2013-06-06 00:00:00 来源:新东方网托福资料下载
7、 Which of the sentences below best expresses the essential information in the highlighted sentence in the passage? Incorrect choices change the meaning in important ways or leave out essential information.
Although direct evidence of recent eruptions is lacking, scientists believe that these volcanoes were active as recently as 100 million years ago.
Scientists estimate that volcanoes active more recently than 100 years ago will still have extensive impact cratering on their slopes.
If, as some evidence suggests, these volcanoes erupted as recently as 100 million years ago, they may continue to be intermittently active.
Although these volcanoes were active as recently as 100 million years ago, there is no direct evidence of recent or ongoing eruptions.
Paragraph 4
Another prominent feature of Mars's surface is cratering. The Mariner spacecraft found that the surface of Mars, as well as that of its two moons, is pitted with impact craters formed by meteoroids falling in from space. As on our Moon, the smaller craters are often filled with surface matter-mostly dust-confirming that Mars is a dry desert world. However, Martian craters get filled in considerably faster than their lunar counterparts. On the Moon, ancient craters less than 100 meters across (corresponding to depths of about 20 meters) have been obliterated, primarily by meteoritic erosion. On Mars, there are relatively few craters less than 5 kilometers in diameter. The Martian atmosphere is an efficient erosive agent, with Martian winds transporting dust from place to place and erasing surface features much faster than meteoritic impacts alone can obliterate them.
8、The word "considerably" in the passage is closest in meaning to
Frequently
Significantly
Clearly
Surprisingly
9、According to paragraph 4, what is demonstrated by the fact that craters fill in much faster on Mars than on the Moon?
Erosion from meteoritic impacts takes place more quickly on Mars than on the Moon.
There is more dust on Mars than on the Moon.
The surface of Mars is a dry desert.
Wind is a powerful eroding force on Mars.
10、In the papragraph 4, why does the author point out that Mars has few ancient craters that are less than 5 kilometer?
To explain why scientists believe that the surface matter fill Martian craters is mostly dust
To explain why scientists believe that the impact craters on Mars were created by meteoroids
To support the claim that Martian atmosphere is an efficient erosive agent
To argue that Mans experienced fewer ancient I impacts than the Moon did
Paragraph 5
As on the Moon, the extent of large impact cratering (i.e.craters too big to have been filled in by erosion since they were formed) serves as an age indicator for the Martian surface. Age estimates ranging from four billion years for Mars's southern highlands to a few hundred million years in the youngest volcanic areas were obtained in this way.
11、According to paragraph 5, what have scientists been able to determine from studies of large impact cratering on Mars?
Some Martian volcanoes are much older ithan was once thought.
The age of Mars's surface can vary from area to area.
Large impact craters are not reliable indicators of age in areas with high volcanic activity.
Some areas of the Martian surface appear to be $Wer than they actually are.
Paragraph 6
The detailed appearance of Martian impact craters provides an important piece of information about conditions just below the planet's surface. Martian craters are surrounded by ejecta (debris formed as a result of an impact) that looks quite different from its lunar counterparts. A comparison of the Copernicus crater on the Moon with the (fairly typical) crater Yuty on Mars demonstrates the differences. The ejecta surrounding the lunar crater is just what one would expect from an explosion ejecting a large volume of dust, soil, and boulders.However, the ejecta on Mars gives the distinct impression of a liquid that has splashed or flowed out of crater. Geologists think that this fluidized ejecta crater indicates that a layer of permafrost, or water ice, lies just a few meters under the surface. Explosive impacts heated and liquefied the ice, resulting in the fluid appearance of the ejecta.
12、 According to paragraph 6, the ejecta of Mars's crater Yuty differs from the ejecta of the Moon's Copernicus crater in that the ejecta of the Yuty crater
Has now become part of a permafrost layer
Contains a large volume of dust, soil and boulders
Suggests that liquid once came out of the surface at the crater site
Was thrown a comparatively long distance from the center of the crater
13、Look at the four squares [■] that indicate where the following sentence could be added to the
passage.
This surface feature has led to speculation about what may lie under Mars's surface.
Where would the sentence best fit? Click on a square to add the sentence to the passage.
Paragraph 6
The detailed appearance of Martian impact craters provides an important piece of information about conditions just below the planet's surface. Martian craters are surrounded by ejecta (debris formed as a result of an impact) that looks quite different from its lunar counterparts. A comparison of the Copernicus crater on the Moon with the (fairly typical) crater Yuty on Mars demonstrates the differences. The ejecta surrounding the lunar crater is just what one would expect from an explosion ejecting a large volume of dust, soil, and boulders. ■ However, the ejecta on Mars gives the distinct impression of a liquid that has splashed or flowed out of crater. ■ Geologists think that this fluidized ejecta crater indicates that a layer of permafrost, or water ice, lies just a few meters under the surface. ■ Explosive impacts heated and liquefied the ice, resulting in the fluid appearance of the ejecta. ■
B
14、 Directions: An introductory sentence for a brief summary of the passage is provided below. Complete the summary by selecting the THREE answer choices that express the most important ideas in the passage. Some answer choices do not belong in the summary because they express ideas that are not presented in the passage or are minor ideas in the passage. This question is worth 2 points.
