]> pere.pagekite.me Git - text-relativity-of-wrong-asimov.git/blob - The_Relativity_of_Wrong.nb.po
Oversatt litt mer.
[text-relativity-of-wrong-asimov.git] / The_Relativity_of_Wrong.nb.po
1 # Copyright (C) 2016 Free Software Foundation, Inc.
2 # This file is distributed under the same license as the PACKAGE package.
3 #
4 # Petter Reinholdtsen <pere@hungry.com>, 2016.
5 msgid ""
6 msgstr ""
7 "Project-Id-Version: \n"
8 "POT-Creation-Date: 2016-07-25 21:53+0200\n"
9 "PO-Revision-Date: 2016-07-26 08:55+0200\n"
10 "Last-Translator: Petter Reinholdtsen <pere@hungry.com>\n"
11 "Language-Team: Norwegian Bokmål <i18n-no@lister.ping.uio.no>\n"
12 "Language: nb\n"
13 "MIME-Version: 1.0\n"
14 "Content-Type: text/plain; charset=UTF-8\n"
15 "Content-Transfer-Encoding: 8bit\n"
16 "Plural-Forms: nplurals=2; plural=(n != 1);\n"
17 "X-Generator: Lokalize 1.5\n"
18
19 #. type: Plain text
20 msgid "From The Skeptical Inquirer, Fall 1989, Vol. 14, No. 1, Pp. 35-44"
21 msgstr "Fra The Skeptical Inquirer, høsten 1989, vol. 14, no. 1, s. 35-44"
22
23 #. type: Plain text
24 msgid "The Relativity of Wrong"
25 msgstr "Relativiteten til galt"
26
27 #. type: Plain text
28 msgid "By Isaac Asimov"
29 msgstr "Av Isaac Asimov. Oversatt til bokmål av Petter Reinholdtsen"
30
31 #. type: Plain text
32 msgid ""
33 "I RECEIVED a letter the other day. It was handwritten in crabbed penmanship "
34 "so that it was very difficult to read. Nevertheless, I tried to make it out "
35 "just in case it might prove to be important. In the first sentence, the "
36 "writer told me he was majoring in English literature, but felt he needed to "
37 "teach me science. (I sighed a bit, for I knew very few English Lit majors "
38 "who are equipped to teach me science, but I am very aware of the vast state "
39 "of my ignorance and I am prepared to learn as much as I can from anyone, so "
40 "I read on.)"
41 msgstr ""
42 "Jeg fikk et brev her om dagen. Det var håndskrevet med knotete håndskrift "
43 "som gjorde det vanskelig å lese. Jeg forsøkte uansett å forstå hva som sto "
44 "der i tilfelle det skulle vise seg å være noe viktig. I den første "
45 "setningen forklarte forfatteren at han hadde hovedfag i engelsk litteratur men "
46 "følte at han trengte å lære meg naturvitenskap. (Jeg sukket litt, da jeg vet "
47 "veldig få med engelsk hovedfag som er utstyrt til å lære meg naturvitenskap. "
48 "Men jeg er godt kjent med det enorme omfanget av alt jeg ikke vet og klar til å "
49 "lære så mye jeg kan fra hvem det skal være, så jeg fortsatte å lese.)"
50
51 #. type: Plain text
52 msgid ""
53 "It seemed that in one of my innumerable essays, I had expressed a certain "
54 "gladness at living in a century in which we finally got the basis of the "
55 "universe straight."
56 msgstr ""
57 "Det virket som om at jeg i et av mine utallige tekster hadde gitt uttrykk "
58 "for en viss glede over å leve i et århundre hvor vi endelig hadde fått "
59 "grunnlaget for universet riktig."
60
61 #. type: Plain text
62 msgid ""
63 "I didn't go into detail in the matter, but what I meant was that we now know "
64 "the basic rules governing the universe, together with the gravitational "
65 "interrelationships of its gross components, as shown in the theory of "
66 "relativity worked out between 1905 and 1916. We also know the basic rules "
67 "governing the subatomic particles and their interrelationships, since these "
68 "are very neatly described by the quantum theory worked out between 1900 and "
69 "1930. What's more, we have found that the galaxies and clusters of galaxies "
70 "are the basic units of the physical universe, as discovered between 1920 and "
71 "1930."
