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OG12 RC117

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楼主
发表于 2012-3-14 12:52:52 | 只看该作者 回帖奖励 |倒序浏览 |阅读模式
如题,请教牛牛指点此题,不大看的懂OG解释。饿晕了,想去吃饭了···
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After evidence was obtained in the 1920s 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.(题目)



117. The authors’ suggestion 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” (lines 34–37) would be most weakened if
which of the following were discovered to be true?
(A) Spiral galaxies are less common than types of
galaxies that contain little nonluminous matter.
(B) Luminous and nonluminous matter are
composed of the same basic elements.
(C) The bright nucleus of a typical spiral galaxy also
contains some nonluminous matter.
(D) The density of the observable universe is
greater than most previous estimates have
suggested.
(E) Some galaxies do not rotate or rotate too slowly
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沙发
 楼主| 发表于 2012-3-14 12:54:03 | 只看该作者
正选选A,关于RC 中的weaken解法,还真有点摸不清头绪。请NN来解答!!!!!
板凳
发表于 2012-3-31 02:13:06 | 只看该作者
我也看了好半天,自己归纳了一下,不知道这样解释可以吗,

117题问削弱其成立的选项,我们可以看成,题干是个结论结果,那我们就削弱其前提原因,而回原文定位时我们就发现L34是说  Our findings suggest that。。。,看到suggest,以及这句话的逻辑关系,我们也可以看出,这个结论是由Our findings 来,那我们找这些发现是什么,根据段落之间的逻辑关系,我们知道第一段对于问题的提出给出作者的解释是,,,,,第二段是说明这个解释的是研究什么得来的--通过研究spiral galaxy's  luminosity and rotational velocity,===结论就是 L30-31de unexpected result,,,,就是说所以星系里,发光团减少,不发光的就增加。 从而你就会看到,文章将spiral 的特性涵盖整个星系的特性,而且文章也在L20说了typical spiral galaxy

回到做题上,为了削弱题干,就得削弱发现得到的结果,而这个结果基于对spiral 的研究,如果它不具有典型性,不包含一些星系共性,研究它的一些现象就不能推而广之整个银河系,那么结论就不正确,那么由结论推出的题干就不成立。

我觉得这个这种题还是找逻辑的上一层吧,这个文章我觉得挺难的,我的阅读很差,唉,不知道怎么克服呢,,,,愁呢,,,,,

对了本题,我要是解释的不怎么样,别见笑呢,我们都好好努力
地板
发表于 2012-4-6 20:15:41 | 只看该作者
我也看了好半天,自己归纳了一下,不知道这样解释可以吗,

117题问削弱其成立的选项,我们可以看成,题干是个结论结果,那我们就削弱其前提原因,而回原文定位时我们就发现L34是说  Our findings suggest that。。。,看到suggest,以及这句话的逻辑关系,我们也可以看出,这个结论是由Our findings 来,那我们找这些发现是什么,根据段落之间的逻辑关系,我们知道第一段对于问题的提出给出作者的解释是,,,,,第二段是说明这个解释的是研究什么得来的--通过研究spiral galaxy's  luminosity and rotational velocity,===结论就是 L30-31de unexpected result,,,,就是说所以星系里,发光团减少,不发光的就增加。 从而你就会看到,文章将spiral 的特性涵盖整个星系的特性,而且文章也在L20说了typical spiral galaxy

回到做题上,为了削弱题干,就得削弱发现得到的结果,而这个结果基于对spiral 的研究,如果它不具有典型性,不包含一些星系共性,研究它的一些现象就不能推而广之整个银河系,那么结论就不正确,那么由结论推出的题干就不成立。

我觉得这个这种题还是找逻辑的上一层吧,这个文章我觉得挺难的,我的阅读很差,唉,不知道怎么克服呢,,,,愁呢,,,,,

对了本题,我要是解释的不怎么样,别见笑呢,我们都好好努力
-- by 会员 goldlily666 (2012/3/31 2:13:06)



同意楼上~
加油!!!
5#
发表于 2012-4-7 19:50:07 | 只看该作者
解释很好,谢谢
6#
 楼主| 发表于 2012-5-4 11:48:11 | 只看该作者
我也看了好半天,自己归纳了一下,不知道这样解释可以吗,

117题问削弱其成立的选项,我们可以看成,题干是个结论结果,那我们就削弱其前提原因,而回原文定位时我们就发现L34是说  Our findings suggest that。。。,看到suggest,以及这句话的逻辑关系,我们也可以看出,这个结论是由Our findings 来,那我们找这些发现是什么,根据段落之间的逻辑关系,我们知道第一段对于问题的提出给出作者的解释是,,,,,第二段是说明这个解释的是研究什么得来的--通过研究spiral galaxy's  luminosity and rotational velocity,===结论就是 L30-31de unexpected result,,,,就是说所以星系里,发光团减少,不发光的就增加。 从而你就会看到,文章将spiral 的特性涵盖整个星系的特性,而且文章也在L20说了typical spiral galaxy

回到做题上,为了削弱题干,就得削弱发现得到的结果,而这个结果基于对spiral 的研究,如果它不具有典型性,不包含一些星系共性,研究它的一些现象就不能推而广之整个银河系,那么结论就不正确,那么由结论推出的题干就不成立。

我觉得这个这种题还是找逻辑的上一层吧,这个文章我觉得挺难的,我的阅读很差,唉,不知道怎么克服呢,,,,愁呢,,,,,

对了本题,我要是解释的不怎么样,别见笑呢,我们都好好努力
-- by 会员 goldlily666 (2012/3/31 2:13:06)



万分感谢!虽然后来好久以后重新看阅读终于懂了···直到一个多月后才看到您的回帖。果然练GMAT就是一个语言和逻辑成长的过程。
7#
 楼主| 发表于 2012-5-4 11:48:25 | 只看该作者
大家一起努力哦~!
8#
发表于 2012-5-19 10:24:21 | 只看该作者
3楼解释的这么好!太谦虚了
9#
发表于 2012-7-29 14:51:31 | 只看该作者
是我看过最清楚的解析了
10#
发表于 2013-11-6 15:25:43 | 只看该作者
goldlily666 发表于 2012-3-31 02:13
我也看了好半天,自己归纳了一下,不知道这样解释可以吗,117题问削弱其成立的选项,我们可以看成,题干是 ...

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