ABOUT THE SPEAKER
James Green - Space physicist
James Green leads NASA's solar system exploration and astrobiology research.

Why you should listen

Dr. James Green began his career at NASA 35 years ago at the Marshall Space Flight Center, where he developed and managed the Space Physics Analysis Network. It provided scientists all over the world rapid access to data and resources. As NASA's Director of Planetary Science he leads NASA's solar system exploration and astrobiology research.

Green received his Ph.D. in Space Physics from the University of Iowa in 1979 and began working in the Magnetospheric Physics Branch at NASA's Marshall Space Flight Center (MSFC) in 1980. At Marshall, Green developed and managed the Space Physics Analysis Network that provided scientists all over the world with rapid access to data, to other scientists, and to specific NASA computer and information resources. In addition, Green was a Safety Diver in the Neutral Buoyancy tank making over 150 dives until left MSFC in 1985.

From 1985 to 1992 Green was the head of the National Space Science Data Center (NSSDC) at Goddard Space Flight Center (GSFC). The NSSDC is NASA's largest space science data archive. In 1992, he became the Chief of the Space Science Data Operations Office until 2005, when he became the Chief of the Science Proposal Support Office. While at GSFC, Green was a co-investigator and the Deputy Project Scientist on the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) mission. He has written over 100 scientific articles in refereed journals involving various aspects of the Earth's and Jupiter's magnetospheres and over 50 technical articles on various aspects of data systems and networks.

In August 2006, Green became the Director of the Planetary Science Division at NASA Headquarters. Over his career, Green has received numerous awards. In 1988, he received the Arthur S. Flemming award given for outstanding individual performance in the federal government and was awarded Japan's Kotani Prize in 1996 in recognition of his international science data management activities.

More profile about the speaker
James Green | Speaker | TED.com
TED Talks Live

James Green: 3 moons and a planet that could have alien life

詹姆斯·格林: 可能存在生命的三个卫星和一个行星

Filmed:
1,837,212 views

地球以外存在生命吗?跟随美国太空总署行星科学主任詹姆斯·格林,一同探索那些太阳系里最可能存在着外星生命的地方。
- Space physicist
James Green leads NASA's solar system exploration and astrobiology research. Full bio

Double-click the English transcript below to play the video.