72 msgstr ""
73 "Jeg gikk ikke i detaljer, men det jeg mente var at vi nå vet de grunnleggende "
74 "reglene som styrer universet og hvordan gravitasjonen for mesteparten virker "
75 "sammen, slik relativitetsteorien utarbeidet mellom 1905 og 1916 viser. Vi "
76 "kjenner også til de grunnleggende reglene som styrer subatomære partikler og "
77 "deres forhold til hverandre, da disse er svært godt beskrevet av "
78 "kvanteteorien som ble utarbeidet mellom 1900 og 1930. I tillegg har vi "
79 "funnet ut at galakser og samlinger av galakser er de grunnleggende enhetene "
80 "som utgjør det fysiske universet, slik det ble oppdaget mellom 1920 og 1930."
81
82 #. type: Plain text
83 msgid "These are all twentieth-century discoveries, you see."
84 msgstr "Disse, ser du, er alle oppdagelser fra det tyvende århundre."
85
86 #. type: Plain text
87 msgid ""
88 "The young specialist in English Lit, having quoted me, went on to lecture me "
89 "severely on the fact that in every century people have thought they "
90 "understood the universe at last, and in every century they were proved to be "
91 "wrong. It follows that the one thing we can say about our modern \"knowledge"
92 "\" is that it is wrong. The young man then quoted with approval what "
93 "Socrates had said on learning that the Delphic oracle had proclaimed him the "
94 "wisest man in Greece. \"If I am the wisest man,\" said Socrates, \"it is "
95 "because I alone know that I know nothing.\" the implication was that I was "
96 "very foolish because I was under the impression I knew a great deal."
97 msgstr ""
98
99 #. type: Plain text
100 msgid ""
101 "My answer to him was, \"John, when people thought the earth was flat, they "
102 "were wrong. When people thought the earth was spherical, they were wrong. "
103 "But if you think that thinking the earth is spherical is just as wrong as "
104 "thinking the earth is flat, then your view is wronger than both of them put "
105 "together.\""
106 msgstr ""
107 "Jeg svarte ham slik: «Da folk tenkte at jorden var flat, John, så tok de "
108 "feil. Når folk tenkte at orden var sfærisk, så tok de feil. Men hvis du "
109 "tror at det å tenke at jorden er sfærisk er like galt som å tenke at jorda er "
110 "flat, så er ditt syn mer feil enn begge to slått sammen.»"
111
112 #. type: Plain text
113 msgid ""
114 "The basic trouble, you see, is that people think that \"right\" and \"wrong"
115 "\" are absolute; that everything that isn't perfectly and completely right "
116 "is totally and equally wrong."
117 msgstr ""
118 "Du forstår, det grunnleggende problemet er at folk tenker at «riktig» og "
119 "«galt» er absolutter. Alt alt som ikke er perfekt og fullstendig riktig er "
120 "fullstendig og likeverdig galt."
121
122 #. type: Plain text
123 msgid ""
124 "However, I don't think that's so. It seems to me that right and wrong are "
125 "fuzzy concepts, and I will devote this essay to an explanation of why I "
126 "think so."
127 msgstr ""
128 "Jeg tror derimot ikke at det er slik. For meg virker det som om riktig og "
129 "feil er uklare konsepter, og jeg vil bruke denne teksten til å forklare "
130 "hvorfor jeg mener dette."
131
132 #. type: Plain text
133 msgid ""
134 "When my friend the English literature expert tells me that in every century "
135 "scientists think they have worked out the universe and are always wrong, "
136 "what I want to know is how wrong are they? Are they always wrong to the same "
137 "degree? Let's take an example."
138 msgstr ""
139
140 #. type: Plain text
141 msgid ""
142 "In the early days of civilization, the general feeling was that the earth "
143 "was flat. This was not because people were stupid, or because they were "
144 "intent on believing silly things. They felt it was flat on the basis of "
145 "sound evidence. It was not just a matter of \"That's how it looks,\" because "
146 "the earth does not look flat. It looks chaotically bumpy, with hills, "
147 "valleys, ravines, cliffs, and so on."
148 msgstr ""
149
150 #. type: Plain text
151 msgid ""
152 "Of course there are plains where, over limited areas, the earth's surface "
153 "does look fairly flat. One of those plains is in the Tigris-Euphrates area, "
154 "where the first historical civilization (one with writing) developed, that "
155 "of the Sumerians."
156 msgstr ""
157
158 #. type: Plain text
159 msgid ""
160 "Perhaps it was the appearance of the plain that persuaded the clever "
161 "Sumerians to accept the generalization that the earth was flat; that if you "
162 "somehow evened out all the elevations and depressions, you would be left "
163 "with flatness. Contributing to the notion may have been the fact that "
164 "stretches of water (ponds and lakes) looked pretty flat on quiet days."
