TPO25阅读之一(托福阅读真题)

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托福阅读TPO25答案解析

托福阅读TPO25答案解析

托福阅读答案1.enormous巨大的,所以正确答案是B,extremely large。

如果不认识,将答案代入原文,原文说在T这个地方有三座非常大的火山,定语从句修饰说T是个什么样的地区,能容下三座大火山的当然是很大的地方。

A 重要、C不寻常和D活跃都不靠谱。

2.注意问的是Olympus M,以这个词做关键词定位至第三句,讲O是最大的,所以正确答案只能是C,比较高,如果不确定可以往下看到最后一句,说三个大的跟O比起来要小点儿,也说明O比较大,其他答案都没说。

3.distinctive有特点的,不同的,所以正确答案是characteristic,dis作为前缀,有分或者否定之意,所以猜出distinctive有不同的意思,这道词汇题代入原文不靠谱,因为几个错误答案带进去也说得通,大家还是抓紧背单词吧。

4.以A的 broad, sloping sides 做关键词定位至第二段第二句的破折号后,正确,不选;B选项的 smaller 定位至第一段尾句,正确,不选;C的channel定位至第二段第三句,正确,不选;D 的数字定位至第一段倒数第二句,但25说的是O,而不是shield volcano,所以D错,是答案。

5.roughly大概,所以正确答案是D的approximately,代入原文,说火星的gravity只有地球的40%,因此火星上山的高度应该大致是地球的2.5倍,其他代入都说不通。

6.以Maxwell为关键词定位至第三段第四句,这句只是在比较,于是往前看,说gravity越低,高度越高,所以作者进行这个比较无外乎想证明这个结论,所以正确答案 A。

C稍有迷惑性,但C的问题在于没有提及高度,只是单纯说不同planet之间gravity的关系,错。

7.提出主干,没有证据,但是如果 blabla,有些火山至少intermittently活跃,完全重复这个意思的只有C,A 后半句的比较错,那句话事实上是条件;B同样因为比较排除;D强调的点与原文相反。

托福TPO25阅读Passage1原文文本+题目+答案解析

托福TPO25阅读Passage1原文文本+题目+答案解析

为了帮助大家高效备考托福,为大家带来托福TPO25阅读Passage1原文文本+题目+答案解析,希望对大家备考有所帮助。

▉托福TPO25阅读Passage1原文文本: The Surface of Mars The surface of Mars shows a wide range of geologic features,including huge volcanoes-the largest known in the solar system-and extensive impact cratering.Three very large volcanoes are found on the Tharsis bulge,an enormous geologic area near Mars’s equator.Northwest of Tharsis is the largest volcano of all:Olympus Mons,with a height of 25 kilometers and measuring some 700 kilometers in diameter at its base.The three large volcanoes on the Tharsis bulge are a little smaller-a “mere”18 kilometers high. None of these volcanoes was formed as a result of collisions between plates of the Martian crust-there is no plate motion on Mars.Instead,they are shield volcanoes-volcanoes with broad,sloping slides formed by molten rock.All four show distinctive lava channels and other flow features similar to those found on shield volcanoes on Earth.Images of the Martian surface reveal many hundreds of volcanoes.Most of the largest volcanoes are associated with the Tharsis bulge,but many smaller ones are found in the northern plains. The great height of Martian volcanoes is a direct consequence of the planet’s low surface gravity.As lava flows and spreads to form a shield volcano,the volcano’s eventual height depends on the new mountain’s ability to support its own weight.The lower the gravity,the lesser the weight and the greater the height of the mountain.It is no accident that Maxwell Mons on Venus and the Hawaiian shield volcanoes on Earth rise to about the same height(about 10 kilometers)above their respective bases-Earth and Venus have similar surface gravity.Mars’s surface gravity is only 40 percent that of Earth,so volcanoes rise roughly 2.5 times as high.Are the Martian shield volcanoes still active?Scientists have no direct evidence for recent or ongoing eruptions,but if these volcanoes were active as recently as 100 million years ago(an estimate of the time of last eruption based on the extent of impact cratering on their slopes),some of them may still be at least intermittently lions of years,though,may pass between eruptions. 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.OnMars,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. 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. 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.■ ▉托福TPO25阅读Passage1题目: Q1 The word“enormous”in the passage is closest in meaning to A.Important B.Extremely large C.Highly unusual D.Active Q2 According to paragraph 1,Olympus Mons differs from volcanoes on the Tharsis bulge in that Olympus Mons A.Has more complex geologic features B.Shows less impact cratering C.Is taller。

