Part from the difficulty discussed in Section XXI, there is a second fundamental difficulty attending classical celestial1 mechanics, which, to the best of my knowledge, was first discussed in detail by the astronomer2 Seeliger. If we ponder over the question as to how the universe, considered as a whole, is to be regarded, the first answer that suggests itself to us is surely this: As regards space (and time) the universe is infinite. There are stars everywhere, so that the density3 of matter, although very variable in detail, is nevertheless on the average everywhere the same. In other words: However far we might travel through space, we should find everywhere an attenuated4 swarm5 of fixed6 stars of approximately the same kind and density.
This view is not in harmony with the theory of Newton. The latter theory rather requires that the universe should have a kind of centre in which the density of the stars is a maximum, and that as we proceed outwards7 from this centre the group-density of the stars should diminish, until finally, at great distances, it is succeeded by an infinite region of emptiness. The stellar universe ought to be a finite island in the infinite ocean of space1.
This conception is in itself not very satisfactory. It is still less satisfactory because it leads to the result that the light emitted by the stars and also individual stars of the stellar system are perpetually passing out into infinite space, never to return, and without ever again coming into interaction with other objects of nature. Such a finite material universe would be destined8 to become gradually but systematically9 impoverished10.
In order to escape this dilemma11, Seeliger suggested a modification12 of Newton’s law, in which he assumes that for great distances the force of attraction between two masses diminishes more rapidly than would result from the inverse13 square law. In this way it is possible for the mean density of matter to be constant everywhere, even to infinity14, without infinitely15 large gravitational fields being produced. We thus free ourselves from the distasteful conception that the material universe ought to possess something of the nature of a centre. Of course we purchase our emancipation16 from the fundamental difficulties mentioned, at the cost of a modification and complication of Newton’s law which has neither empirical nor theoretical foundation. We can imagine innumerable laws which would serve the same purpose, without our being able to state a reason why one of them is to be preferred to the others; for any one of these laws would be founded just as little on more general theoretical principles as is the law of Newton.
1Proof.—According to the theory of Newton, the number of “lines of force” which come from infinity and terminate in a mass m is proportional to the mass m. If, on the average, the Mass density rho 0 is constant throughout tithe17 universe, then a sphere of volume V will enclose the average mass rho 0 upper V. Thus the number of lines of force passing through the surface F of the sphere into its interior is proportional to rho 0 upper V. For unit area of the surface of the sphere the number of lines of force which enters the sphere is thus proportional to rho 0 StartFraction v Over upper F EndFraction or to rho 0 upper R. Hence the intensity18 of the field at the surface would ultimately become infinite with increasing radius19 R of the sphere, which is impossible.
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1 celestial | |
adj.天体的;天上的 | |
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2 astronomer | |
n.天文学家 | |
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3 density | |
n.密集,密度,浓度 | |
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4 attenuated | |
v.(使)变细( attenuate的过去式和过去分词 );(使)变薄;(使)变小;减弱 | |
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5 swarm | |
n.(昆虫)等一大群;vi.成群飞舞;蜂拥而入 | |
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6 fixed | |
adj.固定的,不变的,准备好的;(计算机)固定的 | |
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7 outwards | |
adj.外面的,公开的,向外的;adv.向外;n.外形 | |
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8 destined | |
adj.命中注定的;(for)以…为目的地的 | |
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9 systematically | |
adv.有系统地 | |
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10 impoverished | |
adj.穷困的,无力的,用尽了的v.使(某人)贫穷( impoverish的过去式和过去分词 );使(某物)贫瘠或恶化 | |
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11 dilemma | |
n.困境,进退两难的局面 | |
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12 modification | |
n.修改,改进,缓和,减轻 | |
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13 inverse | |
adj.相反的,倒转的,反转的;n.相反之物;v.倒转 | |
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14 infinity | |
n.无限,无穷,大量 | |
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15 infinitely | |
adv.无限地,无穷地 | |
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16 emancipation | |
n.(从束缚、支配下)解放 | |
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17 tithe | |
n.十分之一税;v.课什一税,缴什一税 | |
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18 intensity | |
n.强烈,剧烈;强度;烈度 | |
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19 radius | |
n.半径,半径范围;有效航程,范围,界限 | |
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