How quantum mechanics explains global warming - Lieven Scheire

530,536 views ・ 2014-07-17

TED-Ed


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翻译人员: Xiangyu Zheng 校对人员: Shan Liu
00:06
You've probably heard that
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你可能听说过
00:07
carbon dioxide is warming the Earth,
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二氧化碳正在让地球变暖
00:10
but how does it work?
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但这是什么原理呢?
00:11
Is it like the glass of a greenhouse
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二氧化碳像是温室的玻璃?
00:13
or like an insulating blanket?
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或者像是隔热的毛毯?
00:15
Well, not entirely.
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其实不全是这样。
00:17
The answer involves a bit
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答案关系到一些
00:19
of quantum mechanics, but don't worry,
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量子力学的知识,但是不用担心
00:22
we'll start with a rainbow.
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让我们从彩虹说起
00:23
If you look closely at sunlight separated
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如果你透过三棱镜
00:25
through a prism,
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仔细观察被分散的阳光
00:27
you'll see dark gaps where bands of color went missing.
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你会看到光谱中有一些暗掉的缺口 一部分颜色的波段消失了
00:30
Where did they go?
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它们去哪里了?
00:31
Before reaching our eyes,
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在到达我们的眼睛之前
00:33
different gases absorbed those
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很多气体就已经吸收掉
00:35
specific parts of the spectrum.
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波谱中特定的一些频段
00:37
For example, oxygen gas snatched up
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例如,氧气夺走了
00:39
some of the dark red light,
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一些深红色光线
00:41
and sodium grabbed two bands of yellow.
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钠夺取了黄色的两个波段
00:44
But why do these gases absorb
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但为什么这些气体会
00:46
specific colors of light?
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吸收特定颜色的光呢?
00:48
This is where we enter the quantum realm.
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我们现在就要进入量子学领域了
00:51
Every atom and molecule has a set number
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每个原子和分子都有
00:53
of possible energy levels for its electrons.
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一定数量的电子能量等级
00:56
To shift its electrons from the ground state
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使电子从基态
00:58
to a higher level,
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跃迁到一个更高的能级
01:00
a molecule needs to gain a certain amount of energy.
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分子需要获得一个特定量的能量
01:03
No more, no less.
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不能多,也不能少
01:06
It gets that energy from light,
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分子从光线中获得这种能量
01:08
which comes in more energy levels than you could count.
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光线里含有数不胜数的能量层级
01:11
Light consists of tiny particles called photons
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光由被称为“光子”的微小粒子组成
01:14
and the amount of energy in each photon
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每个光子里储存的能量
01:16
corresponds to its color.
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与其颜色对应
01:19
Red light has lower energy and longer wavelengths.
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红色光线能量较低,波长较长
01:22
Purple light has higher energy and shorter wavelengths.
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紫色光线能量较高,波长较短
01:25
Sunlight offers all the photons of the rainbow,
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阳光提供了彩虹里所有颜色的光子
01:28
so a gas molecule can choose
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所以一个气体分子可以选择
01:30
the photons that carry the exact amount of energy
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带有它们所需的特定能量值的光子
01:33
needed to shift the molecule to
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用以把分子提升到
01:35
its next energy level.
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下一个能级
01:37
When this match is made,
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匹配上之后
01:38
the photon disappers as the molecule
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光子将消失,因为分子
01:40
gains its energy,
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获取了它的能量
01:41
and we get a small gap in our rainbow.
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从而造成了光谱里的缺口
01:44
If a photon carries too much or too little energy,
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如果一个光子携带的能量太多或太少
01:47
the molecule has no choice but
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分子就只好
01:49
to let it fly past.
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让它飞过
01:51
This is why glass is transparent.
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这就是玻璃透明的原因
01:53
The atoms in glass do not pair well
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玻璃里的原子
01:55
with any of the energy levels in visible light,
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和可见光里的波段不匹配
01:58
so the photons pass through.
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所以这些光子全部直接通过
02:00
So, which photons does carbon dioxide prefer?
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那么,二氧化碳选择吸收哪些光子呢?
02:03
Where is the black line in our rainbow
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彩虹光谱中的哪一条黑线
02:05
that explains global warming?
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能解释全球变暖呢?
02:07
Well, it's not there.
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其实,不在那儿
02:09
Carbon dioxide doesn't absorb light directly
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二氧化碳不直接从阳光中
02:11
from the Sun.
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吸收光线
02:13
It absorbs light from a totally
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它吸收的光线来自一个
02:14
different celestial body.
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完全不同的天体
02:16
One that doesn't appear to be emitting light at all:
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一个看起来根本不发光的天体:
02:19
Earth.
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地球
02:20
If you're wondering why our planet
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如果你在想为什么我们的星球
02:22