00:12
Is there life beyond Earth地球
in our solar太阳能 system系统?
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在地球以外,太阳系里还有生命吗?
00:17
Wow, what a powerful强大 question.
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哇,多么掷地有声的问题!
00:20
You know, as a scientist科学家 --
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作为一名科学家——
行星科学家——
00:22
planetary行星 scientist科学家 --
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我们很久以来都没有认真的
考虑过这个问题。
00:23
we really didn't take that
very seriously认真地 until直到 recently最近.
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00:28
Carl卡尔 Sagan萨根 always said,
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卡尔·萨根
(译注:美国天文学家)常说,
”非凡的断言需要有非凡的证据”。
00:30
"It takes extraordinary非凡 evidence证据
for extraordinary非凡 claims索赔."
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00:36
And the claims索赔 of having life beyond Earth地球
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地球之外有生命的断言
00:41
need to be definitive明确,
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必须是明确的,
必须是响亮的,
00:43
they need to be loud
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还需要证据充分,这样我们才会相信。
00:45
and they need to be everywhere到处
for us to be able能够 to believe it.
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00:50
So how do we make this journey旅程?
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那么,我们要如何开始这段旅行呢?
00:54
What we decided决定 to do
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我们决定
首先去寻找生命的基本要素。
00:55
is first look for
those ingredients配料 for life.
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01:00
The ingredients配料 of life are:
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生命的基本要素是:
液态水——
01:02
liquid液体 water --
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我们需要溶剂,
01:04
we have to have a solvent溶剂,
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不能是冰,必须是液态的。
01:05
can't be ice, has to be liquid液体.
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01:08
We also have to have energy能源.
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我们还需要能量。
有机物质也是必不可少的——
01:10
We also have to have organic有机 material材料 --
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这些都是组成我们的生命体,
01:13
things that make us up,
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以及供我们消耗的东西。
01:16
but also things that we need to consume消耗.
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01:19
So we have to have these elements分子
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环境中必须长期存在
这些元素
01:22
in environments环境 for long periods of time
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01:25
for us to be able能够
to be confident信心 that life,
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才会让我们相信:
生命在诞生的那一刻,
01:28
in that moment时刻 when it starts启动,
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能够迸发出火花,
并且能够成长和演变。
01:31
can spark火花 and then grow增长 and evolve发展.
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01:35
Well, I have to tell you
that early in my career事业,
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我必须坦白,
在我职业生涯早期,
01:39
when we looked看着 at those three elements分子,
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当我们研究这三个要素时,
我并不相信它们能在地球之外
01:41
I didn't believe
that they were beyond Earth地球
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存在足够长的时间,或达到足够的规模。
01:44
in any length长度 of time
and for any real真实 quantity数量.
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为什么?让我们看看太阳系的行星:
01:48
Why? We look at the inner planets行星.
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金星太热——所以没水。
01:50
Venus金星 is way too hot -- it's got no water.
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火星——干旱贫瘠,
01:53
Mars火星 -- dry and arid干旱.
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也不会有水。
01:55
It's got no water.
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在太阳系中比火星更远的地方,
01:57
And beyond Mars火星,
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水全部冻成了固态的冰。
01:58
the water in the solar太阳能 system系统
is all frozen冻结的.
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02:03
But recent最近 observations意见
have changed all that.
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但是最近的观测改变了这一切。
现在它把我们的注意力
带到了正确的地方,
02:07
It's now turning车削 our attention注意
to the right places地方
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让我们去进一步观察,
02:11
for us to take a deeper更深 look
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并且真正开始回答生命的问题。
02:13
and really start开始 to answer回答
our life question.
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02:18
So when we look out into the solar太阳能 system系统,
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那么,当我们探索太阳系时,
生命可能存在于哪里呢?
02:21
where are the possibilities可能性?
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02:23
We're concentrating集中 our attention注意
on four locations地点.
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我们将注意力集中在以下四处:
02:27
The planet行星 Mars火星
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火星
02:29
and then three moons月亮 of the outer planets行星:
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和更远的三个卫星:
02:33
Titan泰坦, Europa欧罗巴 and small Enceladus土卫二.
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泰坦(土卫六),欧罗巴(木卫二)
