscopic behaviour of atoms and molecules
3
Measuring temperature
Properties of materials change with temperature Length Volume Resistance
4
Hotter things become longer
Solids get bigger when they get hot A 1 metre long bar heated by 1 degree gets bigger by Steel ≈0.01 mm Glass ≈ mm Rails expand and may buckle on a hot summer day
5
Hotter things take up more volume -1
Most materials get bigger when they get hot (but not water 0°C -> 4°C gets smaller!) Thermometer relies on a thermal expansion of a liquid (e.g.mercury) Thin tube (Gives big length change for small increase in volume) Large volume of reservoir
6
Hotter things change their resistance
All hotter metals have a higher electrical resistance or conductivity Digital thermometer All hotter semiconductors have a lower electrical resistance key definition between to distinguish metals and insulators!
7
Example You have a (glass) jar and you can’t get the metal lid off.
What should you do: a) ask your girlfriend b) run the jar & lid under cold water c) run the jar & lid under hot water
8
Solution: a) ask your girlfriend b) run the jar & lid under cold water c) run the jar & lid under hot water Because the metal has a substantially higher coefficient of thermal expansion than the glass, heating them will make both of them bigger, but the metal will be more bigger.
9
Insulation Example of good (thermal) insulators
A vacuum, polystyrene, fibreglass, plastic, wood, brick (low density/foam structure, poor electrical conductors) Examples of poor insulators, i.e. good conductors Most metals (but stainless steel better than copper) e.g. gold contact used within IC chips to prevent heating Gases, liquids (high density, “mobile”, good electrical conductors)
10
Temperature and scales
Temperature scales (melting & boiling of water) Degrees Celsius (MP 0°C 100°C) Degrees Kelvin (MP K BP K) Degree Fahrenheit (MP 32° F BP 212°F) Explain how a temperature scale is constructed.
11
The Common Temperature Scales
Fahrenheit & Celsius Celsius & Fahrenheit The Celsius & Fahrenheit scales are based on the phase transition temperatures for pure water
12
Converting between scales
State the relation between Kelvin & Celsius Scales. Kelvin to Celsius K = C C = K Fahrenheit to Celsius (Not IB) F = C x (9/5) + 32 C = (F - 32) x (5/9)
13
Example Convert the following temperatures into °F and K
Boiling water, 100°C Freezing water, 0°C Absolute zero, °C 212°F, K 32°F, K -460°F, 0K
14
Stop here
15
Type of thermometer Change in electrical resistance (convenient but not very linear) Change in length of a bar (bimetallic strip) Change in volume of a liquid Change in volume of gas (very accurate but slow and bulky)
16
Heat and internal energy
Can you describe the difference between the terms. Temperature Heat Internal Energy
17
Temperature & Absolute Temperature
Temperature is a property that determines the direction of thermal energy transfer between two bodies in thermal contact. Absolute temperature is a measure of the average kinetic energy of the molecules of a substance. Average kinetic energy is proportional to absolute temperature in Kelvin.
18
Example What is the kinetic energy of an oxygen molecule at room temperature ( 21˚C)? (k = 1.38x10-23J/K) Since we know the kinetic energy, how is it travelling? This is called the root mean squared speed or rms speed. KE = 3/2 kT = 3/2(1.38x10-23 x 294) = 6.09 x Joules We could equate KE = 1/2 mv2 = KE = 3/2 kT and get v2 = 3kT/m mass must be in kg!!!! Not u.
19
Heat (Energy) Is the flow of energy in or out of a system.
Heat (energy) flows because of temperature difference Bigger temperature difference bigger heat flow Less insulation give more heat flow for the same temperature difference Heat will not flow between two bodies of the same temperature
20
Equilibrium Two objects of different temperature when placed in contact will reach the same temperature + = Cold milk Light brown coffee Hot black coffee
21
Heat transfer = energy transfer
Energy measured in Joules but heat often measured in Calories One cal raises one gram of water from 14.5°C to 15.5°C 1 cal = 4.186J Doing work on something usually makes it hot Joules Experiment! 1st law of thermodynamics heat and work are both forms of energy
22
Sir James Joule James Prescott Joule 1818-1889
Stirring water made it warm Change in temperature proportional to work done Showing equivalence of heat and mechanical energy Also that electrical current flow through a resistor causes heating
23
Joules Experiment
24
Internal Energy Is the total potential and kinetic energy of the molecules in a substance. Potential energy is associated with intermolecular forces. Kinetic energy includes both translational and rotational motion.