托福TPO25综合写作阅读原文+听力原文+满分范文

托福TPO25综合写作阅读原文+听力原文+满分范文

¡¡¡¡ÎªÁ˰ïÖú´ó¼Ò¸ßЧ±¸¿¼Íи££¬Îª´ó¼Ò´øÀ´Íи£TPO25×ÛºÏд×÷ÔĶÁÔ­ÎÄ+ÌýÁ¦Ô­ÎÄ+Âú·Ö·¶ÎÄ£¬Ï£Íû¶Ô´ó¼Ò±¸¿¼ÓÐËù°ïÖú¡£¡¡¡¡Íи£TPO25×ÛºÏд×÷ÔĶÁÔ­ÎÄÎı¾£º¡¡¡¡In 1938 an archaeologist in Iraq acquired a set of clay jars that had been excavated two years earlier by villagers constructing a railroad line. The vessel was about 2,200 years old. Each clay jay contained a copper cylinder surrounding an iron rod. The archaeologist proposed that vessel were ancient electric batteries and even demonstrated that they can produce a small electric current when filled with some liquids. However, it is not likely that the vessels were actually used as electric batteries in ancient times. First of all, if the vessels were used as batteries, they would probably have been attached to some electricity conductors such as metal wires. But there is no evidence that any metal wires were located near the vessels. All that has been excavated are the vessels themselves. Second, the copper cylinders inside the jarslook exactly like copper cylinders discovered in the ruins of Seleucia, an ancientcity located nearby. We know that the copper cylinders from Seleucia were used for holding scrolls of sacred texts, not for generating electricity. Since the cylinders found with the jars have the same shape, it is very likely they were used for holding scrolls as well. That no scrolls were found inside the jars can be explained by the fact that the scrolls simply disintegrated over the centuries. Finally, what could ancient people have done with the electricity that the vessels were supposed to have generated? They had no devices that replied on electricity. As batteries, the vessels would have been completely useless to them.¡¡¡¡Íи£TPO25×ÛºÏд×÷ÌýÁ¦Ô­ÎÄÎı¾£º¡¡¡¡Your reading says that these vessels were not used as batteries in ancient times, but the arguments used in the reading are not convincing. The battery explanation could very well be correct.First, about the absence of wires or other conductors. Remember, vessels were discovered by local people, not archaeologists. These people might have found other material located near the jars. But since they were not trained archaeologists, they may not have recognized the importance of that material. So materials serving as wires or conductors might have been overlooked as uninteresting or even thrown away. We'll never know.Second, it is true that the copper cylinders in the vessels are similar to the cylinders used to hold scrolls, but that does not really prove anything. It's possible that the copper cylinders were originally designed to preserve scrolls. And that some ancient inventor later discovered that if you use them together with iron rods and some liquid in a clay vessel, they will produce electricity. That's how the first ancient battery could have been born.In other words, the copper cylinders could have been originally used for one purpose, but then adapted for another purpose.Finally, there's the question of the possible uses of the battery in the ancient world. Well, the battery could produce a mild shock or tingling sensation when someone touched it. This could very well have beeninterpreted as evidence of some invisible power. You can easily see how people could convince others that they had magical powers through the use of the battery. Also, the battery could have been used for healing. Modern medicine uses mild electric current to stimulate muscles and relieve aches and pains. Ancient doctors may have used to batteries for the same purpose.¡¡¡¡Íи£TPO25×ÛºÏд×÷Âú·Ö·¶ÎÄ£º¡¡¡¡In the reading material, the author states that the vessels found in Iraq in 1938 were not actually used as electric batteries in ancient times. However in the listening material, the professor refutes that the first, according to the reading passage, the author suggests that if they were used as batteries, they would have been attached to some electricity conductors. However in the listening, the professor claims that we should remember that the discovery was made by local people along with some other materials. As they were not trained as archaeologist, they could not recognize the importance of some certain excavations. Perhaps they were overlook as something uninterested and then thrown away. Second, the author in the reading material mentions that the vessels were likely used for holding scrolls. Unfortunately the professor argues that it could not prove anything. It is possible that the vessels may be originally designed to scrolls. However ancient inventor then discovered that if the vessels were used with iron rod and some liquid, it could generate the electricity. So the copper cylinders may be originally used for one purpose but adapted for another purpose. Finally, the author of the reading passage asserts that the vessels would have been completely useless to ancient people as they had no devices that replied on electricity. In the contrary in obviously contradicts with the listening passage in which the professor contends that the battery could generate some mild shock and this also interprets evidence of some invisible power that how people convince others they had the magic power. Also it could be used for healing. In modern society doctors would use batteries to stimulate muscles and release pains. In ancient times people could also do that. In conclusion, according to the listening material, the argument that the vessels could not be used as batteries is unwarranted.¡¡¡¡ÒÔÉÏÊǸø´ó¼ÒÕûÀíµÄÍи£TPO25×ÛºÏд×÷ÔĶÁÔ­ÎÄ+ÌýÁ¦Ô­ÎÄ+Âú·Ö·¶ÎÄ£¬Ï£Íû¶ÔÄãÓÐËù°ïÖú!。

