托福阅读事实信息题是阅读考试中比较常见的一种题型，tpo则是托福阅读备考最权威的材料，所以托福小编综合二者，为大家集中整理了tpo阅读中考察的事实信息题及其对应的解析，供大家参考使用。本文带来的是TPO25-1的事实信息题，一起来看看吧。
TPO25-1The Surface of Mars
Paragraph 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.
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
D.was formed at a later time
解题：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。
【2】这些火山都不是因火星表面的板块碰撞而形成的——火星上并无板块运动。这些火山其实是盾状火山——一种由熔岩形成的斜面宽阔并且坡度平缓的火山。上述4座火山都具有非常明显的熔岩隧道以及其他流动特征，这与地球上的盾状火山相似。火星表面的图像显示那里存在成百上千的火山。那些最大的火山中的大部分都与塔尔西斯隆起有关，但是很多稍小的火山都分布在北部平原地区。
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-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.
9. 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.
解题：以craters fill in much faster on Mars than on the Moon 定位至最后一句，说Martian atmosphere是erosive 的，风搬运尘土并擦掉撞击留下的痕迹，所以正确答案是D。
【4】火星表面的另一个突出特征是陨石坑。水手计划中的宇宙飞船发现在火星表面布满来自太空的流星撞击表面形成的陨石坑，火星的两颗卫星也是如此。与我们的月球类似，那些较小的陨石坑经常被一些物质填满(主要是灰尘)，这表明火星是一个干燥的沙漠世界。然而，与月球相比，火星上的陨石坑被填满的速度明显要快很多。在月球上，那些直径不足100米(对应深度大约在20米)的古老陨石坑主要因流星冲击而形成的尘埃的缘故而被填平了。而在火星上，只有相当少的一部分陨石坑直径小于5千米。火星大气是一种强效的腐蚀剂，加之火星上的风把灰尘从一个地方卷到另一个地方，较之仅仅是因流星冲击而形成的尘埃的作用，(火星上的)地表特征被消除得更快。
Paragraph 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.
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.
解题：B细节题，studies of large impact cratering on Mars 定位至首句，说是age indicator，但遗憾的是，凭这句只能排除 C，所以这道题只能读完这段，还好不长，答案在第二句，说南部和火山地区的不一样，也就是B说的不同地方age不同。
【5】与在我们的月球上相同，那些巨大陨石坑的范围(例如，那些巨大到自形成后尚未被尘埃填满的陨石坑)充当着火星表面年龄指示器的角色。从火星南部高地的40亿年至最年轻的火山地区的几千万年都是用同样的方法估算的。
paragraph 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.
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 crater
解题：C以Yuty做关键词定位至三五两句，第五句说火星的是液体，所以正确答案是C，第四句说月亮的ejecta是dust，soil and boulders，但问题问的是火星，所以答案不是B。
【6】火星表面陨石坑的具体外貌为揭示该行星表面状况提供了非常重要的信息。火星陨石坑周边布满了喷出物(因撞击而形成的碎片)，这与月球上的陨石坑看起来非常不同。对比月球上的哥白尼陨石坑与火星上(相当典型的)尤蒂陨石坑可以看出不同。月球上陨石坑周边的喷出物正如我们以为的那样，一场爆炸喷出的大量的灰尘、土壤和岩石。然而，火星(上的陨石坑周边的)喷出物则因飞溅而出或溢出的液体给人留下了深刻的印象。地质学家认为这种具有流体化喷出物的陨石坑指示了在火星地表下几米处存在永冻土层或水冰。爆炸性的撞击加热并液化了这些冰，结果导致这些喷出物呈现流体状的特征。
以上就是托福阅读TPO25-1中的事实信息题及其解析，大家可以在备考的时候参考复习，希望能够帮助大家的考前准备。最后前程百利祝大家都能取得理想的托福考试成绩。
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