What a planet needs to sustain life | Dave Brain

407,715 views ・ 2016-09-04

TED


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翻译人员: Yangyang Liu 校对人员: Amy Lu
00:12
I'm really glad to be here.
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我很高兴能在这里。
00:15
I'm glad you're here,
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很高兴你们也在这里,
00:16
because that would be a little weird.
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因为这会有点奇怪。
00:19
I'm glad we're all here.
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我很高兴我们都在这里。
00:22
And by "here," I don't mean here.
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我说的"这里",并不是指这里,
00:26
Or here.
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或者这里,
00:28
But here.
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而是这里。
00:29
I mean Earth.
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我指的是地球。
00:31
And by "we," I don't mean those of us in this auditorium,
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我说的"我们"并不是指 我们坐在会场里的人,
00:35
but life,
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而是生命,
00:37
all life on Earth --
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地球上所有的生命。
00:38
(Laughter)
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(笑声)
00:44
from complex to single-celled,
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从复杂的生命到单细胞的生命,
00:46
from mold to mushrooms
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从霉菌到蘑菇,
00:48
to flying bears.
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到会飞的熊。
00:50
(Laughter)
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(笑声)
00:53
The interesting thing is,
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有趣的是,
00:55
Earth is the only place we know of that has life --
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地球是我们已知的 唯一有生命的地方,
00:58
8.7 million species.
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870万种生物。
01:00
We've looked other places,
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我们曾经在其他星球寻找生命,
01:01
maybe not as hard as we should or we could,
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或许没有尽全力,
01:04
but we've looked and haven't found any;
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但我们确实没有发现过。
01:06
Earth is the only place we know of with life.
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地球是我们已知的 唯一有生命的地方,
01:09
Is Earth special?
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地球很特别吗?
01:11
This is a question I've wanted to know the answer to
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从我小时候起,
我就一直想要知道这个问题的答案,
01:14
since I was a small child,
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01:15
and I suspect 80 percent of this auditorium
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我觉得这个会场里80%的人
01:17
has thought the same thing and also wanted to know the answer.
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都曾经思考过同样的问题, 并且想要知道答案。
01:20
To understand whether there are any planets --
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为了知道是否有其他星球
01:23
out there in our solar system or beyond --
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—在我们太阳系中或是之外的—
01:25
that can support life,
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能够支持生命的存在,
01:26
the first step is to understand what life here requires.
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第一步就是要理解生命需要什么。
01:30
It turns out, of all of those 8.7 million species,
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事实表明, 虽然地球上有着870万种生命,
01:34
life only needs three things.
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但生命的存在只需要三样东西。
01:37
On one side, all life on Earth needs energy.
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首先,所有地球上的生命都需要能量。
01:39
Complex life like us derives our energy from the sun,
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复杂的生命,例如我们, 从太阳那里获得能量。
01:43
but life deep underground can get its energy
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但是在地底的生命则 通过其他方式,
01:45
from things like chemical reactions.
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比如化学反应,来获得能量。
01:47
There are a number of different energy sources
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在所有的星球上,
都有很多能够获得能量的方式。
01:49
available on all planets.
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01:51
On the other side,
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另一方面,
01:52
all life needs food or nourishment.
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所有的生命都需要食物和营养。
01:55
And this seems like a tall order, especially if you want a succulent tomato.
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这看起来很难满足,尤其是 如果你想吃一个多汁的番茄。
02:00
(Laughter)
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(笑声)
02:01
However, all life on Earth derives its nourishment
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但是,地球生命所需的全部营养
02:05
from only six chemical elements,
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都只基于六种化学元素,
02:07
and these elements can be found on any planetary body
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这些元素在太阳系中
所有的星体上都可以找到。
02:10
in our solar system.
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02:12
So that leaves the thing in the middle as the tall pole,
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中间那幅图中的东西
反而是最难得到的。
02:15
the thing that's hardest to achieve.
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02:17
Not moose, but water.
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不是那只鹿,而是水。
02:19
(Laughter)
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(笑声)
02:23
Although moose would be pretty cool.
