The dust bunnies that built our planet - Lorin Swint Matthews

247,171 views ・ 2019-09-05

TED-Ed


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譯者: Lilian Chiu 審譯者: Helen Chang
00:07
Consider the spot where you’re sitting.
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想像你現在所坐的這個點。
00:09
Travel backwards in time
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時間旅行回到過去,
00:11
and it might’ve been submerged at the bottom of a shallow sea,
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這個點有可能是位在 一片淺海的底部,
00:15
buried under miles of rock,
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被數英里的岩石給掩埋,
00:17
or floating through a molten, infernal landscape.
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或者漂浮在熱熔的地獄環境。
00:21
But go back far enough—
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但,如果回到夠久的過去——
00:23
about 4.6 billion years,
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大約四十六億年前,
00:26
and you’d be in the middle of an enormous cloud of dust and gas
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你會身處在塵埃和氣體 構成的巨型雲霧中,
00:30
orbiting a newborn star.
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繞著新生的星體運轉。
00:34
This is the setting for some of the biggest, smallest mysteries of physics:
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這是最大、最小物理學之謎 所發生的環境,這個謎就是:
00:39
the mysteries of cosmic dust bunnies.
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宇宙塵兔之謎。
00:43
Seemingly empty regions of space between stars
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在星體之間,看似 空無一物的宇宙區域,
00:47
actually contain clouds of gas and dust,
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其實有著氣體和塵埃所形成的雲,
00:51
usually blown there by supernovas.
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通常是被超級新星炸到那裡去的。
00:54
When a dense cloud reaches a certain threshold called the Jeans mass,
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當雲的密度高到達 「金斯質量」這個門檻值時,
00:59
it collapses in on itself.
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它自己就會崩塌。
01:02
The shrinking cloud rotates faster and faster, and heats up,
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縮小的雲會越轉越快速, 溫度跟著上升,
01:06
eventually becoming hot enough to burn hydrogen in its core.
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最終熱到足以燃燒 它核心區域的氫。
01:11
At this point a star is born.
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在這個時點,星體就誕生了。
01:14
As fusion begins in the new star,
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當新星中的融合開始,
01:16
it sends out jets of gas that blow off the top and bottom of the cloud,
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它就會噴射出氣體, 將雲的頂部和底部吹掉,
01:21
leaving behind an orbiting ring of gas and dust called a protoplanetary disk.
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留下繞行的環狀氣體和塵埃,
稱為「原行星盤」。
01:28
This is a surprisingly windy place;
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這個地方風大得驚人;
01:31
eddies of gas carry particles apart, and send them smashing into each other.
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氣體旋渦會把粒子帶開, 讓它們互相碰撞。
01:36
The dust consists of tiny metal fragments, bits of rock, and, further out, ices.
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塵埃包含了小型的 金屬碎片、小堆岩石,
在更外圍還有冰。
01:43
We’ve observed thousands of these disks in the sky,
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我們已經觀察到天空中 有數千個這種星盤,
01:46
at various stages of development
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處在不同的發展階段,
01:48
as dust clumps together into larger and larger masses.
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塵埃結在一起,質量越來越大。
01:53
Dust grains 100 times smaller than the width of a human hair stick to each other
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比人類頭髮的寬度還要小一百倍的 塵埃粒子會彼此黏在一起,
01:59
through what’s called the van der Waals force.
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讓它們相黏的力量 叫做「凡得瓦爾力」。
02:02
That’s where a cloud of electrons shifts to one side of a molecule,
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此時,電子雲就會 轉移到分子的一邊,
02:06
creating a negative charge on one end, and a positive charge on the other.
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在一端創造出負電荷, 另一端創造出正電荷。
02:11
Opposites attract, but van der Waals can only hold tiny things together.
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異性相吸,但凡得瓦爾力只能夠 將微小的東西結合在一起。
02:16
And there’s a problem: once dust clusters grow to a certain size,
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有一個問題:一旦塵埃群 成長到了某個大小之後,
02:21
the windy atmosphere of a disk should constantly break them up
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星盤大氣中的風很大,
經常使這些塵埃群彼此相撞而散開。
02:25
as they crash into each other.
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02:26
The question of how they continue to grow is the first mystery of dust bunnies.
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它們如何持續成長, 是塵兔的第一個謎。
02:33
One theory looks to electrostatic charge to answer this.
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有個從靜電電荷來解答的理論。
02:37
Energetic gamma rays, x-rays, and UV photons
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高能加馬射線、X 光、UV 光子
02:41
knock electrons off of gas atoms within the disk,
