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Solution to puzzle 4: Equatorial belt

In the diagram below, the belt meets the Earth at a tangent, and therefore the angle between the belt and a radius is 90°.  Consider two lines: one joining the center of the Earth to the high point of the rope; the other joining the center of the Earth to one of the points at which the belt meets the Earth.  Let x be the angle subtended, in radians, between the two lines.  Let a be the distance from the high point of the rope to a point at which the belt meets the Earth.

The Earth, radius r, with equatorial belt, rising to height h above the surface. The belt is shown meeting the Earth, at a tangent.

The length of the belt not in contact with the Earth is 2a.  The corresponding circular arc length is r · 2x.

Let d be the extra length added to the belt: 1 meter in our example.
Then 2a = 2rx + d.
Hence a = rx + d/2, and so a/r = x + d/2r.

We also have, tan x = a/r.
Therefore tan x = x + d/2r.

Given numerical values for d and r, this equation can be solved for x to any required degree of accuracy using the Newton-Raphson Method (or Newton's Method), enabling us to calculate h.  Instead, we will pursue an approximate solution for small values of d = extra belt length.

Assume d/2r is very small, as it is for d = 1, r = 6,400,000.
Then tan x is approximately equal to x, and so x is small.

The Maclaurin series for tan x is: x + x3/3 + ...

Hence x + x3/3 is approximately equal to x + d/2r, and so x3 is approximately equal to 3d/2r.

We also have h = r(sec x − 1).

At this point, we could substitute values for d and r, and calculate x3, and thereby h.  However, we will continue with an approximate solution, to determine the general expression for h in terms of r and small d.

The Maclaurin series for sec x is: 1 + x2/2 + ...
(The cube root of 3d/2r is of the order of 0.01 when d = 1, so this approximation is still acceptable.)
Therefore h is approximately equal to rx2/2.
And so h is approximately equal to (r/2) · (3d/2r)2/3.

Simplifying, h is approximately equal to k · r1/3 · d2/3, where k = (3/2)2/3/2 is approximately equal to 0.65518535.
Since the Earth's radius is a constant, we see that h is proportional to d2/3.

For d = 1, r = 6,400,000, we obtain h is approximately equal to 121.6 meters.


Remarks

Applying the Newton-Raphson Method to f(x) = tan x − x − d/2r = 0, yields the solution x = 0.0061654989, from which h = 121.64473 m, both correct to 8 significant figures.

The above approximate solution, h is approximately equal to (3/2)2/3/2 · 6,400,0001/3 · d2/3, is accurate to within 0.1% for extra belt lengths of up to about 2.3 km.  The table below gives further illustrations, correct to 8 significant figures.

Approximate and exact solutions
Extra belt length (m)Approximate height (m)Exact height (m)Percentage difference
0.0011.21644041.2164405−0.0000056628017
0.015.64621625.6462177−0.000026460023
0.126.20741426.207446−0.00012284293
1121.64404121.64473−0.00057020334
2193.09788193.09962−0.00090513744
5355.68933355.69526−0.0016672651
10564.62162564.63656−0.0026465916
20896.28095896.31860−0.004201135
501650.96361651.0914−0.0077382741
1002620.74142621.0633−0.012283168
2004160.16764160.9789−0.019496863
5007663.09437665.8469−0.035907446
100012164.40412171.340−0.056987112
200019309.78819327.265−0.090430158
500035568.93335628.234−0.16644292
1000056462.16256611.585−0.26394511
2000089628.09590004.599−0.41831634
50000165096.36166373.69−0.76774618
100000262074.14265292.26−1.2130464
200000416016.76424123.55−1.9114198
500000766309.43793794.84−3.4625335
10000001216440.41285617.5−5.3808434
20000001930978.82104894.1−8.2624275
50000003556893.34142952.5−14.145932
64000004193186.25005072.4−16.221268
100000005646216.27106259.6−20.545878

Further reading

  1. Newton's Method Applet

Source: Pete Barnes

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