165 msgstr ""
166
167 #. type: Plain text
168 msgid ""
169 "Another way of looking at it is to ask what is the \"curvature\" of the "
170 "earth's surface Over a considerable length, how much does the surface "
171 "deviate (on the average) from perfect flatness. The flat-earth theory would "
172 "make it seem that the surface doesn't deviate from flatness at all, that its "
173 "curvature is 0 to the mile."
174 msgstr ""
175
176 #. type: Plain text
177 msgid ""
178 "Nowadays, of course, we are taught that the flat-earth theory is wrong; that "
179 "it is all wrong, terribly wrong, absolutely. But it isn't. The curvature of "
180 "the earth is nearly 0 per mile, so that although the flat-earth theory is "
181 "wrong, it happens to be nearly right. That's why the theory lasted so long."
182 msgstr ""
183
184 #. type: Plain text
185 msgid ""
186 "There were reasons, to be sure, to find the flat-earth theory unsatisfactory "
187 "and, about 350 B.C., the Greek philosopher Aristotle summarized them. First, "
188 "certain stars disappeared beyond the Southern Hemisphere as one traveled "
189 "north, and beyond the Northern Hemisphere as one traveled south. Second, the "
190 "earth's shadow on the moon during a lunar eclipse was always the arc of a "
191 "circle. Third, here on the earth itself, ships disappeared beyond the "
192 "horizon hull-first in whatever direction they were traveling."
193 msgstr ""
194
195 #. type: Plain text
196 msgid ""
197 "All three observations could not be reasonably explained if the earth's "
198 "surface were flat, but could be explained by assuming the earth to be a "
199 "sphere."
200 msgstr ""
201
202 #. type: Plain text
203 msgid ""
204 "What's more, Aristotle believed that all solid matter tended to move toward "
205 "a common center, and if solid matter did this, it would end up as a sphere. "
206 "A given volume of matter is, on the average, closer to a common center if it "
207 "is a sphere than if it is any other shape whatever."
208 msgstr ""
209
210 #. type: Plain text
211 msgid ""
212 "About a century after Aristotle, the Greek philosopher Eratosthenes noted "
213 "that the sun cast a shadow of different lengths at different latitudes (all "
214 "the shadows would be the same length if the earth's surface were flat). From "
215 "the difference in shadow length, he calculated the size of the earthly "
216 "sphere and it turned out to be 25,000 miles in circumference."
217 msgstr ""
218
219 #. type: Plain text
220 msgid ""
221 "The curvature of such a sphere is about 0.000126 per mile, a quantity very "
222 "close to 0 per mile, as you can see, and one not easily measured by the "
223 "techniques at the disposal of the ancients. The tiny difference between 0 "
224 "and 0.000126 accounts for the fact that it took so long to pass from the "
225 "flat earth to the spherical earth."
226 msgstr ""
227
228 #. type: Plain text
229 msgid ""
230 "Mind you, even a tiny difference, such as that between 0 and 0.000126, can "
231 "be extremely important. That difference mounts up. The earth cannot be "
232 "mapped over large areas with any accuracy at all if the difference isn't "
233 "taken into account and if the earth isn't considered a sphere rather than a "
234 "flat surface. Long ocean voyages can't be undertaken with any reasonable way "
235 "of locating one's own position in the ocean unless the earth is considered "
236 "spherical rather than flat."
237 msgstr ""
238
239 #. type: Plain text
240 msgid ""
241 "Furthermore, the flat earth presupposes the possibility of an infinite "
242 "earth, or of the existence of an \"end\" to the surface. The spherical "
243 "earth, however, postulates an earth that is both endless and yet finite, and "
244 "it is the latter postulate that is consistent with all later findings."
245 msgstr ""
246
247 #. type: Plain text
248 msgid ""
249 "So, although the flat-earth theory is only slightly wrong and is a credit to "
250 "its inventors, all things considered, it is wrong enough to be discarded in "
251 "favor of the spherical-earth theory."
252 msgstr ""
253
254 #. type: Plain text
255 msgid "And yet is the earth a sphere?"
256 msgstr "Men er virkelig jorden en sfære?"
257
258 #. type: Plain text
259 msgid ""
260 "No, it is not a sphere; not in the strict mathematical sense. A sphere has "
261 "certain mathematical properties - for instance, all diameters (that is, all "
262 "straight lines that pass from one point on its surface, through the center, "
263 "to another point on its surface) have the same length."