和小小的恩赛拉多斯(土卫二)。
02:38
So what about Mars火星?
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火星到底是什么情况呢?
让我们看看证据。
02:40
Let's go through通过 the evidence证据.
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02:43
Well, Mars火星 we thought
was initially原来 moon-like月亮般的:
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起初我们以为火星像月亮一样:
布满陨石坑,荒凉,没有生命。
02:47
full充分 of craters陨石坑, arid干旱 and a dead world世界.
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02:52
And so about 15 years年份 ago,
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大约在15年前,
我们开始了一系列登陆火星的任务,
02:55
we started开始 a series系列
of missions任务 to go to Mars火星
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去查看那里过去是否有水存在过,
02:58
and see if water existed存在
on Mars火星 in its past过去
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还因此改变了它的地质。
03:03
that changed its geology地质学.
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我们应该可以观察得到。
03:05
We ought应该 to be able能够 to notice注意 that.
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03:08
And indeed确实 we started开始
to be surprised诧异 right away.
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而实际上,我们一开始就很惊讶。
高清图片显示,
那里有三角洲,河谷和沟渠,
03:11
Our higher更高 resolution解析度 images图片
show显示 deltas三角洲 and river valleys山谷 and gulleys溪沟
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它们过去都曾存在过。
03:16
that were there in the past过去.
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事实上,
03:19
And in fact事实,
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好奇号探测车
03:20
Curiosity好奇心 --
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在火星表面上漫游已经有三年了——
03:21
which哪一个 has been roving漫游 on the surface表面
now for about three years年份 --
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我们看到它停在一条古老的河床上,
03:26
has really shown显示 us that it's sitting坐在
in an ancient river bed,
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那里曾有过湍急的水流。
03:31
where water flowed流入 rapidly急速.
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03:34
And not for a little while,
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时间还不短,
可能曾持续过数亿年之久。
03:35
perhaps也许 hundreds数以百计 of millions百万 of years年份.
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03:39
And if everything was there,
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如果所有要素都存在,
包括有机物在内,
03:40
including包含 organics有机物,
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也许生命曾在那里诞生过。
03:41
perhaps也许 life had started开始.
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好奇号还在红土上打了洞,
03:43
Curiosity好奇心 has also
drilled in that red soil
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并且发现了其他物质。
03:46
and brought up other material材料.
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我们看到后非常兴奋,
03:48
And we were really excited兴奋
when we saw that.
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因为那不是红色的物质,
03:51
Because it wasn't red Mars火星,
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而是灰色的,
03:53
it was gray灰色 material材料,
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火星地表下面是灰色的。
03:54
it's gray灰色 Mars火星.
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我们把挖出来的东西带回探测车,
03:56
We brought it into the rover流浪者,
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03:57
we tasted it,
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仔细地分析了它,
你们猜怎么着?
03:59
and guess猜测 what?
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我们分析出了有机物——
04:00
We tasted organics有机物 --
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碳,氢,氧,
04:02
carbon, hydrogen, oxygen,
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氮,磷,硫——
04:05
nitrogen, phosphorus, sulfur --
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统统都有。
04:07
they were all there.
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所以过去的火星
04:09
So Mars火星 in its past过去,
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曾有很多的水,
04:11
with a lot of water,
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也许存在过很长时间,
04:13
perhaps也许 plenty丰富 of time,
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可能有过生命,
04:15
could have had life,
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可能有过生命的火花,
04:16
could have had that spark火花,
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04:18
could have grown长大的.
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还可能繁衍过一段时间。
那时候的生命还在么?
04:20
And is that life still there?
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我们不知道。
04:22
We don't know that.
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但是几年前,
04:24
But a few少数 years年份 ago
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我们开始观察一些陨石坑。
04:26
we started开始 to look at a number of craters陨石坑.
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在夏季,
04:29
During the summer夏季,
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陨石坑的边沿会出现深色的线条。
04:30
dark黑暗 lines线 would appear出现
down the sides双方 of these craters陨石坑.
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随着我们观察得越多,
04:34
The more we looked看着,
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看到的陨石坑越多,
04:36
the more craters陨石坑 we saw,
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这样的特征也越多。
04:37
the more of these features特征.
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04:38
