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103 Trigonometry Problems

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54 <strong>103</strong> <strong>Trigonometry</strong> <strong>Problems</strong><br />

(a) How far from the equatorial plane is Exeter, assuming that one travels through<br />

Earth’s interior? What if one travels on Earth’s surface?<br />

(b) How far does Earth’s rotation carry the citizens of Exeter during a single day?<br />

Solution: Let N be the foot of the perpendicular line segment from E to the equatorial<br />

plane. Then ̸ EON = 43 ◦ . In right triangle EON, |EN| =|EO| sin 43 ◦ =<br />

3960 sin 43 ◦ ≈ 2700.714; that is, the z coordinate of Exeter is about 2700.714<br />

miles. If one travels on Earth’s surface, we extend segment ON through N to meet<br />

the equator at M. Then |ÊM| = ̸ EON<br />

360 ◦ · 2π · 3960 ≈ 2971.947; that is, exeter is<br />

about 2971.947 miles away from the equator, assuming that one travels on Earth’s<br />

surface.<br />

z<br />

C<br />

E<br />

O<br />

N<br />

M<br />

y<br />

x<br />

Figure 1.53.<br />

Let C denote the latitudinal circle of 43 ◦ , and let C be the center of C. During a<br />

single day (and night; that is, a complete day of 24 hours), Earth’s rotation carries<br />

the citizens of Exeter through one revolution along the circle C. (If we fix Earth,<br />

then E travels along C for a complete revolution.) Hence, the distance sought is<br />

2π ·|CE| =2π ·|ON| =7920π cos 43 ◦ ≈ 18197.114 miles. (What a long free<br />

ride!)<br />

It is not difficult to see that points E and N have the same x and y coordinates,<br />

and that N lies on a circle centered at O with radius 3960 cos 43 ◦ . Now we set up<br />

the x and y axes. The primary meridian is the great semicircle that passes through<br />

Greenwich, England, on its way from the North Pole to the South Pole. The x axis is<br />

set in such a way that the intersection of the primary meridian and the equator is at<br />

(3960, 0, 0). This point is in the South Atlantic Ocean, near the coast of Ghana. The<br />

y axis is set such that the positive x, y, and z axes follow the right-hand rule. When<br />

we turn the primary meridian around the z axis, we obtain all the semicircles with the<br />

segment connecting the North Pole and the South Pole as their common diameter.

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