What is the universe made of? - Dennis Wildfogel

宇宙由甚麼組成? - 丹尼斯.萬弗喬

500,656 views ・ 2014-02-25

TED-Ed


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譯者: Toby Wong 審譯者: Becky Ma
00:07
All the material objects around you
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你身邊一切事物
00:08
are composed of submicroscopic units
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都是由極微細的單位組成
00:10
we call molecules.
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這些單位稱為分子
00:12
And molecules in turn are composed
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而分子則由一粒一粒原子組成
00:13
of individual atoms.
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00:15
Molecules frequently break apart
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分子不斷分裂
00:16
and then form new molecules.
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然後又組成新分子
00:19
On the other hand,
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另一方面
00:20
virtually all the atoms you come in to contact with
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你一生中所接觸到的原子
00:22
through the course of your life,
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00:23
the ones in the ground beneath you,
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大地、空氣、食物
00:25
the air you breath, the food you eat,
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00:27
those that make up every living thing, including you,
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組成你和一切生物的原子
00:29
have existed for billions of years
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已存在數以億年
00:31
and were created in places very unlike our planet.
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發源地與地球非常不同
00:34
How those atoms came about is what I want to share with you.
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以下說的就是原子如何誔生
00:38
It all started 14 billion years ago
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一切源於一百四十億年前
00:39
with an event we call The Big Bang,
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發生了宇宙大爆炸
00:41
which resulted in a universe consisting of gas alone.
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產生了只有氣體的宇宙
00:44
There were no stars and no planets.
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無恆星亦無行星
00:46
The gas was made up only of atoms
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氣體只由原子組成
00:48
belonging to the simplest elements.
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那些原子屬於最簡單的元素
00:50
It was about 75 percent hydrogen
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當中75%為氫
00:52
and almost all the rest was helium.
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其餘多為氦
00:54
No elements like carbon, oxygen or nitrogen existed.
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仍未有碳、氧或氮等元素
00:57
No iron, silver or gold.
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亦無鐵、銀或金
00:59
In some places, the density of this gas was slightly higher than in others.
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氣體密度有些地方稍高
01:03
Due to gravity, those places attracted even more gas,
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因萬有引力而吸引更多氣體
01:05
which further strengthened the pull of gravity,
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引力因而更強
01:07
which then drew more gas in, and so on.
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再吸引更多氣體,循環不息
01:10
Eventually, large dense gas balls formed,
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最後形成大氣團
01:13
shrinking under their own gravity
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氣團因自身引力而萎縮
01:15
and consequently heating up on the inside.
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結果內部發熱
01:18
At some point, the core of such a ball
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氣團核心熱到若干程度
01:19
gets hot enough that nuclear fusion occurs.
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就發生核融合
01:22
Hydrogen atoms smash together to form helium,
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氫原子融合為氦
01:24
accompanied by a great release of energy,
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同時釋放巨大能量
01:27
strong enough to counteract the shrinking force of the gravity.
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大得可對抗向內拉扯的引力
01:30
When the energy pushing out from the fusion reactions
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融合所生向外推的能量
01:32
matches the gravity pulling all the gas inwards,
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足以對抗向內拉扯的引力時
01:35
an equilibrium occurs.
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就會達平衡狀態
01:37
From this a star is born.
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恆星就自此而生
01:39
Over its lifetime,
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巨大恆星一生之中
01:40
the fusion reactions in the core of a massive star
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核心的融合反應不只產生氦
01:42
will produce not only helium,
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01:44
but also carbon, oxygen, nitrogen
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亦產生週期表中各元素
01:46
and all the other elements in the periodic table up to iron.
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自碳、氧、氮至鐵止
01:50
But eventually, the core's fuel runs out,
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但核心最終將耗盡燃料
01:52
leaving it to collapse completely.
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完全崩潰
01:54
That causes an unbelievably powerful explosion
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崩潰造成巨大爆炸
01:56
we call a supernova.
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這爆炸稱為超新星爆發
01:58
Now there are two things to note
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對超新星如何產生元素
01:59
about how supernovas create elements.
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有兩點須注意
02:01
First, this explosion releases so much energy
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一, 爆炸釋放巨大能源
02:04
that fusion goes wild
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使融合能力變強
02:05
forming elements with atoms even heavier than iron
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產生較鐵更重的原子
02:08
like silver, gold and uranium.
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如銀、金及鈾
02:10
Second, all the elements that had been accumulating
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二,聚於恆星核心的所有元素
02:12
in the core of the star,
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02:14
like carbon, oxygen, nitrogen, iron,
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如碳、氧、氮、鐵
02:16
as well as all of those formed in the supernova explosion,
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和超新星爆炸所產生的所有元素
02:19
are ejected in to interstellar space
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均被排進星際空間
02:21
where they mix with the gas that's already there.
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與空間已有的氣體混合
02:24
History then repeats itself.
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然後前事重演
02:26
Gas clouds, now containing many elements
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氣團現在含多種元素
02:28
besides the original hydrogen and helium,
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不單只有氫和氦
02:31
have higher density areas
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密度較高區域
02:32
that attract more matter, and so on.
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吸引更多物質,如此類推
02:34
As before, new stars result.
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如前所述,產生新星
02:37
Our sun was born this way about 5 billion years ago.
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太陽就在五十億年前如此產生
02:40
That means that the gas it arose from
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即是說,產生太陽旳氣團
02:42
had itself been enriched with many elements
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自宇宙開始,超新星爆發時
02:44
from supernova explosions since the universe began.
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吸收過多種元素
02:47
So that's how the sun wound up with all the elements.
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所以現在太陽所有元素俱備
02:50
It's still mostly hydrogen at 71 percent,
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但氫仍佔71%
02:52
with most of the rest being helium at 27 percent.
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其餘27%為氦
02:55
But bear in mind
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但請緊記
02:56
that while the first stars were made up
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首批恆星產生時
02:57
of hydrogen and helium alone,
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只有氫和氦
02:59
the remaining elements in the periodic table
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週期表中其餘元素
03:01
make up two percent of the sun.
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只佔太陽2%
03:03
And what about Earth?
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地球又如何?
03:05
Planets form as an incidental process to star formation
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行星是恆星產生過程的副產品
03:07
out of the same gas cloud as the star itself.
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來自同一氣體
03:11
Small planets like ours don't have enough gravity
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地球等小行星
03:13
to hold on to much hydrogen or helium gas
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引力不足以捉緊氫或氦氣
03:15
since both of those are very light.
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因氫、氦均極輕
03:17
So, even though carbon, nitrogen, oxygen and so on
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雖然碳、氮、氧等元素
03:20
made up only two percent of the gas cloud from which Earth was formed,
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在產生地球的氣團中只佔2%
03:23
these heavier elements form the bulk of our planet
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這些較重的元素組成地球大部份
03:26
and everything on it.
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也組成地球各種物體一大部份
03:28
Think about this:
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試想想:
03:29
with the exception of hydrogen and some helium,
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除氫和氦外
03:31
the ground you walk on,
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你腳下大地
03:33
the air you breath, you,
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所吸空氣,還有你
03:35
everything is made of atoms
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當中的原子均來自恆星
03:36
that were created inside stars.
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03:38
When scientists first worked this out
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二十世紀前半
03:40
over the first half of the 20th Century,
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科學家有此發現時
03:42
the famous astronomer Harlow Shapley commented,
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著名太空人沙普利曾說
03:45
"We are brothers of the boulders, cousins of the clouds."
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「人與石為兄弟,與雲為表親」
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