Is there a limit to technological progress? - Clément Vidal

761,337 views ・ 2016-12-19

TED-Ed


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審譯者: Bruce Sung
00:06
Many generations have felt they’ve reached the pinnacle
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許多世代的人都認為
他們的科技進步已到達頂峰
00:09
of technological advancement.
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00:11
Yet look back 100 years and the technologies we take for granted today
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然而回首百年前
今天我們視為理所當然的科技
00:16
would seem like impossible magic.
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在當時被視為不可能的魔法
00:19
So will there be a point where we reach an actual limit of technological progress?
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所以,真的會在某個時間點
我們將觸及科技的極限嗎?
00:26
And if so, are we anywhere near that limit now?
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如果是這樣,我們現在距離 科技的極限有多遠呢?
00:30
Half a century ago, Russian astronomer Nikolai Kardashev was asking
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半個世紀前
俄羅斯天文學家尼古拉·卡爾達肖夫
問了類似的問題
00:35
similar questions when he came up with a way to measure technological progress;
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他想出一個測量科技進步的方法
00:40
even when we have no idea exactly what it might look like.
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即使當時我們無法得知 未來會是什麼樣子
00:44
Anything we do in the future will require energy.
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未來我們做的任何事情都需要能源
00:47
So Kardashev’s scale classifies potential civilizations,
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卡爾達肖夫將潛在的文明進行分級
00:51
whether alien civilizations out there in the universe or our own,
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不論是宇宙的外星文明 或是我們自己的
00:55
into three levels based on energy consumption.
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都能依照能源消耗量分為三個等級
00:59
The tiny amount of energy we currently consume pales
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我們目前消耗的少量能源
01:02
next to what we leave untapped.
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比起尚未開發的部分,根本微不足道
01:04
A type I, or planetary civilization, can access all the energy resources
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第一級文明,也稱為「行星文明」
能運用所有行星本身的能源
01:10
of its home planet.
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01:12
In our case, this is the 174,000 terawatts
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以我們為例,地球從太陽接收了 174,000 兆瓦的能量
01:16
Earth receives from the sun.
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01:18
We currently only harness about 15 terawatts of it,
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目前我們僅僅取得其中的十五兆瓦
01:22
mostly by burning solar energy stored in fossil fuels.
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大部分是藉由燃燒 儲存著太陽能的化石燃料
01:26
To approach becoming a type I civilization,
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為了要更趨近第一級文明
01:29
we would need to capture solar energy more directly and efficiently
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我們必須更直接 更有效率地取得太陽能
01:33
by covering the planet with solar panels.
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方法是以太陽能電池板覆蓋地球
01:36
Based on the most optimistic models,
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根據最樂觀的模型推測
01:38
we might get there within just four centuries.
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我們大概能在四個世紀後達成目標
01:41
What would be next?
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接下來呢?
01:43
Well, the Earth only gets a sliver of the sun’s energy,
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由於地球只能獲得 所有太陽能量的微小部分
01:46
while the rest of its 400 yottawatts is wasted in dead space.
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400 X 10 的 24 次方瓦的能量 絕大部分在太空中被浪費
01:51
But a type II, or stellar civilization,
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但是在第二級文明 或稱為「恆星文明」
01:54
would make the most of its home stars energy.
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就能善用恆星大部分的能源
01:57
Instead of installing solar panels around a planet,
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取代了原本圍繞著行星 安裝太陽能板的方式
02:00
a type II civilization would install them directly orbiting its star,
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第二級文明直接以太陽能板 包圍整個恆星
02:05
forming a theoretical structure called a Dyson sphere.
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所形成的這個理論結構 稱為「戴森球體」
02:09
And the third step, a type III civilization,
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然後下一步呢?
第三級「星系文明」
02:12
would harness all the energy of its home galaxy.
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能夠取得它本身所處星系的所有能源
02:16
But we can also think of progress in the opposite way.
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然而,我們也能從另一個方向 來衡量科技進程
02:19
How small can we go?
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我們能達到多小呢?
在那方面,英國的 宇宙學家約翰 · 巴羅