Volcanoes and impact craters are major features of Martian geology.
A. Plate motion on Mars, once considered to have played no role in shaping the planets surface, is
now seen as being directly associated with the planet's earliest volcanoes.
B.Mars has shield volcanoes, some of which are extremely tall because of the planet"s low surface
gravity.
C. Although the erosive power of the Martian atmosphere ensures that Mars has fewer craters than the
Moon does, impact craters are prominent on Mars' s surface.
D. Scientists cannot yet reliably estimate the age of the Martian surface because mere has been too
much erosion of it.
E. Scientists have been surprised to discover that conditions just below the surface of Mars are very
similar to conditions just below the surface of the Moon
F. Studies of crater ejecta have revealed the possibility of a layer of permafrost below the surface of
Mars.
本文关键字: 托福阅读
资料下载
2021-2025托福机经试题|答案|范文下载
发布时间:2024-02-21关注新东方在线托福
回复【XDF】获取
托福全科备考资料大礼包
发布时间:2024-02-21关注新东方在线托福
回复【XDF】获取
托福正价课试听课程包
发布时间:2024-02-21关注新东方在线托福
回复【XDF】获取
托福定制备考规划
发布时间:2024-02-21关注新东方在线托福
回复【XDF】获取
托福TPO免费模考
发布时间:2024-02-21关注新东方在线托福
回复【XDF】获取
托福免费水平测试
发布时间:2024-02-21关注新东方在线托福
回复【XDF】获取
托福写作新题型模拟题+范文汇总[ETS发布]
发布时间:2023-07-30关注新东方在线托福
回复【XDF】获取
2023全年托福机经PDF版下载
发布时间:2023-06-17关注新东方在线托福
回复【XDF】获取
2022全年托福机经PDF版下载
发布时间:2023-06-17关注新东方在线托福
回复【XDF】获取
2022全年写作托福机经整理
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
2022年托福考后题目回忆
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
托福口语黄金80题附录音
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
新东方IBT写作网络课堂录音[.rar]
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
21天托福听力提升计划
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
不怕跑题偏题,这份写作资料请收好
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
托福阅读提分技巧锦囊妙计
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
口语拖后腿?因为你缺少这套万能句式资料
发布时间:2019-11-01关注新东方在线托福
回复【XDF】获取
攻破托福听力难关的资料包
发布时间:2023-01-13关注新东方在线托福
回复【XDF】获取
看剧学英语,经典美剧一键获取
发布时间:2019-11-01关注新东方在线托福
回复【XDF】获取
原版外刊资源合集|精心打包整理
发布时间:2019-11-01关注新东方在线托福
回复【XDF】获取
关注新东方在线托福,
回复【XDF】获取大礼包

版权及免责声明
1,"新东方在线"上的内容,包括文章、资料、资讯等, 本网注明"稿件来源:新东方在线"的,其版权 均为"新东方在线"或北京新东方迅程网络科技有限公司所有 ,任何公司、媒体、网站或个人未经授权不得转载、链接、转贴或以其他方式使用。已经得到 "新东方在线"许可 的媒体、网站,在使用时必须注明"稿件来源:新东方",违者本网站将依法追究责任。
2, "新东方在线" 未注明"稿件来源:新东方"的 文章、资料、资讯等 均为转载稿,本网站转载出于传递更多信息之目的,并不意味着赞同其观点或证实其内容的真实性。如其他媒体、网站或个人从本网站下载使用,必须保留本网站注明的"稿件来源",并自负版权等法律责任。如擅自篡改为 " 稿件来源:新东方 " ,本网站将依法追究其法律责任。
3,如本网转载稿涉及版权等问题,请作者见稿后在两周内与新东方在线联系。
资料下载
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关注新东方在线托福
回复【XDF】获取
关于我们 - 商务合作 - 广告服务 - 代理商区域 - 客服中心 - 在线留言 - 退换货说明 - 合作伙伴 - 联系我们 - 人员招聘 - 网站地图 - 热点关注 - 寓乐优学
新东方教育科技集团旗下成员公司 全国客服专线:400-676-3300
Copyright (C) 2000-2013 koolearn.com Inc. All rights reserved. 新东方在线 版权所有
京ICP证050421号 京ICP备05067669号 京公网安备11010802017616号 网络视听许可证0110531号