The history of our world in 18 minutes | David Christian | TED

8,196,821 views ・ 2011-04-11

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譯者: K. C. Peng 審譯者: zhang haohan
首先, 一則錄影
00:16
First, a video.
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00:24
Yes, it is a scrambled egg.
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是的, 這是關於打蛋
但當你注視它
00:29
But as you look at it,
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00:30
I hope you'll begin to feel just slightly uneasy.
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我希望你們會開始
感到一絲絲的不自在
00:36
Because you may notice that what's actually happening
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因為你會注意到實際上發生的是
蛋在重新回到有序的狀態
00:40
is that the egg is unscrambling itself.
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00:42
And you'll now see the yolk and the white have separated.
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看到蛋白蛋黃分離
00:44
And now they're going to be poured back into the egg.
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接著是灌回到蛋殼之中
我們非常清楚
00:48
And we all know in our heart of hearts
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00:50
that this is not the way the universe works.
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宇宙不會是這樣運行的
00:54
A scrambled egg is mush -- tasty mush -- but it's mush.
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打散的蛋 是濃稠的
00:57
An egg is a beautiful, sophisticated thing
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蛋是美麗的 是複雜的
01:00
that can create even more sophisticated things,
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也能產生更複雜的
01:02
such as chickens.
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像是小雞
01:04
And we know in our heart of hearts
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我們也非常明白
01:06
that the universe does not travel from mush to complexity.
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宇宙不是從稠狀混亂
到複雜的運行
01:10
In fact, this gut instinct
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事實上, 本能直覺
01:12
is reflected in one of the most fundamental laws of physics,
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是反映了一些基本物理定律
01:15
the second law of thermodynamics, or the law of entropy.
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熱力學的第二定律或熵變定理
基本上是說
01:19
What that says basically
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01:20
is that the general tendency of the universe
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宇宙的一般通則
是從較有規則
01:24
is to move from order and structure
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與結構的狀態
01:27
to lack of order, lack of structure --
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演變成缺乏規律與結構的方向
也就是向 濃稠狀混亂
01:30
in fact, to mush.
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01:31
And that's why that video feels a bit strange.
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那也就是剛剛錄影片段
看起來奇怪的地方
01:35
And yet, look around us.
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同樣地
看看我們的四周
01:39
What we see around us is staggering complexity.
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到處所見
都是驚人的複雜
01:43
Eric Beinhocker estimates that in New York City alone,
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Eric Beinhocker 估計光紐約市
01:46
there are some 10 billion SKUs, or distinct commodities, being traded.
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就有近100億項物品在進行交易
01:50
That's hundreds of times as many species as there are on Earth.
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是數百倍地球所有生物
的實際數量
01:55
And they're being traded by a species of almost seven billion individuals,
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而這些交易只是由一種近
70億數量的生物物種
01:59
who are linked by trade, travel, and the Internet
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被交易 旅行 與 網路 所串聯
02:02
into a global system of stupendous complexity.
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成一全球系統
的驚人複雜性
02:07
So here's a great puzzle:
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這就是個偉大的迷惑:
宇宙中
02:10
in a universe ruled by the second law of thermodynamics,
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由熱力學的第二定律所主宰
02:14
how is it possible
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又是怎麼可能
02:16
to generate the sort of complexity I've described,
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產生剛剛所描述的複雜
02:19
the sort of complexity represented by you and me
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由你我所代表的複雜
以及這會議中心的一切呢?
02:23
and the convention center?
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答案似乎是
02:26
Well, the answer seems to be,
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02:28
the universe can create complexity,
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宇宙能創造出複雜性
02:31
but with great difficulty.
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但帶著些困難度
02:33
In pockets,
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口袋裡
02:34
there appear what my colleague, Fred Spier,
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有著我的同事, Fred Spier,
02:37
calls "Goldilocks conditions" --
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所稱的 Goldilocks (適宜)條件
02:39
not too hot, not too cold,
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既不過熱 也不過冷
02:41
just right for the creation of complexity.
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條件剛剛好 適宜創造出複雜性
02:44
And slightly more complex things appear.