02:22
To that end, British cosmologist John Barrow,
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02:24
classified civilizations by the size of objects they control.
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根據文明能控制的 物體大小來進行分級
02:28
That ranges from mechanical structures at our own scale,
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範圍由大到我們自身大小相仿的機械
02:32
to the building blocks of our own biology, down to unlocking atoms themselves.
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小到組成我們身體的生物結構
甚至可以小到分解原子
02:37
We’ve currently touched the atomic level,
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我們現有的科技觸及原子層級 但還不能完全控制它們
02:39
though our control remains limited.
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02:42
But we potentially could go much smaller in the future.
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但我們未來有可能探索更微小的世界
02:45
To get a sense of the extent to which that’s true,
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底下的例子能讓你感受到 真實世界的尺度
02:48
the observable universe is 26 orders of magnitude
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目前所能觀測得到的宇宙 是人體體積的「10 的 26 次方」倍
02:52
larger than a human body.
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02:54
That means if you zoomed out by a factor of 10, 26 times,
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意思是,每次放大十倍 連續放大 26 次
02:58
you’d be at the scale of the universe.
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就能達到宇宙的規模
但為了達到最小的尺度 也就是「普朗克長度」
03:01
But to reach the minimum length scale known as the Planck length,
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03:05
you would need to zoom in 35 times.
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你需要縮小 35 次
03:08
As physicist Richard Feynman once said,
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如同物理學家理察·費曼所言: 「在微小世界仍有許多的空間。」
03:10
there’s plenty of room at the bottom.
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03:13
Instead of one or the other, it’s likely that our civilization
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未來人類的文明 並非兩者只能取其一
03:16
will continue to develop along both Kardashev and Barrow scales.
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可能依循卡爾達肖夫和巴羅 二者的衡量方式繼續發展
03:21
Precision on a smaller scale lets us use energy more efficiently
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精確地控制微小尺度 能讓我們更有效地使用能源
03:25
and unlocks new energy sources like nuclear fusion or even antimatter.
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並開發新能源,例如「核融合」
甚至是「反物質」
03:30
And this increased energy lets us expand and build on a larger scale.
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增加的能源,能讓我們在 巨大尺度上持續擴張和建設
03:36
A truly advanced civilization then would harness both stellar energy
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真正先進的文明
會同時運用恆星能量以及次原子科技
03:40
and subatomic technologies.
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03:43
But these predictions weren't made just for us humans.
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這些預測不只是適用於人類
03:46
They double as a possible means of detecting intelligent life
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它們也可以作為
偵測宇宙智慧生命的方法
03:49
in the universe.
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03:51
If we find a Dyson sphere around a distant star,
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如果我們在遙遠的恆星外圍 發現戴森球體的結構
03:54
that's a pretty compelling sign of life.
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那會是個很有說服力的生命跡象
03:56
Or what if instead of a structure that passively soaked up
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或者,如果外星文明所建造的結構體
04:00
all of a star’s energy like a plant,
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並不只是像植物那樣 只能被動地接收能量
04:02
an alien civilization built one that actively sucked the energy
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而是像蜂鳥主動吸取恆星能量, 那我們該怎麼辦?
04:06
out of the star like a hummingbird?
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04:09
Frighteningly enough, we’ve observed super dense celestial bodies
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可怕的是,我們已經能觀測到 超高密度的天體
04:13
about the size of a planet that drain energy out of a much bigger star.
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他們的大小跟行星一樣
卻能從比它更大的恆星吸取能量
04:18
It would be much too premature to conclude that this is evidence of life
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當然現在還無法斷言
那是宇宙中具有其他生命的證據
04:22
in the universe.
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04:23
There are also explanations for these observations
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對於這些觀測結果
04:25
that don’t involve alien life forms.
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還有其他各種解釋 是無關外來生命形式的
04:27
But that doesn’t stop us from asking: what if?
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但這並不會阻止我們繼續問:
「如果這樣......會怎樣?」
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