TPO25-Passage 1

TPO25-Passage 1

5. The word “roughly” in the passage is closest in meaning to A. typically B. frequently C. actually D. approximately
6. In paragraph 3, why does the author compare Maxwell Mons on Venus to the Hawaiian shield volcanoes on Earth? A. To help explain the relationship between surface gravity and volcano height B. To explain why Mars’s surface gravity is only 40 percent of Earth’s C. To point out differences between the surface gravity of Earth and the surface gravity of Venus D. To argue that there are more similarities than differences between volcanoes on different planets
3. According to paragraphs 1 and 2, which of the following is NOT true of the shield volcanoes on the Tharsis bulge? A. They have broad, sloping sides. B. They are smaller than the largest volcano on Mars. C. They have channels that resemble the lava channels of volcanoes on Earth. D. They are over 25 kilometers tall.

托福阅读TPO25-1 The Surface of Mars

托福阅读TPO25-1 The Surface of Mars

Tpo25The Surface of MarsThe surface of Mars shows a wide rangeof geologic features, including huge volcanoes-the largest known in the solar system-and extensive impact cratering. Three very large volcanoes are found on the Tharsis bulge, an enormousgeologic area near Mars’s equator. Northwest of Tharsis is the largest volcano of all: Olympus Mons, with a height of 25 kilometers and measuring some 700 kilometers in diameter at its base. The three large volcanoes on the Tharsis bulge are a little smaller-a “mere” 18 kilometers high.None of these volcanoes was formed as a result of collisions between platesof the Martian crust-there is no plate motion on Mars. Instead, they are shield volcanoes — volcanoes with broad, sloping slides formed by molten rock. All four show distinctivelava channels and other flow features similar to those found on shield volcanoes on Earth. Images of the Martian surface reveal many hundreds of volcanoes. Most of the largest volcanoes are associated with the Tharsis bulge, but many smaller ones are found in the northern plains.The great height of Martian volcanoes is a directconsequence of the planet’s low surface gravity. As lava flows and spreads to form a shi eld volcano, the volcano’s eventual height depends on the new mountain’s ability to support its own weight. The lower the gravity, the lesser the weight and the greater the height of the mountain. It is no accident that Maxwell Mons on Venus and the Hawaiian shield volcanoes on Earth rise to about the same height (about 10 kilometers) above their respective bases-Earth and Venus have similar surface gravity. Mars’s surface gravity is only 40 percent that of Earth, so volcanoes rise roughly2.5 times as high. Are the Martian shield volcanoes still active? Scientists have no direct evidence for recent or ongoing eruptions, but if these volcanoes were active as recently as 100 million years ago (an estimate of the time of last eruption based on the extent of impact cratering on their slopes), some of them may still be at least intermittently lions of years, though, may pass between eruptions.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 considerablyfaster 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.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) servesas an age indicator for the Martian surface. Age estimates ranging from four billion years for Mars’s southern highla nds to a few hundred million years in the youngest volcanic areas were obtained in this way.The detailed appearance of Martian impact craters provides an important piece of information aboutconditions just below the planet’s surface. Martian craters are surrounded by ejecta (debris formed as aresult of an impact) that looks quite different from its lunar counterparts. A comparison ofthe Copernicuscrater on the Moon with the (fairly typical) crater Yuty on Mars demonstrates the differences. The ejectasurrounding 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 orflowed out of crater. Geologists think that this fluidized ejecta crater indicates that a layer of permafrost, orwater ice, lies just a few meters under the surface. Explosive impacts heated and liquefied the ice, resultingin the fluid appearance of the ejecta.Paragraph 1:The surface of Mars shows a wide rangeof geologic features, including huge volcanoes-the largest known in the solar system-and extensive impact cratering. Three very large volcanoes are found on the Tharsis bulge, ant of Tharsis is the largest volcano of all: Olympus Mons, with a height of 25 kilometers and measuring some 700 kilometers in diameter at its base. The three large volcanoes on the Tharsis bulge are a little smaller-a “mere” 18 kilometers high.1. The wo○ Important○ Extremely large○ Highly unusual○ Active2. According to paragraph 1, Olympus Mons differs from volcanoes on the Tharsis bulge in that Olympus Mons○ Has more complex geologic features○ Shows less impact cratering○ Is taller○ Was formed at a later timeParagraph 2:None of these volcanoes was formed as a result of collisions between platesof the Martian crust-there is no plate motion on Mars. Instead, they are shield volcanoes-volcanoes with broad, sloping slides formed by molten rock. All four showreveal many hundreds of volcanoes. Most of the largest volcanoes are associated with the Tharsis bulge, but many smaller ones are found in the northern plains.3. meaning to○ Deep○Complex○ Characteristic○ Ancient4. According to paragraphs 1 and 2, which of the following is NOT true of the shield volcanoes on the Tharsis bulge?