【阅读】0925跃渡整理（1001更新，41篇原始，35篇考古）

oatmilk

jujuba808 发表于 2017-9-26 10:15
等不及了，周四考试。我整理了一下，希望大家帮忙考古

目录 一、upstream.. 2 二、水库/地下水 ...

这个是925之后，你自己根据各位构筑帖子整理的吗？还是。。。。好棒

oatmilk

谢谢整理君，速度赞

Yungll

9.28???谢谢分享～～

maggieljj

感谢~求明天上午也更新一波~

daraxi

qiuqiuyu 发表于 2017-9-26 14:20
看了好多回忆觉得就是29楼那个裤诶！

29楼怎么就看到一个笑脸啊

qiuqiuyu

daraxi 发表于 2017-9-26 17:45
29楼怎么就看到一个笑脸啊

好像他删掉了…觉得不准确？

elizabethwoo

好想知道29楼之前发的啥

momo_s

dark matter 疑似原文

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.

Chloehxttt

感谢！！！