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1 From The Skeptical Inquirer, Fall 1989, Vol. 14, No. 1, Pp. 35-44
2
3 The Relativity of Wrong
4
5 By Isaac Asimov
6
7 I RECEIVED a letter the other day. It was handwritten in crabbed
8 penmanship so that it was very difficult to read. Nevertheless, I
9 tried to make it out just in case it might prove to be important. In
10 the first sentence, the writer told me he was majoring in English
11 literature, but felt he needed to teach me science. (I sighed a bit,
12 for I knew very few English Lit majors who are equipped to teach me
13 science, but I am very aware of the vast state of my ignorance and I
14 am prepared to learn as much as I can from anyone, so I read on.)
15
16 It seemed that in one of my innumerable essays, I had expressed a
17 certain gladness at living in a century in which we finally got the
18 basis of the universe straight.
19
20 I didn't go into detail in the matter, but what I meant was that we
21 now know the basic rules governing the universe, together with the
22 gravitational interrelationships of its gross components, as shown in
23 the theory of relativity worked out between 1905 and 1916. We also
24 know the basic rules governing the subatomic particles and their
25 interrelationships, since these are very neatly described by the
26 quantum theory worked out between 1900 and 1930. What's more, we have
27 found that the galaxies and clusters of galaxies are the basic units
28 of the physical universe, as discovered between 1920 and 1930.
29
30 These are all twentieth-century discoveries, you see.
31
32 The young specialist in English Lit, having quoted me, went on to
33 lecture me severely on the fact that in every century people have
34 thought they understood the universe at last, and in every century
35 they were proved to be wrong. It follows that the one thing we can say
36 about our modern "knowledge" is that it is wrong. The young man then
37 quoted with approval what Socrates had said on learning that the
38 Delphic oracle had proclaimed him the wisest man in Greece. "If I am
39 the wisest man," said Socrates, "it is because I alone know that I
40 know nothing." the implication was that I was very foolish because I
41 was under the impression I knew a great deal.
42
43 My answer to him was, "John, when people thought the earth was flat,
44 they were wrong. When people thought the earth was spherical, they
45 were wrong. But if you think that thinking the earth is spherical is
46 just as wrong as thinking the earth is flat, then your view is wronger
47 than both of them put together."
48
49 The basic trouble, you see, is that people think that "right" and
50 "wrong" are absolute; that everything that isn't perfectly and
51 completely right is totally and equally wrong.
52
53 However, I don't think that's so. It seems to me that right and wrong
54 are fuzzy concepts, and I will devote this essay to an explanation of
55 why I think so.
56
57 When my friend the English literature expert tells me that in every
58 century scientists think they have worked out the universe and are
59 always wrong, what I want to know is how wrong are they? Are they
60 always wrong to the same degree? Let's take an example.
61
62 In the early days of civilization, the general feeling was that the
63 earth was flat. This was not because people were stupid, or because
64 they were intent on believing silly things. They felt it was flat on
65 the basis of sound evidence. It was not just a matter of "That's how
66 it looks," because the earth does not look flat. It looks chaotically
67 bumpy, with hills, valleys, ravines, cliffs, and so on.
68
69 Of course there are plains where, over limited areas, the earth's
70 surface does look fairly flat. One of those plains is in the
71 Tigris-Euphrates area, where the first historical civilization (one
72 with writing) developed, that of the Sumerians.
73
74 Perhaps it was the appearance of the plain that persuaded the clever
75 Sumerians to accept the generalization that the earth was flat; that
76 if you somehow evened out all the elevations and depressions, you
77 would be left with flatness. Contributing to the notion may have been
78 the fact that stretches of water (ponds and lakes) looked pretty flat
79 on quiet days.
80
81 Another way of looking at it is to ask what is the "curvature" of the
82 earth's surface. Over a considerable length, how much does the surface
83 deviate (on the average) from perfect flatness. The flat-earth theory
84 would make it seem that the surface doesn't deviate from flatness at
85 all, that its curvature is 0 to the mile.
86
87 Nowadays, of course, we are taught that the flat-earth theory is
88 wrong; that it is all wrong, terribly wrong, absolutely. But it
89 isn't. The curvature of the earth is nearly 0 per mile, so that
90 although the flat-earth theory is wrong, it happens to be nearly
91 right. That's why the theory lasted so long.