264 msgstr ""
265 "Nei, den er ikke en sfære, ikke i matematisk forstand. En sfære har visse "
266 "matematiske egenskaper - for eksempel har alle diametre (dvs. alle rette "
267 "linjer som går fra et punkt på overflaten, gjennom sentrum, til et annet "
268 "punkt på overflaten) samme lengde."
269
270 #. type: Plain text
271 msgid ""
272 "That, however, is not true of the earth. Various diameters of the earth "
273 "differ in length."
274 msgstr ""
275 "Dette er derimot ikke riktig for jorden. Forskjellige diametre gjennom "
276 "jorden har ulik lengde."
277
278 #. type: Plain text
279 msgid ""
280 "What gave people the notion the earth wasn't a true sphere? To begin with, "
281 "the sun and the moon have outlines that are perfect circles within the "
282 "limits of measurement in the early days of the telescope. This is "
283 "consistent with the supposition that the sun and the moon are perfectly "
284 "spherical in shape."
285 msgstr ""
286
287 #. type: Plain text
288 msgid ""
289 "However, when Jupiter and Saturn were observed by the first telescopic "
290 "observers, it became quickly apparent that the outlines of those planets "
291 "were not circles, but distinct ellipses. That meant that Jupiter and Saturn "
292 "were not true spheres."
293 msgstr ""
294
295 #. type: Plain text
296 msgid ""
297 "Isaac Newton, toward the end of the seventeenth century, showed that a "
298 "massive body would form a sphere under the pull of gravitational forces "
299 "(exactly as Aristotle had argued), but only if it were not rotating. If it "
300 "were rotating, a centrifugal effect would be set up that would lift the "
301 "body's substance against gravity, and this effect would be greater the "
302 "closer to the equator you progressed. The effect would also be greater the "
303 "more rapidly a spherical object rotated, and Jupiter and Saturn rotated very "
304 "rapidly indeed."
305 msgstr ""
306
307 #. type: Plain text
308 msgid ""
309 "The earth rotated much more slowly than Jupiter or Saturn so the effect "
310 "should be smaller, but it should still be there. Actual measurements of the "
311 "curvature of the earth were carried out in the eighteenth century and Newton "
312 "was proved correct."
313 msgstr ""
314
315 #. type: Plain text
316 msgid ""
317 "The earth has an equatorial bulge, in other words. It is flattened at the "
318 "poles. It is an \"oblate spheroid\" rather than a sphere. This means that "
319 "the various diameters of the earth differ in length. The longest diameters "
320 "are any of those that stretch from one point on the equator to an opposite "
321 "point on the equator. This \"equatorial diameter\" is 12,755 kilometers "
322 "(7,927 miles). The shortest diameter is from the North Pole to the South "
323 "Pole and this \"polar diameter\" is 12,711 kilometers (7,900 miles)."
324 msgstr ""
325
326 #. type: Plain text
327 msgid ""
328 "The difference between the longest and shortest diameters is 44 kilometers "
329 "(27 miles), and that means that the \"oblateness\" of the earth (its "
330 "departure from true sphericity) is 44/12755, or 0.0034. This amounts to l/3 "
331 "of 1 percent."
332 msgstr ""
333
334 #. type: Plain text
335 msgid ""
336 "To put it another way, on a flat surface, curvature is 0 per mile "
337 "everywhere. On the earth's spherical surface, curvature is 0.000126 per mile "
338 "everywhere (or 8 inches per mile). On the earth's oblate spheroidal surface, "
339 "the curvature varies from 7.973 inches to the mile to 8.027 inches to the "
340 "mile."
341 msgstr ""
342
343 #. type: Plain text
344 msgid ""
345 "The correction in going from spherical to oblate spheroidal is much smaller "
346 "than going from flat to spherical. Therefore, although the notion of the "
347 "earth as a sphere is wrong, strictly speaking, it is not as wrong as the "
348 "notion of the earth as flat."
349 msgstr ""
350
351 #. type: Plain text
352 msgid ""
353 "Even the oblate-spheroidal notion of the earth is wrong, strictly speaking. "
354 "In 1958, when the satellite Vanguard I was put into orbit about the earth, "
355 "it was able to measure the local gravitational pull of the earth--and "
356 "therefore its shape--with unprecedented precision. It turned out that the "
357 "equatorial bulge south of the equator was slightly bulgier than the bulge "
358 "north of the equator, and that the South Pole sea level was slightly nearer "
359 "the center of the earth than the North Pole sea level was."
