Temperature and Kinetic Theory

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Presentation transcript:

Temperature and Kinetic Theory Chapter 13

Thermal Physics Thermal physics is the study of Temperature Heat How these affect matter

Thermal Physics, cont Concerned with the concepts of energy transfers between a system and its environment Concerns itself with the physical and chemical transformations of matter in all of its forms: solid, liquid, and gas

Heat The process by which energy is exchanged between objects because of temperature differences is called heat Objects are in thermal contact if energy can be exchanged between them Thermal equilibrium exists when two objects in thermal contact with each other cease to exchange energy

Zeroth Law of Thermodynamics If objects A and B are separately in thermal equilibrium with a third object, C, then A and B are in thermal equilibrium with each other. Allows a definition of temperature

Temperature from the Zeroth Law Two objects in thermal equilibrium with each other are at the same temperature Temperature is the property that determines whether or not an object is in thermal equilibrium with other objects

Thermometers Used to measure the temperature of an object or a system Make use of physical properties that change with temperature Many physical properties can be used volume of a liquid length of a solid pressure of a gas held at constant volume volume of a gas held at constant pressure electric resistance of a conductor color of a very hot object

Thermometers, cont A mercury thermometer is an example of a common thermometer The level of the mercury rises due to thermal expansion Temperature can be defined by the height of the mercury column

Temperature Scales Thermometers can be calibrated by placing them in thermal contact with an environment that remains at constant temperature Environment could be mixture of ice and water in thermal equilibrium Also commonly used is water and steam in thermal equilibrium

Celsius Scale Temperature of an ice-water mixture is defined as 0º C This is the freezing point of water Temperature of a water-steam mixture is defined as 100º C This is the boiling point of water Distance between these points is divided into 100 segments or degrees

Pressure-Temperature Graph All gases extrapolate to the same temperature at zero pressure This temperature is absolute zero

Kelvin Scale When the pressure of a gas goes to zero, its temperature is –273.15º C This temperature is called absolute zero This is the zero point of the Kelvin scale –273.15º C = 0 K To convert: TC = TK – 273.15 The size of the degree in the Kelvin scale is the same as the size of a Celsius degree

Modern Definition of Kelvin Scale Defined in terms of two points Agreed upon by International Committee on Weights and Measures in 1954 First point is absolute zero Second point is the triple point of water Triple point is the single point where water can exist as solid, liquid, and gas Single temperature and pressure Occurs at 0.01º C and P = 4.58 mm Hg

Modern Definition of Kelvin Scale, cont The temperature of the triple point on the Kelvin scale is 273.16 K Therefore, the current definition of of the Kelvin is defined as 1/273.16 of the temperature of the triple point of water

Some Kelvin Temperatures Some representative Kelvin temperatures

Fahrenheit Scales Most common scale used in the US Temperature of the freezing point is 32º Temperature of the boiling point is 212º 180 divisions between the points

Comparing Temperature Scales

Converting Among Temperature Scales

Thermometers and Temperature Scales Example: (a) “Room temperature” is often taken to be 68°F. What is this on the Celsius scale? (b) The temperature of the filament in a lightbulb is about 1800°C. What is this on the Fahrenheit scale?

Thermal Expansion The thermal expansion of an object is a consequence of the change in the average separation between its constituent atoms or molecules At ordinary temperatures, molecules vibrate with a small amplitude As temperature increases, the amplitude increases This causes the overall object as a whole to expand

Linear Expansion For small changes in temperature , the coefficient of linear expansion, depends on the material See table These are average coefficients, they can vary somewhat with temperature

Applications of Thermal Expansion – Bimetallic Strip Thermostats Use a bimetallic strip Two metals expand differently Since they have different coefficients of expansion

Area Expansion Two dimensions expand according to g is the coefficient of area expansion

Volume Expansion Three dimensions expand For liquids, the coefficient of volume expansion is given in the table

More Applications of Thermal Expansion Pyrex Glass Thermal stresses are smaller than for ordinary glass Sea levels Warming the oceans will increase the volume of the oceans

Unusual Behavior of Water As the temperature of water increases from 0ºC to 4 ºC, it contracts and its density increases Above 4 ºC, water exhibits the expected expansion with increasing temperature Maximum density of water is 1000 kg/m3 at 4 ºC

Thermal Expansion Example: It is observed that 55.50 mL of water at 20°C completely fills a container to the brim. When the container and the water are heated to 60°C, 0.35 g of water is lost. What is the coefficient of volume expansion of the container?

