How quantum mechanics explains global warming - Lieven Scheire

530,536 views ใƒป 2014-07-17

TED-Ed


์•„๋ž˜ ์˜๋ฌธ์ž๋ง‰์„ ๋”๋ธ”ํด๋ฆญํ•˜์‹œ๋ฉด ์˜์ƒ์ด ์žฌ์ƒ๋ฉ๋‹ˆ๋‹ค.

๋ฒˆ์—ญ: ๋™์šฑ ์ฒœ ๊ฒ€ํ† : jimin Hyun
00:06
You've probably heard that
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๋‹น์‹ ์€ ์•„๋งˆ ๋“ค์–ด ๋ดค์„ ๊ฒƒ์ž…๋‹ˆ๋‹ค.
00:07
carbon dioxide is warming the Earth,
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์ด์‚ฐํ™”ํƒ„์†Œ๊ฐ€ ์ง€๊ตฌ๋ฅผ ์˜จ๋‚œํ•˜๊ฒŒ ํ•œ๋‹ค๋Š” ๊ฒƒ์„์š”.
00:10
but how does it work?
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ํ•˜์ง€๋งŒ ์–ด๋–ป๊ฒŒ ์ด๊ฒƒ์ด ์ผ์–ด ๋‚ ๊นŒ์š”?
00:11
Is it like the glass of a greenhouse
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์ด๊ฒƒ์ด ๋งˆ์น˜ ์˜จ์‹ค์˜ ํ’€,
00:13
or like an insulating blanket?
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๋˜๋Š” ์ฐจ๋‹จํ•˜๋Š” ๋‹ด์š” ๊ฐ™์€ ๊ฑธ๊นŒ์š”?
00:15
Well, not entirely.
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๊ธ€์Ž„์š”, ์ •ํ™•ํ•˜์ง„ ์•Š์Šต๋‹ˆ๋‹ค.
00:17
The answer involves a bit
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์ •๋‹ต์€ ์–‘์ž์—ญํ•™์„ ์กฐ๊ธˆ ํฌํ•จํ•ฉ๋‹ˆ๋‹ค.
00:19
of quantum mechanics, but don't worry,
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ํ•˜์ง€๋งŒ ๊ฑฑ์ •ํ•˜์ง€ ๋งˆ์„ธ์š”.
00:22
we'll start with a rainbow.
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์šฐ๋ฆฐ ๋ฌด์ง€๊ฐœ๋ถ€ํ„ฐ ์‹œ์ž‘ํ•  ๊ฒ๋‹ˆ๋‹ค.
00:23
If you look closely at sunlight separated
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๋‹น์‹ ์ด ๋งŒ์•ฝ ํ”„๋ฆฌ์ฆ˜์„ ํ†ตํ•ด
00:25
through a prism,
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๋ถ„๋ฆฌ๋œ ํ–‡๋น›์„ ๊ฐ€๊นŒ์ด์„œ ๋ณธ๋‹ค๋ฉด,
00:27
you'll see dark gaps where bands of color went missing.
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์ƒ‰๊น” ๋ ๊ฐ€ ์‚ฌ๋ผ์ง„ ๋ถ€๋ถ„์˜ ์–ด๋‘์šด ํ‹ˆ์„ ๋ณผ ์ˆ˜ ์žˆ์„ ๊ฒƒ์ž…๋‹ˆ๋‹ค.
00:30
Where did they go?
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๊ทธ๋“ค์€ ์–ด๋””๋กœ ๊ฐ”์„๊นŒ์š”?
00:31
Before reaching our eyes,
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์šฐ๋ฆฌ์˜ ๋ˆˆ์— ๋‹ฟ๊ธฐ ์ „์—,
00:33
different gases absorbed those
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๊ฐ๊ฐ ๋‹ค๋ฅธ ๊ฐ€์Šค๊ฐ€
00:35
specific parts of the spectrum.