25
Three Phases – Atomic Model
Three States of Ordinary Matter Solid ® liquid ® gas
26
Atomic Model of Matter Comparing Molecular Forces
Solid – Largest molecular forces Liquid Gas – Weakest molecular forces When the kinetic energy of the molecules become comparable to the energy required for separation the molecules change there position and separate (PE increase). This is a phase transition Melting or vaporizing
27
Avogadro constant One mole a any substance is that quantity of the substance whose mass in grams is numerically equal to the substances molar mass, μ. EX: The moloar mass of O2 is 32 g mol-1 NA = 6.02 x 1023 molecules mol-1
28
Example How many grams are there in a quantity of oxygen gas containing 1.2 x 1025 molecules? The number of moles is (1.20 x 1025)/6.02 x 1023 = mol Since the molar mass is 32 g mol-1 The mass is x 32 = 638 g or kg
29
Example So, how fast is that O2 molecule traveling? O2 = 32 g/mole
v2 = 3kT/m (rms speed of a molecule) m = 0.032/(6.023 x 1023) = 5.3x10-26 kg v2 = 3(1.38 x 10-23J/K)(294)/(5.3x10-26 kg) v = 479 m/sec
30
Transferring heat energy
3 mechanisms Conduction Heat transfer through material Convection Heat transfer by movement of hot material Radiation Heat transfer by light
31
Conduction of heat Conduction in solids Conduction in metal
Heat energy causes atoms to vibrate, a vibrating atom passes this vibration to the next Conduction in metal Heat energy causes electrons to gain energy, electrons travel through metal (conduction) and carry heat energy with them Metals are good conductors of both heat and electricity
32
Conduction of heat The atoms at the bottom are at a higher temperature and will oscillating more strongly than those at the top.
33
Rate of heat flow Heat flow (H) is energy transfer per unit time, depends on Temperature difference Thermal conductivity (k) k (copper) = 385 W/(m K) k (glass) = 0.8 W/(m K) k (air) =0.02 W/(m K) A TH TC L
34
Example Two rods of the same cross-sectional area are joined together. The right rod is a better conductor of heat than the rod at left. The ends are kept at fixed temperatures. In which rod is the rate of heat transfer the largest? Is the temperature at the joining point lower are higher than 54 ˚C? Heat entering the joint must equal the heat leaving the joint. (Conservation of Energy). Hence, the rate of heat transfer is the same. Since the second conductor is poor a much larger temperature gradient can be maintained. Thus, the temperature at the junction will be larger.
35
Thermal conduction vs thermal resistance
Also can use thermal resistance, cf Can make equation of heat flow more general
36
Convection of heat “Hot air rises” (and takes its heat with it!)
Radiators
37
Convection of heat “Hot air rises” (and takes its heat with it!)
Cumulus clouds
38
Figure 16-11 Alternating Land and Sea Breezes
39
Convection of heat Hurricanes Plate tectonics
40
Radiation of heat Don’t confuse with radioactivity
Instead realize that light carries heat (e.g. the sun heats the earth) Anything above absolute zero radiates heat P a AT4 Stefan-Boltzmann law.
41
Radiation of heat involves the generation and absorption of photons. Unlike conduction or convection, however, radiation requires no intervening medium to transport the heat. All objects radiate energy continuously in the form of electromagnetic waves The hotter an object the more power it radiate sand the shorter the wavelength of the peak emission wavelength
42
Not all things emit heat the same
Heat emission from an object area A P = AesT4 s = Stafan’s constant = 5.6x10-8 W/(m2 K4) e = emissivity of a body, 0 -1 ecopper = 0.3 ecarcoal ≈ 1
43
Example Estimate the upper limit to the heat emission of the sun
Suns temperature 7000k Sun’s radius 7x108m Emission, P = AesT4 Area = 4pr2 = 6.2 x 1018 m2 Emissivity ≈ 1 H = 6.2 x 1018 x 5.6x10-8 x 70004 Sun’s output = 8.3 x 1026 W
44
Are heat emitter also good absorbers?
Black and dull on the surface Best emitter/absorber Charcoal Blackbody radiators perfect absorber & emitter White and polished/shiny Good Reflectors Stay cool in the summer
45
Figure 16-12 The Thermos Bottle
Discuss the operation of a thermos making reference to methods of heat exchange.
46
Assignment Questions from Packet. 1, 2, 3, 5, 7, 10, 11, 12, 14, 18, 19.
47
The “colour” of heat Peak wavelength of light emitted depends on temperature Spectrum includes all wavelength longer than the peak but not many above 20°C - peak in infrared (need thermal imaging camera to see body heat) 800°C - peak in red (electric coil, fire glows reds) 3000° - peak in blue (but includes green and red light hence appears white) 2.7K peak in micro-wave (background emission in the universe left over from the Big Bang)
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.