This passage was excerpted from material published in 1996.
When a large body strikes a planet or moon, material is ejected, thereby creating a hole in the planet and a local deficit of mass. This deficit shows up as a gravity anomaly: the removal of the material that has been ejected to make the hole results in an area of slightly lower gravity than surrounding areas. One would therefore expect that all of the large multi-ring impact basins on the surface of Earth's Moon would show such negative gravity anomalies, since they are, essentially, large holes in the lunar surface. Yet data collected in 1994 by the Clementine spacecraft show that many of these lunar basins have no anomalously low gravity and some even have anomalously high gravity.Scientists speculate that early in lunar history, when large impactors struck the Moon's surface, causing millions of cubic kilometers of crustal debris to be ejected, denser material from the Moon's mantle rose up beneath the impactors almost immediately, compensating for the ejected material and thus leaving no low gravity anomaly in the resulting basin. Later, however, as the Moon grew cooler and less elastic, rebound from large impactors would have been only partial and incomplete. Thus today such gravitational compensation probably would not occur: the outer layer of the Moon is too cold and stiff.
The passage suggests that if the scientists mentioned in the highlighted text are correct in their speculations, the large multi-ring impact basins on the Moon with the most significant negative gravity anomalies probably
were not formed early in the Moon's history
were not formed by the massive ejection of crustal debris
are closely surrounded by other impact basins with anomalously low gravity
were created by the impact of multiple large impactors
were formed when the Moon was relatively elastic
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正确答案是 E。因为文中提到,当月球早期受到大型撞击物的冲击,会导致数百万立方公里的地壳碎片被喷射出来,而这些碎片会被密度更高的来自月球地幔的物质立即补上,因此导致最终形成的盆地不会有低引力异常。然而,当月球变得冷而且比较僵硬时,撞击物的反弹力不完整,也就是说,今天发生撞击时,不太可能发生这种引力补偿,因为月球外层太冷而且太僵硬了。所以,答案是 E,这些大型多圈撞击盆地在月球相对比较有弹性时形成。
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