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ํŠน์ •ํ•œ ๋ถ€๋ถ„์˜ ์ŠคํŽ™ํŠธ๋Ÿผ์— ํก์ˆ˜๋ฉ๋‹ˆ๋‹ค.
00:37
For example, oxygen gas snatched up
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์˜ˆ๋ฅผ ๋“ค์–ด, ์‚ฐ์†Œ๋Š”
00:39
some of the dark red light,
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์–ด๋‘์šด ๋ถ‰์€ ๋น›์„ ๋„๊ณ ,
00:41
and sodium grabbed two bands of yellow.
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๋‚˜ํŠธ๋ฅจ์€ ๋‘๊ฐœ์˜ ๋…ธ๋ž€์ƒ‰ ๋ ๋ฅผ ๋ณด์ž…๋‹ˆ๋‹ค.
00:44
But why do these gases absorb
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ํ•˜์ง€๋งŒ ์™œ ์ด๋Ÿฌํ•œ ๊ฐ€์Šค๊ฐ€
00:46
specific colors of light?
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ํŠน์ •ํ•œ ์ƒ‰๊น”์˜ ๋น›์„ ํก์ˆ˜ํ• ๊นŒ์š”?
00:48
This is where we enter the quantum realm.
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์ด๊ฒƒ์€ ์šฐ๋ฆฌ๊ฐ€ ์–‘์ž์˜ ์˜์—ญ์— ๋“ค์–ด์˜จ ๊ฒƒ์ž…๋‹ˆ๋‹ค.
00:51
Every atom and molecule has a set number
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๋ชจ๋“  ์›์ž์™€ ๋ถ„์ž๋Š” ๋ฒˆํ˜ธ๋ฅผ ๊ฐ€์ง€๊ณ  ์žˆ์Šต๋‹ˆ๋‹ค.
00:53
of possible energy levels for its electrons.
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์ „์ž์˜ ๊ฐ€๋Šฅํ•œ ์—๋„ˆ์ง€ ์ˆ˜์ค€์— ๋งž๋Š”
00:56
To shift its electrons from the ground state
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์ด๊ฒƒ์˜ ์ „์ž๋ฅผ ๊ธฐ์ €(๋‚ฎ์€ ์—๋„ˆ์ง€) ์ƒํƒœ์—์„œ
00:58
to a higher level,
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๋†’์€ ์—๋„ˆ์ง€ ์ˆ˜์ค€์œผ๋กœ ์ด๋™์‹œํ‚ค๊ธฐ ์œ„ํ•ด์„œ
01:00
a molecule needs to gain a certain amount of energy.
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๋ถ„์ž๋Š” ํŠน์ •ํ•œ ์–‘์˜ ์—๋„ˆ์ง€๋ฅผ ๋ชจ์„ ํ•„์š”๊ฐ€ ์žˆ์Šต๋‹ˆ๋‹ค.
01:03
No more, no less.
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๋” ๋งŽ์ง€๋„, ์ ์ง€๋„ ์•Š๊ฒŒ์š”.
01:06
It gets that energy from light,
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์ด๊ฒƒ์€ ๊ทธ ์—๋„ˆ์ง€๋ฅผ ๋น›์—์„œ ์–ป์Šต๋‹ˆ๋‹ค.
01:08
which comes in more energy levels than you could count.
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๋‹น์‹ ์ด ์…€์ˆ˜ ์žˆ๋Š” ์ˆ˜์ค€๋ณด๋‹ค ๋” ๋งŽ์€ ์—๋„ˆ์ง€๋ฅผ ์–ป์Šต๋‹ˆ๋‹ค.
01:11
Light consists of tiny particles called photons
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๋น›์€ ๊ด‘์ž(photons)๋ผ๊ณ  ๋ถˆ๋ฆฌ๋Š” ์ž‘์€ ์ž…์ž๋กœ ๊ตฌ์„ฑ๋˜์–ด ์žˆ์Šต๋‹ˆ๋‹ค.