Ideal Gas A gas does not have a fixed volume or pressure In a container, the gas expands to fill the container Most gases at room temperature and pressure behave approximately as an ideal gas

Assumptions of an Ideal Gas # of molecules is large, and separation between them is large Random Movement Newton’s Laws Exert no long-range force on one another Elastic Collisions Walls Identical

The Gas Laws and Absolute Temperature The relationship between the volume, pressure, temperature, and mass of a gas is called an equation of state. We will deal here with gases that are not too dense. Boyle’s Law: the volume of a given amount of gas is inversely proportional to the pressure as long as the temperature is constant.

The Gas Laws and Absolute Temperature The volume is linearly proportional to the temperature, as long as the temperature is somewhat above the condensation point and the pressure is constant: Extrapolating, the volume becomes zero at −273.15°C; this temperature is called absolute zero.

The Gas Laws and Absolute Temperature Finally, when the volume is constant, the pressure is directly proportional to the temperature:

The Ideal Gas Law We can combine the three relations just derived into a single relation: What about the amount of gas present? If the temperature and pressure are constant, the volume is proportional to the amount of gas:

Moles It’s convenient to express the amount of gas in a given volume in terms of the number of moles, n One mole is the amount of the substance that contains as many particles as there are atoms in 12 g of carbon-12 1 mol H2 has a mass of 2 g 1 mol Ne has a mass of 20 g 1 mol CO2 has a mass of 44 g

Ideal Gas Law Equation

Ideal Gas Law PV = n R T R is the Universal Gas Constant R = 8.31 J / mole.K R = 0.0821 L. atm / mole.K Is the equation of state for an ideal gas

Ideal Gas Law, Alternative Version P V = N kB T kB is Boltzmann’s Constant kB = R / NA = 1.38 x 10-23 J/ K N is the total number of molecules n = N / NA n is the number of moles N is the number of molecules

Avogadro’s Number The number of particles in a mole is called Avogadro’s Number NA=6.02 x 1023 particles / mole Defined so that 12 g of carbon contains NA atoms

Avogadro’s Number and Masses The mass in grams of one Avogadro's number of an element is numerically the same as the mass of one atom of the element, expressed in atomic mass units, u Carbon has a mass of 12 u 12 g of carbon consists of NA atoms of carbon Holds for molecules, also

Ideal gas Example: 5 kg of CO2 occupy a volume of 500L at a pressure of 2 atm. What is the temperature? If the volume is increased to 750L and the temperature is kept constant, what is the new pressure?

Kinetic Theory of Gases – Assumptions The number of molecules in the gas is large and the average separation between them is large compared to their dimensions The molecules obey Newton’s laws of motion, but as a whole they move randomly

Kinetic Theory of Gases – Assumptions, cont. The molecules interact only by short-range forces during elastic collisions The molecules make elastic collisions with the walls The gas under consideration is a pure substance, all the molecules are identical

Kinetic Theory and the Molecular Interpretation of Temperature The force exerted on the wall by the collision of one molecule is Then the force due to all molecules colliding with that wall is

Kinetic Theory and the Molecular Interpretation of Temperature The averages of the squares of the speeds in all three directions are equal: So the pressure is: (13-6)

Kinetic Theory and the Molecular Interpretation of Temperature Rewriting, (13-7) so (13-8) The average translational kinetic energy of the molecules in an ideal gas is directly proportional to the temperature of the gas.

Announcements Homework #12 (no late HW) Chapter 12: 4, 13, 49 Chapter 13: 1, 4, 10, 33 Due: today Homework #13 (Extra Credit – no late HW) Chapter 14: 2, 9, 12, 24 Chapter 15: 2, 10 Due: 5/11 (library drop box – before 4pm) Final May 14 6:00 – 7:50 1- 8.5x11 or 4 – 3x5 Ch 1-15 (limited)

Kinetic Theory and the Molecular Interpretation of Temperature We can invert this to find the average speed of molecules in a gas as a function of temperature: (13-9)

Speed of the Molecules Expressed as the root-mean-square (rms) speed At a given temperature, lighter molecules move faster, on average, than heavier ones Lighter molecules can more easily reach escape speed from the earth

Some rms Speeds

Maxwell Distribution A system of gas at a given temperature will exhibit a variety of speeds Three speeds are of interest: Most probable Average rms

Maxwell Distribution, cont For every gas, vmp < vav < vrms As the temperature rises, these three speeds shift to the right The total area under the curve on the graph equals the total number of molecules

Kinetic Theory of Molecules Example Calculate the rms speed of helium atoms near the surface of the Sun at a temperature of about 6000 K.