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虽然那只鹿也很酷。
02:25
(Laughter)
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(笑声)
02:26
And not frozen water, and not water in a gaseous state, but liquid water.
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并且不是固态,也不是气态的水, 而是液态的水。
02:32
This is what life needs to survive, all life.
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水是所有生命的前提。
02:35
And many solar system bodies don't have liquid water,
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很多太阳系的天体上没有液态水,
02:39
and so we don't look there.
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所以就可以排除了。
02:40
Other solar system bodies might have abundant liquid water,
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其他的太阳系天体可能有充足的液态水,
02:43
even more than Earth,
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甚至比地球上还多,
02:45
but it's trapped beneath an icy shell,
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但是那些水被阻隔在冰盖下面,
02:47
and so it's hard to access, it's hard to get to,
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因此很难得到并加以利用。
02:49
it's hard to even find out if there's any life there.
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即使那里有生命,我们也很难找到。
02:53
So that leaves a few bodies that we should think about.
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所以只需要考虑 剩下的很少几个星球。
02:56
So let's make the problem simpler for ourselves.
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让我们进一步简化,
02:58
Let's think only about liquid water on the surface of a planet.
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先只考虑星球表面上 存在液态水的问题。
03:02
There are only three bodies to think about in our solar system,
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在太阳系中,只有三个星球的表面
03:05
with regard to liquid water on the surface of a planet,
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可能存在液态水,
03:07
and in order of distance from the sun, it's: Venus, Earth and Mars.
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按照距离太阳的远近, 他们是:金星、地球、火星。
03:13
You want to have an atmosphere for water to be liquid.
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你需要一个让水保持液态的大气层,
03:16
You have to be very careful with that atmosphere.
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需要非常小心这个大气层,
03:19
You can't have too much atmosphere, too thick or too warm an atmosphere,
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不能太多,不能太厚,不能太热,
03:22
because then you end up too hot like Venus,
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因为如果太热,像金星一样,
03:25
and you can't have liquid water.
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就无法保持液态水。
03:27
But if you have too little atmosphere and it's too thin and too cold,
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但如果大气太少,太薄或太冷,
03:31
you end up like Mars, too cold.
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结果就像火星,太冷。
03:33
So Venus is too hot, Mars is too cold,
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所以金星太热,火星太冷,
03:36
and Earth is just right.
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地球刚刚好。
03:37
You can look at these images behind me and you can see automatically
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从我身后的图片,你很容易看出
03:41
where life can survive in our solar system.
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哪个星球能让生命存活。
03:44
It's a Goldilocks-type problem,
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这是个“金发姑娘问题”,
03:45
and it's so simple that a child could understand it.
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即使是小孩子也会明白。
03:49
However,
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但是,
03:51
I'd like to remind you of two things
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我想提醒你们,
金发姑娘的故事中, 有两件我们不太在意的事,
03:54
from the Goldilocks story that we may not think about so often
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03:57
but that I think are really relevant here.
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在这里却非常关键。
04:00
Number one:
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第一:
04:02
if Mama Bear's bowl is too cold
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如果金发姑娘走进房间的时候,
04:05
when Goldilocks walks into the room,
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熊妈妈的碗太凉,
04:08
does that mean it's always been too cold?
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是否意味着碗会一直很凉呢?
04:11
Or could it have been just right at some other time?
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会不会某一个时间, 它的温度会变得刚刚好呢?
04:15
When Goldilocks walks into the room determines the answer
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金发姑娘走进房间的时间,
决定了我们能获得什么样的答案。
04:19
that we get in the story.
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04:21
And the same is true with planets.
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对于行星是同样的道理,
04:22
They're not static things. They change.
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他们不是一成不变的,他们在改变,
04:24
They vary. They evolve.
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在变化,在发展。
04:26
And atmospheres do the same.
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大气层也是一样。
04:28
So let me give you an example.
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我举个例子,
04:30
Here's one of my favorite pictures of Mars.