01:14
and the amount of energy in each photon
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๊ทธ๋ฆฌ๊ณ  ๊ฐ๊ฐ์˜ ๊ด‘์ž ์—๋„ˆ์ง€ ์–‘์€
01:16
corresponds to its color.
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๊ทธ๊ฒƒ์˜ ์ƒ‰๊น”๊ณผ ๋“ค์–ด๋งž์Šต๋‹ˆ๋‹ค.
01:19
Red light has lower energy and longer wavelengths.
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๋ถ‰์€์ƒ‰์€ ๋‚ฎ์€ ์—๋„ˆ์ง€์™€ ๊ธด ํŒŒ์žฅ์„ ๋ณด์ด๊ณ .
01:22
Purple light has higher energy and shorter wavelengths.
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๋ณด๋ผ์ƒ‰์€ ๋†’์€ ์—๋„ˆ์ง€์™€ ์งง์€ ํŒŒ์žฅ์„ ๋ณด์ž…๋‹ˆ๋‹ค.
01:25
Sunlight offers all the photons of the rainbow,
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ํ–‡๋น›์€ ๋ฌด์ง€๊ฐœ์˜ ๋ชจ๋“  ๊ด‘์ž๋ฅผ ์ œ๊ณตํ•ฉ๋‹ˆ๋‹ค.
01:28
so a gas molecule can choose
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๊ทธ๋ž˜์„œ ๊ฐ€์Šค ๋ถ„์ž๋Š” ์„ ํƒ์„ ํ• ์ˆ˜ ์žˆ์Šต๋‹ˆ๋‹ค.
01:30
the photons that carry the exact amount of energy
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๊ทธ ๊ด‘์ž๋Š” ๋ถ„์ž๊ฐ€ ๋‹ค์Œ ์—๋„ˆ์ง€ ์ˆ˜์ค€์œผ๋กœ
01:33
needed to shift the molecule to
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์ด๋™ํ•˜๋Š”๋ฐ ํ•„์š”ํ•œ
01:35
its next energy level.
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์ •ํ™•ํ•œ ์–‘์˜ ์—๋„ˆ์ง€๋ฅผ ์šด๋ฐ˜ํ•ฉ๋‹ˆ๋‹ค.
01:37
When this match is made,
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์ด ์—ฐ๊ฒฐ์ด ๋งŒ๋“ค์–ด ์งˆ๋•Œ,
01:38
the photon disappers as the molecule
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๊ด‘์ž๋Š” ์—๋„ˆ์ง€๋ฅผ ์–ป์œผ๋ฉฐ
01:40
gains its energy,
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๋ถ„์ž๋กœ ์‚ฌ๋ผ์ง‘๋‹ˆ๋‹ค.
01:41
and we get a small gap in our rainbow.
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๊ทธ๋ฆฌ๊ณ  ๋ฌด์ง€๊ฐœ์— ์ž‘์€ ํ‹ˆ์ด ์ƒ๊น๋‹ˆ๋‹ค.
01:44
If a photon carries too much or too little energy,
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๋งŒ์•ฝ ๊ด‘์ž๊ฐ€ ๋„ˆ๋ฌด๋งŽ์€, ๋˜๋Š” ๋„ˆ๋ฌด ์ ์€ ์—๋„ˆ์ง€๋ฅผ ๊ฐ€์ ธ์™”๋‹ค๋ฉด,
01:47
the molecule has no choice but
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๋ถ„์ž๋Š” ์„ ํƒ์„ ํ•˜์ง€ ์•Š๊ณ 
01:49
to let it fly past.
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์ง€๋‚˜๊ฐ€๋„๋ก ๋‚ด๋ฒ„๋ ค ๋‘ก๋‹ˆ๋‹ค.
01:51
This is why glass is transparent.
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์ด๊ฒƒ์€ ์œ ๋ฆฌ๊ฐ€ ํˆฌ๋ช…ํ•œ ์ด์œ ์ž…๋‹ˆ๋‹ค.
