Sunlight is way older than you think - Sten Odenwald

732,768 views ・ 2015-05-12

TED-Ed


请双击下面的英文字幕来播放视频。

翻译人员: Xinlong Zhang 校对人员: Kai Ma
00:06
You may know that it takes light a zippy eight minutes
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或许你知道太阳光从太阳表面
00:10
to reach us from the surface of the Sun,
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到达地球需要8分钟
00:13
so how long do you think it takes light
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但是你认为太阳光要多久
00:15
to travel from the Sun's core to its surface?
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从太阳中心到达太阳表面呢
几秒钟 顶多一分钟?
00:18
A few seconds or a minute at most?
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00:21
Well, oddly enough, the answer is many thousands of years.
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扶好下巴 答案是需要好几千年
00:25
Here's why.
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这里是解释
00:27
Photons are produced by the nuclear reactions deep in the core of our Sun.
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光子在太阳中心深处通过核反应产生
00:32
As the photons flow out of the core, they interact with matter and lose energy,
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光子从太阳中心流出
与物质相互作用损失能量
00:37
becoming longer wavelength forms of light.
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形成波长更长的光波
00:40
They start out as gamma rays in the core,
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光波在核心以伽马射线形式产生
00:43
but end up as x-rays, ultraviolet or visible light as they near the surface.
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但是在表面却衰减为X射线紫外线或者可见光
00:49
However, that journey is neither simple nor direct.
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然而过程十分复杂
00:54
Upon being born, each photon travels at a speed of 300,000 kilometers per second
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光子刚刚产生时候速度是每秒30万千米
01:01
until it collides with a proton and is diverted in another direction,
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直到它撞击到另一个光子并且改变方向
01:06
acting like a bullet ricocheting off of every charged particle it strikes.
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好比子弹一样
每次撞击改变一次方向
经过无数次撞击
01:11
The question of how far this photon gets from the center of the Sun
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光子到达表面到底要经过多久
01:15
after each collision
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01:17
is known as the random walk problem.
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就是一个随机漫步问题
01:20
The answer is given by this formula:
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这个公式会告诉我们答案
01:22
distance equals step size times the square root of the number of steps.
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距离等于步长乘以步数的平方根 (一步指撞击间隔)
01:28
So if you were taking a random walk from your front door
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如果你从你家前门出发
01:31
with a one meter stride each second,
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每秒走一米并且每次随机换一次方向
01:33
it would take you a million steps and eleven days
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会花费你11天时间 经过100万米的路程
01:37
just to travel one kilometer.
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才能离开1千米远的距离
01:40
So then how long does it take for a photon generated in the center of the sun
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所以光子要用多久
才能从太阳中心到达地球
01:45
to reach you?
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01:47
We know the mass of the Sun
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我们知道太阳的质量
01:49
and can use that to calculate the number of protons within it.
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可以通过质量计算光子的数量
01:53
Let's assume for a second that all the Sun's protons are evenly spread out,
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不妨假设这一秒钟内光子均匀扩散
01:57
making the average distance between them about 1.0 x 10^-10 meters.
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假设它们每次传播0.1纳米的距离
02:04
To random walk the 690,000 kilometers from the core to the solar surface
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从太阳核心到表面是69万千米的距离
02:11
would then require 3.9 x 10^37 steps,
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用随机漫步的话3.9X10^37步
02:17
giving a total travel time of 400 billion years.
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大概需要4千亿年的时间
02:22
Hmm, that can't be right.
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桥豆麻袋 这不科学啊
02:24
The Sun is only 4.6 billion years old, so what went wrong?
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太阳公公才460万岁好嘛 所以一定是哪里出问题了
02:28
Two things:
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这里有两点
02:30
The Sun isn't actually of uniform density
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第一 太阳并不是均匀的
02:33
and photons will miss quite a few protons between every collision.
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第二 每次撞击之间光子会失去一些质子
02:38
In actuality, a photon's energy,
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实际上 在这个过程中
02:41
which changes over the course of its journey,
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光子的能量是在不断变化的
02:43
determines how likely it is to interact with a proton.
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并且能量决定着与质子反应的可能性
02:47
On the density question,
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在密度这个问题上
02:48
our models show that the Sun has a hot core,
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我们假设的是
02:51
where the fusion reactions occur.
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溶解反应在太阳的核心中发生
02:54
Surrounding that is the radiative zone,
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围绕核心的是辐射传播区域
02:56
followed by the convective zone, which extends all the way to the surface.
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再其外是通向表面的对流区域
03:01
The material in the core is much denser than lead,
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核心的物质比金属铅还要密集
03:04
while the hot plasma near the surface is a million times less dense
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表面附近的连续密度等离子体
03:09
with a continuum of densities in between.
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相比之下稀疏了100万倍
03:12
And here's the photon-energy relationship.
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这是光子-能量的关系
03:15
For a photon that carries a small amount of energy,
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对于携带少量能量的光子而言
03:18
a proton is effectively huge,
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质子的影响是巨大的
03:21
and it's much more likely to cause the photon to ricochet.
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很可能引起光子的反弹
03:24
And for a high-energy photon, the opposite is true.
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对于携带大量能量的光子而言
03:28
Protons are effectively tiny.
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质子的影响就很微小
03:30
Photons start off at very high energies
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光子出发时相对于到达表面时候而言
03:33
compared to when they're finally radiated from the Sun's surface.
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携带大量的能量
03:37
Now when we use a computer and a sophisticated solar interior model
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现在我们用电脑运算一下先进的太阳内部模型
03:42
to calculate the random walk equation with these changing quantities,
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计算出随机路程中数量的变化
03:46
it spits out the following number: 170,000 years.
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答案是17万年
03:52
Future discoveries about the Sun may refine this number further,
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未来的发现也许会精确这个数字
03:56
but for now, to the best of our understanding,
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但是现在我们最好的理解是
03:59
the light that's hitting your eyes today
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今天我们看到的阳光
04:01
spent 170,000 years pinballing its way towards the Sun's surface,
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经历了17万年跌跌撞撞的路途
04:07
plus eight miniscule minutes in space.
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别忘了还要再加上8分钟的太空之旅
04:10
In other words, that photon began its journey two ice ages ago,
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也就是说 在两个冰河世纪之前 人类刚开始穿衣服的时候
04:15
around the same time when humans first started wearing clothes.
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今天的阳光就已经启程了
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