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更約略複雜的事就發生了
02:46
And where you have slightly more complex things,
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有了複雜的發生
02:48
you can get slightly more complex things.
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才能有再約略複雜的事接著發生
就這樣 複雜性一步一步
02:51
And in this way, complexity builds stage by stage.
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建構起來
每一步都是神奇的
02:56
Each stage is magical
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02:58
because it creates the impression of something utterly new
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因為一切都是創建新奇的事物
一切都是無中生有
03:02
appearing almost out of nowhere in the universe.
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03:04
We refer in big history to these moments as threshold moments.
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在大歷史中 我們稱這些階段為
閥值時段
每一個閥值
03:09
And at each threshold, the going gets tougher.
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是愈來愈難
03:12
The complex things get more fragile,
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複雜的事是 更脆弱
03:15
more vulnerable;
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更易破碎
03:17
the Goldilocks conditions get more stringent,
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Goldilocks (適宜)條件是更嚴峻
03:20
and it's more difficult to create complexity.
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更困難
創建下一個複雜性
03:24
Now, we, as extremely complex creatures,
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現在呢, 身為極度複雜物種
極度需要知道這個關於
03:28
desperately need to know this story
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03:30
of how the universe creates complexity despite the second law,
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宇宙變得複雜的故事
除了是第二定律
03:34
and why complexity means vulnerability and fragility.
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以及為何複雜性
意味著脆弱性
與不穩定
03:40
And that's the story that we tell in big history.
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這些就是我們想解的大歷史
03:43
But to do it, you have do something
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為了達成它 我們必須先做些其他事
03:45
that may, at first sight, seem completely impossible.
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這事乍看之下是完全不可能的
就是你得盤查整個宇宙的歷史
03:48
You have to survey the whole history of the universe.
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03:52
So let's do it.
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所以 進行吧!
03:54
(Laughter)
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(笑聲)
03:56
Let's begin by winding the timeline back
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讓我們把時間往回撥
03:59
13.7 billion years,
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到137億年前
04:02
to the beginning of time.
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也就是時間的開始
04:12
Around us, there's nothing.
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四周是什麼也沒有
04:14
There's not even time or space.
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根本沒有時間與空間
04:18
Imagine the darkest, emptiest thing you can
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先想像能想像的最黑暗與空無的狀況
再更加無數倍的狀況
04:22
and cube it a gazillion times and that's where we are.
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那才是所處的狀態
04:25
And then suddenly,
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突然間
04:28
bang!
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砰! 一個宇宙出現 一個完整的宇宙
04:29
A universe appears, an entire universe.
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04:31
And we've crossed our first threshold.
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我們第一次越過閥值
04:33
The universe is tiny; it's smaller than an atom.
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那個宇宙是非常小 比一個原子還小
04:35
It's incredibly hot.
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卻是極度的高溫高能量
04:37
It contains everything that's in today's universe,
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它包含今日所有存在宇宙的東西
04:39
so you can imagine, it's busting.
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所以你可以想像 那是非常爆滿
04:41
And it's expanding at incredible speed.
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它開始以極快的速度膨脹
04:44
And at first, it's just a blur,
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一開始只是模糊渾沌
04:46
but very quickly distinct things begin to appear in that blur.
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但是渾沌中一些明晰的物質出現
04:49
Within the first second,
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就在第一秒內
04:51
energy itself shatters into distinct forces
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能量自己分裂出不同的作用力
04:54
including electromagnetism and gravity.
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包括電磁力與重力
能量開始做些神奇的事
04:57
And energy does something else quite magical:
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04:59
it congeals to form matter --
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它凝結成物質
有夸克就是後來組成質子等
05:03
quarks that will create protons
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有輕子就是含電子等
05:05
and leptons that include electrons.
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05:07
And all of that happens in the first second.
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這些都發生在第一秒內
05:09
Now we move forward 380,000 years.
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再往前撥快38萬年
05:14
That's twice as long as humans have been on this planet.
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是人類出現於地球上的兩倍長的時間
05:17
And now simple atoms appear of hydrogen and helium.