01:53
The atoms in glass do not pair well
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์œ ๋ฆฌ์•ˆ์˜ ์›์ž๋Š” ๊ฐ€์‹œ๊ด‘์„ ์˜
01:55
with any of the energy levels in visible light,
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์–ด๋–ค ์—๋„ˆ์ง€ ์ค€์œ„์—๋„ ์ง์„ ์ด๋ฃจ์ง€ ์•Š์Šต๋‹ˆ๋‹ค.
01:58
so the photons pass through.
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๋”ฐ๋ผ์„œ ๊ด‘์ž๋Š” ํ†ต๊ณผํ•ฉ๋‹ˆ๋‹ค.
02:00
So, which photons does carbon dioxide prefer?
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๊ทธ๋ž˜์„œ, ์ด์‚ฐํ™”ํƒ„์†Œ์— ์ ์ ˆํ•œ ๊ด‘์ž๋Š” ๋ฌด์—‡์ผ๊นŒ์š”?
02:03
Where is the black line in our rainbow
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์ง€๊ตฌ ์˜จ๋‚œํ™”๋ฅผ ์„ค๋ช…ํ•˜๋Š”
02:05
that explains global warming?
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๋ฌด์ง€๊ฐœ์˜ ๊ฒ€์€ ์„ ์€ ์–ด๋”” ์žˆ์„๊นŒ์š”?
02:07
Well, it's not there.
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๊ธ€์Œ์š”, ๊ทธ๊ฒƒ์€ ๋ฌด์ง€๊ฐœ์— ์—†์Šต๋‹ˆ๋‹ค.
02:09
Carbon dioxide doesn't absorb light directly
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์ด์‚ฐํ™”ํƒ„์†Œ๋Š” ํƒœ์–‘์œผ๋กœ๋ถ€ํ„ฐ
02:11
from the Sun.
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์ง์ ‘ ๋น›์„ ํ ์ˆ˜ํ•˜์ง€ ์•Š์Šต๋‹ˆ๋‹ค.
02:13
It absorbs light from a totally
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์ด์‚ฐํ™”ํƒ„์†Œ๋Š” ์™„์ „ํžˆ ๋‹ค๋ฅธ ์ฒœ์ฒด๋กœ๋ถ€ํ„ฐ
02:14
different celestial body.
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๋น›์„ ํก์ˆ˜ํ•ฉ๋‹ˆ๋‹ค.
02:16
One that doesn't appear to be emitting light at all:
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ํ•˜์ง€๋งŒ ๋น›์„ ์ „ํ˜€ ๋ฐฉ์ถœ ํ•˜์ง€ ์•Š๊ณ  ๋‚˜ํƒ€๋‚˜๋Š” ๊ฒƒ์ด ์žˆ์Šต๋‹ˆ๋‹ค.
02:19
Earth.
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๊ทธ๊ฒƒ์€ ๋ฐ”๋กœ ์ง€๊ตฌ์ž…๋‹ˆ๋‹ค.
02:20
If you're wondering why our planet
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๋‹น์‹ ์€ ์™œ ์ง€๊ตฌ๊ฐ€
02:22
doesn't seem to be glowing,
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ํƒ€๋Š” ๊ฒƒ ์ฒ˜๋Ÿผ ๋ณด์ด์ง€ ์•Š๋Š”์ง€ ๊ถ๊ธˆํ•  ๊ฒƒ ์ž…๋‹ˆ๋‹ค.
02:23
it's because the Earth doesn't emit visible light.
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๊ทธ๊ฒƒ์€ ์ง€๊ตฌ๊ฐ€ ๊ฐ€์‹œ๊ด‘์„ ์„ ๋ฐฉ์ถœํ•˜์ง€ ์•Š๊ธฐ ๋•Œ๋ฌธ์ž…๋‹ˆ๋‹ค.
