TOEFL 6 (READING PASSAGE 2) TOEFL READING PRACTICE WITH ANSWERS

 

TOEFL READING PRACTICE WITH ANSWERS TOEFL 6 (READING PASSAGE 2)

 

Questions 9-19 Stars may be spheres, but not every celestial object is spherical. Objects in the universe show a variety of shapes: round planets (some with rings), tailed comets, wispy cosmic gas and dust clouds, ringed nebulae, pinwheel-shaped spiral galaxies, and so on. But none of the shapes on this list describes the largest single entities in the universe. These are the double radio sources, galaxies with huge clouds of radio emission that dwarf the visible galaxies, sometimes by a factor of a hundred or more. Stretching over distances greater than a million light-years, these radio-emitting regions resemble twin turbulent gas clouds, typically forming dumbbell-like shapes with the visible galaxy (when it is visible) in the center. These double radio sources present astronomers with a puzzle. Their radio emission arises from the synchrotron process, in which electrons accelerated to nearly the speed of light move through magnetic fields. However, in view of the rate at which the radio sources emit energy, they should disappear in a few million years as their electrons slow down and cease producing radiation. Somehow new electrons must be continually accelerated to nearly the speed of light, otherwise, by now almost none of the double radio sources would be observed. With the advent of high-resolution radio interferometers during the late 1970's, part of the answer became clear: the electrons are produced in jets that are shot out in opposite directions from the center of galaxy. Remarkably narrow and highly directional, the jets move outward at speeds close to the speed of light. When the jets strike the highly rarefied gas that permcales intergalactic space, the fast-moving electrons lose their highly directional motion and form vast clouds of radio-emitting gas. Cosmic jets have ranked among the hottest topics of astronomical research in recent years as astronomers strive to understand where they come from. Why should a galaxy eject matter at such tremendous speeds in two narrow jets? And why are such jets not seen in the Milky Way?   9. The word "celestial" in line 1 could best be replaced by (A) visible (B) astronomical (C) glowing (D) scientific 10. The word "entities" in line 4 is closest in meaning to (A) factors (B) processes (C) objects (D) puzzle 11. In the first paragraph, the author describes objects in the universe in terms of their (A) color (B) origin (C) location (D) shape 12. Which of the following is the best representation of the clouds of radio emission described in the first paragraph? (A) （图） (B) （图） (C) （图） (D) （图） 13. According to the passage, scientists do not fully understand why double radio sources (A) have not eventually disappeared (B) cannot be observed with a telescope (C) are beginning to slow down (D) are not as big as some planets and stars 14. The word "their" in line 22 refers to (A) speeds (B) directions (C) electrons (D) clouds 15. According to the passage, what happens when electrons and gas collide in space? (A) The gas becomes more condensed (B) The gas becomes less radiated (C) The electrons disperse (D) The electrons become negatively charged 16. The author suggests that astronomers consider the study of cosmic jets to be (A) an obsolete scientific field (B) an unprofitable venture (C) an intriguing challenge (D) a subjective debate 17. In what lines does the passage compare the size of double radio sources with that of other galaxies? (A) Lines 4-6 (B) Lines 12-14 (C) Lines 19-20 (D) Lines 23-24 18. Where in the passage does the author mention a technology that aided in the understanding of double radio sources? (A) Line 2 (B) Line 7 (C) Line 17 (D) Line 21 19. The paragraph following the passage most likely discusses (A) specific double radio sources (B) an explanation of the synchrotron process (C) possible reasons for the presence of cosmic jets (D) the discovery of the first double radiosources.

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ANSWER KEY

9.       B 10.     D 11.      D 12.     A 13.     A 14.     C 15.     C 16.     C 17.     A 18.     C 19.     C