托福黄金阅读12.3版本：火星上的流水

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　　Photographic evidence suggests that liquid water once existed in great quantity on the surface of Mars. Two types of flow features are seen: runoff channels and outflow channels. Runoff channels are found in the southern highlands. These flow features are extensive systems—sometimes hundreds of kilometers in total length—of interconnecting, twisting channels that seem to merge into larger, wider channels. They bear a strong resemblance to river systems on Earth, and geologists think that they are dried-up beds of long-gone rivers that once carried rainfall on Mars from the mountains down into the valleys. Runoff channels on Mars speak of a time 4 billion years ago (the age of the Martian highlands), when the atmosphere was thicker, the surface warmer, and liquid water widespread.

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　　Outflow channels are probably relics of catastrophic flooding on Mars long ago. They appear only in equatorial regions and generally do not form extensive interconnected networks. Instead, they are probably the paths taken by huge volumes of water draining from the southern highlands into the northern plains. The onrushing water arising from these flash floods likely also formed the odd teardrop-shaped “islands” (resembling the miniature versions seen in the wet sand of our beaches at low tide) that have been found on the plains close to the ends of the outflow channels. Judging from the width and depth of the channels, the flow rates must have been truly enormous—perhaps as much as a hundred times greater than the 105 tons per second carried by the great Amazon river. Flooding shaped the outflow channels approximately 3 billion years ago, about the same times as the northern volcanic plains formed.

　　Some scientists speculate that Mars may have enjoyed an extended early Period during which rivers, lakes, and perhaps even oceans adorned its surface. A 2003 Mars Global Surveyor image shows what mission specialists think may be a delta—a fan-shaped network of channels and sediments where a river once flowed into a larger body of water, in this case a lake filling a crater in the southern highlands. Other researchers go even further, suggesting that the data provide evidence for large open expenses of water on the early Martian surface. A computer-generated view of the Martian north polar region shows the extent of what may have been an ancient ocean covering much of the northern lowlands. The Hellas Basin, which measures some 3,000 kilometers across and has a floor that lies nearly 9 kilometers below the basin’s rim, is another candidate for an ancient Martian sea.

　　These ideas remain controversial. Proponents point to features such as the terraced “beaches” shown in one image, which could conceivably have been left behind as a lake or ocean evaporated and the shoreline receded. But detractors maintain that the terraces could also have been created by geological activity, perhaps related to the geologic forces that depressed the Northern Hemisphere far below the level of the south, in which case they have nothing whatever to do with Martian water. Furthermore, Mars Global Surveyor data released in 2003 seem to indicate that the Martian surface contains too few carbonate rock layers—layers containing compounds of carbon and oxygen—that should have been formed in abundance in an ancient ocean. Their absence supports the picture of a cold, dry Mars that never experienced the extended mild period required to form lakes and oceans. However, more recent data imply that at least some parts of the planet did in fact experience long periods in the past during which liquid water existed on the surface.

　　Aside from some small-scale gullies (channels) found since 2000, which are inconclusive, astronomers have no direct evidence for liquid water anywhere on the surface of Mars today, and the amount of water vapor in the Martian atmosphere is tiny. Yet even setting aside the unproven hints of ancient oceans, the extent of the outflow channels suggests that a huge total volume of water existed on Mars in the past. Where did all the water go? The answer may be that virtually all the water on Mars is now locked in the permafrost layer under the surface, with more contained in the planet’s polar caps.

　　Paragraph 1: Photographic evidence suggests that liquid water once existed in great quantity on the surface of Mars. Two types of flow features are seen: runoff channels and outflow channels. Runoff channels are found in the southern highlands. These flow features are extensive systems—sometimes hundreds of kilometers in total length—of interconnecting, twisting channels that seem to merge into larger, wider channels. They bear a strong resemblance to river systems on Earth, and geologists think that they are dried-up beds of long-gone rivers that once carried rainfall on Mars from the mountains down into the valleys. Runoff channels on Mars speak of a time 4 billion years ago (the age of the Martian highlands), when the atmosphere was thicker, the surface warmer, and liquid water widespread.