02:27
It emits infared light.
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์ง€๊ตฌ๋Š” ์ ์™ธ์„ ์„ ๋ฐฉ์ถœํ•ฉ๋‹ˆ๋‹ค.
02:29
The light that our eyes can see,
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๋ฌด์ง€๊ฐœ์˜ ๋ชจ๋“  ์ƒ‰์„ ํฌํ•จํ•ด์„œ
02:30
including all of the colors of the rainbow,
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์šฐ๋ฆฌ๊ฐ€ ๋ณผ์ˆ˜ ์žˆ๋Š” ๋น›์€
02:32
is just a small part of the larger spectrum
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๋ผ๋””์˜คํŒŒ, ๋งˆ์ดํฌ๋กœํŒŒ,
02:35
of electromagnetic radiation,
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์ ์™ธ์„ , ์ž์™ธ์„ ,x์„ ,
02:37
which includes radio waves, microwaves,
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๊ทธ๋ฆฌ๊ณ  ๊ฐ๋งˆ์„ ์„ ํฌํ•จํ•˜๋Š”
02:40
infrared, ultraviolet, x-rays,
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์ „์ž๊ธฐ ๋ฐฉ์‚ฌ์„ ์˜
02:43
and gamma rays.
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๊ฑฐ๋Œ€ํ•œ ์ŠคํŽ™ํŠธ๋Ÿผ์˜ ํ•œ ์ž‘์€ ๋ถ€๋ถ„์ผ ๋ฟ์ž…๋‹ˆ๋‹ค.
02:45
It may seem strange to think of these things as light,
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๊ทธ๊ฒƒ๋“ค์„ ๋น›์œผ๋กœ ์ƒ๊ฐํ•˜๋Š” ๊ฒƒ์€ ์ด์ƒํ•ด ๋ณด์ผ์ง€๋„ ๋ชจ๋ฆ…๋‹ˆ๋‹ค.
02:47
but there is no fundamental difference
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ํ•˜์ง€๋งŒ ๊ฐ€์‹œ๊ด‘์„ ๊ณผ ๋‹ค๋ฅธ ์ „์ž๊ธฐ ๋ฐฉ์‚ฌ์„ ๊ณผ๋Š”
02:49
between visible light and other electromagnetic radiation.
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๊ทผ๋ณธ์ ์ธ ์ฐจ์ด์ ์ด ์—†์Šต๋‹ˆ๋‹ค.
02:53
It's the same energy,
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๊ทธ๊ฒƒ๋“ค์€ ๊ฐ™์€ ์—๋„ˆ์ง€์ž…๋‹ˆ๋‹ค.
02:54
but at a higher or lower level.
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ํ•˜์ง€๋งŒ ๋” ๋†’๊ฑฐ๋‚˜ ๋” ๋‚ฎ์€ ๋‹จ๊ณ„์— ์กด์žฌํ•ฉ๋‹ˆ๋‹ค.
02:56
In fact, it's a bit presumptuous to define
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์‚ฌ์‹ค, ์šฐ๋ฆฌ ์ž์‹ ์˜ ํ•œ๊ณ„๋กœ ๊ฐ€์‹œ๊ด‘์„ ์˜ ์กฐ๊ฑด์„ ๊ฒฐ์ •ํ•˜๋Š” ๊ฒƒ์€
02:58
the term visible light by our own limitations.
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์•ฝ๊ฐ„ ์ฃผ์ œ๋„˜๋Š” ๊ฒƒ ์ž…๋‹ˆ๋‹ค.
03:01
After all, infrared light is visible to snakes,
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์™œ๋ƒํ•˜๋ฉด ์ ์™ธ์„ ์€ ๋ฑ€๋“ค์—๊ฒŒ ๋ณด์ผ ์ˆ˜ ์žˆ๊ณ 
03:04
and ultraviolet light is visible to birds.
