PHYS 1220, Engineering Physics, Chapter 17 Temperature and Heat Instructor: TeYu Chien Department of Physics and Astronomy University of Wyoming

Similar documents
Chapter 18 Temperature, Heat, and the First Law of Thermodynamics. Thermodynamics and Statistical Physics

Chapters 16 Temperature and Heat

Chapter 18. Temperature, Heat, and the First Law of Thermodynamics Temperature

Chapter 16 Temperature and Heat

Chapter 16. Copyright 2010 Pearson Education, Inc.

18.13 Review & Summary

Thermodynamics. Thermodynamics is the study of the collective properties of a system containing many bodies (typically of order 10 23!

Lecture Outlines Chapter 16. Physics, 3 rd Edition James S. Walker

Chapter 16 Temperature and Heat

Chapter 14 Temperature and Heat

Chapter 2 Heat, Temperature and the First Law of Thermodynamics

Figure 1.1. Relation between Celsius and Fahrenheit scales. From Figure 1.1. (1.1)

Calorimetry: Problem Solving with Heat Exchanges (method 1)

Chapter 1 - Temperature and Heat

Physics 2: Fluid Mechanics and Thermodynamics

Physics 201. Professor P. Q. Hung. 311B, Physics Building. Physics 201 p. 1/3

Lecture 22. Temperature and Heat

Lecture 2: Zero law of thermodynamics

Chapter 17 Temperature and heat

Physics 2: Fluid Mechanics and Thermodynamics

Handout 10: Heat and heat transfer. Heat capacity

General Physics (PHY 2130)

Thermal Radiation Heat Transfer Mechanisms

Chapter 14 Temperature and Heat

Chapter 10 Temperature and Heat

For more info visit

Chapter 11. Energy in Thermal Processes

First Law of Thermodynamics Second Law of Thermodynamics Mechanical Equivalent of Heat Zeroth Law of Thermodynamics Thermal Expansion of Solids

Kinetic Theory continued

Chapters 17 &19 Temperature, Thermal Expansion and The Ideal Gas Law

Physics 100 Lecture 5. Laws of Thermodynamics February 5, 2018

Kinetic Theory continued

A). Yes. B). No. Q15 Is it possible for a solid metal ball to float in mercury?

Chapter 12. Temperature and Heat. continued

Honors Physics. Notes Nov 16, 20 Heat. Persans 1

Temperature and Its Measurement

Chapter 17. Temperature. Dr. Armen Kocharian

PHYSICS 149: Lecture 26

Chapter 11. Important to distinguish between them. They are not interchangeable. They mean very different things when used in physics Internal Energy

(Heat capacity c is also called specific heat) this means that the heat capacity number c for water is 1 calorie/gram-k.

Chapter 13 Temperature, Heat Transfer, and the First Law of Thermodynamics

Bernoulli s Principle. Application: Lift. Bernoulli s Principle. Main Points 3/13/15. Demo: Blowing on a sheet of paper

Chapter 10. Thermal Physics

Chapter 17. Work, Heat, and the First Law of Thermodynamics Topics: Chapter Goal: Conservation of Energy Work in Ideal-Gas Processes

Introduction to Thermodynamics

Preview. Heat Section 1. Section 1 Temperature and Thermal Equilibrium. Section 2 Defining Heat. Section 3 Changes in Temperature and Phase

Thermal contact. Heat absorbed and released. Temperature and Heat. Review of lecture 1. Can β be negative?

Chapter 11. Energy in Thermal Processes

Physics 53. Thermal Physics 1. Statistics are like a bikini. What they reveal is suggestive; what they conceal is vital.