　　1. The word merge in the passage is closest in meaning to

　　○expand

　　○separate

　　○straighten out

　　○combine

　　2. What does the discussion in paragraph 1 of runoff channels in the southern highlands suggest about Mars?

　　○The atmosphere of Mars was once thinner than it is today.

　　○Large amounts of rain once fell on parts of Mars.

　　○The river systems of Mars were once more extensive than Earth’s.

　　○The rivers of Mars began to dry up about 4 billion years ago.

　　Paragraph 2: Outflow channels are probably relics of catastrophic flooding on Mars long ago. They appear only in equatorial regions and generally do not form extensive interconnected networks. Instead, they are probably the paths taken by huge volumes of water draining from the southern highlands into the northern plains. The onrushing water arising from these flash floods likely also formed the odd teardrop-shaped “islands” (resembling the miniature versions seen in the wet sand of our beaches at low tide) that have been found on the plains close to the ends of the outflow channels. Judging from the width and depth of the channels, the flow rates must have been truly enormous—perhaps as much as a hundred times greater than the 105 tons per second carried by the great Amazon river. Flooding shaped the outflow channels approximately 3 billion years ago, about the same times as the northern volcanic plains formed.

　　3. The word relics in the passage is closest in meaning to

　　○remains

　　○sites

　　○requirements

　　○sources

　　4. The word miniature in the passage is closest in meaning to

　　○temporary

　　○small

　　○multiple

　　○familiar

　　5. In paragraph 2, why does the author include the information that 105 tons of water flow through the Amazon river per second?

　　○To emphasize the great size of the volume of water that seems to have flowed through Mars’ outflow channels

　　○To indicate data used by scientists to estimate how long ago Mars’ outflow channels were formed

　　○To argue that flash floods on Mars may have been powerful enough to cause tear-shaped “islands” to form

　　○To argue that the force of flood waters on Mars was powerful enough to shape the northern volcanic plains

　　6. According to paragraph 2, all of the following are true of the outflow channels on Mars EXCEPT:

　　○They formed at around the same time that volcanic activity was occurring on the northern plains.

　　○They are found only on certain parts of the Martian surface.

　　○They sometimes empty onto what appear to have once been the wet sands of tidal beaches.

　　○They are thought to have carried water northward from the equatorial regions.

　　Paragraph 3: Some scientists speculate that Mars may have enjoyed an extended early Period during which rivers, lakes, and perhaps even oceans adorned its surface. A 2003 Mars Global Surveyor image shows what mission specialists think may be a delta—a fan-shaped network of channels and sediments where a river once flowed into a larger body of water, in this case a lake filling a crater in the southern highlands. Other researchers go even further, suggesting that the data provide evidence for large open expenses of water on the early Martian surface. A computer-generated view of the Martian north polar region shows the extent of what may have been an ancient ocean covering much of the northern lowlands. The Hellas Basin, which measures some 3,000 kilometers across and has a floor that lies nearly 9 kilometers below the basin’s rim, is another candidate for an ancient Martian sea.

　　7. All of the following questions about geological features on Mars are answered in paragraph 3 EXCEPT:

　　○What are some regions of Mars that may have once been covered with an ocean?

　　○Where do mission scientists believe that the river forming the delta emptied?

　　○Approximately how many craters on Mars do mission scientists believe may once have been lakes filled with water?

　　○During what period of Mars’ history do some scientists think it may have had large bodies of water?