○ They have broad, sloping sides.○ They are smaller than the largest volcano on Mars.○ They have channels that resemble the lava channels of volcanoes on Earth.○ They are over 25 kilometers tall.Paragraph 3:The great height of Martian volcanoes is a direct consequence of the planet’s low surfacegravity. As lava flows and spreads to form a shield volcano, the volcano’s eventual height depends on thenew mountain’s ability to support its own weight. The lower the gravity, the lesser the weight and the greaterthe height of the mountain. It is no accident that Maxwell Mons on Venus and the Hawaiian shield volcanoeson Earth rise to about the same height (about 10 kilometers) above their respective bases-Earth and Venus5. n the passage is closest in meaning to○ Typically○ Frequently○ Actually○ Approximately6. In paragraph 3, why does the author compare Maxwell Mons on Venus to the Hawaiian shieldvolcanoes on Earth?○ To help explain the relationship between surface gravity and volcano height○To explain why Mars’s surface gravity is only 40 percent of Earth’s○ To point out differences between the surface gravity of Earth and the surface gravity of Venus○ To argue that there are more similarities than differences between volcanoes on different planets7. Which of the sentences below best expresses the essential information in the highlighted sentence inthe 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 wereactive as recently as 100 million years ago.○ Scientists estimate that volcanoes active more recently than 100 years ago will still have extensiveimpact cratering on their slopes.○ If, as some evidence suggests, these volcanoes erupted as recently as 100 million years ago, theymay continue to be intermittently active.○Although these volcanoes were active as recently as 100 million years ago, there is no directevidence 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-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.○ Frequently○ Significantly○ Clearly○ Surprisingly9. 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 paragraph 4, why does the author point out that Mars has few ancient craters that are less than 5 kilometers in diameter?○ To explain why scientists believe that the surface matter filling 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 the Martian atmosphere is an efficient erosive agent○ To argue that Mars experienced fewer ancient impacts than the Moon didParagraph 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) servesas 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 than 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 older than they actually are.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 ofthe 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 o f 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, resulti ng 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 crater13. 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.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 sentences 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.Drag your answer choices to the spaces where they belong. To remove an answer choice, click on it. To review the passage, click VIEW NEXT.Volcanoes and impact craters are major features of Martian geology.Answer Choices●●●○Plate motion on Mars, once considered to have played no role in shaping the planet’s surface, is now seen as being directly associated with the planet’s earliest volcanoes.○Mars has shield volcanoes, some of which are extremely tall because of the planet’s low surface gravity.○ Although the erosive power of the Martian atmosphere ensures that Mars has fewer craters than the Moon does, impact cr aters are prominent on Mars’ s surface.○Scientists cannot yet reliably estimate the age of the Martian surfacebecause there has been too much erosion of it.○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○Studies of crater ejecta have revealed the possibility of a layer of permafrost below the surface of Mars.参考答案:1.22. 33. 34. 45.46. 17. 38.29. 410. 311. 212. 313. 214. Mars has shield volcanoes, ... Although the erosive power... Studies of crater ejecta have...。