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現在 簡單的原子出現了
氫與氦
05:23
Now I want to pause for a moment,
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讓我暫停一下下
05:25
380,000 years after the origins of the universe,
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宇宙開始後的38萬年
05:28
because we actually know quite a lot about the universe at this stage.
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就目前為止我們
對這段宇宙歷史是知道相當多的
05:32
We know above all that it was extremely simple.
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我們也知道一切都是相當簡單的物理
05:35
It consisted of huge clouds of hydrogen and helium atoms,
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有著龐大雲霧般的
氫與氦原子
05:39
and they have no structure.
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還不成結構狀態
05:41
They're really a sort of cosmic mush.
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它們真的只是一種宇宙渾沌
05:44
But that's not completely true.
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又不完全是
05:46
Recent studies
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根據最近研究
05:48
by satellites such as the WMAP satellite
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WMAP衛星的觀測
05:51
have shown that, in fact,
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顯示背景輻射 有少許的不同
05:52
there are just tiny differences in that background.
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05:55
What you see here,
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就如此所示
05:57
the blue areas are about a thousandth of a degree cooler
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藍色區域有著相差千分之一度的冷
相較於紅色區域
06:01
than the red areas.
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只有著些許不同
06:03
These are tiny differences,
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06:04
but it was enough for the universe to move on
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卻足夠讓宇宙演化
06:06
to the next stage of building complexity.
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進入下一階段的複雜度
06:08
And this is how it works.
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就是這麼的進展
06:10
Gravity is more powerful where there's more stuff.
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重力當有更多物質聚集
作用更強
06:15
So where you get slightly denser areas,
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只要有密度分配不均的情況
重力就開始作用
06:18
gravity starts compacting clouds of hydrogen and helium atoms.
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拉近 氫和氦原子團
所以可以想像 初期的宇宙 開始分出
06:22
So we can imagine the early universe breaking up into a billion clouds.
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無數的 小雲團
06:25
And each cloud is compacted,
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每一個雲團都是緊實的
06:27
gravity gets more powerful as density increases,
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而重力又隨密度增加而增加作用
06:30
the temperature begins to rise at the center of each cloud,
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雲團核心處的溫度開始升高
然後在雲團中的核心處
06:33
and then, at the center,
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06:34
the temperature crosses the threshold temperature
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溫度越過了臨界溫度
06:37
of 10 million degrees,
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約為1000萬度
06:39
protons start to fuse,
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質子開始融合
06:41
there's a huge release of energy,
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也釋放出巨大能量
06:44
and --
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碰!
06:45
bam!
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06:46
We have our first stars.
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有了第一個恆星了
06:48
From about 200 million years after the Big Bang,
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約當自宇宙開始後的2億年
06:52
stars begin to appear all through the universe,
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恆星開始出現在宇宙四處
幾十億的星星
06:56
billions of them.
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06:57
And the universe is now significantly more interesting
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宇宙開始有趣多了
07:00
and more complex.
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也更複雜
07:03
Stars will create the Goldilocks conditions
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恆星會產生最適宜狀態
再越過兩個門階
07:06
for crossing two new thresholds.
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07:08
When very large stars die,
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當大型恆星死亡
會是極高溫狀態
07:11
they create temperatures so high
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07:13
that protons begin to fuse in all sorts of exotic combinations,
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質子開始結合成各種奇特的組合
也建構出週期表的所有元素
07:17
to form all the elements of the periodic table.
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如果 你也像我帶著一只金戒指
07:20
If, like me, you're wearing a gold ring,
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07:22
it was forged in a supernova explosion.
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它被超新星爆炸所偽造
07:25
So now the universe is chemically more complex.
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所以 現在的宇宙就化學的觀點是更複雜的
就化學上複雜的宇宙
07:29
And in a chemically more complex universe,
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07:31
it's possible to make more things.
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具備製造更多事物的條件
07:33
And what starts happening is that, around young suns,
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接著發生的是
在一些年輕的恆星中
07:37
young stars,
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年輕的星球
07:39
all these elements combine, they swirl around,
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所有元素結合 環旋
07:41
the energy of the star stirs them around,
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星球的能量 擾動它們
形成粒子 形成雪片
07:44
they form particles, they form snowflakes, they form little dust motes,
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形成小小的沙塵
形成岩石 形成小行星
07:49
they form rocks, they form asteroids,
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最後形成行星與衛星
07:51
and eventually, they form planets and moons.
