GRE阅读理解具体的做题步骤

　　虽然GRE考试的阅读理解部分是比较难的，只要我们掌握具体的一些做题步骤还是可以拿到高分的。一起来看看小编为大家整理收集了GRE考试阅读理解题具体的做题步骤吧，欢迎大家阅读!

GRE阅读理解做题步骤

　　GRE阅读理解5大做题步骤

　　第一步：读原文

　　GRE阅读的基本做题方法，就是先读原文再看题目，看过题目后再根据题目定位回原文，所以读原文是做一篇阅读的第一步。有些读者已经养成了先读题目再看原文的阅读习惯，其实，做题的顺序要因阅读特点和出题方式而异，GRE阅读题目的出题顺序和原文几乎没有任何联系，也就是说第一道题可能考了原文的末尾，而最后一道题可能考的是原文的开始，故先读题目再读原文对做题没有任何帮助，反而有可能扰乱读者理解原文内在的逻辑结构。

　　第二步：读原文的同时对重点、考点做标记

　　做标记是指在读文章的时候用简单的符号记录所读重点内容，这应该和读GRE阅读文章同步进行，标记可以轻轻做在试卷边缘，也可以另外写在草稿纸上。所标记的主要目的是为了读完选项之后能快速、准确的定位，这个步骤要求读者熟悉常考考点，对应做标记的内容烂熟于胸，这样才能不费时间的给自己下一步的定位作准标记。

　　第三步：读题干、选项

　　读GRE阅读题干的过程也是个找题干特征的过程，看看题干所述和自己所做标记的内容有没有联系，如果有，则可以直接定位，故定位最主要的基础是题干与标记之间的联系。有时候题干可能没有可以捕捉的特征，这时读者不妨从选项下手，选项中也时常会有明显的特征反映出它与原文中的重点内容之间的相关性。

　　第四步：定位

　　定位指的是确定考题针对GRE阅读原文中什么位置的内容发问，通常通过题干和选项的特征词来找，判断了原文所述的位置之后，就可以找原文和答案之间的对应关系了，绝大多数题目都可以通过找题干和选项的特征词准确的定位到原文某处。

　　第五步：排除干扰选项后按照文字对应原则选答案

　　GRE考试的'备选答案都是五个，通常很少有考题能让读者非常直接的判断出正确答案，总有1-2个迷惑性比较大的选项，所以，考生不妨先竖读各选相，排除一些明显错误的选项，然后再对剩下的进行细致的比较，通过原文和选项之间的文字对应关系，进行选择。

　　GRE阅读理解备考技巧

　　1.解剖文章的首段

　　GRE考试中阅读部分需要考生积极主动地解读文章的第1段，阅读时尽量记住作者提出的问题(现象或观点)，和一些关于文章内容的概念和词汇，如这篇文章讲的是生物化学，日本企业文化还是黑人运动。文章的论题是什么，作者想说什么?

　　2.分析作者思路

　　在脑子里或者在草稿纸上画一个新GRE阅读文章的结构思路题。各个段落的目的是什么，主题又是什么-再次提醒，考察的是你的答题能力而非阅读能力。你不必完全掌握整篇GRE阅读理解文章，了解文章中的每一个细节(其实，你也没有那么多时间)。相反，你应该只读文章段落的第1句，而快速浏览其余部分。当你“读”完这篇文章时，你就能对文章的结构思路有总体的把握。

　　3.语气词过渡词要重点留意

　　在快速阅读文章时，特别留意段落开头或者结尾可能出现的语气词和过渡词。这样做有助于你对作者思路的把握，从而快速掌握文章大意。

　　4.总结文章大意

　　在回答问题前，花几秒钟总结一下文章的思路和主题。

　　5.开始答题

　　根据你对文章的整体思路来答题。将问题(或选项)定位到文章中具体的某个段落甚至具体的句子。这里，你可以比第3个步骤更仔细。

　　GRE阅读理解练习题

　　Hotter and more massive than the Sun, stars called “stragglers” are puzzling to astronomers because such rapidly burning stars would not be expected to persist in ancient star clusters. Some researchers believe that the typical blue stragglers formed when two ancient, lower-mass stars collide and merge form more massive, hotter star. Peter Leonard theorizes alternatively that in low density globular clusters, where mergers between single stars occur too infrequently to account for the observed quantity of blue stragglers, these stragglers are created instead by a group of stars. He suggests that a pair of stars already orbiting each other presents a larger target for a third star or another pair. Once this new grouping forms, close encounters between the stars could prompt any two to merge as a blue straggler. Leonard’s model predicts that each blue straggler has a distant orbiting companion—as appears true of many blue stragglers in the M67 cluster of the Milky Way galaxy.

　　1. The reference to a “larger target” serves primarily to suggest why a

　　A. blue straggler would be more likely to collide and merge with another star than would be a lower-mass star

　　B. pair of stars would be more likely to encounter other stars than would the typical blue straggler

　　C. pair of stars would be more likely to interact with other stars than would a single star

　　D. blue straggler would be more likely to interact with a pair of stars than it would with a third star

　　E. third star would be more likely to encounter a pair than it would to encounter a blue straggler

　　2. Information presented in the passage suggests which of the following about blue stragglers?

　　A. They originate from stars that are hotter and more massive than the Sun.

　　B. They are burning more rapidly than other types of stars observed in ancient star clusters.

　　C. They are older than most other types of stars within the same star cluster.

　　D. They are less numerous in low-density globular clusters than are pairs of stars.

　　E. They generally originate from the oldest stars among those found in ancient star clusters.

　　3. The passage cites which of the following as evidence undermining the theory presented in the second sentence?

　　A. A discrepancy between the number of mergers between single stars in certain low-density globular clusters and that in other low-density globular clusters

　　B. A discrepancy between the heat and mass of blue stragglers formed by one type of process and the heat and mass of blue stragglers formed by another type of process

　　C. A discrepancy between the frequency of star mergers in low-density globular clusters and those in high-density globular clusters

　　D. A discrepancy between the amount of heat and mass of ancient single stars and that of blue stragglers

　　E. A discrepancy between the number of mergers between single stars in certain star clusters and the number of blue stragglers in those clusters

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