TPO25

TPO25

TPO 25 Conversation 1advisor [ædˈvaɪzɚ]n. 顾问approval [ə'pruvl]n. 同意;批准dean [din] n. 系主任;学院院长submit [səb'mɪt]v. 提交;递交elective [ɪ'lɛktɪv] n. 选修科目globalization [ˌɡləubəlai'zeiʃən]n. 全球化faculty ['fæklti] n. 全体教员seminar ['sɛmɪnɑr] n. 研讨会Lecture 1consequence ['kɑnsəkwɛns]n. 结果;后果fuel ['fjuəl]n. 燃料radical ['rædɪkl]adj. 彻底的;基本的debate [dɪ'bet]v. 争论;辩论latitude['lætɪtud]n. 纬度glacial ['ɡleʃl]adj. 冰川的swing [swɪŋ]n. 改变fragment ['fræɡmənt]v. 使破碎;分裂retreat [rɪ'trit]v. 撤退;改变slice [slaɪs]v. 切成薄片;切开prairie ['prɛri]n. 大草原quarter ['kwɔrtɚ]n. 四分之一viable [ˈvaɪəbəl]adj. 能生存的;可行的rescue ['rɛskju]n. 营救;救援proliferate[prə'lɪfə'ret] v. 繁殖invasive [ɪn'vesɪv]adj. 侵略性的;攻击性的choke [tʃok]v. 窒息;抑制hog [hɔɡ] v. 独占sugarcane [ˈʃʊɡɚˌken]n. 甘蔗plantation [plæn'teʃən]n. 种植园continent ['kɑntɪnənt]n. 大陆;洲intimate ['ɪntɪmət]adj. 亲密的fungus ['fʌŋɡəs] n. 真菌;霉菌insect ['ɪnsɛkt]n. 昆虫;虫子pollination ['pɑləneʃən] n. 授粉migration [maɪ'ɡreʃən]n. 移民ultimate ['ʌltəmət] adj. 最后的oversight ['ovɚsaɪt]n. 监管;看管permit [pɚ'mɪt]n. 许可证;执照invertebrate [ɪn'vɝtɪbret]adj. 无脊椎的pest [pɛst]n. 害虫eliminate [ɪ'lɪmɪnet]v. 消除;除去maverick ['mævərɪk]adj. 标新立异的Lecture 2religious [rɪ'lɪdʒəs]adj. 宗教的;虔诚的ceremony ['sɛrə'moni]n. 仪式;礼节ethnomusicologist ['ɛθnomjʊzɪkɑ'lɑdʒɪkəl]n. 人种音乐学notable ['notəbl]adj. 显著的;著名的folk [fok] adj. 民间的Conversation 2pattern ['pætɚn]n. 模式;图案overwhelming [ˌovɚˈhwɛlmɪŋ]adj.势不可挡的;无法抗拒的skim [skɪm]v. 掠过;撇去substantial [səb'stænʃl]adj. 大量的assignment [ə'saɪnmənt]n. 分配;任务adaptation[ˌædæp'teʃən] n. 改编;改编成的作品anatomy [ə'nætəmi]n. 分解;解剖circulatory ['sɝkjələtɔri]a dj. 循环的mammal ['mæml] n. 哺乳动物capacity [kə'pæsəti]n. 能力metabolic [ˌmɛtə'bɑlɪk]adj. 新陈代谢的kidney ['kɪdni]n. 肾Lecture 3Hieroglyph ['haɪərəɡlɪf]n. 象形文字monument ['mɑnjumənt]n. 纪念碑temple [ˈtɛmpəl]n. 寺院;庙宇abruptly [ə'brʌptli] adv. 突然地mystify['mɪstə'fai] v. 迷惑;使神秘化archaeology [ˌɑrkɪ'ɑlədʒi]n. 考古学decipher [dɪ'saɪfɚ]v. 辨认alphabet ['ælfə'bɛt]n. 字母表demotic [dɪ'mɑtɪk]adj. 通俗的elaborate [ɪ'læbəret]adj. 详尽的;复杂的mundane [mʌnˈden] adj. 世俗的;普通的administrative [əd'mɪnɪstretɪv]adj. 行政的;管理的remarkable [rɪ'mɑrkəbl]adj. 非凡的;卓越的essentially [ɪ'sɛnʃəli] adv. 本质上;本来interpret [ɪn'tɝprɪt] v. 解释;诠释attempt [ə'tɛmpt]v. 企图;尝试symbol ['sɪmbl]n. 符号;标志suspect ['sʌspɛkt] v. 怀疑;猜想phonetic [fəˈnɛtɪk] adj. 语音的pictograph ['pɪktoɡræf] n. 象形文字concept ['kɑnsɛpt] n. 观念;想法dominant ['dɑmɪnənt]adj. 主要的dismiss [dɪs'mɪs]v. 解散;屏除anomaly [ə'nɑməli] n. 异常;反常dynasty ['daɪnəsti] n. 朝代;王朝critic ['krɪtɪk]n. 评论家;批评家disprove [ˌdɪs'pruv]v. 证明... 是不对的linguistic [lɪŋ'gwɪstɪk]adj. 语言的;语言学的crack [kræk] v. 破解fluent ['fluənt]adj. 流利的;流畅的breakthrough ['brek'θrʊ]n. 突破,突破性进展confirm [kən'fɝm]v. 证实;确定Lecture 4assign [ə'saɪn]v. 分配;指定;指派hypothesis [haɪ'pɑθəsɪs]n. 假说;假设chase [tʃes]v. 奔跑;追赶pounce [paʊns]v. 猛扑;突然袭击pup [pʌp]n. 小海豹handicap['hændɪ'kæp]v. 妨碍fake [fek] adj. 假的submissive [səb'mɪsɪv]adj. 服从的;顺从的posture ['pɑstʃɚ]n. 姿势;态度flexibility[ˌflɛksə'bɪləti]n. 灵活性;弹性pretend [prɪ'tɛnd] v. 假装notion ['noʃən]n. 观念;概念persuasive [pɚ'swesɪv]adj. 有说服力的;令人信服的intensity [ɪn'tɛnsəti]n. 强度reversal [rɪ'vɝsl]n. 翻转;倒转fill out 填写look over 检查;查看Rosetta Stone 罗塞塔石碑rather than 而不是other than 除了take ... into account 考虑... 的因素cope with 处理。