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07:53
And that is how our solar system was formed,
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這也就是我們太陽系統的形成
07:56
four and a half billion years ago.
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約是45億年前
岩石建構的行星 如地球
08:00
Rocky planets like our Earth are significantly more complex than stars
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會比其他星球 更複雜
08:05
because they contain a much greater diversity of materials.
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因為有著更多元的的物質
08:08
So we've crossed a fourth threshold of complexity.
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我們也就越過複雜度 第四階的門檻
08:12
Now, the going gets tougher.
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愈來愈困難了
08:16
The next stage introduces entities that are significantly more fragile,
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下個階段的複雜 是個體
更脆弱
08:20
significantly more vulnerable,
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更容易受傷
08:22
but they're also much more creative
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卻也更有創造性
08:25
and much more capable of generating further complexity.
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更能產生更多的複雜度
08:28
I'm talking, of course, about living organisms.
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這裡說的 當然就是
有生命的實體
08:32
Living organisms are created by chemistry.
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生物體都是由化學變化產生
08:34
We are huge packages of chemicals.
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我們就是一大包的化學物集合體
08:38
So, chemistry is dominated by the electromagnetic force.
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而化學主要是靠電磁作用力
08:41
That operates over smaller scales than gravity,
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作用距離比重力作用的小很多
08:43
which explains why you and I are smaller than stars or planets.
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也解釋了為何你和我
比星球是小很多很多
又是怎樣的理想化學狀態呢?
08:48
Now, what are the ideal conditions for chemistry?
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08:50
What are the Goldilocks conditions?
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也就是所謂的最適條件?
08:52
Well, first, you need energy,
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首先, 需要能源
但又不能過多
08:55
but not too much.
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08:56
In the center of a star, there's so much energy
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星球的中心能量是高的
08:58
that any atoms that combine will just get busted apart again.
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任何結合的原子 又都會再爆開
又不能太少的能量
09:02
But not too little.
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09:03
In intergalactic space,
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星河之間的太空 就是太少的能量
09:04
there's so little energy that atoms can't combine.
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原子無法結合一起
09:08
What you want is just the right amount,
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所需的就是適當的能量
09:10
and planets, it turns out, are just right,
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行星 就剛剛好有著適當能量
09:12
because they're close to stars, but not too close.
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因為它們是接近恆星 又不是過近
09:15
You also need a great diversity of chemical elements,
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也同時需要多種化學元素
也需要一些液體 像水
09:19
and you need liquids, such as water.
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為什麼?
09:22
Why?
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09:23
Well, in gases, atoms move past each other so fast
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因為在氣相態 原子與原子的移動過於快速
很難結合
09:27
that they can't hitch up.
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09:28
In solids,
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固相態
09:30
atoms are stuck together, they can't move.
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又因連在一起 無法移動
09:33
In liquids,
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液相態呢
09:35
they can cruise and cuddle
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允許四處遊蕩與集結
連結成各種分子
09:38
and link up to form molecules.
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那到哪裡找到如此的 最適狀態?
09:41
Now, where do you find such Goldilocks conditions?
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09:43
Well, planets are great,
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其實行星就是好的
09:45
and our early Earth was almost perfect.
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我們的地球
就算是幾乎完美
它有著與恆星剛剛好的距離
09:50
It was just the right distance from its star
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能有著巨大的海洋
09:52
to contain huge oceans of liquid water.
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09:54
And deep beneath those oceans,
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在海洋深處
09:56
at cracks in the Earth's crust,
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地殼縫隙
09:58
you've got heat seeping up from inside the Earth,
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地熱往上傳遞
10:01
and you've got a great diversity of elements.
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又有著多種的元素
10:03
So at those deep oceanic vents,
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所以在深海縫隙
10:05
fantastic chemistry began to happen,
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神奇的化學反應開始了
10:08
and atoms combined in all sorts of exotic combinations.