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这是我最喜欢的一张火星的照片,
04:32
It's not the highest resolution image, it's not the sexiest image,
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它的分辨率不算最高, 也不算最漂亮,
04:35
it's not the most recent image,
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也不是最近的照片,
04:37
but it's an image that shows riverbeds cut into the surface of the planet;
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但它展示了火星表面的河床。
04:41
riverbeds carved by flowing, liquid water;
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这些河床是由流动的液态水,
04:45
riverbeds that take hundreds or thousands or tens of thousands of years to form.
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经过成千上万年的侵蚀所形成。
04:50
This can't happen on Mars today.
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但如今火星上不会再形成河床了,
04:52
The atmosphere of Mars today is too thin and too cold
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现在火星的大气层太薄太冷,
04:54
for water to be stable as a liquid.
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液态水已经无法稳定存在。
04:56
This one image tells you that the atmosphere of Mars changed,
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这张图显示了火星大气的变化,
05:01
and it changed in big ways.
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并且是巨大的变化。
05:03
And it changed from a state that we would define as habitable,
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它从一个我们认为 可居住的状态变化而来,
05:08
because the three requirements for life were present long ago.
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因为它很久以前呈现出了 那三个生命存活的要素。
05:13
Where did that atmosphere go
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那个可以维持液态水的 大气层哪去了?
05:15
that allowed water to be liquid at the surface?
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05:17
Well, one idea is it escaped away to space.
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一种观点是大气逃逸到了太空,
05:21
Atmospheric particles got enough energy to break free
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大气粒子获得了脱离星球重力的能量,
05:24
from the gravity of the planet,
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05:25
escaping away to space, never to return.
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逃逸到太空,再也无法回来。
05:28
And this happens with all bodies with atmospheres.
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在所有存在大气层的天体上都会发生。
05:31
Comets have tails
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彗星的尾巴,
05:32
that are incredibly visible reminders of atmospheric escape.
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就是大气逃逸的一种直观表现。
05:35
But Venus also has an atmosphere that escapes with time,
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但金星同样有正在逃逸的大气层,
05:39
and Mars and Earth as well.
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火星和地球也一样,
05:40
It's just a matter of degree and a matter of scale.
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只是逃逸的程度和规模的问题。
05:44
So we'd like to figure out how much escaped over time
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我们希望计算出逃逸的速度,
05:46
so we can explain this transition.
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以解释这种变迁。
05:48
How do atmospheres get their energy for escape?
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大气如何获得逃逸的能量?
05:51
How do particles get enough energy to escape?
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粒子是怎么获得足够能量的?
05:53
There are two ways, if we're going to reduce things a little bit.
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简而言之有两种方式,
05:56
Number one, sunlight.
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第一,太阳光。
05:58
Light emitted from the sun can be absorbed by atmospheric particles
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太阳发出的光可以被大气粒子吸收
06:01
and warm the particles.
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并被加温。
06:03
Yes, I'm dancing, but they --
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是的,我在跳舞,但它们…
06:05
(Laughter)
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(笑声)
06:07
Oh my God, not even at my wedding.
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天哪,我结婚那天都没跳过舞。
06:09
(Laughter)
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(笑声)
06:11
They get enough energy to escape and break free
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通过加温,它们获得了冲破星球重力
06:14
from the gravity of the planet just by warming.
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以逃逸的足够能量。
06:16
A second way they can get energy is from the solar wind.
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它们可以获得能量的第二种方式是, 太阳风。
06:19
These are particles, mass, material, spit out from the surface of the sun,
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太阳表面会发射出例子、质量、材料,
06:24
and they go screaming through the solar system
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它们以400千米每秒的速度
06:27
at 400 kilometers per second,
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在太阳系中冲撞,
06:29
sometimes faster during solar storms,
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有太阳风暴时会更快。
06:31
and they go hurtling through interplanetary space
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它们在星际空间中,
06:34
towards planets and their atmospheres,
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朝着行星和大气层飞奔,
06:37
and they may provide energy
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它们也会为大气粒子 的逃逸提供能量。
06:38
for atmospheric particles to escape as well.
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06:41
This is something that I'm interested in,
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我对这个很感兴趣,
06:43
because it relates to habitability.
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因为这会和可居住相关。
06:45
I mentioned that there were two things about the Goldilocks story
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我刚才提到金发姑娘故事中
06:48
that I wanted to bring to your attention and remind you about,
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有两个我们需要关注的问题,
06:51
and the second one is a little bit more subtle.
