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Chapter 2 Review of Forces and Moments - Brown University

Chapter 2 Review of Forces and Moments - Brown University

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TABLE OF POSITIONS OF CENTER OF MASS FOR COMMON OBJECTS<br />

Rectangular prism Circular cylinder Half-cylinder<br />

Solid hemisphere Thin hemispherical shell Cone<br />

Triangular Prism<br />

Thin triangular laminate<br />

Some subtleties about gravitational interactions<br />

There are some situations where the simple equations in the preceding section don’t work. Surveyors<br />

know perfectly well that the earth is no-where near spherical; its density is also not uniform. The earth’s<br />

gravitational field can be quite severely distorted near large mountains, for example. So using the simple<br />

gravitational formulas in surveying applications (e.g. to find the `vertical’ direction) can lead to large<br />

errors.<br />

Also, the center <strong>of</strong> gravity <strong>of</strong> an object is not the same as its center <strong>of</strong> mass. Gravity is actually a<br />

distributed force. When two nearby objects exert a gravitational force on each other, every point in one<br />

body is attracted towards every point inside its neighbor. The distributed force can be replaced by a<br />

single, statically equivalent force, but the point where the equivalent force acts depends on the relative<br />

positions <strong>of</strong> the two objects, <strong>and</strong> is not generally a fixed point in either solid. One consequence <strong>of</strong> this<br />

behavior is that gravity can cause rotational accelerations, as well as linear accelerations. For example,<br />

the resultant force <strong>of</strong> gravity exerted on the earth by the sun <strong>and</strong> moon does not act at the center <strong>of</strong> mass<br />

<strong>of</strong> the earth. As a result, the earth precesses – that is to say, its axis <strong>of</strong> rotation changes with time.

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