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New trends in physics teaching, v.4; The ... - unesdoc - Unesco

New trends in physics teaching, v.4; The ... - unesdoc - Unesco

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<strong>New</strong> Trends <strong>in</strong> Physics Teach<strong>in</strong>g IV<br />

We, the teachers of <strong>physics</strong>, must help our students to understand - we must put them <strong>in</strong>to a<br />

position <strong>in</strong> which they can <strong>in</strong>terpret what they read or what they are told about energy <strong>in</strong> the<br />

press, by the oil companies, by the trade unions (to see coal m<strong>in</strong>ers lead<strong>in</strong>g an anti-nuclear lobby<br />

is surely worthy of sceptical comment) and all the other pressure groups.<br />

As teachers, we must have access to reliable <strong>in</strong>formation about energy <strong>in</strong> the global context,<br />

and about the effect of that knowledge on the approaches we might adopt <strong>in</strong> our teach<strong>in</strong>g. That<br />

is the purpose of this first half of the part on Energy. However, the part is largely concerned with<br />

the impersonal and a few comments on the energy needs of human be<strong>in</strong>gs might be welcome.<br />

<strong>The</strong> energy unit which is most familiar to the men and women <strong>in</strong> the street is the kilowatt-hour<br />

of the electricity bill. Although it is, of course, 3600 kilojoules, its very familiarity makes it an<br />

attractive unit when one wishes to relate energy to a human context.<br />

An average requirement of energy for a human be<strong>in</strong>g is around 10 000 kJ per day. That is just<br />

under 3 kWh. And the rate of supply is just over 0.1 kW.<br />

If I switch a 100 W electric lamp on for 24 hours, that lamp converts energy at a rate of 0.1<br />

kW; and, <strong>in</strong> 24 hours, wil use 8640 kJ or 2.4 kWh.<br />

So you and I live by convert<strong>in</strong>g energy at about the same rate that a 100 W lamp converts<br />

energy.<br />

We derive this energy for liv<strong>in</strong>g from our food. Any biology text will supply details of the<br />

energy which is available to us from various foodstuffs. However, those textbooks usually omit<br />

to po<strong>in</strong>t out that the foods themselves require energy for their production and that this too has<br />

to be paid for. Consider a loaf of bread - a staple item <strong>in</strong> so many lands. Accord<strong>in</strong>g to P. Chapman<br />

[ 11 a typical loaf of about 1.4 kg provides its consumer with about 14 000 kJ or nearly 4 kWh.<br />

To make that loaf from the wheat (allow<strong>in</strong>g for the farmer’s, the miller’s, the baker’s and the<br />

shopkeeper’s usage of energy) requires 20000 kJ (5.5 kWh).<br />

<strong>The</strong> field of wheat from which the bread was derived may be thought of as a solar farm consum<strong>in</strong>g<br />

solar energy and stor<strong>in</strong>g it up <strong>in</strong> the gra<strong>in</strong>. We human be<strong>in</strong>gs then extract about 3.5 kWh<br />

(12 500 kJ) from each kilogram of the harvested crop. If we were to burn the crop we should<br />

get three times as much. But not <strong>in</strong> so useful a form. <strong>The</strong> energy would have been degraded.<br />

<strong>The</strong> energy we extract from the loaf of bread has, through the process of photosynthesis,<br />

been derived from solar radiation. Measurements from space craft confirm that the Earth receives<br />

energy from the Sun at a rate of about 1.4 kW per square metre. Tak<strong>in</strong>g the Earth’s diametric<br />

plane as of area 1.23 X lOI4 m2, the total <strong>in</strong>put of energy to the Earth is 17.2 X 1OI6 W. S<strong>in</strong>ce,<br />

over a long period of years the mean temperature of the Earth has rema<strong>in</strong>ed very close to its<br />

present value (280 K), we must conclude that just as much energy is radiated back <strong>in</strong>to space as<br />

is received. Figure 1 gives details of the <strong>in</strong>terven<strong>in</strong>g energy flows.<br />

Of course, Stefan’s Law describes the process of radiat<strong>in</strong>g the energy back <strong>in</strong>to space.<br />

and<br />

Divid<strong>in</strong>g Eq. 2 by Eq. 1<br />

E = kT4 Eq. 1<br />

AE = k4T3AT Eq. 2<br />

AA E = 4r AT<br />

or Eq. 3<br />

4

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