Recap. There are 3 different temperature scales: Celsius, Kelvin, and Fahrenheit

Chapter 14 Heat. Lecture PowerPoints. Chapter 14 Physics: Principles with Applications, 7 th edition Giancoli

Physics 111. Lecture 35 (Walker: ) Thermal Physics I: Temperature Thermal Expansion. April 29, Temperature (T)

Phy 212: General Physics II

Rate in Thermal Systems

Page 1 SPH3U. Heat. What is Heat? Thermal Physics. Waterloo Collegiate Institute. Some Definitions. Still More Heat

Zeroth Law of Thermodynamics

Thermal Equilibrium. Zeroth Law of Thermodynamics 2/4/2019. Temperature

Chapter 9. Preview. Objectives Defining Temperature. Thermal Equilibrium. Thermal Expansion Measuring Temperature. Section 1 Temperature and

Core Concepts. PowerPoint Lectures to accompany Physical Science, 8e. Chapter 4 Heat and Temperature. New Symbols for this Chapter 2/14/2011

0 o K is called absolute zero. Water Freezes: 273 o K Water Boils: 373 o K

TEMPERATURE. 8. Temperature and Heat 1

Zeroth Law of Thermodynamics

Thermodynamics 2013/2014, lecturer: Martin Zápotocký

Energy, Temperature, & Heat. Energy, Temperature, & Heat. Temperature Scales 1/17/11

PROGRAM OF PHYSICS. Lecturer: Dr. DO Xuan Hoi Room A

The Kinetic Theory of Matter. Temperature. Temperature. Temperature. Temperature. Chapter 6 HEAT

Physics 111. Lecture 42 (Walker: 18.9) Entropy & Disorder Final Review. May 15, 2009

S15--AP Phys Q4--Heat-Thermo Ch13_14_15 PRACTICE

Lecture PowerPoints. Chapter 14 Physics: Principles with Applications, 6 th edition Giancoli

General Physics I. Lecture 23: Basic Concepts of Thermodynamics

7. (2) Of these elements, which has the greatest number of atoms in a mole? a. hydrogen (H) b. oxygen (O) c. iron (Fe) d. gold (Au) e. all tie.

Applied Natural Sciences

Physics 1501 Lecture 35

Temperature and Thermometers. Temperature is a measure of how hot or cold something is. Most materials expand when heated.

Lecture 3: Light and Temperature

Effect of Temperature on Materials. June 20, Kamran M. Nemati. Phase Diagram

1. How much heat was needed to raise the bullet to its final temperature?

10 TEMPERATURE, THERMAL EXPANSION, IDEAL GAS LAW, AND KINETIC THEORY OF GASES.

Fluids Bernoulli s equation

Lecture PowerPoints. Chapter 13 Physics: Principles with Applications, 7 th edition Giancoli

Atomic Theory, Temperature and Thermal Expansion

Physics 408 Final Exam

Chapter 14 Heat and Temperature Notes

Chapter 7 Notes. Matter is made of tiny particles in constant motion

Chapter 12. Temperature and Heat

High temperature He is hot

Mechanisms of heat transfer

Section 2. Energy Fundamentals

Heat What is heat? Work = 2. PdV 1

Heat Transfer. Phys101 Lectures 33, 34. Key points: Heat as Energy Transfer Specific Heat Heat Transfer: Conduction, Convection, Radiation.

Thermodynamics System Surrounding Boundary State, Property Process Quasi Actual Equilibrium English

Ch. 7: Thermochemistry

- Apply closed system energy balances, observe sign convention for work and heat transfer.

Chapter 4: Heat Capacity and Heat Transfer

Topic 5: Energetics. Heat & Calorimetry. Thursday, March 22, 2012

Thermodynamics 2018/2019, lecturer: Martin Zápotocký

Temperature and Heat. Two systems of temperature. Temperature conversions. PHY heat - J. Hedberg

Chapter 10: Thermal Physics

Temperature. Temperature Scales. Temperature (cont d) CHAPTER 14 Heat and Temperature

Hence. The second law describes the direction of energy transfer in spontaneous processes

Transcription:

