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2012年12月2日托福阅读真题解析

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2021-02-13 17:53
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2012



12



2


日 托福阅读真题解析





阅读


1





版本


1


:宇 宙的两个理论,一个说物质会变化但总量不变,一个是会膨胀,最后说一个


遥远的恒星的 发现说明后一个理论更正确;




< /p>


版本


2


:讲的是


universe expanding


的两种理论,一个是


density


在变小。另一种是


density


不变。因为不断


new creation


补充变大 的空间,然后发现了一种


q.


它表明前一种理

< br>论更可信。





解析:





big-bang model





widely held theory of the evolution of the universe. Its essential feature is the


emergence of the universe from a state of extremely high temperature and density- the


so-called big bang that occurred at least 10,000,000,000 years ago. Although this type of


universe was proposed by Alexander Friedmann and Abbé


Georges Lema?tre in the


1920s, the modern version was developed by George Gamow and colleagues in the


1940s.





The big-bang model is based on two assumptions. The first is that Albert Einstein's


general theory of relativity correctly describes the gravitational interaction of all matter.


The second assumption, called the cosmological principle, states that an observer's view


of the universe depends neither on the direction in which he looks nor on his location. This


principle applies only to the large-scale properties of the universe, but it does imply that


the universe has no edge, so that the big-bang origin occurred not at a particular point in


space but rather throughout space at the same time. These two assumptions make it


possible to calculate the history of the cosmos after a certain epoch called the Planck time.


Scientists have yet to determine what prevailed before Planck time.





According to the big-bang model, the universe expanded rapidly from a highly


compressed primordial state, which resulted in a significant decrease in density and


temperature. Soon afterward, the dominance of matter over antimatter (as observed today)


may have been established by processes that also predict proton decay. During this stage


many types of elementary particles may have been present. After a few seconds, the


universe cooled enough to allow the formation of certain nuclei. The theory predicts that


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definite amounts of hydrogen, helium, and lithium were produced. Their abundances


agree with what is observed today. About 1,000,000 years later the universe was


sufficiently cool for atoms to form. The radiation that also filled the universe was then free


to travel through space. This remnant of the early universe is the microwave background


radiation (three degree background radiation) discovered in 1965 by Arno A. Penzias and


Robert W. Wilson.





In addition to accounting for the presence of ordinary matter and radiation, the model


predicts that the present universe should also be filled with neutrinos, fundamental


particles with no mass or electric charge. The possibility exists that other relics from the


early universe may eventually be discovered.





expanding universe





dynamic state of the extragalactic realm, the discovery of which has transformed


20th-century cosmology. The development of general relativity and its application to


cosmology by Albert Einstein, Wilhelm de Sitter, and other theoreticians, along with the


detection of extragalactic redshift (a shift to the longer wavelengths of light from galaxies


beyond the Milky Way) by VestoSlipher, led to the realization in the 1920s that all galaxies


are receding. Edwin Hubble correlated these observations in mathematical form to


provide evidence that the universe is expanding. The discovery of the 2.7 K background


radiation in 1965 by Arno A. Penzias and Robert W. Wilson is regarded as convincing


evidence that the universe originated approximately 15 billion years ago in a very dense


and hot state referred to as the big bang (seebig-bang model).





Observations so far have not succeeded in determining whether the universe is open


(of infinite extent in space) or closed (of finite extent) and whether the universe in the


future will continue to expand indefinitely or will eventually collapse back into an extremely


dense, congested state. See also cosmology.






阅读


2





版本


1


:草 原上的三种食草动物,斑马羊,还有一个


B


。他们吃草的不同的 部分。把草的各


个部分坐对比,斑马的


diet


最没营养,因为蛋白质少,题目问你斑马怎么吃饱。羊吃的最有营


养题目问你为 什么。然后讲过渡放牧,他们之间没有竞争,相处的较和谐。羊反而会


prefer



些已经被斑马吃过的草地而不是全新的草地





版本


2


:讲了非洲的一片地区有很多种大型食草的哺乳动物,斑马,羚羊和一个什么


white


的东西看上去像牛他们在吃草的时候会互补,


因为他们吃的是植物不同的地方。


其中羚羊获取得


营养 的最多,斑马的营养最少,但是斑马靠一个大的胃储存的多。





解析:



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OG


测试题非常相似,请参考


--




Feeding Habits of East African Herbivores




Buffalo, zebras, wildebeests, topi, and Thomson's gazelles live in huge groups that


together make up some 90 percent of the total weight of mammals living on the Serengeti


Plain of East Africa. They are all herbivores (plant-eating animals), and they all appear to be


living on the same diet of grasses, herbs, and small bushes. This appearance, however, is


illusory. When biologist Richard Bell and his colleagues analyzed the stomach contents of four


of the five species (they did not study buffalo), they found that each species was living on a


different part of the vegetation. The different vegetational parts differ in their food qualities:


lower down, there are succulent, nutritious leaves; higher up are the harder stems. There are


also sparsely distributed, highly nutritious fruits, and Bell found that only the Thomson's


gazelles eat much of these. The other three species differ in the proportion of lower leaves and


higher stems that they eat: zebras eat the most stem matter, wildebeests eat the most leaves,


and topi are intermediate.




How are we to understand their different feeding preferences? The answer lies in two


associated differences among the species, in their digestive systems and body sizes.


According to their digestive systems, these herbivores can be divided into two categories: the


nonruminants (such as the zebra, which has a digestive system like a horse) and the


ruminants (such as the wildebeest, topi, and gazelle, which are like the cow). Nonruminants


cannot extract much energy from the hard parts of a plant; however, this is more than made up


for by the fast speed at which food passes throughtheir guts. Thus, when there is only a short


supply of poor- quality food, the wildebeest, topi, and gazelle enjoy an advantage. They are


ruminants and have a special structure (the rumen) in their stomachs, which contains


microorganisms that can break down the hard parts of plants. Food passes only slowly through


the ruminant's gut because ruminating-digesting the hard parts-takes time. The ruminant


continually regurgitates food from its stomach back to its mouth to chew it up further (that is


what a cow is doing when


almost to a liquid can the food pass through the rumen and on through the gut. Larger particles


cannot pass through until they have been chewed down to size. Therefore, when food is in


short supply, a ruminant can last longer than a nonruminant because it can derive more


energy out of the same food. The difference can partially explain the eating habits of the


Serengeti herbivores. The zebra chooses areas where there is more low-quality food. It


migrates first to unexploited areas and chomps the abundant low-quality stems before moving


on. It is a fast-in/fast-out feeder, relying on a high output of incompletely digested food. By the


time the wildebeests (and other ruminants) arrive, the grazing and trampling of the zebras will


have worn the vegetation down. As the ruminants then set to work, they eat down to the lower,


leafier parts of the vegetation. All of this fits in with the differences in stomach contents with


which we began.


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