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原子組合成未有的化合物
10:12
But of course, life is more than just exotic chemistry.
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當然 生命本身
不是只是非比尋常的化學
你要如何穩定這些
10:17
How do you stabilize those huge molecules
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不穩定的
10:20
that seem to be viable?
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巨大的分子群?
10:22
Well, it's here that life introduces an entirely new trick.
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在這時候 生命引入
一整個新把戲
10:28
You don't stabilize the individual;
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並不是穩定每一個體
10:30
you stabilize the template,
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而是穩定樣版:
10:32
the thing that carries information,
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就是攜帶訊息的
與日後可複製的樣版
10:35
and you allow the template to copy itself.
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DNA 就是這
10:37
And DNA, of course, is the beautiful molecule
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美麗攜帶訊息
10:40
that contains that information.
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的化學分子
10:42
You'll be familiar with the double helix of DNA.
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大家都熟悉雙螺旋體的 DNA
10:45
Each rung contains information.
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每一連接橫桿都帶著資訊
DNA有著如何製作
10:48
So, DNA contains information about how to make living organisms.
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生命體的訊息
以及如何自行複製自己
10:53
And DNA also copies itself.
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所以生物開始複製
10:55
So, it copies itself
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10:56
and scatters the templates through the ocean.
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將資訊經由海洋傳遞
同時資訊也傳開了
10:59
So the information spreads.
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請留意 資訊將扮演一個重要部份
11:01
Notice that information has become part of our story.
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而DNA精彩的部分是
11:04
The real beauty of DNA though is in its imperfections.
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在於它的不完美
11:07
As it copies itself, once in every billion rungs,
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當它在複製時
十億分之一的機會
11:11
there tends to be an error.
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會產生複製錯誤
11:13
And what that means is that DNA is, in effect, learning.
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也就是說
DNA 會自我學習
11:18
It's accumulating new ways of making living organisms
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累積製造新的生命體的方式
因為一些錯誤的確能存用
11:21
because some of those errors work.
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所以 DNA 一直學習
11:23
So DNA's learning
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11:24
and it's building greater diversity and greater complexity.
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它一直建構更多元更複雜的架構
11:27
And we can see this happening over the last four billion years.
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過去40億年來, 這都一直在發生
11:30
For most of that time of life on Earth,
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地球的大多數時間
生物體多是以簡單的
11:33
living organisms have been relatively simple --
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單細胞存在的
11:35
single cells.
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11:36
But they had great diversity, and, inside, great complexity.
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但仍是非常多元
與複雜
11:40
Then from about 600 to 800 million years ago,
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從6~8億年前開始
11:43
multi-celled organisms appear.
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多細胞生物出現
11:45
You get fungi, you get fish,
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有了真菌類 有了魚類
有了植物類
11:48
you get plants,
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11:49
you get amphibia, you get reptiles,
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有了兩棲類 有了爬蟲類
11:52
and then, of course, you get the dinosaurs.
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當然 也有了恐龍
11:55
And occasionally, there are disasters.
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偶而 會有災難
11:59
Sixty-five million years ago,
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6千5百萬年前
12:01
an asteroid landed on Earth
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隕石墬落到地球
12:03
near the Yucatan Peninsula,
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靠近Yucatan 半島
12:05
creating conditions equivalent to those of a nuclear war,
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創造出相當於核子戰爭的威力
12:08
and the dinosaurs were wiped out.
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恐龍滅絕
對恐龍來說是壞消息
12:11
Terrible news for the dinosaurs,
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12:14
but great news for our mammalian ancestors,
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卻是哺乳動物祖先的好消息
才能在恐龍
12:18
who flourished
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12:19
in the niches left empty by the dinosaurs.
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留下的生存縫隙繁衍
12:22
And we human beings are part of that creative evolutionary pulse
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人類
也是那6千5百萬年開始進化的
一部分
12:28
that began 65 million years ago
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12:30
with the landing of an asteroid.
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就在隕石落下後
12:33
Humans appeared about 200,000 years ago.
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人類出現在20萬年前
12:36
And I believe we count as a threshold in this great story.
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我相信人類
發展就是宇宙進化的一個階段
12:40
Let me explain why.
