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譯者: Aaron Shoo
審譯者: Adrienne Lin
00:06
You've probably heard that
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你可能有聽說,
00:07
carbon dioxide is warming the Earth,
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二氧化碳正在暖化地球。
00:10
but how does it work?
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但是怎麼做到的呢?
00:11
Is it like the glass of a greenhouse
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它們是像溫室的玻璃,
00:13
or like an insulating blanket?
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還是像隔熱毯?
00:15
Well, not entirely.
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嗯,也不全然是。
00:17
The answer involves a bit
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實際情況涉及一點點「量子力學」。
00:19
of quantum mechanics, but don't worry,
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不過別緊張,
00:22
we'll start with a rainbow.
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讓我們先從彩虹開始。
00:23
If you look closely at sunlight separated
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如果仔細看太陽光
被三稜鏡折射出的光譜,
00:25
through a prism,
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你會看見色塊之間,
有黑色的間隔。
00:27
you'll see dark gaps where bands of color went missing.
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00:30
Where did they go?
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那些顏色跑去哪了?
00:31
Before reaching our eyes,
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在色光進入我們的眼睛前,
00:33
different gases absorbed those
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空氣中的氣體分子
就把特定的色光吸收了。
00:35
specific parts of the spectrum.
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00:37
For example, oxygen gas snatched up
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比如說,
氧氣會把暗紅光吃掉;
00:39
some of the dark red light,
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00:41
and sodium grabbed two bands of yellow.
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鈉會吸掉一部分黃光。
00:44
But why do these gases absorb
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可是為什麼氣體要吸收色光呢?
00:46
specific colors of light?
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00:48
This is where we enter the quantum realm.
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這就要靠量子力學解釋了。
00:51
Every atom and molecule has a set number
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每個原子或分子,
都有固定的「能階」,
00:53
of possible energy levels for its electrons.
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容納一定的電子。
00:56
To shift its electrons from the ground state
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「基態」時的電子要從低能階
00:58
to a higher level,
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「躍遷」到高能階時,
01:00
a molecule needs to gain a certain amount of energy.
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分子必須要吸收特定的能量。
01:03
No more, no less.
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不能太多也不能太少。
01:06
It gets that energy from light,
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它從光獲取能量,
01:08
which comes in more energy levels than you could count.
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這些能量可以帶來
你意想不到的能階改變。
01:11
Light consists of tiny particles called photons
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光中攜帶稱為「光子」的粒子,
01:14
and the amount of energy in each photon
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不同色光的光子帶有不同能量。
01:16
corresponds to its color.
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紅光的能量低、波長長,
01:19
Red light has lower energy and longer wavelengths.
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01:22
Purple light has higher energy and shorter wavelengths.
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紫光能量高、波長短。
01:25
Sunlight offers all the photons of the rainbow,
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陽光包含了所有色光的光子,
01:28
so a gas molecule can choose
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所以氣體可以自由選擇,
01:30
the photons that carry the exact amount of energy
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分子要躍遷到更高能階時
01:33
needed to shift the molecule to
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所需的光子和能量。
01:35
its next energy level.
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01:37
When this match is made,
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當光子的能量被分子吸收,
01:38
the photon disappers as the molecule
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光子就會消失,
01:40
gains its energy,
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01:41
and we get a small gap in our rainbow.
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我們就只看得到色塊間的黑線。
01:44
If a photon carries too much or too little energy,
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如果光子攜帶太多或太少的能量,
01:47
the molecule has no choice but
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分子就會放過它、隨它去。
01:49
to let it fly past.
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所以玻璃是透明的,
01:51
This is why glass is transparent.
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01:53
The atoms in glass do not pair well
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因為玻璃裡的原子在可見光中,
01:55
with any of the energy levels in visible light,
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老找不到適合的光子,
01:58
so the photons pass through.
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只好讓它們都通過。
02:00
So, which photons does carbon dioxide prefer?
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那二氧化碳喜歡哪種光子呢?
02:03
Where is the black line in our rainbow
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彩虹光譜中的哪條黑線,
02:05
that explains global warming?
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代表全球暖化的進行呢?
02:07
Well, it's not there.
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嗯,一條也不是。
02:09
Carbon dioxide doesn't absorb light directly
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因為二氧化碳不從日光
直接吸收光子,
02:11
from the Sun.
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而是吸收另一個天體的光,
02:13
It absorbs light from a totally
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02:14
different celestial body.
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一個不太算是發光天體的星球:
02:16
One that doesn't appear to be emitting light at all:
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02:19
Earth.
