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托福考试托福阅读练习题:排除列举题6
发布时间:2013/7/12 22:57:35 来源:城市网学院 编辑:admin

  In July of 1994, an astounding series of events took place. The world anxiously
  
  watched as, every few hours, a hurtling chunk of #et plunged into the atmosphere of
  
  Jupiter. All of the twenty-odd fragments, collectively called #et Shoemaker-Levy 9
  
  Line after its discoverers, were once part of the same object, now dismembered and strung out
  
  (5)  along the same orbit. This #etary train, glistening like a string of pearls, had been first
  
  glimpsed only a few months before its fateful impact with Jupiter, and rather quickly
  
  scientists had predicted that the fragments were on a collision course with the giant
  
  planet. The impact caused an explosion clearly visible from Earth, a bright flaming fire
  
  that quickly expanded as each icy mass incinerated itself. When each fragment slammed
  
  (10) at 60 kilometers per second into the dense atmosphere, its immense kinetic energy was
  
  transformed into heat, p

roducing a superheated fireball that was ejected back through the
  
  tunnel the fragment had made a few seconds earlier. The residues form these explo-
  
  sions left huge black marks on the face of Jupiter, some of which have stretched out to
  
  from dark ribbons.
  
  (15)  Although this impact event was of considerable scientific importance, it especially piqued
  
  public curiosity and interest. Photographs of each collision made the evening television
  
  newscast and were posted on the Internet. This was possibly the most open scientific
  
  endeavor in history. The face of the largest planet in the solar system was changed before
  
  our very eyes. And for the very first time, most of humanity came to fully appreciate the
  
  (20) fact that we ourselves live on a similar target, a world subject to catstrophe by random
  
  assaults from celestial bodies. That realization was a surprise to many, but it should not
  
  have been. One of the great truths revealed by the last few decades of planetary explo-
  
  ration is that collisions between bodies of all sizes are relatively #monplace, at least in
  
  geologic terms, and were even more frequent in the early solar system.

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