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讓我來做解釋
12:42
We've seen that DNA learns in a sense,
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我們已經見到DNA是會學習的
12:45
it accumulates information.
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它會累積資訊
12:47
But it is so slow.
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卻是非常緩慢的
DNA會累積資訊
12:50
DNA accumulates information through random errors,
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經由隨機的錯誤
12:53
some of which just happen to work.
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有的錯誤剛好適用
12:56
But DNA had actually generated a faster way of learning:
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另外DNA有更快的方式在學習
是經由有腦的生物體
12:59
it had produced organisms with brains,
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13:01
and those organisms can learn in real time.
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這種生物就能即時的學習
便能由腦累積資訊 學習
13:05
They accumulate information, they learn.
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13:07
The sad thing is, when they die,
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可悲的是
當他們死去 資訊也跟著失去
13:10
the information dies with them.
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13:12
Now what makes humans different is human language.
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所以造就人類的不同
就是人類的語言能力
13:16
We are blessed with a language, a system of communication,
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我們有幸能有語言 是個溝通的系統
是有力與正確的傳達
13:19
so powerful and so precise
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13:21
that we can share what we've learned with such precision
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3158
我們能正確分享我們所學的
能集合成一集體智慧
13:25
that it can accumulate in the collective memory.
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也就是說
13:28
And that means
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13:29
it can outlast the individuals who learned that information,
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資訊能夠超過個體的壽命
能以世代的方式傳遞
13:33
and it can accumulate from generation to generation.
277
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3173
13:36
And that's why, as a species, we're so creative and so powerful,
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4056
也因為這 我們這樣的物種 才這麼有創造力
能有這麼大的能耐
13:40
and that's why we have a history.
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2056
也是這樣我們能記下歷史
40億年來 我們似乎是唯一有
13:43
We seem to be the only species in four billion years
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此天賦的物種
13:46
to have this gift.
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我稱此能力為
13:48
I call this ability collective learning.
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集體式學習
13:51
It's what makes us different.
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這就是造就我們不同的
13:53
We can see it at work in the earliest stages of human history.
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我們能明顯
這能力在早期人類歷史中呈現
13:57
We evolved as a species in the savanna lands of Africa,
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3287
我們是以整個物種的方式進化
即使是在 早期非洲沙瓦那平原時代
14:01
but then you see humans migrating into new environments,
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接著 也看到人類移居到新環境 ---
14:04
into desert lands, into jungles,
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2150
進入沙漠地帶 進入叢林
14:06
into the Ice Age tundra of Siberia --
288
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2436
進入冰河期的西伯利亞凍土平原
非常非常艱辛的環境 ---
14:09
tough, tough environment --
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1445
14:10
into the Americas, into Australasia.
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2333
進入美洲 進入澳洲
每一次的移居 就伴隨著學習
14:13
Each migration involved learning --
291
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學習如何開墾新環境
14:15
learning new ways of exploiting the environment,
292
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14:17
new ways of dealing with their surroundings.
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學習新方法與週遭共榮
14:19
Then 10,000 years ago,
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一萬年前
14:21
exploiting a sudden change in global climate
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在上個冰河期的末期
面對了突然的氣候變遷
14:24
with the end of the last ice age,
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1572
人類開始學會農耕
14:26
humans learned to farm.
297
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1581
14:28
Farming was an energy bonanza.
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2436
農耕就是 能源的礦藏
開發這樣的能源
14:31
And exploiting that energy, human populations multiplied.
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人類數目開始增加
14:34
Human societies got larger, denser, more interconnected.
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人類社會也跟著增大與密集
更加相互關連
從約500年前
14:39
And then from about 500 years ago,
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14:42
humans began to link up globally
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人類開始有全球性的相連
14:44
through shipping, through trains,
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經由船運 與 鐵路
14:46
through telegraph, through the Internet,
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經由電報 與 網際網路
14:49
until now we seem to form a single global brain
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到現在 我們形成了
來自近70億人
的單一全球腦袋
14:54
of almost seven billion individuals.
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2132
這個腦是以極高速的方式在學習
14:56
And that brain is learning at warp speed.