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์ž์™ธ์„ ์€ ์ƒˆ๋“ค์—๊ฒŒ ๋ณด์ด๊ธฐ ๋•Œ๋ฌธ์ž…๋‹ˆ๋‹ค.
03:07
If our eyes were adapted to see light of
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๋งŒ์•ฝ ์šฐ๋ฆฌ์˜ ๋ˆˆ์ด 1900 ๋ฉ”๊ฐ€ํ—ค๋ฅด์ธ ์˜ ๋น›์œผ๋กœ ๋ณด๋Š”๋ฐ์—
03:09
1900 megahertz, then a mobile phone
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์ ์‘๋˜์–ด ์žˆ๋‹ค๋ฉด
03:12
would be a flashlight,
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์ „ํ™”๊ธฐ๋Š” ์„ฌ๊ด‘์ฒ˜๋Ÿผ ๋ณด์ผ๊ฒƒ ์ด๊ณ 
03:13
and a cell phone tower
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์ „ํ™” ๊ธฐ์ง€๊ตญ์€
03:14
would look like a huge lantern.
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ํฐ ๋žœํ„ด์ฒ˜๋Ÿผ ๋ณด์ผ๊ฒƒ ์ž…๋‹ˆ๋‹ค.
03:17
Earth emits infrared radiation
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๋ชจ๋“  ๋ฌผ์ฒด๋Š” ์ ˆ๋Œ€์˜๋„์—์„œ
03:19
because every object with a temperature
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๋น›์„ ๋ฐœ์‚ฐํ•  ๊ฒƒ์ด๊ธฐ ๋•Œ๋ฌธ์—
03:21
above absolute zero will emit light.
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์ง€๊ตฌ๋Š” ์ ์™ธ์„ ์„ ๋ฐฉ์ถœํ•  ๊ฒƒ์ž…๋‹ˆ๋‹ค.
03:24
This is called thermal radiation.
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์ด๊ฒƒ์€ ์—ด ์ ์™ธ์„ ์ด๋ผ๊ณ  ๋ถˆ๋ฆฝ๋‹ˆ๋‹ค.
03:26
The hotter an object gets,
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ํ•œ ๋ฌผ์ฒด๊ฐ€ ๋œจ๊ฑฐ์›Œ ์งˆ์ˆ˜๋ก
03:28
the higher frequency the light it emits.
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๋” ๋†’์€ ์ฃผํŒŒ์ˆ˜์˜ ๋น›์ด ๋ฐฉ์ถœ๋  ๊ฒƒ์ž…๋‹ˆ๋‹ค.
03:30
When you heat a piece of iron,
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๋‹น์‹ ์ด ์ฒ  ์กฐ๊ฐ์„ ๊ฐ€์—ดํ•˜๋ฉด ๊ฐ€์—ดํ•  ์ˆ˜๋ก
03:32
it will emit more and more frequencies of infrared light,
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๋”๋†’์€ ์ฃผํŒŒ์ˆ˜์˜ ์ ์™ธ์„ ์„ ๋ฐฉ์ถœํ•  ๊ฒƒ์ด๊ณ ,
03:35
and then, at a temperature of around 450 degrees Celsius,
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์„ญ์”จ 450๋„ ๋ถ€๊ทผ์—์„œ,
03:40
its light will reach the visible spectrum.
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๊ฐ€์‹œ๊ด‘์„ ์˜ ์ŠคํŽ™ํŠธ๋Ÿผ์— ๋„๋‹ฌํ•  ๊ฒƒ์ž…๋‹ˆ๋‹ค.
03:43
At first, it will look red hot.
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์ฒ˜์Œ์—” ๋นจ๊ฐ›๊ณ  ๋œจ๊ฒ๊ฒŒ ๋ณด์ผ ๊ฒƒ์ž…๋‹ˆ๋‹ค.