We now know more than a dozen of them.
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现在已知的已经超过十二个了。
04:42
A few少数 months个月 ago the fairy仙女 tale故事 came来了 true真正.
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几个月前,童话故事成真了!
我们向世界宣布,
我们已经知道这些条纹是什么了。
04:46
We announced公布 to the world世界
that we know what these streaks条纹 are.
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是液态水。
04:50
It's liquid液体 water.
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04:53
These craters陨石坑 are weeping
during the summer夏季.
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这些陨石坑在夏天浸出水分。
这些液态水顺着陨石坑向下流。
04:56
Liquid液体 water is flowing流动
down these craters陨石坑.
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我们接下来要做什么——
05:00
So what are we going to do now --
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在发现了液态水之后?
05:02
now that we see the water?
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05:04
Well, it tells告诉 us that Mars火星 has
all the ingredients配料 necessary必要 for life.
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这说明火星拥有生命的所有必需成分。
在过去,可能它的北半球有三分之二
05:09
In its past过去 it had perhaps也许
two-thirds三分之二 of its northern北方 hemisphere半球 --
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都曾是海洋。
05:14
there was an ocean海洋.
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现在它有冒出的水流。
05:15
It has weeping water right now.
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星球表面有液态水。
05:17
Liquid液体 water on its surface表面.
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它有有机物。
05:19
It has organics有机物.
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它有一切合适(孕育生命)的条件。
05:21
It has all the right conditions条件.
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05:24
So what are we going to do next下一个?
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那么我们接下来要做什么呢?
我们将开展一系列任务
05:26
We're going to launch发射 a series系列 of missions任务
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开始寻找火星上的生命。
05:28
to begin开始 that search搜索 for life on Mars火星.
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现在行动要比以往
任何时候都更有吸引力。
05:32
And now it's more appealing吸引人的
than ever before.
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05:35
As we move移动 out into the solar太阳能 system系统,
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在离地球更远的太阳系里,
有一个小小的土卫二。
05:38
here's这里的 the tiny moon月亮 Enceladus土卫二.
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它不在我们以往公认的宜居区域内,
05:41
This is not in what we call
the traditional传统 habitable可居住 zone,
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也就是靠近太阳的区域。
05:44
this area around the sun太阳.
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这里离太阳很远。
05:46
This is much further进一步 out.
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这个星球应该像个
被冰层覆盖的硅酸盐核心。
05:48
This object目的 should be
ice over a silicate硅酸盐 core核心.
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05:54
But what did we find?
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但我们找到了什么?
自2006年起,卡西尼太空船就在那里,
05:55
Cassini卡西尼 was there since以来 2006,
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在飞过土卫二的几年后,再回过头看,
05:58
and after a couple一对 years年份
looked看着 back after it flew by Enceladus土卫二
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我们都大吃一惊。
06:03
and surprised诧异 us all.
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06:04
Enceladus土卫二 is blasting爆破 sheets床单 of water
out into the solar太阳能 system系统
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土卫二在向太阳系喷出一片片的水,
再回落到它的表面。
06:10
and sloshing晃动 back down onto the moon月亮.
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06:13
What a fabulous极好 environment环境.
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多么美妙的环境啊。
卡西尼太空船几个月前
又从这些飞溅的水流中穿过,
06:15
Cassini卡西尼 just a few少数 months个月 ago
also flew through通过 the plume,
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它检测到了硅酸盐颗粒。
06:20
and it measured测量 silicate硅酸盐 particles粒子.
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06:23
Where does the silica二氧化硅 come from?
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这些硅从哪来的?
它肯定是从海底来的。
06:25
It must必须 come from the ocean海洋 floor地板.
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06:28
The tidal潮汐 energy能源 is generated产生 by Saturn土星,
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土星产生的潮汐动能
拉扯,挤压着这个星球——
06:31
pulling and squeezing挤压 this moon月亮 --
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正融化那里的冰,
06:34
is melting融化 that ice,
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形成着海洋。
06:35
creating创建 an ocean海洋.
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这潮汐能同样
拉扯挤压着硅酸盐核心。
06:37
But it's also doing that to the core核心.
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06:40
Now, the only thing that we can think of
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我们唯一能想到
地球上类似的现象是——
06:42
that does that here on Earth地球
as an analogy比喻 ...
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06:46
are hydrothermal热液 vents通风口.
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深海热泉。
06:49
Hydrothermal水热 vents通风口 deep in our ocean海洋
were discovered发现 in 1977.
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深海热泉在1977年的时候
在海洋深处被发现。
海洋学家们对此非常惊讶。
