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Imagine the disc of our galaxy1, if you just took a disc of stars and put it there, gravity would tend to make this disc collapse/ into itself and it would immediately just fall together. That is not what we see with the galaxy.
What’s actually going on is the stars are orbiting around the center and that is what keeps them from falling in, in much the same way that the Earth is orbiting around the Sun.
The planets in our solar system are in a delicate balance between gravity pulling them towards the Sun and their orbital velocity2 wanting to pull them outwards3 into space.
To keep in balance, planets / further from the Sun must orbit more slowly. If you go to / more distant planets at the edge of the solar system, they are going around the Sun much more slowly than the Earth is, and that’s because / the gravity is weaker. The same holds true for stars in the Milky4 Way. All of them are orbiting / the center of the galaxy. But the stars in the outer arm should be travelling more slowly then those closer to the galaxy’s heart.
What’s interesting, that is not what’s going on. The stars in the outer parts of the galaxy are spinning around just as quickly as those in the inner parts. And they are not the only ones, it’s not just our galaxy, it is every galaxy we look at. Every galaxy we look at seems to be spinning too fast in its outer part. These speeding stars should be flying out of the galaxy altogether. But they are not. That is a puzzle. This means that there is a lot more mass there that we just can’t see.
It’s this mass that must produce the gravity that hold these stars in their orbits. But when astronomers5 look for the mass, there appears to be nothing there. It’s led cosmologists like John Premark to an astounding6 conclusion.
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1 galaxy | |
n.星系;银河系;一群(杰出或著名的人物) | |
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2 velocity | |
n.速度,速率 | |
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3 outwards | |
adj.外面的,公开的,向外的;adv.向外;n.外形 | |
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4 milky | |
adj.牛奶的,多奶的;乳白色的 | |
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5 astronomers | |
n.天文学者,天文学家( astronomer的名词复数 ) | |
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6 astounding | |
adj.使人震惊的vt.使震惊,使大吃一惊astound的现在分词) | |
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