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Physics for Geologists, Second edition

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10 Basic concepts<br />

relating them by equating the exponents. It must be emphasized, though,<br />

that if we omit any components, we may finish with the wrong answer. An<br />

example will make this clear.<br />

If we did not know the equation on page 1 relating depth to pressure, p,<br />

in a static homogeneous liquid, we might assume that it is a function of mass<br />

density, p, the acceleration due to gravity, g, and the volume, v, and write<br />

p = f (p, g, v)<br />

This can be written in dimensional <strong>for</strong>m<br />

from which we write the indicial equations<br />

<strong>for</strong>M: 1 = a<br />

<strong>for</strong>L: -I=-3a+b+3c<br />

<strong>for</strong> T : - 2 = -2b.<br />

(say, pressure is a function of p, g and v).<br />

The solution of these simultaneous equations is a = 1, b = 1, and substitu-<br />

tion of these into the indicial equation <strong>for</strong> L gives c = 4. This tells us that it<br />

is not volume but length that is involved, and that that length is clearly the<br />

depth at which p is required:<br />

and the function is<br />

where B is a dimensionless constant. A few measurements would establish<br />

that the dimensionless constant<br />

<strong>for</strong> a liquid of constant density.<br />

Take another example, the results of which we will use later. The tension in<br />

a string as we twirl a stone around in a horizontal orbit, or the gravitational<br />

<strong>for</strong>ce that keeps a satellite in orbit, is called the centripetal <strong>for</strong>ce. What is<br />

the equation <strong>for</strong> the centripetal <strong>for</strong>ce required to keep an artificial satellite<br />

in a circular orbit? This <strong>for</strong>ce is clearly a function of the mass of the object,<br />

Copyright 2002 by Richard E. Chapman

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