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[原始] 叁号,叁战,七百四~机经加心得~

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11#
发表于 2010-11-3 22:55:23 | 只看该作者
祝福LZ!希望明天能顺利!
12#
 楼主| 发表于 2010-11-3 23:49:18 | 只看该作者
算谓语?
sisters 是复数 要做sisters谓语也得复数了。。
那应该是主句的谓语吧。那后头。。providing...
-- by 会员 cutewen (2010/11/3 22:37:17)



前面biography才是主语吧。。。
13#
 楼主| 发表于 2010-11-3 23:50:16 | 只看该作者
一上来就看到LZ这篇
我今天超级无比的沮丧,因为GWD总是超时10分钟,都好多套了,做得还很赶。
想问一下,实战和GWD比,哪个更纠结一点?
-- by 会员 zoukan (2010/11/3 22:46:18)



今天是我考的最高的一次,但是也是我觉得最容易的一次
不知道为啥,可能心态问题吧,昨天的模考帮了大忙~
14#
发表于 2010-11-4 00:52:34 | 只看该作者
LZ遇到的暗物质应该是这篇吧:
V1
密度跟行星差不多,但是是太阳的1/10 占宇宙重量的90%  balabala
第二段讲观测,说传统方法很难观测到,天文爱好者观测 dark物质通过他们和发亮的星星之间是时产生的一种类似于日食(及光亮度下降)的现象,定义现象A
第三段讲观测到的A明显比预计的要多,说他们的观测方法需要改进,而且在改进之前他们并不愿意公开他们的研究结果、
问题1. 天文爱好者为什么对dark物质感兴趣  我选的:因为可以dark物质account for宇宙的大部分质量
问题2. 为什么要改进观测方法
    我选的:因为他们不知道现在overestimated多少
15#
发表于 2010-11-4 00:55:10 | 只看该作者
OG11上面有一篇非常相近的,麻烦LZ确认一下:
After evidence was obtained in the 1920’s that the universe is expanding, it became reasonable to ask: will the universe continue to expand indefinitely, or is there enough mass in it for the mutual attraction of its constituents to bring this expansion to a halt? It can be calculated that the critical density of matter needed to brake the expansion and “close” the universe is equivalent to three hydrogen atoms per cubic meter. But the density of the observable universe—luminous matter in the form of galaxies—comes to only a fraction of this. If the expansion of the universe is to stop, there must be enough invisible matter in the universe to exceed the luminous matter in density by a factor of roughly 70.
Our contribution to the search for this “missing matter” has been to study the rotational velocity of galaxies at various distances from their center of rotation. It has been known for some time that outside the bright nucleus of a typical spiral galaxy luminosity falls off rapidly with distance from the center. If luminosity were a true indicator of mass, most of the mass would be concentrated toward the center. Outside the nucleus the rotational velocity would decrease geometrically with distance from the center, in conformity with Kepler’s law. Instead we have found that the rotational velocity in spiral galaxies either remains constant with increasing distance from the center or increases slightly. This unexpected result indicates that the falloff in luminous mass with distance from the center is balanced by an increase in nonluminous mass.
Our findings suggest that as much as 90 percent of the mass of the universe is not radiating at any wavelength with enough intensity to be detected on the Earth. Such dark matter could be in the form of extremely dim stars of low mass, of large planets like Jupiter, or of black holes, either small or massive. While it has not yet been determined whether this mass is sufficient to “close” the universe, some physicists consider it significant that estimates are converging on the critical value.
16#
 楼主| 发表于 2010-11-4 01:05:43 | 只看该作者
LZ遇到的暗物质应该是这篇吧:
V1
密度跟行星差不多,但是是太阳的1/10 占宇宙重量的90%  balabala
第二段讲观测,说传统方法很难观测到,天文爱好者观测 dark物质通过他们和发亮的星星之间是时产生的一种类似于日食(及光亮度下降)的现象,定义现象A
第三段讲观测到的A明显比预计的要多,说他们的观测方法需要改进,而且在改进之前他们并不愿意公开他们的研究结果、
问题1. 天文爱好者为什么对dark物质感兴趣  我选的:因为可以dark物质account for宇宙的大部分质量
问题2. 为什么要改进观测方法
    我选的:因为他们不知道现在overestimated多少
-- by 会员 XYXB (2010/11/4 0:52:34)



是的。。。
但是感觉问题不是我遇到的题目。。。

而且楼上不是原文~~
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