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第二个问题会更微妙。
06:53
If Papa Bear's bowl is too hot,
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如果熊爸爸的碗太烫,
06:58
and Mama Bear's bowl is too cold,
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而熊妈妈的碗太凉,
07:03
shouldn't Baby Bear's bowl be even colder
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如果按这个规律,
熊宝宝的碗不是应该更凉吗?
07:07
if we're following the trend?
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07:10
This thing that you've accepted your entire life,
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这件你一直没怀疑的事,
07:12
when you think about it a little bit more, may not be so simple.
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如果仔细一想,可能没那么简单。
07:16
And of course, distance of a planet from the sun determines its temperature.
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当然, 大气温度取决于行星和太阳的距离,
07:20
This has to play into habitability.
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这也决定了可居住性。
07:22
But maybe there are other things we should be thinking about.
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但可能有其他我们需要考虑的事,
07:25
Maybe it's the bowls themselves
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可能碗本身,
07:27
that are also helping to determine the outcome in the story,
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也可以决定故事的结局,
07:30
what is just right.
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这恰恰是事实。
07:32
I could talk to you about a lot of different characteristics
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我讲一个不太一样的特性,
07:35
of these three planets
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它可以影响这三个行星的可居住性,
07:36
that may influence habitability,
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07:38
but for selfish reasons related to my own research
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但由于我的一点私心, 因为这是我自己的研究,
07:41
and the fact that I'm standing up here holding the clicker and you're not --
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并且遥控器在我这儿 而不在你们手里,
07:44
(Laughter)
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(笑声)
07:45
I would like to talk for just a minute or two
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我想花一两分钟
07:47
about magnetic fields.
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聊一下磁场。
07:49
Earth has one; Venus and Mars do not.
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地球有磁场,而金星和火星没有。
07:52
Magnetic fields are generated in the deep interior of a planet
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磁场是从星球的内部产生,
07:55
by electrically conducting churning fluid material
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由电荷驱动旋转的流体,
07:59
that creates this big old magnetic field that surrounds Earth.
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形成了地球周围的 巨大而古老的磁场。
08:02
If you have a compass, you know which way north is.
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你用指南针可以分辨出哪里是北,
08:05
Venus and Mars don't have that.
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但金星和火星没有磁场,
08:06
If you have a compass on Venus and Mars,
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如果你在金星和火星上用指南针,
08:08
congratulations, you're lost.
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恭喜,你迷路了。
08:09
(Laughter)
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(笑声)
08:11
Does this influence habitability?
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这会影响可居住性吗?
08:15
Well, how might it?
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会怎么影响?
08:17
Many scientists think that a magnetic field of a planet
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有些科学家认为 行星的磁场为大气层提供保护,
08:19
serves as a shield for the atmosphere,
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08:22
deflecting solar wind particles around the planet
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通过力场效应影响带电粒子,
08:25
in a bit of a force field-type effect
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08:27
having to do with electric charge of those particles.
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从而改变太阳风粒子的方向。
08:30
I like to think of it instead as a salad bar sneeze guard for planets.
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我倒喜欢把它比喻成 食品柜台的防喷嚏罩。
08:34
(Laughter)
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(笑声)
08:36
And yes, my colleagues who watch this later will realize
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是的,我的同事看到这个后,
08:40
this is the first time in the history of our community
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会发现这是我们圈里有史以来
08:42
that the solar wind has been equated with mucus.
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第一次把太阳风等同成喷嚏口水。
08:45
(Laughter)
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(笑声)
08:48
OK, so the effect, then, is that Earth may have been protected
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因此,地球可能因为存在磁场,
08:52
for billions of years,
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08:53
because we've had a magnetic field.
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而被保护了数十亿年,
08:55
Atmosphere hasn't been able to escape.
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使得大气层无法逃逸。
08:57
Mars, on the other hand, has been unprotected
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然而火星没有受到这样的保护,
08:59
because of its lack of magnetic field,
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因为没有磁场,
09:01
and over billions of years,
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经历了数十亿年,
09:03
maybe enough atmosphere has been stripped away
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足够的大气层逃逸出去
09:05
to account for a transition from a habitable planet
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使得它变成了不可居住的星球,
09:08
to the planet that we see today.