03:45
And with even more heat,
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๊ทธ๋ฆฌ๊ณ  ๋” ๋œจ๊ฒ๊ฒŒ ๊ฐ€์—ด ํ•  ์ˆ˜๋ก,
03:46
it will glow white
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๊ฐ€์‹œ๊ด‘์„ ์˜ ๋ชจ๋“  ์ฃผํŒŒ์ˆ˜๋“ค๋กœ
03:48
with all of the frequencies of visible light.
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ํ•˜์–—๊ฒŒ ๋น›๋‚  ๊ฒƒ์ž…๋‹ˆ๋‹ค.
03:51
This is how traditional light bulbs
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์ด๊ฒƒ์€ ์ „ํ†ต์ ์ธ ์ „๊ตฌ๊ฐ€
03:52
were designed to work
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์–ด๋–ป๊ฒŒ ์ž‘๋™ํ•˜๊ฒŒ ๋””์ž์ธ ๋˜์—ˆ๊ณ ,
03:54
and why they're so wasteful.
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์™œ ๊ทธ๋“ค์ด ์“ธ๋ชจ๊ฐ€ ์—†๋Š”์ง€๋ฅผ ์•Œ๋ ค์ฃผ๋Š”๊ฒƒ ์ž…๋‹ˆ๋‹ค.
03:56
95% of the light they emit is invisible to our eyes.
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๋ฐฉ์ถœ๋˜๋Š” ๋น›์˜ 95์ฒ˜์„ผํŠธ๋Š” ๋ˆˆ์— ๋ณด์ด์ง€ ์•Š์Šต๋‹ˆ๋‹ค.
04:00
It's wasted as heat.
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๊ทธ๊ฒƒ๋“ค์€ ์—ด์—๋„ˆ์ง€๋กœ ๋‚ญ๋น„๋ฉ๋‹ˆ๋‹ค.
04:02
Earth's infrared radiation would escape to space
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๋Œ€๊ธฐ์•ˆ์—์„œ,
04:04
if there weren't greenhouse gas molecules
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์˜จ์‹ค๊ฐ€์Šค์˜ ๋ถ„์ž๋“ค์ด ์—†๋‹ค๋ฉด,
04:07
in our atmophere.
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์ง€๊ตฌ์˜ ์ ์™ธ์„ ์€ ์šฐ์ฃผ๋กœ ๋ฐฉ์ถœ๋  ๊ฒƒ์ž…๋‹ˆ๋‹ค.
04:09
Just as oxygen gas prefers the dark red photons,
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๋‹จ์ง€ ์‚ฐ์†Œ๊ฐ€ ์–ด๋‘ก๊ณ  ๋ถ‰์€ ๊ด‘์ž๋ฅผ ์„ ํ˜ธํ•˜๋Š” ๊ฒƒ ์ฒ˜๋Ÿผ,
04:11
carbon dioxide and other greenhouse gases
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์ด์‚ฐํ™”ํƒ„์†Œ์™€ ๋‹ค๋ฅธ ์˜จ์‹ค๊ฐ€์Šค๋“ค์€
04:14
match with infrared photons.
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์ ์™ธ์„  ๊ด‘์ž์™€ ์—ฐ๊ฒฐ๋ฉ๋‹ˆ๋‹ค.
04:17
They provide the right amount of energy
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๊ทธ๋“ค์€ ๊ธฐ์ฒด๋ถ„์ž๋“ค์„ ๋” ๋†’์€ ์—๋„ˆ์ง€ ์ค€์œ„๋กœ ์˜ฌ๋ฆฌ๊ธฐ ์œ„ํ•ด
04:18
to shift the gas molecules into their higher energy level.
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์ ๋‹นํ•œ ์–‘์˜ ์—๋„ˆ์ง€๋ฅผ ๊ณต๊ธ‰ํ•ฉ๋‹ˆ๋‹ค.
