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  • The earth receives about 90 petajoules of energy from the sun every second.

    地球每秒接收到太陽約九京焦耳的能量,

  • That’s a lotenough to satisfy all human energy needs thousands of times over.

    粉多的,足以滿足數千倍於全人類使用的能量。

  • However, the earth also radiates an equal amount of energy back into space as heat.

    然而同時,地球也向太空放出等量的熱能

  • (An almost equal amount, anyway -- the Earth is gradually heating up, but that's another

    (幾乎等量啦,地球正在暖化,此事暫且不提。)

  • story.)

    (幾乎等量啦,地球正在暖化,此事暫且不提。)

  • So if energy in equals energy out, how can we possibly be using any energy to do anything?

    如果輸入等於輸出,我們哪來的能量做各種事情?

  • What matters, it turns out, isn’t simply energyit’s useful energy.

    事實上這不只關係到能量,而是「可用的能量」。

  • And energy is useful when it comes packaged in a low-entropy form.

    當能量在低熵狀態則容易使用。

  • The total amount of energy in any closed system can’t change, of course -- energy is conserved.

    一個封閉系統內的能量當然不會改變─能量守恆嘛,

  • But that energy can be in different states of usefulness.

    但能量從有用到沒用有各種層級。

  • There is useful energy in the water behind a dam, which will flow until the level is

    水壩後頭的水釋放可用能量,直到兩邊水位等高,

  • the same on both sides, but will never go backup.”

    但絕對不會倒流回去。

  • Or in hot tea, which will melt a cold ice cube until they reach a medium temperature.

    或一杯熱茶,把裡面的冰塊融化,直到兩者溫度相同,

  • You never see tepid tea spontaneously generate an ice cube while heating up, even though

    你不可能目睹微熱的紅茶自動加溫、自動生出冰塊,

  • the total energy would be the same.

    即使總能量仍然一致。

  • So, useful energy is low entropy, out-of-equilibrium energy that can be put to work, to turn a

    因此有用的能量熵較低,不平衡的能量可以做功,

  • turbine or push a piston or melt an ice cube.

    轉動渦輪以推動活塞,或融化冰塊。

  • Useless energy, meanwhile, can’t be put to work.

    除非這能量無法做功,

  • It’s out there in the form of waste heat or noise or the potential energy of a ball

    以廢熱、噪音或地上一顆靜止球球的位能等形式,

  • just sitting on the ground: we can't really do anything with it.

    對我們來講都一無是處。

  • For example, gasoline and air carry useful, low-entropy energy.

    好比說,汽油和空氣都帶有低熵的可用能量,

  • By burning them together, we can accelerate a car, drive for a while, then put on the

    當燃燒使它們結合,我們能藉此加速汽車、開一段路、

  • brakes and stop.

    踩煞車停止。

  • The total energy of the world remains constant during the trip, but useful chemical energy

    整趟旅程中,世界上的能量總和不便,但有用的化學能

  • is converted into useless, high-entropy heat and noise.

    被轉換成沒用、高熵的熱與聲音。

  • The energy is still there, but we can't reclaim it to power any more cars, as convenient as

    能量還是在,但我們無法利用它駕車如之前那般方便。

  • that would be.

    能量還是在,但我們無法利用它駕車如之前那般方便。

  • And thus it is with the earth.

    地球也是同一種原理。

  • The sun sends us energy in a convenient, useful, low-entropy form, mainly as photons of visible

    太陽給我們有用、低熵的能量, 主要是以可見光子的形式。

  • light.

    太陽給我們有用、低熵的能量, 主要是以可見光子的形式。

  • This energy gets absorbed and used and degraded by various processes here on Earth, until

    這股能量經由地球上的各種過程被吸收、使用、衰敗,

  • we radiate it away in a much higher-entropy form: lots of infrared photons.

    直到我們把它們以高熵形式散發出去:大量紅外光子。

  • For every visible photon we receive, the Earth radiates about twenty infrared photons out

    地球每接收一個可見光子,大約就會放出20個紅外光子

  • into space.

    至太空中。

  • Even though there’s a balance of energy in with energy out, the entropy of the energy

    即便能量輸入和輸出平衡,能量的熵仍增加了20倍。

  • has gone up twenty times.

    即便能量輸入和輸出平衡,能量的熵仍增加了20倍。

  • The Sun, in fact, is only a source of useful energy because it's a hot, bright spot in

    事實上,太陽本身之所以是有用的能源, 正因為它是個明亮的熱點,處在寒冷、黑暗的太空中。

  • a cold, dark sky.

    事實上,太陽本身之所以是有用的能源, 正因為它是個明亮的熱點,處在寒冷、黑暗的太空中。

  • If the whole sky were the temperature of the Sun, our planet would receive a lot more energy,

    若太空各處的溫度都和太陽一樣, 地球會接收到非常多的能量,

  • but the Earth would quickly average out to a state of high-entropy equilibrium, with

    但地球很快會陷入高熵的能量平衡,

  • everything at the temperature of the Sun.

    整個星球都變得跟太陽一樣熱。

  • So things like driving or living would be impossiblenot because there’s insufficient

    開車或生存會變得不可能─不是因為能量太少,

  • energy, but because you can’t do anything when all the energy has averaged out.

    而是你沒辦法使用已經平衡的能量。

  • In equilibrium, all energy is equally useless, nothing ever changes, and time's arrow ceases

    在平衡狀態下,所有能量都沒有用,事物永遠不變,

  • to have any meaning.

    時間之箭將不再有任何意義。

  • Hey, Henry here, thanks for watching.

    安安我是Henry,感謝收看。

  • This is the fourth video in a series about time and entropy made in collaboration with

    本片是和物理學家Sean Carroll合作關於時間與熵

  • physicist Sean Carroll.

    系列影片的第四集。

  • The series is supported with funding from Google’s Making and Science initiative,

    本系列由 Google’s Making and Science initiative贊助播出,

  • which seeks to encourage more young people (and people of all ages) to learn about and

    為了鼓勵更多年輕人(和全年齡的人們)學習

  • fall in love with science and the world around them, and the videos are based off of Sean’s

    並愛上科學和這個世界,本片基於Sean所著

  • bookThe Big Picture: On the Origins of Life, Meaning, and the Universe Itself,”

    《The Big Picture: On the Origins of Life, Meaning, and the Universe Itself》。

  • which you can find online or in bookstores around the world.

    你可以在線上或世界各地的書店找到。

The earth receives about 90 petajoules of energy from the sun every second.

地球每秒接收到太陽約九京焦耳的能量,

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