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就是今天我们看到的样子。
09:11
Other scientists think that magnetic fields
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其他科学家认为磁场
09:14
may act more like the sails on a ship,
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更像是船上的帆,
09:16
enabling the planet to interact with more energy from the solar wind
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让行星可以通过太阳风 获得更多能量,
09:22
than the planet would have been able to interact with by itself.
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比星球自己产生的更多。
09:25
The sails may gather energy from the solar wind.
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船帆可能从太阳风中收集能量。
09:27
The magnetic field may gather energy from the solar wind
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但磁场从太阳风中吸收能量,
09:30
that allows even more atmospheric escape to happen.
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会让更多的大气逃逸。
09:33
It's an idea that has to be tested,
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这个想法还有待验证,
09:36
but the effect and how it works
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但它的影响和原理也是显而易见的。
09:37
seems apparent.
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09:39
That's because we know
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因为我们知道,
09:40
energy from the solar wind is being deposited into our atmosphere
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太阳风中的能量会被存储到 地球的大气中。
09:43
here on Earth.
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09:44
That energy is conducted along magnetic field lines
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这些能量随着磁场被导入两极,
09:47
down into the polar regions,
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09:48
resulting in incredibly beautiful aurora.
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形成绚丽无比的极光。
09:50
If you've ever experienced them, it's magnificent.
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如果你体验过,那真是非常壮丽。
09:53
We know the energy is getting in.
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我们知道能量正在源源不断的进入,
09:55
We're trying to measure how many particles are getting out
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我们也试着测量有多少粒子跑出去,
09:58
and if the magnetic field is influencing this in any way.
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以及磁场是不是在影响这个过程。
10:02
So I've posed a problem for you here,
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所以我刚刚抛给各位一个问题,
10:05
but I don't have a solution yet.
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但我还没有答案,
10:06
We don't have a solution.
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我们没有答案,
10:08
But we're working on it. How are we working on it?
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但我们正在努力。 我们怎么做的呢?
10:11
Well, we've sent spacecraft to all three planets.
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我们往三颗行星都发射了航天器。
10:13
Some of them are orbiting now,
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有些已经在轨运行了,
10:14
including the MAVEN spacecraft which is currently orbiting Mars,
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包括正围绕火星运行的 MAVEN 航天器,
10:18
which I'm involved with and which is led here,
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这个项目由这里的 科罗拉多大学主导,
10:21
out of the University of Colorado.
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我也参与了这个项目。
10:23
It's designed to measure atmospheric escape.
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它被设计用来观测大气逃逸,
10:26
We have similar measurements from Venus and Earth.
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在金星和地球, 我们也有类似的测量项目。
10:28
Once we have all our measurements,
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一旦我们完成测量,
10:30
we can combine all these together, and we can understand
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综合分析这些数据,我们就可以了解
10:33
how all three planets interact with their space environment,
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这三颗行星是如何与他们的太空环境
10:36
with the surroundings.
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以及自身周围的环境相互作用。
10:38
And we can decide whether magnetic fields are important for habitability
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我们也可以清楚, 磁场对可居住性是否关键。
10:41
or not.
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10:42
Once we have that answer, why should you care?
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一旦我们有了答案, 你们为什么会在意?
10:45
I mean, I care deeply ...
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我是说,我很在意…
10:48
And financially as well, but deeply.
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财务上很在意,但也确实很在意…
10:50
(Laughter)
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(笑声)
10:52
First of all, an answer to this question
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首先,这个问题的答案
10:54
will teach us more about these three planets,
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会告诉我们更多关于 这三颗行星的事情,
10:56
Venus, Earth and Mars,
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金星、地球、火星,
10:58
not only about how they interact with their environment today,
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不只是它们今天如何与 周边环境互相作用,
11:00
but how they were billions of years ago,
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更多是几十亿年前的情形,
11:02
whether they were habitable long ago or not.
