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OFFICIAL51 According to paragraph 2, what is one difference between Earth and Venus?

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Surface Fluids on Venus and Earth
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A fluid is a substance, such as a liquid or gas, in which the component particles (usually molecules) can move past one another. Fluids flow easily and conform to the shape of their containers. The geologic processes related to the movement of fluids on a planet's surface can completely resurface a planet many times. These processes derive their energy from the Sun and the gravitational forces of the planet itself. As these fluids interact with surface materials, they move particles about or react chemically with them to modify or produce materials. On a solid planet with a hydrosphere and an atmosphere, only a tiny fraction of the planetary mass flows as surface fluids. Yet the movements of these fluids can drastically alter a planet. Consider Venus and Earth, both terrestrial planets with atmospheres.

Venus and Earth are commonly regarded as twin planets but not identical twins. They are about the same size, are composed of roughly the same mix of materials, and may have been comparably endowed at their beginning with carbon dioxide and water. However, the twins evolved differently largely because of differences in their distance from the Sun. With a significant amount of internal heat, Venus may continue to be geologically active with volcanoes, rifting, and folding. However, it lacks any sign of a hydrologic system (water circulation and distribution): there are no streams, lakes oceans or glaciers. Space probes suggest that Venus may have started with as much water as Earth, but it was unable to keep its water in liquid form. Because Venus receives more heat from the Sun, water released from the interior evaporated and rose to the upper atmosphere where the Sun's ultraviolet rays broke the molecules apart. Much of the freed hydrogen escaped into space, and Venus lost its water. Without water, Venus became less and less like Earth and kept an atmosphere filled with carbon dioxide. The carbon dioxide acts as a blanket, creating an intense greenhouse effect and driving surface temperatures high enough to melt lead and to prohibit the formation of carbonate minerals. Volcanoes continually vented more carbon dioxide into the atmosphere. On Earth, liquid water removes carbon dioxide from the atmosphere and combines it with calcium, from rock weathering, to form carbonate sedimentary rocks. Without liquid water to remove carbon from the atmosphere, the level of carbon dioxide in the atmosphere of Venus remains high.

Like Venus, Earth is large enough to be geologically active and for its gravitational field to hold an atmosphere. Unlike Venus, it is just the right distance from the Sun so that temperature ranges allow water to exist as a liquid, a solid, and a gas. Water is thus extremely mobile and moves rapidly over the planet in a continuous hydrologic cycle. Heated by the Sun, the water moves in great cycles from the oceans to the atmosphere, over the landscape in river systems, and ultimately back to the oceans. As a result, Earth's surface has been continually changed and eroded into delicate systems of river valleys - a remarkable contrast to the surfaces of other planetary bodies where impact craters dominate. Few areas on Earth have been untouched by flowing water. As a result, river valleys are the dominant feature of its landscape. Similarly, wind action has scoured fine particles away from large areas, depositing them elsewhere as vast sand seas dominated by dunes or in sheets of loess (fine-grained soil deposits). These fluid movements are caused by gravity flow systems energized by heat from the Sun. Other geologic changes occur when the gases in the atmosphere or water react with rocks at the surface to form new chemical compounds with different properties. An important example of this process was the removal of most of Earths carbon dioxide from its atmosphere to form carbonate rocks. However, if Earth were a little closer to the Sun, its oceans would evaporate; if it were farther from the Sun, the oceans would freeze solid. Because liquid water was present, self-replicating molecules of carbon, hydrogen, and oxygen developed life early in Earth's history and have radically modified its surface, blanketing huge parts of the continents with greenery. Life thrives on this planet, and it helped create the planet's oxygen- and nitrogen-rich atmosphere and moderate temperatures.

5.According to paragraph 2, what is one difference between Earth and Venus?

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正确答案:B
题目解析:
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【题目翻译】根据第2段,地球和金星之间的一个区别是什么? A:地球大气中的水比金星少。 B:地球有水文系统,但金星没有。 C:地球的地质活动不如金星活跃。 D:地球的二氧化碳比金星多。 【判定题型】:题目问的是文章中的具体细节信息,故根据题目问法可以判断本题为事实信息题。 【关键词定位】题目问以下哪一项是地球与金星的不同之处。因为第二段整段都在描写金星与地球的不同,所以无法通过题干关键词进行定位,只能逐一来看选项 【逻辑分析】在段落内找地球和金星的不同。 【选项分析】 A选项:地球大气层所含水分比金星大气层少。但是第二段中提到金星从太阳那里接收到更多热量,内部的水分被蒸发,所以失去了水。故A选项与原文信息矛盾,错误。 B选项:地球有水文系统,而金星没有。根据关键词“hydrologic system”,定位到这句话“However, it lacks any sign of a hydrologic system (water circulation and distribution): there are no streams, lakes oceans or glaciers.”这句话提到金星上没有任何水文系统。再往下看,“Space probes suggest that Venus may have started with as much water as Earth, but it was unable to keep its water in liquid form.”这句话说一开始金星和地球一样是有水的,但是金星无法将水分以液态形式保存。我们可以从侧面得出地球上有水。故B选项符合原文,正确。 C选项:地球的地质活跃度没有金星高。第二段中确实提到金星上火山、裂陷、折叠等地质活动一直很活跃。但没有将它与地球金星比较,故比较关系不存在,C选项排除。 D选项:地球比金星有更多二氧化碳。根据第二段,我们只能知道金星的大气层“filled with carbon dioxide”,但无法知道地球和金星上二氧化碳总数谁多谁少,文中未提及比较关系,故D排除。

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