托福TPO25 section1 翻译

托福TPO25 section1 翻译

TPO25 Coversation1ProfessorHi, Mark. What can I do for you?你好,Mark. 我能为你做点什么?StudentI am just filling out this approval for graduation form for the dean's office, and I don't know, I hope I will be able to graduate next semester.我正在填写要交给系主任办公室的毕业批准表格,我不知道会不会批准,希望下个学期我能够毕业。

ProfessorWell, as long as you've met the departmental requirements and you submit the form on time, you shouldn't have any problem. Make sure you include all the classes you will have taken for your degree in finance and the electives too.只要你满足院系里的毕业要求然后按时提交表格,你就应该没有问题。

请确认你把所有上过的金融专业的课都算在内还有那些选修课。

StudentYeah, but as I look over the form, I got confused because of the way, um…they've changed the requirements. So now I am not sure I will be qualified to graduate next semester. I know I would, before, under the old requirements.是的,但是看了这份表格之后,我有些困惑,因为他们改变了要求。

托福阅读TPO25(试题+答案+译文)第1篇:ThesurfaceofMars

托福阅读TPO25(试题+答案+译文)第1篇:ThesurfaceofMars

托福阅读TPO25(试题+答案+译文)第1篇:ThesurfaceofMarsTPO是我们常用的托福模考工具,对我们的备考很有价值,下面小编给大家带来托福阅读TPO25(试题+答案+译文)第1篇:The surface of Mars。

托福阅读原文【1】The surface of Mars shows a wide range of geologic features, including huge volcanoes-the largest known in the solar system-and extensive impact cratering. Three very large volcanoes are found on the Tharsis bulge, an enormous geologic area near Mars’s equator. Northwest of Tharsis is the largest volcano of all: Olympus Mons, with a height of 25 kilometers and measuring some 700 kilometers in diameter at its base. The three large volcanoes on the Tharsis bulge are a little smaller-a “mere”18 kilometers high.【2】None of these volcanoes was formed as a result of collisions between plates of the Martian crust-there is no plate motion on Mars. Instead, they are shield volcanoes — volcanoes with broad, sloping slides formed by molten rock. All four show distinctive lava channels and other flow features similar to those found on shield volcanoes on Earth. Images of the Martian surface reveal many hundreds of volcanoes. Most of the largest volcanoes are associated with the Tharsis bulge, but many smaller ones are found in the northern plains.【3】The great height of Martian volcanoes is a direct consequence of the planet’s low surface gravity. As lava flows and spreads to form a shield volcano, the volcano’s eventual height depends on the new mountain’s ability to support its own weight. The lower the gravity, the lesser the weight and thegreater the height of the mountain. It is no accident that Maxwell Mons on Venus and the Hawaiian shield volcanoes on Earth rise to about the same height (about 10 kilometers) above their respective bases-Earth and Venus have similar surface gravity. Mars’s surface gravity is only 40 percent that of Earth, so volcanoes rise roughly 2.5 times as high. Are the Martian shield volcanoes still active? Scientists have no direct evidence for recent or ongoing eruptions, but if these volcanoes were active as recently as 100 million years ago (an estimate of the time of last eruption based on the extent of impact cratering on their slopes), some of them may still be at least intermittently active. Millions of years, though, may pass between eruptions.【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.【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.【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.托福阅读试题1.The word “enormous”(paragraph 1)in the passage is closest in meaning toA.importantB.extremely largeC.highly unusualD.active2.According to paragraph 1, Olympus Mons differs from volcanoes on the Tharsis bulge in that Olympus MonsA.has more complex geologic featuresB.shows less impact crateringC.is tallerD.was formed at a later time3.The word “distinctive”(paragraph 1)in the passage is closest in meaning toA.deep.plex.C.characteristic.D.ancient.4.According to paragraphs 1 and 2, which of the following is NOT true of the shield volcanoes on the Tharsis bulge?A.They have broad, sloping sides.B.They are smaller than the largest volcano on Mars.C.They have channels that resemble the lava channels of volcanoes on Earth.D.They are over 25 kilometers tall.5.The word “roughly” in the passage is closest in meaning toA.typically.B.frequently.C.actually.D.approximately.6.In