托福阅读真题Official 50 Passage 3（五）

托福阅读真题Official 50 Passage 3（五）

Star Death

Until the early-to mid-twentieth century,scientists believed that stars generate energy by shrinking.As stars contracted,it was thought,they would get hotter and hotter,giving off light in the process.This could not be the primary way that stars shine,however.If it were,they would scarcely last a million years,rather than the billions of years in age that we know they are.We now know that stars are fueled by nuclear fusion.Each time fusion takes place,energy is released as a by-product.This energy,expelled into space,is what we see as starlight.The fusion process begins when two hydrogen nuclei smash together to form a particle called the deuteron(a combination of a positive proton and a neutral neutron).Deuterons readily combine with additional protons to form helium.Helium,in turn,can fuse together to form heavier elements,such as carbon.In a typical star,merger after merger takes place until significant quantities of heavy elements are built up.

We must distinguish,at this point,between two different stellar types:Population I and Population II,the latter being much older than the former.These groups can also be distinguished by their locations.Our galaxy,the Milky Way,is shaped like a flat disk surrounding a central bulge.Whereas Population I stars are found mainly in the galactic disk,Population II stars mostly reside in the central bulge of the galaxy and in the halo surrounding this bulge.

Population II stars date to the early stages of the universe.Formed when the cosmos was filled with hydrogen and helium gases,they initially contained virtually no heavy elements.They shine until their fusible material is exhausted.When Population II stars die,their material is spread out into space.Some of this dust is eventually incorporated into newly formed Population I stars.Though Population I stars consist mostly of hydrogen and helium gas,they also contain heavy elements(heavier than helium),which comprise about 1 or 2 percent of their mass.These heavier materials are fused from the lighter elements that the stars have collected.Thus,Population I stars contain material that once belonged to stars from previous generations.The Sun is a good example of a Population I star.

What will happen when the Sun dies.In several billion years,our mother star will burn much brighter.It will expend more and more of its nuclear fuel,until little is left of its original hydrogen.Then,at some point in the far future,all nuclear reactions in the Sun’s center will cease.

Once the Sun passes into its“postnuclear”phase,it will separate effectively into two different regions:an inner zone and an outer zone.While no more hydrogen fuel will remain in the inner zone,there will be a small amount left in the outer zone.Rapidly,changes will begin to take place that will serve to tear the Sun apart.The inner zone,its nuclear fires no longer burning,will begin to collapse under the influence of its own weight and will contract into a tiny hot core,dense and dim.An opposite fate will await the outer region,a loosely held-together ball of gas.A shock wave caused by the inner zone’s contraction will send ripples through the dying star,pushing the stellar exterior’s material farther and farther outward.The outer envelope will then grow rapidly,increasing,in a short interval,hundreds of times in size.As it expands,it will cool down by thousands of degrees.Eventually,the Sun will become a red giant star,cool and bright.It will be so large that it will occupy the whole space that used to be the Earth’s orbit and so brilliant that it would be able to be seen with the naked eye thousands of light-years away.It will exist that way for millions of years,gradually releasing the material of its outer envelope into space.Finally,nothing will be left of the gaseous exterior of the Sun;all that will remain will be the hot,white core.The Sun will have become a white dwarf star.The core will shrink,giving off the last of its energy,and the Sun will finally die.

Question 9 of 14

Why does the author ask the question“What will happen when the Sun dies?”?

A.To identify the most serious question concerning star death that scientists must address

B.To introduce the topic that the rest of the passage will discuss

C.To suggest that scientists remain uncertain about some aspects of star death

D.To suggest that the Sun may not be a good example of a Population I star

正确答案：B

题目详解

题型分类：修辞目的题

题干分析：考察一个段落的主旨。

选项分析：

根据题干内容，定位到第四段第一句。第四段全部的内容都是在描述太阳的衰亡过程，说明这个问题是在引出第四段的内容，即B选项。

A选项the most serious question后文没有说到。

C选项uncertain about some aspects后文没有提到。

D选项not be a good example of a Population I star后文没有提到。

Question 10 of 14

According to paragraph 5,once the Sun is in its“postnuclear”phase,the outer zone will differ from the inner zone in that the outer zone will

A.undergo a much less dramatic change in size

B.maintain more nearly constant temperatures

C.cease to be a site of energy-generating activity

D.still contain some amount of hydrogen

Paragraph 5 is marked with an arrow

正确答案：D

题目详解

题型分类：事实信息题

原文定位：根据once the Sun is in its“postnuclear”phase定位到第五段第一句和第二句。

选项分析：

第二句a small amount left in the outer zone对应D选项及题干the outer zone will still contain some amount of hydrogen。

A选项a much less dramatic change in size无中生有。文中没有对比内外区域的大小变化。

B选项nearly constant temperatures与原文cool down by thousands of degrees信息相反。

C选项，原文说的是The inner zone,its nuclear fires no longer burning，而没有说外部区域会停止释放能量。