　　8. According to paragraph 3, images of Mars’ surface have been interpreted as support for the idea that

　　○the polar regions of Mars were once more extensive than they are now

　　○a large part of the northern lowlands may once have been under water

　　○deltas were once a common feature of the Martian landscape

　　○the shape of the Hellas Basin has changed considerably over time

　　Paragraph 4: These ideas remain controversial. Proponents point to features such as the terraced “beaches” shown in one image, which could conceivably have been left behind as a lake or ocean evaporated and the shoreline receded. But detractors maintain that the terraces could also have been created by geological activity, perhaps related to the geologic forces that depressed the Northern Hemisphere far below the level of the south, in which case they have nothing whatever to do with Martian water. Furthermore, Mars Global Surveyor data released in 2003 seem to indicate that the Martian surface contains too few carbonate rock layers—layers containing compounds of carbon and oxygen―that should have been formed in abundance in an ancient ocean. Their absence supports the picture of a cold, dry Mars that never experienced the extended mild period required to form lakes and oceans. However, more recent data imply that at least some parts of the planet did in fact experience long periods in the past during which liquid water existed on the surface.

　　9. 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.

　　○But detractors argue that geological activity may be responsible for the water associated with the terraces.

　　○But detractors argue that the terraces may have been formed by geological activity rather than by the presence of water.

　　○But detractors argue that the terraces may be related to geological forces in the Northern Hemisphere of Mars, rather than to Martian water in the south.

　　○But detractors argue that geological forces depressed the Northern Hemisphere so far below the level of the south that the terraces could not have been formed by water.

　　10. According to paragraph 4, what do the 2003 Global Surveyor data suggest About Mars?

　　○Ancient oceans on Mars contained only small amounts of carbon.

　　○The climate of Mars may not have been suitable for the formation of large bodies of water.

　　○Liquid water may have existed on some parts of Mars’ surface for long periods of time.

　　○The ancient oceans that formed on Mars dried up during periods of cold, dry weather.

　　Paragraph 5: Aside from some small-scale gullies (channels) found since2000, which are inconclusive, astronomers have no direct evidence for liquid water anywhere on the surface of Mars today, and the amount of water vapor in the Martian atmosphere is tiny. Yet even setting aside the unproven hints of ancient oceans, the extent of the past. Where did all the water go? The answer may be that virtually all the water on Mars is now locked in the permafrost layer under the surface, with more contained in the planet’s polar caps.

　　11. The word hints in the passage is closest in meaning to

　　○clues

　　○features

　　○arguments

　　○effects

　　Paragraph 2: Outflow channels are probably relics of catastrophic flooding on Mars long ago. They appear only in equatorial regions and generally do not form extensive interconnected networks. Instead, they are probably the paths taken by huge volumes of water draining from the southern highlands into the northern plains. The onrushing water arising from these flash floods likely also formed the odd teardrop-shaped “islands” (resembling the miniature versions seen in the wet sand of our beaches at low tide) that have been found on the plains close to the ends of the outflow channels. Judging from the width and depth of the channels, the flow rates must have been truly enormous―perhaps as much as a hundred times greater than the 105 tons per second carried by the great Amazon river. Flooding shaped the outflow channels approximately 3 billion years ago, about the same times as the northern volcanic plains formed.

　　12. Look at the four squares that indicate where the following sentence could be added to the passage.These landscape features differ from runoff channels in a number of ways.Where would the sentence best fit?

　　13. 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 that are not presented in the passage or are minor ideas in the passage. This question is worth 2 points.

　　There is much debate concerning whether Mars once had water.

　　Answer choices

　　○Mars’ runoff and outflow channels are large-scale, distinctive features that suggest that large quantities of liquid water once flowed on Mars.

　　○Although some researchers claim that Mars may once have had oceans, others dispute this, pointing to an absence of evidence or offering alternative interpretations of evidence.

　　○Various types of images have been used to demonstrate that most of Martian surface contains evidence of flowing water.

　　○The runoff and outflow channels of Mars apparently carried a higher volume of water and formed more extensive networks than do Earth’s river systems.

　　○There is very little evidence of liquid water on Mars today, and it is assumed that all the water that once existed on the planet is frozen beneath its surface.