paragraph 3, why does the author compare Maxwell Mons on Venus to the Hawaiian shield volcanoes on Earth?A.To help explain the relationship between surface gravity and volcano height.B.To explain why Mars’s surface gravity is only 40 percent of Earth’s.C.To point out differences between the surface gravity of Earth and the surface gravity of Venus.D.To argue that there are more similarities than differences between volcanoes on different planets.7.Which of the sentences below best expresses the essential information in the highlighted sentence in the passage? Incorrect choices change the meaningin important ways or leave out essential information.A.Although direct evidence of recent eruptions is lacking, scientists believe that these volcanoes were active as recently as 100 million years ago.B.Scientists estimate that volcanoes active more recently than 100 years ago will still have extensive impact cratering on their slopes.C.If, as some evidence suggests, these volcanoes erupted as recently as 100 million years ago, they may continue to be intermittently active.D.Although these volcanoes were active as recently as 100 million years ago, there is no direct evidence of recent or ongoing eruptions.8.The word “considerably”(paragraph 3)in the passage is closest in meaning toA.frequently.B.significantly.C.clearly.D.surprisingly.9.According to paragraph 4, what is demonstrated by the fact that cratersfill in much faster on Mars than on the Moon?A.Erosion from meteoritic impacts takes place more quickly on Mars than on the Moon.B.There is more dust on Mars than on the Moon.C.The surface of Mars is a dry desert.D.Wind is a powerful eroding force on Mars.10.In paragraph 4, why does the author point out that Marshas few ancient craters that are less than 5 kilometers in diameter?A.To explain why scientists believe that the surface matter filling Martian craters is mostly dust.B.To explain why scientists believe that the impact craters on Mars were created by meteoroids.C.To support the claim that the Martian atmosphere is an efficient erosive agent.D.To argue that Mars experienced fewer ancient impacts than the Moon did.11.According to paragraph 5, what have scientists been able to determinefrom studies of large impact cratering on Mars?A.Some Martian volcanoes are much older than was once thought.B.The age of Mars’s surface can vary from area to area.rge impact craters are not reliable indicators of age in areas with high volcanic activity.D.Some areas of the Martian surface appear to be older than they actually are.12.According to paragraph 6, the ejecta of Mars’s crater Yuty differs fromthe ejecta of the Moon’s Copernicus crater in that the ejecta of the Yuty craterA.Has now become part of a permafrost layer.B.Contains a large volume of dust, soil and boulders.C.Suggests that liquid once came out of the surface at the crater site.D.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.Where would the sentence best fit? Click on a square to add the sentence tothe passage. This surface feature has led to speculation about what may lie under Mars’s surface.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. ■【A】However, the ejecta on Mars gives the distinct impression of a liquid that has splashed or flowed out of crater. ■【B】Geologists think that this fluidized ejecta crater indicates that a layer of permafrost, or water ice, lies just a few meters under the surface. ■【C】Explosive impacts heated and liquefied the ice, resulting in the fluid appearance of the ejecta. ■【D】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 sentences 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.Drag your answer choices to the spaces where they belong. To remove an answer choice, click on it. To review the passage, click VIEW NEXT.Volcanoes and impact craters are major features of Martiangeology.A.Plate motion on Mars, once considered to have played no role in shaping the planet’s s urface, is now seen as beingdirectly 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 there 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 MoonF.Studies of crater ejecta have revealed the possibility of a layer of permafrost below the surface of Mars.托福阅读答案1.enormous 巨大的,所以正确答案是B,extremely large。

