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        2017年10月14日托福閱讀考試小范圍預(yù)測(cè)

        字號(hào):


              趁著10月14日考試還沒(méi)來(lái)臨,好好準(zhǔn)備托福考試吧!下面是小編搜集的2017年10月14日托福閱讀考試小范圍預(yù)測(cè)的相關(guān)資訊,希望可以幫助考生度過(guò)考試的難關(guān),歡迎參考!
              2017年10月14日托福閱讀考試小范圍預(yù)測(cè)
              天文類Surface Fluids on Venus and Earth
              參考閱讀:
              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 atmosphere.
              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 remainshigh.
              ...
              Origin of the Solar System
              Comets
            文化藝術(shù)類
              The Origins of Writing
              Live Performance
              The Origins of Theater
              The Development of Printing
            地質(zhì)類
              Early Theories of Continental Drift
              Attempts at Determining Earth’s Age
              How Soil is Formed
              Earth’s Energy Cycle
              Thermal Stratification
            環(huán)境類
              The Climate of Japan
              The Role of the Ocean in Controlling Climate
            經(jīng)濟(jì)類
              Effects of the Commercial Revolution
              Seventeenth-Century European Economic Growth
            考古類
              Environmental Impact of the Anasazi
              The Collapse of the Mays
              The Chaco Phenomenon
            科學(xué)類
              The Birth of Photography
              Early American Printing Industry
            農(nóng)業(yè)類
              Agricultural Society in Eighteenth- Century British America
              Water Management in Early Agriculture
            社會(huì)類
              Population Growth in Nineteenth-Century Europe
              Hunting and the Setting of Inner Eurasia
            生物類
              Extinctions at the End of the Cretaceous
              The Cambrian Explosion
              The Extinction of the Dinosaurs
              How Animals in Rain Forests Make Themselves Heard
              Sociality in Animals
              Dinosaurs and Parental Care
              Habitat Selection
              Temperature Regulation in Marine Organisms
              Cell Theory
              Poikilotherms
              Forest Succession
              The Role of Diapause
              The Identification of the Genetic Material
              How Plants and Animals Arrived in the Hawaiian Islands
              Constraints on Natural Selection
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