92
93 There were reasons, to be sure, to find the flat-earth theory
94 unsatisfactory and, about 350 B.C., the Greek philosopher Aristotle
95 summarized them. First, certain stars disappeared beyond the Southern
96 Hemisphere as one traveled north, and beyond the Northern Hemisphere
97 as one traveled south. Second, the earth's shadow on the moon during a
98 lunar eclipse was always the arc of a circle. Third, here on the earth
99 itself, ships disappeared beyond the horizon hull-first in whatever
100 direction they were traveling.
101
102 All three observations could not be reasonably explained if the
103 earth's surface were flat, but could be explained by assuming the
104 earth to be a sphere.
105
106 What's more, Aristotle believed that all solid matter tended to move
107 toward a common center, and if solid matter did this, it would end up
108 as a sphere. A given volume of matter is, on the average, closer to a
109 common center if it is a sphere than if it is any other shape
110 whatever.
111
112 About a century after Aristotle, the Greek philosopher Eratosthenes
113 noted that the sun cast a shadow of different lengths at different
114 latitudes (all the shadows would be the same length if the earth's
115 surface were flat). From the difference in shadow length, he
116 calculated the size of the earthly sphere and it turned out to be
117 25,000 miles in circumference.
118
119 The curvature of such a sphere is about 0.000126 per mile, a quantity
120 very close to 0 per mile, as you can see, and one not easily measured
121 by the techniques at the disposal of the ancients. The tiny difference
122 between 0 and 0.000126 accounts for the fact that it took so long to
123 pass from the flat earth to the spherical earth.
124
125 Mind you, even a tiny difference, such as that between 0 and 0.000126,
126 can be extremely important. That difference mounts up. The earth
127 cannot be mapped over large areas with any accuracy at all if the
128 difference isn't taken into account and if the earth isn't considered
129 a sphere rather than a flat surface. Long ocean voyages can't be
130 undertaken with any reasonable way of locating one's own position in
131 the ocean unless the earth is considered spherical rather than flat.
132
133 Furthermore, the flat earth presupposes the possibility of an infinite
134 earth, or of the existence of an "end" to the surface. The spherical
135 earth, however, postulates an earth that is both endless and yet
136 finite, and it is the latter postulate that is consistent with all
137 later findings.
138
139 So, although the flat-earth theory is only slightly wrong and is a
140 credit to its inventors, all things considered, it is wrong enough to
141 be discarded in favor of the spherical-earth theory.
142
143 And yet is the earth a sphere?
144
145 No, it is not a sphere; not in the strict mathematical sense. A sphere
146 has certain mathematical properties - for instance, all diameters
147 (that is, all straight lines that pass from one point on its surface,
148 through the center, to another point on its surface) have the same
149 length.
150
151 That, however, is not true of the earth. Various diameters of the
152 earth differ in length.
153
154 What gave people the notion the earth wasn't a true sphere? To begin
155 with, the sun and the moon have outlines that are perfect circles
156 within the limits of measurement in the early days of the telescope.
157 This is consistent with the supposition that the sun and the moon are
158 perfectly spherical in shape.
159
160 However, when Jupiter and Saturn were observed by the first telescopic
161 observers, it became quickly apparent that the outlines of those
162 planets were not circles, but distinct ellipses. That meant that
163 Jupiter and Saturn were not true spheres.
164
165 Isaac Newton, toward the end of the seventeenth century, showed that a
166 massive body would form a sphere under the pull of gravitational
167 forces (exactly as Aristotle had argued), but only if it were not
168 rotating. If it were rotating, a centrifugal effect would be set up
169 that would lift the body's substance against gravity, and this effect
170 would be greater the closer to the equator you progressed. The effect
171 would also be greater the more rapidly a spherical object rotated, and
172 Jupiter and Saturn rotated very rapidly indeed.
173
174 The earth rotated much more slowly than Jupiter or Saturn so the
175 effect should be smaller, but it should still be there. Actual
176 measurements of the curvature of the earth were carried out in the
177 eighteenth century and Newton was proved correct.
178
179 The earth has an equatorial bulge, in other words. It is flattened at
180 the poles. It is an "oblate spheroid" rather than a sphere. This means
181 that the various diameters of the earth differ in length. The longest
182 diameters are any of those that stretch from one point on the equator
183 to an opposite point on the equator. This "equatorial diameter" is
184 12,755 kilometers (7,927 miles). The shortest diameter is from the
185 North Pole to the South Pole and this "polar diameter" is 12,711
186 kilometers (7,900 miles).
