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翻译人员: Yuchen Lu
校对人员: Lipeng Chen
00:06
We know about our universe’s past:
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我们了解宇宙的过往:
00:09
the Big Bang theory predicts that all
matter, time, and space
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大爆炸原理预测了
所有的物质、时间和空间
00:14
began in an incredibly tiny, compact
state about 14 billion years ago.
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都始于140亿年前的极小极紧密的状态。
00:20
And we know about the present:
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我们了解宇宙的当下,
00:22
scientists’ observations of the movement
of galaxies
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科学家们对于银河运动的观察
00:25
tell us that the universe is expanding
at an accelerated rate.
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告诉我们宇宙正在加速扩张。
00:30
But what about the future?
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但是未来呢?
00:31
Do we know how our universe
is going to end?
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我们知道我们的宇宙将会如何终结吗?
00:35
Cosmologists have three
possible answers for this question,
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宇宙学家们关于这个问题有三种可能的回答:
00:38
called the Big Freeze,
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大冻结、
00:40
the Big Rip and the Big Crunch.
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大撕裂和大挤压。
00:43
To understand these three scenarios,
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为了理解这三种设想,
00:46
imagine two objects representing galaxies.
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请想象一下两个物体代表银河。
00:49
A short, tight rubber band is
holding them together—
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一根橡皮筋将它们定在一起——
00:53
that’s the attractive force of gravity.
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这就是引力。
00:56
Meanwhile, two hooks are
pulling them apart—
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同时,两个钩子将它们分开——
00:59
that’s the repulsive force
expanding the universe.
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这就是扩展宇宙的斥力。
01:03
Copy this system over and over again,
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如果这个系统复制下去,
01:06
and you have something
approximating the real universe.
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你就会得到一个近似宇宙的模型。
01:09
The outcome of the battle between
these two opposing forces
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这一对相反作用力的结果
01:13
determines how the end of the
universe will play out.
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决定了宇宙的尽头在哪里。
01:16
The Big Freeze scenario is what happens
if the force pulling the objects apart
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大冻结学说指的是
01:22
is just strong enough to stretch the
rubber band until it loses its elasticity.
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这个拉力刚好大到让皮筋失去弹力。
01:27
The expansion wouldn’t be able to
accelerate anymore,
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这样,宇宙的扩张就不会再加速,
01:30
but the universe would keep
getting bigger.
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但宇宙还是会继续变大。
01:33
Clusters of galaxies would separate.
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银河系会散开。
01:36
The objects within the galaxies–
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银河系中的物体——
01:38
suns, planets, and solar systems
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恒星、行星和星系
01:41
would move away from each other,
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会远离彼此,
01:42
until galaxies dissolved into
lonely objects
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直到银河系彻底分解,
01:45
floating separately in the vast space.
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漂浮在广阔的宇宙中。
01:48
The light they emit would be redshifted
to long wavelengths
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它们发出的光会被红移成长波,
01:51
with very low, faint energies,
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所含的能量很少,很模糊。
01:54
and the gas emanating from them
would be too thin to create new stars.
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它们放出的气体太薄,
无法让人看见星星。
01:59
The universe would become
darker and colder,
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宇宙会变得黑暗寒冷,
02:02
approaching a frozen state
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趋近于冰冻的状态,
02:03
also known as the Big Chill,
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这也叫做宇宙大寒,
02:05
or the Heat Death of the Universe.
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或者热寂。
02:08
But what if the repulsive force
is so strong
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但如果这对斥力非常强大呢?
02:11
that it stretches the rubber band
past its elastic limit,
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大到使皮筋超出弹力极限,
02:15
and actually tears it?
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然后拉断。
02:16
If the expansion of the universe
continues to accelerate,
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如果宇宙的扩张继续加速,
02:19
it will eventually overcome not only
the gravitational force –
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这个拉力最终不仅会克服重力影响——
02:23
tearing apart galaxies and solar systems–
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导致银河系和太阳系分离——
02:26
but also the electromagnetic, weak,
and strong nuclear forces
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还会克服强核力和弱核力,
02:30
which hold atoms and nuclei together.
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这两种力是保持原子和核子的。
02:33
As a result,
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其结果是,
02:34
the matter that makes up stars
breaks into tiny pieces.
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形成星球的物质会变成细小的碎片。
02:38
Even atoms and subatomic particles
will be destroyed.
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甚至于原子和亚原子颗粒都会被摧毁。
02:42
That’s the Big Rip.
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这就是大撕裂。
02:44
What about the third scenario,
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那第三种情况呢?
02:46
where the rubber band wins out?
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如果是皮筋比较有力量会怎么样?
02:48
That corresponds to a possible future
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这就对应了一个未来
可能会出现的情况——
02:51
in which the force of gravity brings the
universe’s expansion to a halt—
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重力让宇宙的扩张停止,
02:55
and then reverses it.
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然后往回收。
02:58
Galaxies would start rushing
towards each other,
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星系会开始互相靠拢。
03:01
and as they clumped together
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在它们凝结在一起的同时,
03:02
their gravitational pull would
get even stronger.
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它们的重力会变得更加强大。
03:06
Stars too would hurtle
together and collide.
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星球也会互相猛烈碰撞。
03:09
Temperatures would rise as space
would get tighter and tighter.
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温度会随着宇宙变小而升高。
03:13
The size of the universe would plummet
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宇宙会骤然变小,
03:15
until everything compressed into such
a small space
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直到所有东西都压缩成一个小空间。
03:19
that even atoms and subatomic particles
would have to crunch together.
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甚至原子和亚原子都会被压碎。
03:24
The result would be an incredibly dense,
hot, compact universe —
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宇宙最终会变得稠密,异常得热和紧密,
03:29
a lot like the state that
preceded the Big Bang.
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这与大爆炸之前的状态很相似。
03:32
This is the Big Crunch.
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这就是大挤压。
03:35
Could this tiny point of matter explode
in another Big Bang?
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这个点上的物质会不会又一次大爆炸?
03:39
Could the universe expand and contract
over and over again,
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宇宙会不会重复地扩张和收缩,
03:43
repeating its entire history?
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重演整段历史呢?
03:45
The theory describing such a universe
is known as the Big Bounce.
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描述上述现象的原理叫作大反弹。
03:50
In fact, there’s no way to tell how many
bounces could’ve already happened—
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事实上,我们不知道宇宙
已经经过了几次反弹,
03:54
or how many might happen in the future.
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或者将来会发生几次。
03:57
Each bounce would wipe away any record
of the universe’s previous history.
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每一次反弹都会清除宇宙之前的所有历史。
04:03
Which one of those scenarios
will be the real one?
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这些情况中哪一个是真实的?
04:06
The answer depends on the exact shape
of the universe,
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答案取决于宇宙的准确形状,
04:09
the amount of dark energy it holds,
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它含有的暗物质的数量,
04:11
and changes in its expansion rate.
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和它扩张率的变化。
04:14
As of now, our observations suggest
that we’re heading for a Big Freeze.
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到现在为止,我们的观察显示
我们正往大冻结的方向前进。
04:18
But the good news is that we’ve probably
got about 10 to the 100th power years
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但好消息是还要过十的一百次方年,
04:24
before the chill sets in —
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寒冷才会降临。
04:26
so don’t start stocking up
on mittens just yet.
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所以,先别急着囤手套。
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