　　○While numerous gullies have been discovered on Mars since 2000, many astronomers dismiss them as evidence that Mars once had liquid water.

　　参考答案：

　　1. ○4

　　2. ○2

　　3. ○1

　　4. ○2

　　5. ○1

　　6. ○3

　　7. ○3

　　8.○2

　　9. ○2

　　10. ○2

　　11. ○1

　　12. ○1

　　13. ○1, 2, 5

　　参考译文

　　刘文勇ibt黄金阅读12.3版本：火星上的流水

　　来自照片的证据显示在火星的表面曾有过大量的液态水。两种流动形式已经被发现：径流通道和外流通道。 径流通道发现于南部的高地。这些流动形式有着庞大的系统——有时竟有数百千米长——他们相互交错，扭转， 并可能汇入更大更宽的通道中。它们和地球上的河流系统非常相似，地质学家们认为它们是以前曾将火星上的雨 水从高山携带到峡谷中的那些河流干涸后的遗迹。火星上的径流通道存在于4 百万年以前(就是火星高地的年龄)， 那时候火星的大气层更厚，地表更暖和，并且液态水分布很广。

　　外流通道可能是很久以前火星上洪灾的遗迹。它们只形成于赤道附近，并一般没有形成广泛的交错的网络。 相反，它们可能是携带大量水从南部高地到北部平原的排水系统。由泛滥的洪水而产生的激流可能也形成奇怪的 泪滴状小岛(就像是在低潮时湿沙地或海滩上看到的缩小版本一样)，已经在靠近出流通道末尾处的平原上被看 到。从这些通道的宽度和深度可判断，当时流速一定很大——有可能是亚马逊河的每秒钟105 吨的流量的一百多 倍。大约在三百万年以前，北部火山平原形成的同时，洪水改变了外流通道的形状。

　　一些科学家认为早期的火星上广泛存在着河流，湖泊甚至是海洋。一份2003 年的对火星全球的调查照片显 示了一个科学家们认为是三角洲的构造——一个扇形的沉积物和水流通道的网络，河流可能是从这里流入了一个 更大的水体;在这种情况下，它可能是南部高地的一个火山口湖泊。其他研究者做了更大胆的猜测，他们认为那 些数据表明早期在火星表面存在大量的水。一张关于火星北部极地地区的电脑图片说明有可能有一个古老的海洋 覆盖了大部分北部的低洼处。那座有大约3000 公里宽，9 公里深的Hellas 盆地也可能是火星海洋。

　　这些观点仍然有争议。支持者们指出照片里显示的台地“海滩”可以是由湖泊或者海洋蒸发干涸之后或者海 退之后形成的。但是反对者认为这些台地也可能是由于地质活动造成的，即由于北半球的地质压力要远比南半球 的小得多而造成的，在这种情况下，他们就和火星水系没有任何关系。而且，2003 发布的火星全球调查数据也表 明火星表面含有太少的碳化岩层——含有碳氧化合物的岩层——他们应该是在古代海洋中大量形成的。这些岩层 的缺失支持了火星是一个又冷又干燥的星球这一说法，并且不可能拥有形成湖泊和海洋的温和气候。然而，更多 的数据现在表明至少该星球上的一些部分表面的确在过去的很长时间内存在液态水。

　　除了在2000 年发现了一些小规模的、不确定的溪谷以外，宇航员到目前为止还没有在星球的什么地方找到 液态水存在的直接证据。而且火星大气中的水蒸气的含量也是微乎其微的。然而就算不考虑尚未证明的古代海洋 存在的观点，出流通道的广泛存在就足以证明在火星上曾有大量的水体，水都去了哪里呢?答案可能是火星上所 有的水实际上现在已经封存在其地下的永久冻层中，并且在极地地区最多。

　　以上就是新东方在线为大家总结的托福黄金阅读12.3版本：火星上的流水的相关内容，最后预祝大家在托福考试中取得优异的成绩!

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