360 msgstr ""
361
362 #. type: Plain text
363 msgid ""
364 "There seemed no other way of describing this than by saying the earth was "
365 "pear-shaped, and at once many people decided that the earth was nothing like "
366 "a sphere but was shaped like a Bartlett pear dangling in space. Actually, "
367 "the pear-like deviation from oblate-spheroid perfect was a matter of yards "
368 "rather than miles, and the adjustment of curvature was in the millionths of "
369 "an inch per mile."
370 msgstr ""
371
372 #. type: Plain text
373 msgid ""
374 "In short, my English Lit friend, living in a mental world of absolute rights "
375 "and wrongs, may be imagining that because all theories are wrong, the earth "
376 "may be thought spherical now, but cubical next century, and a hollow "
377 "icosahedron the next, and a doughnut shape the one after."
378 msgstr ""
379
380 #. type: Plain text
381 msgid ""
382 "What actually happens is that once scientists get hold of a good concept "
383 "they gradually refine and extend it with greater and greater subtlety as "
384 "their instruments of measurement improve. Theories are not so much wrong as "
385 "incomplete."
386 msgstr ""
387
388 #. type: Plain text
389 msgid ""
390 "This can be pointed out in many cases other than just the shape of the "
391 "earth. Even when a new theory seems to represent a revolution, it usually "
392 "arises out of small refinements. If something more than a small refinement "
393 "were needed, then the old theory would never have endured."
394 msgstr ""
395
396 #. type: Plain text
397 msgid ""
398 "Copernicus switched from an earth-centered planetary system to a sun-"
399 "centered one. In doing so, he switched from something that was obvious to "
400 "something that was apparently ridiculous. However, it was a matter of "
401 "finding better ways of calculating the motion of the planets in the sky, and "
402 "eventually the geocentric theory was just left behind. It was precisely "
403 "because the old theory gave results that were fairly good by the measurement "
404 "standards of the time that kept it in being so long."
405 msgstr ""
406
407 #. type: Plain text
408 msgid ""
409 "Again, it is because the geological formations of the earth change so slowly "
410 "and the living things upon it evolve so slowly that it seemed reasonable at "
411 "first to suppose that there was no change and that the earth and life always "
412 "existed as they do today. If that were so, it would make no difference "
413 "whether the earth and life were billions of years old or thousands. "
414 "Thousands were easier to grasp."
415 msgstr ""
416
417 #. type: Plain text
418 msgid ""
419 "But when careful observation showed that the earth and life were changing at "
420 "a rate that was very tiny but not zero, then it became clear that the earth "
421 "and life had to be very old. Modern geology came into being, and so did the "
422 "notion of biological evolution."
423 msgstr ""
424
425 #. type: Plain text
426 msgid ""
427 "If the rate of change were more rapid, geology and evolution would have "
428 "reached their modern state in ancient times. It is only because the "
429 "difference between the rate of change in a static universe and the rate of "
430 "change in an evolutionary one is that between zero and very nearly zero that "
431 "the creationists can continue propagating their folly."
432 msgstr ""
433
434 #. type: Plain text
435 msgid ""
436 "Since the refinements in theory grow smaller and smaller, even quite ancient "
437 "theories must have been sufficiently right to allow advances to be made; "
438 "advances that were not wiped out by subsequent refinements."
439 msgstr ""
440
441 #. type: Plain text
442 msgid ""
443 "The Greeks introduced the notion of latitude and longitude, for instance, "
444 "and made reasonable maps of the Mediterranean basin even without taking "
445 "sphericity into account, and we still use latitude and longitude today."
446 msgstr ""
447 "Grekerne introduserte for eksempel begrepene lengdegrad og breddegrad, og "
448 "laget fornuftige kart over middelhavet, uten å ta hensyn til sfæriskiskhet, "
449 "og vi bruker fortsatt lengdegrad og breddegrad i dag."
450
451 #. type: Plain text
452 msgid ""
453 "The Sumerians were probably the first to establish the principle that "
454 "planetary movements in the sky exhibit regularity and can be predicted, and "
455 "they proceeded to work out ways of doing so even though they assumed the "
456 "earth to be the center of the universe. Their measurements have been "
457 "enormously refined but the principle remains."
458 msgstr ""
459
460 #. type: Plain text
461 msgid ""
462 "Naturally, the theories we now have might be considered wrong in the "
463 "simplistic sense of my English Lit correspondent, but in a much truer and "
464 "subtler sense, they need only be considered incomplete."
465 msgstr ""
466