307
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3162
15:00
And in the last 200 years, something else has happened.
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在過去的200年 另外的事情也發生了
我們發現了另一能源礦藏
15:03
We've stumbled on another energy bonanza
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就是化石石油
15:05
in fossil fuels.
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1127
化石石油加上集體式學習
15:07
So fossil fuels and collective learning together
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15:09
explain the staggering complexity we see around us.
312
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3524
解釋了驚人的
週遭的複雜性
15:16
So --
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1000
所以 我們在此
15:18
Here we are,
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1317
回到會議中心
15:20
back at the convention center.
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1524
15:21
We've been on a journey, a return journey, of 13.7 billion years.
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我們經歷過一個回溯的旅程
到137億年前
15:26
I hope you agree this is a powerful story.
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希望你也認同這個震撼故事
15:29
And it's a story in which humans play an astonishing and creative role.
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4665
是個人類扮演著
驚人與創意的角色
15:34
But it also contains warnings.
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2215
它也帶來警訊
15:37
Collective learning is a very, very powerful force,
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集合的智慧是個非常巨大的力量
15:41
and it's not clear that we humans are in charge of it.
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但不明確的是
我們人類是否能控制它
我記得在英格蘭的童年
15:47
I remember very vividly as a child growing up in England,
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經過古巴飛彈危機
15:50
living through the Cuban Missile Crisis.
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2020
15:52
For a few days, the entire biosphere
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3611
有那麼幾天
整個生物圈
15:56
seemed to be on the verge of destruction.
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2299
似乎濒臨全球毀滅
15:59
And the same weapons are still here,
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3165
但是同樣的武器仍然存在
16:02
and they are still armed.
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他們仍然武裝
我們是否能避開那陷阱
16:05
If we avoid that trap, others are waiting for us.
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3232
其他國也在觀望
16:08
We're burning fossil fuels at such a rate
329
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2589
我們使用化石石油的快速
16:11
that we seem to be undermining the Goldilocks conditions
330
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就好像忽略所謂的最適狀態
16:14
that made it possible for human civilizations
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2228
那最適狀態才造就了人類文明
16:16
to flourish over the last 10,000 years.
332
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3082
綻放了過去一萬年
16:20
So what big history can do
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所以這個大歷史能作的是
16:22
is show us the nature of our complexity and fragility
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3321
告訴我們自己的複雜與脆弱
以及我們所面對的危機
16:26
and the dangers that face us,
335
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1924
它也同樣昭示我們
16:28
but it can also show us our power with collective learning.
336
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我們有著集體式的智慧力量
16:32
And now, finally --
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最後
16:35
this is what I want.
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2155
我想說的是
16:39
I want my grandson, Daniel,
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3032
我希望我的孫子 Daniel
16:42
and his friends and his generation,
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2757
及他的朋友與全球
的這代人
16:45
throughout the world,
341
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能知道這個大歷史故事
16:47
to know the story of big history,
342
1007102
2840
16:49
and to know it so well
343
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2039
清楚到
他們明瞭
16:52
that they understand both the challenges that face us
344
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3666
我們所面臨的挑戰
16:55
and the opportunities that face us.
345
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與所面臨的機會
16:58
And that's why a group of us
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1880
那也就是我們之中一群人
17:00
are building a free, online syllabus
347
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在建構線上教學大綱
有關於大歷史
17:03
in big history
348
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1318
17:04
for high-school students throughout the world.
349
1024542
2151
針對全球高中生
我們相信大歷史
17:07
We believe that big history
350
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2436
17:09
will be a vital intellectual tool for them,
351
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2551
在Daniel 及他的同世代
17:12
as Daniel and his generation
352
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2843
面對挑戰
17:15
face the huge challenges
353
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2348
與無窮機會
17:17
and also the huge opportunities
354
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2055
面對下一個
17:19
ahead of them at this threshold moment
355
1039578
3455
美麗地球上的進化門檻
會成為他們的一個智慧的工具
17:23
in the history of our beautiful planet.
356
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3179
17:26
I thank you for your attention.
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謝謝聆聽
17:28
(Applause)
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4695
(掌聲)
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