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地球。
02:20
If you're wondering why our planet
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可曾想過為什麼
02:22
doesn't seem to be glowing,
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地球不像恆星閃閃發光?
02:23
it's because the Earth doesn't emit visible light.
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那是因為地球不發出可見光,
只射出紅外線。
02:27
It emits infared light.
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02:29
The light that our eyes can see,
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我們肉眼可見的光,
02:30
including all of the colors of the rainbow,
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包括彩虹中的所有色光,
02:32
is just a small part of the larger spectrum
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只是廣大「電磁輻射」
02:35
of electromagnetic radiation,
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光譜中的一小部分。
02:37
which includes radio waves, microwaves,
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另外還有無線電波、微波、
02:40
infrared, ultraviolet, x-rays,
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紅外線、紫外線、X光和伽瑪射線。
02:43
and gamma rays.
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你可能覺得這些不是光,
02:45
It may seem strange to think of these things as light,
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02:47
but there is no fundamental difference
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但它們本質上並沒有不同;
02:49
between visible light and other electromagnetic radiation.
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可見光和其他電磁輻射,
同為能量的一種,
02:53
It's the same energy,
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差別只在能量高低。
02:54
but at a higher or lower level.
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02:56
In fact, it's a bit presumptuous to define
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再說,
用人類的眼光去定義
可見光也有失公允。
02:58
the term visible light by our own limitations.
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03:01
After all, infrared light is visible to snakes,
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因為蛇其實看得見紅外線,
03:04
and ultraviolet light is visible to birds.
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鳥類也看得到紫外線。
03:07
If our eyes were adapted to see light of
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如果我們的眼睛
能看見1900兆赫的光,
03:09
1900 megahertz, then a mobile phone
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那手機就會像一支支手電筒,
03:12
would be a flashlight,
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03:13
and a cell phone tower
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基地台就會像大燈籠。
03:14
would look like a huge lantern.
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03:17
Earth emits infrared radiation
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地球發出紅外線,
03:19
because every object with a temperature
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因為任何有溫度的物體
都會「發光」,
03:21
above absolute zero will emit light.
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03:24
This is called thermal radiation.
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就是所謂的「熱輻射」。
03:26
The hotter an object gets,
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當物體的溫度越高,
03:28
the higher frequency the light it emits.
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發出的光頻率就越高。
03:30
When you heat a piece of iron,
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當你燒熱一塊鐵,
03:32
it will emit more and more frequencies of infrared light,
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它會發出越來越高頻的紅外線。
03:35
and then, at a temperature of around 450 degrees Celsius,
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當溫度達攝氏450度左右,
03:40
its light will reach the visible spectrum.
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就會轉變為可見光。
一開始我們會看到燒得通紅,
03:43
At first, it will look red hot.
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03:45
And with even more heat,
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當溫度持續上升,
03:46
it will glow white
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開始發出白光,
03:48
with all of the frequencies of visible light.
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也就是所有的可見光。
這就是傳統燈泡的原理,
03:51
This is how traditional light bulbs
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03:52
were designed to work
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03:54
and why they're so wasteful.
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而且很耗能的原因。
03:56
95% of the light they emit is invisible to our eyes.
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發出95%以上的光
是我們肉眼不可見的,
04:00
It's wasted as heat.
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只會一直散發熱能。
04:02
Earth's infrared radiation would escape to space
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如果大氣中沒有溫室氣體,
04:04
if there weren't greenhouse gas molecules
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地球的紅外線就會跑到宇宙。
04:07
in our atmophere.
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就像氧氣喜歡暗紅光,
04:09
Just as oxygen gas prefers the dark red photons,
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04:11
carbon dioxide and other greenhouse gases
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二氧化碳和其他溫室氣體
04:14
match with infrared photons.
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會和紅外線的光子結合。
它們提供剛剛好的能量
04:17
They provide the right amount of energy
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04:18
to shift the gas molecules into their higher energy level.
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讓氣體分子轉換到更高能階。
04:22
Shortly after a carbon dioxide molecule
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當二氧化碳分子吸收紅外線光子,
04:24
absorbs an infrared photon,
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04:26
it will fall back to its previous energy level,
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它會降回原來的能階,
04:29
and spit a photon back out in a random direction.
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再往隨機方向丟出一顆光子。
04:32
Some of that energy then returns
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部分的能量又會回到地球,
04:34
to Earth's surface,
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造成暖化。
04:36
causing warming.
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04:37
The more carbon dioxide in the atmosphere,
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大氣中的二氧化碳越多,
04:39
the more likely that infrared photons
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紅外線光子就越會被留在地球,
04:41
will land back on Earth
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04:43
and change our climate.
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並改變我們的氣候。
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