PHYS 1220, Engineering Physics, Chapter 17 Temperature and Heat Instructor: TeYu Chien Department of Physics and Astronomy University of Wyoming Goal of this chapter is to learn the nature of Temperature and Heat. - What is Temperature and what is heat? Temperature is a quantitative measurement of hotness/coldness; while Heat is a form of energy that could alter the value of temperature. Thermal equilibrium is a state that two objects reach the same temperature by exchanging heat. Zeroth law of thermodynamics: If two separated systems/objects are each in thermal equilibrium with a third system/object simultaneously. All three systems/objects are in thermal equilibrium with each other, and thus all three have same temperature. Note: Zeroth law of thermodynamics is the basis why thermometer works. Thermometer is, in fact, measuring its own temperature (will discussed later). With Zeroth law, we know that the measured temperature is also the temperature of the object that has thermal equilibrium with the thermometer.

- How temperature is measured? Use anything that has significant reactions/changes upon change of temperature. - Typical temperature scales Fahrenheit, Celsius, and Kelvin T F = 9 5 T C +32 (or T C = 5 9 (T F 32) ) T K =T C +273.15 In constant volume gas thermometer: T 2 T 1 = p 2 p 1 the unit of Kelvin. (Will discuss more in Chapter 18), where T 1, and T 2 are in

- How to describe thermal expansion of solid materials? Δ L=α L 0 ΔT (Linear thermal expansion) (similar equation as temperature-dependent resistance or resistivity in metal: R(T )=R 0 [1+α(T T 0 )] ) ΔV =βv 0 ΔT (Volume thermal expansion) Note: β=3 α Note #2: Volume of materials as function of temperature typically is not a linear function (does not change proportionally). These equations above are approximation in small temperature range.

- What is heat? How it is related to temperature? How to calculate? Unit: 1 cal=4.186 J ; 1 kcal=1000 cal=4186 J ; 1 Btu=252 cal=1055 J Specific heat: c= 1 dq (amount of energy needed to increase a unit m dt J temperature of the material with a unit mass) ( kg K, cal Btu, ) g C o lb F o Specific heat is a material-dependent quantity. Q=mc ΔT Q=nMc ΔT =nc ΔT (n: number of moles; M: molar mass; C: molar heat capacity) Note: molar heat capacity, C, is another form of specific heat with different unit. (amount of energy needed to increase a unit temperature of the material with mole of molecules)

- Phase changes We know when boiling water, the water could reach a maximum temperature ~ 100 C o and start boiling. Even if you keep heating, the temperature is not changing. If the temperature does not increase, where does the heat go to? The energy goes to help materials change phase phase change. liquid vapor ; or solid liquid are two phase changes for H 2 O at 1 atm. Q=mL (L: latent heat) L liq vap =2.256 10 6 J /kg=539cal / g=970 Btu/lb L sol liq =3.34 10 5 J /kg=79.6cal / g=143 Btu/lb - How heat transfer? Three major mechanisms: (1) Conduction; (2) Convection; and (3) Radiation

- Conduction: Conduction is based on the heat flow in material (very similar to electron conductivity in current) H = dq dt =ka T T H L L ( I = V R =V V H L = 1 ρ L ρ A V V H L L A k in the above equation is called thermal conductivity - Convection: Convection is based on the flow of fluid that carries heat away with it. - Radiation: Radiation is based on electromagnetic waves that carry energy in or out of the system. Thus, this method requires NO contacts with other object NOR fluid (such as air). H = Ae σ T 4 (Stefan-Boltzmann law) (A: area of the surface of the object) e: emissivity (describing how easy the radiation could be emitted out of the object. It is ranging from 0 to 1, with 1 as easiest and 0 as hardest) σ=5.670400 10 8 W /m 2 K 4 (Stefan-Boltzmann constant) Note: the object could emit radiation, and also absorb radiation. For absorption, use same equation (Stefan-Boltzmann law), but change temperature to surrounding environment temperature, T s. ) Math Preview for Chapter 18: rms (root-mean-square) Integrations with a Gaussian function Questions to think about for Chapter 18: What does it mean as temperature and heat for atoms or molecules in gas or solid materials?