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The Evolutionary Origin of PlantsThe evolutionary history of plants has been marked by a series of adaptations. The ancestors of plants were photosynthetic single-celled organisms that gave rise to plants presumably lacked true roots, stems, leaves, and complex reproductive structures such as flowers. All of these features appeared later in the evolutionary history of plants. Of today’s different groups of algae, green algae are probably the most similar to ancestral plants. This supposition stems from the close phylogenetic (natural evolutionary) relationship between the two groups. DNA comparisons have shown that green algae are plants’ closest living relatives. In addition, other lines of evidence support the hypothesis that land plants evolved from ancestral green algae used the same type of chlorophyll and accessory pigments in photosynthesis as do land plants. This would not be true of red and brown algae. Green algae store food as starch, as do land plants and have cell walls made of cellulose, similar in composition to those of land plants. Again, the good storage and cell wall molecules of red and brown algae are different.Today green algae live mainly in freshwater, suggesting that their early evolutionary history may have occurred in freshwater habitats. If so, the green algae would have been subjected to environmental pressures that resulted in adaptations that enhanced their potential to give rise to land-dwelling or organisms.█The environmental conditions of freshwater habitats, unlike those of ocean habitats, are highly variable. █Water temperature can fluctuate seasonally or even daily and changing level of rainfall can lead to fluctuations in the concentration of chemical in the water or even to period in which the aquatic habitat dries up. █Ancient fresh water green algae must have evolved features that enable them to withstand extremes of temperature and periods of dryness. █These adaptations served their descendant well as they invaded land.selection had shaped the adaptations that helped plants overcome the obstacles to terrestrial living, plants prospered and diversified.When plants pioneered the land, they faced a range of challenges posed by terrestrial environments. On land, the supportive buoyancy of water is missing, the plant is no longer bathed in a nutrient solution, and air tends to dry things out. These conditions favored the evolution of the structures that support the body, vessels that transport water and nutrients to all parts of plant, and structures that conserve water. The resulting adaptations to dry land include some structural features that arose early in plant evolution; now these features are common to virtually all land plant. They include roots or root like structures, a waxy cuticle that covers the surfaces of leaves and stems and limits the evaporation of water, and pores called stomata in leaves and stems that allow gas exchange but close when water is scarce, thus reducing water loss. Other adaptations occurred later in the transition to terrestrial life and now wide spread but not universal among plants. These include conducting vessels that transport water and minerals upward from the roots and that move the photosynthetic products from the leaves to the rest of the plant body and the stiffening substance lignin, which support the plant body, helping it expose maximum surface area to sunlight.These adaptations allowed an increasing diversity of plant forms to exploit dry land. Life on land, however, also required new methods of transporting sperm to eggs. Unlike aquatic and marine forms, land plants cannot always rely on water currents to carrytheir sex cells and disperse their fertilized eggs. So the most successful groups of land plants are those that evolved methods of fertilized sex cell dispersal that are independent of water and structures that protest developing embryos from drying out. Protected embryos and waterless dispersal of sex cells were achieved with the origin of seed plans and the key evolutionary innovations that they introduced: pollen, seeds, and later, flowers and fruits.Paragraph 1:1.The word “presumably” in the passage is closest inmeaning toB. supposedlyC. obviouslyD. usually2. According to paragraph 1, all of the following are true of ancestral plants EXCEPTA. They had cellulose-based cell walls.B. They were closely related to green algaeC. They were able to store nutrientsD. They had a sophisticated multicellular structure.Paragraph 2:3.The phrase “subjected to” in the passage is closest inA. restricted byB. distant fromC. exposed toD. combined withParagraph 3:4.What can be inferred from paragraph 3 about ancient green algae?A. They lived in a generally wet environment that was sometimes dayB. They adapted better to changes in water temperature than did to other changes in the environment.C. They inhabited areas that were close to the ocean.D. They had lived primarily on landParagraph 4:5. The word “desolate” in the passage is closest in meaning toA. dustyB. hardenedC. desertedD. dried out6.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.A. Terrestrial plants had the advantages of not having rivals and having easy access to photosynthetic materialB. The abundance of photosynthetic material made life on land easier for pioneering plantsC. Once plants had eliminated their competitors and their predators, their evolutionary process proceeded smoothly.D. Plant evolution eliminated competitors and made the process of photosynthesis more efficient.7. According to paragraph 4, which of the following is true about the terrestrial world at the time it was colonized by plants?A. it was exposed to high levels of solar radiationB. it contained a limited supply of carbon dioxideC. it had developed 400million years earlierD. it lacked the presence of any organismsParagraph 5:8. the word “posed” in the passage is closest in meaning toA. sharedB. presentedC. strengthened9. According to paragraph 5, all of the following are problems that early terrestrial plants had to overcome ExceptA. a tendency to become dryB. the inability to limit surface sunlightC. the absence of a structure to support the body of the plantD. the inability to transport water and minerals through the plant10. What purpose does paragraph 5 serve in the larger discussion of the origins of terrestrial plants?A. To emphasize how long it took for ancestral plants to adjust to life on landB. To disprove the argument that land plants adapted easily to their new terrestrial environmentC. To explain how plant colonization changed the physical environment of the terrestrial worldD. To describe how ancestral plants solved the problems they confirmed in colonizingParagraph 6:11. According to Paragraph 6, The adaptation made by terrestrial plants had which of the follow ing effect?’A. Plants developed reproductive strategies usable in both land and water environmentB. the plant diversity achieved in water environments diminished on landC. seed plants became the dominant species among plantsD. a greater range of plants was able to develop12. Which of the following best describes the author’s presentation of the information about land plantsA. the author provided and overview of the evolutionary relationships between specific species of algae and land plantsB. The author discusses the transformation plants underwent in the process of changing from an aquatic to a terrestrial environmentC. the author establishes a pattern of similarity between major land and water pant groupsD. The author resents evidence to support the hypothesis that plants first fully evolved in water before finding their way to land13. Look at the four squares [█] that indicate where the following sentence could be added to the passage.Scientists believe that chemical changes and a thicker exterior, among other things, may have helped ancient algae overcome the conditions in their environment.Where would the sentence best fit? Click on a square to add the sentence to the passage.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 sentences 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.In moving from water to land, ancestral plants overcame many obstacles in order to survive.Answer Choice:A. Neither brown nor red algae are likely to be ancestors of plants because of their difference in pigmentationB. The instability of freshwater habitats caused marine algae to develop adaptations to their harsh environment.C. The colonization of land by plants was a major revolution in the history of Earth.D. Terrestrial plants adjusted to life on land by undergoing structural changes that enabled them to support themselves, resist drying, and exchange gases.E. To colonize new terrestrial habitats, plants needed to create a way of reproducing without water.F. Once plants had overcome the challenges posed by terrestrial life, they prospered by becoming less diverse.。

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