doesn't seem to be glowing,
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看起来不发光
02:23
it's because the Earth doesn't emit visible light.
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那是因为地球不发射可见光
02:27
It emits infared light.
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它发射的是红外光
02:29
The light that our eyes can see,
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我们眼睛能看得见的光
02:30
including all of the colors of the rainbow,
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包括彩虹里的所有颜色
02:32
is just a small part of the larger spectrum
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都只是电磁辐射大光谱里的
02:35
of electromagnetic radiation,
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一小部分
02:37
which includes radio waves, microwaves,
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大光谱里有无线电波,微波
02:40
infrared, ultraviolet, x-rays,
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红外线,紫外线,X射线
02:43
and gamma rays.
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和伽马射线
02:45
It may seem strange to think of these things as light,
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把这些都当成是光线可能有点奇怪
02:47
but there is no fundamental difference
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但是可见光和电磁射线之间
02:49
between visible light and other electromagnetic radiation.
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没有根本的区别
02:53
It's the same energy,
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它们都是能量
02:54
but at a higher or lower level.
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只不过在能级上有高低之分
02:56
In fact, it's a bit presumptuous to define
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其实,我们用自身的局限来定义“可见光”
02:58
the term visible light by our own limitations.
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是有点自大的
03:01
After all, infrared light is visible to snakes,
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毕竟,蛇类看得见红外线
03:04
and ultraviolet light is visible to birds.
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鸟类看得见紫外线
03:07
If our eyes were adapted to see light of
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如果我们的眼睛能看见1900兆赫的光线
03:09
1900 megahertz, then a mobile phone
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那么一个移动电话
03:12
would be a flashlight,
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将会变成手电
03:13
and a cell phone tower
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而一个手机信号塔
03:14
would look like a huge lantern.
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将看起来像个大灯笼
03:17
Earth emits infrared radiation
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地球发出红外射线
03:19
because every object with a temperature
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因为每个温度在绝对零度之上的物体
03:21
above absolute zero will emit light.
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都会发出光线
03:24
This is called thermal radiation.
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这被称作“热辐射”
03:26
The hotter an object gets,
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一个物体越热
03:28
the higher frequency the light it emits.
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它发出的光线频率越高
03:30
When you heat a piece of iron,
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当你加热铁的时候
03:32
it will emit more and more frequencies of infrared light,
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它将会发出越来越高频率的红外光
03:35
and then, at a temperature of around 450 degrees Celsius,
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然后,当温度达到450摄氏度时
03:40
its light will reach the visible spectrum.
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它发出的光将达到可见光范围
03:43
At first, it will look red hot.
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刚开始,它看起来是赤热的红色
03:45
And with even more heat,
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得到更多热量时
03:46
it will glow white
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它发的光将变白
03:48
with all of the frequencies of visible light.
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发出可见光波段里所有的光
03:51
This is how traditional light bulbs
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这是传统灯泡的
03:52
were designed to work
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设计原理
03:54
and why they're so wasteful.
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也是为什么它们如此浪费能源
03:56
95% of the light they emit is invisible to our eyes.
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它们发出的光中95%都是我们眼睛看不见的光
04:00
It's wasted as heat.
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它以热量的形式浪费掉了
04:02
Earth's infrared radiation would escape to space
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如果我们的大气层中
04:04
if there weren't greenhouse gas molecules
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没有温室气体分子的话
04:07
in our atmophere.
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地球的红外射线会逃到太空中
04:09
Just as oxygen gas prefers the dark red photons,
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就像氧气偏爱深红色光子一样
04:11
carbon dioxide and other greenhouse gases
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二氧化碳和其它温室气体
04:14
match with infrared photons.
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和红外线光子匹配
04:17
They provide the right amount of energy
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它们提供了正好合适的能量
04:18
to shift the gas molecules into their higher energy level.
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用来使气体分子升到它们更高一层的能级
04:22
Shortly after a carbon dioxide molecule
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当一个二氧化碳分子
04:24
absorbs an infrared photon,
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吸收了红外光子之后
04:26
it will fall back to its previous energy level,
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不久它便会回到之前的能级
04:29
and spit a photon back out in a random direction.
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并分离出一个光子,以随机的方向射出
04:32
Some of that energy then returns
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这些能量的一部分
04:34
to Earth's surface,
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就返回了地球表面
04:36
causing warming.
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导致变暖
04:37
The more carbon dioxide in the atmosphere,
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大气层里的二氧化碳越多
04:39
the more likely that infrared photons
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红外光子反回到地球表面的
04:41
will land back on Earth
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可能性就越大
04:43
and change our climate.
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使我们的气候随之改变
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