After evidence was obtained in the 1920’s that the universe is expanding, it became reasonable to ask: will the universe continue to expand indefinitely, or is there enough mass in it for the mutual attraction of its constituents to bring this expansion to a halt? It can be calculated that the critical density of matter needed to brake the expansion and “close” the universe is equivalent to three hydrogen atoms per cubic meter. But the density of the observable universe-luminous matter in the form of galaxies-comes to only a fraction of this. If the expansion of the universe is to stop, there must be enough invisible matter in the universe to exceed the luminous matter in density by a factor of roughly 70. Our contribution to the search for this “missing matter” has been to study the rotational velocity of galaxies at various distances from their center of rotation. It has been known for some time that outside the bright nucleus of a typical spiral galaxy luminosity falls off rapidly with distance from the center. If luminosity were a true indicator of mass, most of the mass would be concentrated toward the center. Outside the nucleus the rotational velocity would decrease geometrically with distance from the center, in conformity with Kepler’s law. Instead we have found that the rotational velocity in spiral galaxies either remains constant with increasing distance from the center or increases slightly. This unexpected result indicates that the falloff in luminous mass with distance from the center is balanced by an increase in nonluminous mass. Our findings suggest that as much as 90 percent of the mass of the universe is not radiating at any wavelength with enough intensity to be detected on the Earth. Such dark matter could be in the form of extremely dim stars of low mass, of large planets like Jupiter, or of black holes, either small or massive. While it has not yet been determined whether this mass is sufficient to “close” the universe, some physicists consider it significant that estimates are converging on the critical value.
113 The passage suggests that the results of the authors' study have changed their ideas about which of the following characteristics of spiral galaxies? 1 The relative luminosity of different regions 2The relative rotational velocity of different regions 3The relative distribution of matter in different regions A I only B II only C III only D II and III only E I, II, and III 答案选D,我想知道3在文中如何看出change,在那里定位distribution of matter? 114 The authors' suggestion that "as much as 90 percent of the mass of the universe is not radiating at any wavelength with enough intensity to be detected on the Earth" (lines 39-42) would be most weakened if which of the following were discovered to be true? (A) Spiral galaxies are less common than types of galaxies that contain little nonluminous matter. (B) Luminous and nonluminous matter are composed of the same basic elements. (C) The bright nucleus of a typical spiral galaxy also contains some nonluminous matter. (D) The density of the observable universe is greater than most previous estimates have suggested. (E) Some galaxies do not rotate or rotate too slowly for their rotational velocity to be measured. 答案选A,解释这样写到:
The authors' conclusion about nonluminous matter is based on their study of the rotational velocity of spiral galaxies. If spiral galaxies were found to be atypical of galaxies, then it would be possible that, in those other galaxies, nonluminous matter does not increase as luminous matter decreases. If this were the case, the authors' conclusion would be based on a sample of galaxies not representative of the whole, and their argument would be seriously weakened. A Correct. The authors' conclusion assumes that spiral galaxies are typical of all galaxies; information calling that assumption into question weakens the argument. 不太明白黄色部分的结论在文中如何提到的,而又怎样推出了A答案? 请大家指点,谢谢! |