Home-immediately access 800+ free online publications. Download CD3WD (680 Megabytes) and distribute it to the 3rd World. CD3WD is a 3rd World Development private-sector initiative, mastered by Software Developer Alex Weir and hosted by GNUveau_Networks (From globally distributed organizations, to supercomputers, to a small home server, if it's Linux, we know it.)

Creating Learning Networks for African Teachers

UNESCO PROJECT (Contract No. 408.302.9)

Home | Computer Literacy | Common Applications | Pedagogy & Internet | Infrastructure Guide

Background

COMMON APPLICATIONS

Spreadsheets
Tutorial
Introduction
Worksheets
Columns & Rows
Charts

Examples
Refraction of Light
Solving Polynomial Equations
Workers' Database
Base Converter

Activities

Links

Databases
Tutorial

Introduction

Example
Periodic Table

Links

Word Processing
Tutorial

Introduction
Text
Page Properties
Printing
Quit

Examples
Address list
Time table
Newsletter
Repeat Patterns
Logos

Practical Questions

HTML Editors
Tutorial
Basic html
Netscape
Composer


Examples
Teaching Syllabus
Teachers' Notes
Subject Website Lists
Students Website

Art
Principles of Art
Elements of Art
Coloured Pencil Paintings
Pastel Paintings
Book cover
Posters


Scanning an image


        KINETIC THEORY (CON'T)
Assessment objectives

By the  end of this topic, the student should be able to:

      • Explain what is meant by kinetic theory of gases.
      • Explain quantitatively why a gas exerts pressure on the walls

      • of its container.
      • Derive the expression P = 1  r <c2> stating any assumptions made.
        •                               3
      • Relate the mean kinetic energy of a gas to its absolute temperature.
      • Use the formula  P = 1r <c2> to deduce Avogadro's Hypothesis,

      •                                 3
        Boyle's law, Charles's law, Dalton's law of partial pressures and Graham's
        law of diffusion.
      • Distinguish between a real and an ideal gas.
      • Account for the difference between equations PV = RT and

      • ( P + )(V - b) = RT
                 v2
      • Define critical temperature Tc of a gas.
      • Draw  labelled P-V diagrams to show the behaviour of a real gas under

      • compression for temperatures above and below the critical temperature.
      • Distinguish between a gas and a vapour.
      • Distinguish between saturated an unsaturated vapour and define saturated

      • vapour pressure.(s.v.p)
      • Explain the occurrence of saturated vapour pressure using molecular theory.
      • Use kinetic theory to explain the effect of volume and temperature change

      • on s.v.p.
      • Distinguish the behaviour of saturated vapours from that of unsaturated ones.
      • Use Dalton's law of partial pressures to solve problems on s.v.p
      • Relate variation of s.v.p to boiling point.
      • Describe an experiment to measure the variation of s.v.p of water with

      • temperature.

7.6 Thermodynamics                   (12 Periods)

    Work done by an expanding gas
    Internal Energy
    First law of thermodynamics DQ = DU + DW
    Principle specific heat capacities, the relation Cp-Cv = R
    Isothermal and adiabatic changes of a gas inlcuding work done
        by a gas on such a process.
Assessment objectives

By the  end of this topic, the student should be able to:

      • State the component of the internal energy of a real gas and the factors

      • on which they depend.
      • Define an ideal gas and show that the internal energy of an ideal gas has no

      • potential energy component.
      • Explain the meanings of terms: isovolumetric, isobaric, isothermal, and

      • adiabatic changes.
      • Derive the expression W = Pdv for the work done when a gas expands and

      • relate it to the area under the P-V curve.
      • State the first law of thermodynamics and apply it to isobaric processes.
      • Explain why a gas has more than one specific heat capacity.
      • Define specific heat capacity of a gas at constant pressure and constant

      • volume.
      • Explain why the molar principle heat capacity at constant pressure Cp

      • is greater than that at at constant volume Cv.
      • Derive the expression Cp-Cv = R
      • Relate g = Cp/Cv to atomicity of a gas.
      • Represent isovolumetric, isobaric, isothermal, and adiabatic processes on

      • a P-V sketch.
      • State the conditions necessary in practice to achieve isothermal and adiabatic

      • processes.
      • State and use the equations relating
      • Derive expressions for the work done in isothermal and adiabatic processes.
      • Solve problems involving isovolumetric, isobaric, isothermal, and adiabatic

      • processes.


  7.7  Transfer of Heat Energy

    Thermal Conduction.
      - Mechanism of thermal conduction in insulators and in metals.
    Thermal conductivity.
    The relation DQ = k A  DT
                             Dt              Dx
    Measurement of thermal conductivity of good and bad conductors of heat.
    Convection as a consequence of change of density.
    Radiation as a form of energy.
      •  Blackbody radiation
      •  Energy distribution in the spectrum of blackbody radiation.
      •  Stefan's law   E = sT4.
      •  Wein's displacement law, lmT = 2.9x10-3 mK.
      •  Surface temperature of the sun.
      •  Survey of the electromagnetic spectrum.
Assessment objectives:

By the  end of this topic, the student should be able to:

      • Explain the mechanism of heat conduction in gases, liquids metallic

      • and non-metallic solids.
      • State the factors which determine the rate of heat transfer through

      • a material.
      • Define thermal conductivity k of a material.
      • Draw a sketch graph to show the variation of temperature with length

      • along a lagged and an unlagged metal bar.
      • Perform and describe an experiment to determine thermal conductivity

      • of a good conductor of  heat like copper and a poor conductor of heat
        like glass.
      • Solve problems involving conduction of heat.
      • Describe and explain the process of convection.
      • State properties of infra-red radiation and describe how it can be detected.
      • Define a blackbody and blackbody radiation.
      • Describe how an approximate blackbody can be realised in practice.
      • Draw sketch graphs to show variation of relative intensity with wavelength

      • and describe their special features.
      • State and use Wein's displacement law and Stefan's law in calculations, including

      • the estimation of the temperature of the sun.
      • State Prevost's theory of heat exchanges and apply it in calculations.
      • Arrange the components of the electromagnetic spectrum in order of

      • decreasing wavelength.
             


Presentation Software | Spreadsheets | Databases | Word Processing | HTML Editors
Computer Literacy | Common Applications | Pedagogy & Internet | Infrastructure Guides | Home