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很久以前它们是否是可居住的。
11:04
It will teach us about atmospheres
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它会告诉更多关于围绕着我们、
11:06
that surround us and that are close.
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与我们息息相关的大气层的事情。
11:09
But moreover, what we learn from these planets
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此外,从这些行星身上学到的经验,
11:11
can be applied to atmospheres everywhere,
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可以用在其他任何星球的大气层。
11:14
including planets that we're now observing around other stars.
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包括我们正在观测的 其他恒星系的行星,
11:17
For example, the Kepler spacecraft,
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比如,建造并管理于博尔德的 开普勒望远镜,
11:19
which is built and controlled here in Boulder,
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11:22
has been observing a postage stamp-sized region of the sky
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近几年一直在观测
一块邮票大小的天空区域,
11:25
for a couple years now,
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11:27
and it's found thousands of planets --
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它已经发现了几千颗行星,
11:29
in one postage stamp-sized region of the sky
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仅仅在一块邮票大小的天空,
11:32
that we don't think is any different from any other part of the sky.
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和别的区域并没有什么不同。
11:36
We've gone, in 20 years,
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在这20年里,
11:38
from knowing of zero planets outside of our solar system,
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我们从对太阳系外的行星一无所知,
11:42
to now having so many,
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到目前我们知道这么多,
11:44
that we don't know which ones to investigate first.
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以至于我们不知道该从哪一个下手。
11:49
Any lever will help.
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每一条线索都很重要。
11:52
In fact, based on observations that Kepler's taken
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事实上,从开普勒的观测
11:56
and other similar observations,
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以及其他类似的观测中,
11:58
we now believe that,
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我们目前相信,
11:59
of the 200 billion stars in the Milky Way galaxy alone,
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仅在银河系的2000亿颗恒星中,
12:04
on average, every star has at least one planet.
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通常每颗恒星都至少有一颗行星。
12:10
In addition to that,
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除此之外,
12:12
estimates suggest there are somewhere between 40 billion and 100 billion
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这些行星中, 据估算有400亿至1000亿颗
12:18
of those planets that we would define as habitable
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可以被定义为可居住的,
12:23
in just our galaxy.
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这仅仅是在我们的银河系。
12:26
We have the observations of those planets,
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我们在观察这些行星,
12:28
but we just don't know which ones are habitable yet.
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但我们还不知道哪些是适合居住的。
12:31
It's a little bit like being trapped on a red spot --
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就像被困在这个红点上一样,
12:34
(Laughter)
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(笑声)
12:35
on a stage
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在台上,
12:38
and knowing that there are other worlds out there
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并且知道这外面有其他的世界,
12:43
and desperately wanting to know more about them,
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拼命想要了解它们,
12:47
wanting to interrogate them and find out if maybe just one or two of them
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想调查并找到是否有那么一两个
12:51
are a little bit like you.
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和你有点像。
12:54
You can't do that. You can't go there, not yet.
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但你做不到, 你还无法到达那里。
12:56
And so you have to use the tools that you've developed around you
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所以你只能用你身边的工具,
13:00
for Venus, Earth and Mars,
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金星,地球,火星,
13:02
and you have to apply them to these other situations,
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用他们来推演其他的情况,
13:05
and hope that you're making reasonable inferences from the data,
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并祈祷你正在做有意义的尝试,
13:09
and that you're going to be able to determine the best candidates
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你将可以做出最佳的判断,
13:12
for habitable planets, and those that are not.
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关于哪些星球可居住,哪些不可以。
13:16
In the end, and for now, at least,
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最终,至少是目前,
13:18
this is our red spot, right here.
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这是我们的红点,就在这里。
13:22
This is the only planet that we know of that's habitable,
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这是我们唯一知道的宜居的星球,
13:25
although very soon we may come to know of more.
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虽然可能很快就会发现还有其他的。
13:28
But for now, this is the only habitable planet,
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但目前,这是唯一宜居的星球,
13:31
and this is our red spot.
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这是我们的红点。
13:33
I'm really glad we're here.
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我很高兴我们在这里。
13:36
Thanks.
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谢谢。
13:37
(Applause)
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(掌声)
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