187
188 The difference between the longest and shortest diameters is 44
189 kilometers (27 miles), and that means that the "oblateness" of the
190 earth (its departure from true sphericity) is 44/12755, or
191 0.0034. This amounts to 1/3 of 1 percent.
192
193 To put it another way, on a flat surface, curvature is 0 per mile
194 everywhere. On the earth's spherical surface, curvature is 0.000126
195 per mile everywhere (or 8 inches per mile). On the earth's oblate
196 spheroidal surface, the curvature varies from 7.973 inches to the mile
197 to 8.027 inches to the mile.
198
199 The correction in going from spherical to oblate spheroidal is much
200 smaller than going from flat to spherical. Therefore, although the
201 notion of the earth as a sphere is wrong, strictly speaking, it is not
202 as wrong as the notion of the earth as flat.
203
204 Even the oblate-spheroidal notion of the earth is wrong, strictly
205 speaking. In 1958, when the satellite Vanguard I was put into orbit
206 about the earth, it was able to measure the local gravitational pull
207 of the earth--and therefore its shape--with unprecedented
208 precision. It turned out that the equatorial bulge south of the
209 equator was slightly bulgier than the bulge north of the equator, and
210 that the South Pole sea level was slightly nearer the center of the
211 earth than the North Pole sea level was.
212
213 There seemed no other way of describing this than by saying the earth
214 was pear-shaped, and at once many people decided that the earth was
215 nothing like a sphere but was shaped like a Bartlett pear dangling in
216 space. Actually, the pear-like deviation from oblate-spheroid perfect
217 was a matter of yards rather than miles, and the adjustment of
218 curvature was in the millionths of an inch per mile.
219
220 In short, my English Lit friend, living in a mental world of absolute
221 rights and wrongs, may be imagining that because all theories are
222 wrong, the earth may be thought spherical now, but cubical next
223 century, and a hollow icosahedron the next, and a doughnut shape the
224 one after.
225
226 What actually happens is that once scientists get hold of a good
227 concept they gradually refine and extend it with greater and greater
228 subtlety as their instruments of measurement improve. Theories are not
229 so much wrong as incomplete.
230
231 This can be pointed out in many cases other than just the shape of the
232 earth. Even when a new theory seems to represent a revolution, it
233 usually arises out of small refinements. If something more than a
234 small refinement were needed, then the old theory would never have
235 endured.
236
237 Copernicus switched from an earth-centered planetary system to a
238 sun-centered one. In doing so, he switched from something that was
239 obvious to something that was apparently ridiculous. However, it was a
240 matter of finding better ways of calculating the motion of the planets
241 in the sky, and eventually the geocentric theory was just left behind.
242 It was precisely because the old theory gave results that were fairly
243 good by the measurement standards of the time that kept it in being so
244 long.
245
246 Again, it is because the geological formations of the earth change so
247 slowly and the living things upon it evolve so slowly that it seemed
248 reasonable at first to suppose that there was no change and that the
249 earth and life always existed as they do today. If that were so, it
250 would make no difference whether the earth and life were billions of
251 years old or thousands. Thousands were easier to grasp.
252
253 But when careful observation showed that the earth and life were
254 changing at a rate that was very tiny but not zero, then it became
255 clear that the earth and life had to be very old. Modern geology came
256 into being, and so did the notion of biological evolution.
257
258 If the rate of change were more rapid, geology and evolution would
259 have reached their modern state in ancient times. It is only because
260 the difference between the rate of change in a static universe and the
261 rate of change in an evolutionary one is that between zero and very
262 nearly zero that the creationists can continue propagating their
263 folly.
264
265 Since the refinements in theory grow smaller and smaller, even quite
266 ancient theories must have been sufficiently right to allow advances
267 to be made; advances that were not wiped out by subsequent
268 refinements.
269
270 The Greeks introduced the notion of latitude and longitude, for
271 instance, and made reasonable maps of the Mediterranean basin even
272 without taking sphericity into account, and we still use latitude and
273 longitude today.
274
275 The Sumerians were probably the first to establish the principle that
276 planetary movements in the sky exhibit regularity and can be
277 predicted, and they proceeded to work out ways of doing so even though
278 they assumed the earth to be the center of the universe. Their
279 measurements have been enormously refined but the principle remains.
280
281 Naturally, the theories we now have might be considered wrong in the
282 simplistic sense of my English Lit correspondent, but in a much truer
283 and subtler sense, they need only be considered incomplete.