04:22
Shortly after a carbon dioxide molecule
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์ด์‚ฐํ™” ํƒ„์†Œ ๋ถ„์ž๊ฐ€
04:24
absorbs an infrared photon,
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์ ์™ธ์„  ๊ด‘์ž๋ฅผ ํก์ˆ˜ํ•œ ์ž ์‹œ ํ›„์—,
04:26
it will fall back to its previous energy level,
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์ด์ „์˜ ์—๋„ˆ์ง€ ์ค€์œ„๋กœ ๋‹ค์‹œ ๋–จ์–ด์งˆ ๊ฒƒ์ž…๋‹ˆ๋‹ค.
04:29
and spit a photon back out in a random direction.
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๊ทธ๋ฆฌ๊ณ  ์ž„์˜์˜ ๋ฐฉํ–ฅ๋Œ€๋กœ ๊ด‘์ž๋ฅผ ๋ฑ‰์–ด๋‚ผ ๊ฒƒ์ž…๋‹ˆ๋‹ค.
04:32
Some of that energy then returns
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์ง€๊ตฌ์˜ ํ‘œ๋ฉด์œผ๋กœ ๋Œ์•„๊ฐ€๋Š”
04:34
to Earth's surface,
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๋ช‡๋ช‡ ์—๋„ˆ์ง€๋“ค์€
04:36
causing warming.
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์ง€๊ตฌ ์˜จ๋‚œํ™”๋ฅผ ์ผ์œผํ‚ต๋‹ˆ๋‹ค.
04:37
The more carbon dioxide in the atmosphere,
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๋Œ€๊ธฐ์— ๋” ๋งŽ์€ ์ด์‚ฐํ™”ํƒ„์†Œ๊ฐ€ ์žˆ์„์ˆ˜๋ก
04:39
the more likely that infrared photons
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๋” ๋งŽ์€ ์ ์™ธ์„  ๊ด‘์ž๊ฐ€ ๋“ค์–ด์™€
04:41
will land back on Earth
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์ง€๊ตฌ์— ์ •์ฐฉํ•˜์—ฌ
04:43
and change our climate.
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๊ธฐํ›„๋ฅผ ๋ฐ”๊ฟ€ ๊ฐ€๋Šฅ์„ฑ์ด ๋†’์•„์ง‘๋‹ˆ๋‹ค.
์ด ์›น์‚ฌ์ดํŠธ ์ •๋ณด

์ด ์‚ฌ์ดํŠธ๋Š” ์˜์–ด ํ•™์Šต์— ์œ ์šฉํ•œ YouTube ๋™์˜์ƒ์„ ์†Œ๊ฐœํ•ฉ๋‹ˆ๋‹ค. ์ „ ์„ธ๊ณ„ ์ตœ๊ณ ์˜ ์„ ์ƒ๋‹˜๋“ค์ด ๊ฐ€๋ฅด์น˜๋Š” ์˜์–ด ์ˆ˜์—…์„ ๋ณด๊ฒŒ ๋  ๊ฒƒ์ž…๋‹ˆ๋‹ค. ๊ฐ ๋™์˜์ƒ ํŽ˜์ด์ง€์— ํ‘œ์‹œ๋˜๋Š” ์˜์–ด ์ž๋ง‰์„ ๋”๋ธ” ํด๋ฆญํ•˜๋ฉด ๊ทธ๊ณณ์—์„œ ๋™์˜์ƒ์ด ์žฌ์ƒ๋ฉ๋‹ˆ๋‹ค. ๋น„๋””์˜ค ์žฌ์ƒ์— ๋งž์ถฐ ์ž๋ง‰์ด ์Šคํฌ๋กค๋ฉ๋‹ˆ๋‹ค. ์˜๊ฒฌ์ด๋‚˜ ์š”์ฒญ์ด ์žˆ๋Š” ๊ฒฝ์šฐ ์ด ๋ฌธ์˜ ์–‘์‹์„ ์‚ฌ์šฉํ•˜์—ฌ ๋ฌธ์˜ํ•˜์‹ญ์‹œ์˜ค.

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