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在星盤中將電子 從氣體原子中打掉,
02:45
creating positive ions and negative electrons.
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創造出正離子和負電子,
02:49
Electrons run into and stick to dust,
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電子碰到塵埃就會黏住塵埃,
02:52
making it negatively charged.
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讓它帶負電。
02:54
Now, when the wind pushes clusters together,
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當風把塵埃群推到一起時,
02:57
like repels like and slows them down as they collide.
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同性相斥,且當它們 相撞時會讓它們慢下來。
03:02
With gentle collisions they won’t fragment,
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輕輕碰撞不會讓它們破碎,
03:04
but if the repulsion is too strong, they’ll never grow.
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但如果相斥太強, 它們就永遠不會成長。
03:08
One theory suggests that high energy particles
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有一種理論指出,高能粒子
03:12
can knock more electrons off of some dust clumps,
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能把更多電子從塵埃團中給除去,
03:15
leaving them positively charged.
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讓塵埃團帶正電。
03:17
Opposites again attract, and clusters grow rapidly.
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異性相吸,塵埃群就會快速成長。
03:22
But before long we reach another set of mysteries.
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但,不久,我們又 碰到了另一組謎。
03:26
We know from evidence found in meteorites
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從隕石找到的證據顯示,
03:28
that these fluffy dust bunnies eventually get heated, melted
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這些蓬鬆的塵兔最終 會被加溫、熔化,
03:33
and then cooled into solid pellets called chondrules.
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接著冷卻,成為固態顆粒, 叫做隕石球粒。
03:38
And we have no idea how or why that happens.
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我們不知道這是怎麼發生的, 也不知道為什麼發生。
03:42
Furthermore, once those pellets do form, how do they stick together?
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此外,一旦那些顆粒真的形成了, 它們要如何黏在一起?
03:47
The electrostatic forces from before are too weak,
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之前的靜電力太弱了,
03:50
and small rocks can’t be held together by gravity either.
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小岩石無法靠引力就結合在一起。
03:55
Gravity increases proportionally to the mass of the objects involved.
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物體間的引力 和物體的質量成正比。
04:00
That’s why you could effortlessly escape an asteroid the size of a small mountain
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那就是為什麼你可以毫不費力, 光靠雙腿產生的力量,
04:05
using just the force generated by your legs.
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就脫離小山大小的小行星。
04:08
So if not gravity, then what?
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如果不是引力,那是什麼?
04:11
Perhaps it’s dust.
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也許是塵埃。
04:13
A fluffy dust rim collected around the outside of the pellets
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在顆粒外部集結的蓬鬆塵埃外緣
04:17
could act like Velcro.
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可能會有魔鬼沾的功能。
04:19
There’s evidence for this in meteors,
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在隕石中有找到相關證據,
04:22
where we find many chondrules surrounded by a thin rim of very fine material–
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我們發現許多隕石球粒被薄薄一層 非常好的材質給包住——
04:28
possibly condensed dust.
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有可能是高密度的塵埃。
04:31
Eventually the chondrule pellets get cemented together inside larger rocks,
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最終,隕石球粒的顆粒會在 更大的岩石中被黏結起來,
04:36
which at about 1 kilometer across
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這些岩石大約有一公里寬,
04:39
are finally large enough to hold themselves together through gravity.
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終於,這些顆粒因此就夠大, 足以用引力持續結合在一起了。
04:43
They continue to collide and grow into larger and larger bodies,
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它們繼續碰撞, 成長成更大的物體,
04:48
including the planets we know today.
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包括我們現今所知的行星。
04:51
Ultimately, the seeds of everything familiar–
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最終,我們熟悉的一切——
04:54
the size of our planet, its position within the solar system,
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我們行星的大小, 在太陽系中的位置,
04:57
and its elemental composition–
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以及組成的元素——
04:59
were determined by an uncountably large series of random collisions.
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其根源是由一大連串 隨機撞擊所決定的。
05:05
Change the dust cloud just a bit,
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若塵雲有稍微改變一點點,
05:08
and perhaps the conditions wouldn’t have been right
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也許就不會有對的條件
05:10
for the formation of life on our planet.
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讓我們的星球上出現生命了。
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