06:55
Oceanographers海洋学家 were completely全然 surprised诧异.
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06:58
And now there are thousands数千
of these below下面 the ocean海洋.
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如今在海洋之下
有成千上万这样的深海热泉。
07:03
What do we find?
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我们找到了什么?
当海洋学家们研究这些深海热泉时发现
07:04
The oceanographers海洋学家, when they go
and look at these hydrothermal热液 vents通风口,
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那里有富饶的生命,
07:07
they're teeming丰富的 with life,
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不管水是酸性的还是碱性的——
07:09
regardless而不管 of whether是否 the water
is acidic酸性 or alkaline碱性 --
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这不重要。
07:13
doesn't matter.
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地球上的深海热泉是生命的绝佳住所。
07:15
So hydrothermal热液 vents通风口 are
a fabulous极好 abode住所 for life here on Earth地球.
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07:20
So what about Enceladus土卫二?
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那么土卫二呢?
07:23
Well, we believe because it has water
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我们相信因为它有水,
并且在相当长的一段时间里拥有水,
07:26
and has had it for
a significant重大 period of time,
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07:29
and we believe it has hydrothermal热液 vents通风口
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加上我们认为它有深海热泉,
以及适合的有机物质。
07:33
with perhaps也许 the right organic有机 material材料,
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07:36
it is a place地点 where life could exist存在.
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那是一个生命可能存在的地方。
并且不仅仅是微生物——
07:40
And not just microbial微生物 --
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可能存在更复杂的生命,
因为它有足够的时间去进化。
07:42
maybe more complex复杂
because it's had time to evolve发展.
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07:47
Another另一个 moon月亮, very similar类似,
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另一个非常相似的卫星,
木卫二。
07:50
is Europa欧罗巴.
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伽利略号在1996年时探访了木星系统,
07:52
Galileo伽利略 visited参观 Jupiter's木星 system系统 in 1996
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对木卫二进行了详细的观察。
07:58
and made制作 fabulous极好 observations意见 of Europa欧罗巴.
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08:01
Europa欧罗巴, we also know,
has an under-the-ice下的冰 crust脆皮 ocean海洋.
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我们知道木卫二拥有
存在于冰层下的海洋。
伽利略号告诉了我们这些,
但我们从未看到过任何的片状水。
08:06
Galileo伽利略 mission任务 told us that,
but we never saw any plumes羽毛.
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因为我们从未找寻过它们。
08:11
But we didn't look for them.
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08:13
Hubble哈勃,
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哈勃望远镜
就在几年前
08:14
just a couple一对 years年份 ago,
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观察木卫二时,
08:16
observing观察 Europa欧罗巴,
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看到了片状水,
08:19
saw plumes羽毛 of water
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它们从南半球的裂缝中喷洒出来,
08:21
spraying from the cracks裂缝
in the southern南部的 hemisphere半球,
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就跟土卫二一模一样。
08:24
just exactly究竟 like Enceladus土卫二.
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08:29
These moons月亮,
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这些卫星
不在我们称作传统宜居地的区域,
08:31
which哪一个 are not in what we call
a traditional传统 habitable可居住 zone,
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而在太阳系更远的地方,
08:35
that are out in the solar太阳能 system系统,
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却拥有着液态水。
08:37
have liquid液体 water.
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如果那里有有机物的话,
08:39
And if there are organics有机物 there,
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那里就可能有生命。
08:41
there may可能 be life.
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08:43
This is a fabulous极好 set of discoveries发现
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这是一系列绝佳的发现,
因为这些卫星已经在这样的环境中
08:45
because these moons月亮
have been in this environment环境 like that
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存在了数十亿年。
08:50
for billions数十亿 of years年份.
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08:53
Life started开始 here on Earth地球, we believe,
after about the first 500 million百万,
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我们相信地球上的生命
开始于地球形成5亿年之后,
08:58
and look where we are.
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看看现在的我们(进化的程度)。
09:01
These moons月亮 are fabulous极好 moons月亮.
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这些卫星让人难以置信。
09:04
Another另一个 moon月亮 that we're
looking at is Titan泰坦.
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我们在研究的另一个卫星是土卫六。
09:08
Titan泰坦 is a huge巨大 moon月亮 of Saturn土星.
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土卫六是土星的一个非常大的卫星。
它可能比水星还要大很多。
09:10
It perhaps也许 is much larger
than the planet行星 Mercury.
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09:14
It has an extensive广泛 atmosphere大气层.
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它有着广阔的大气层。
非常的广阔——
09:17
It's so extensive广泛 --
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主要成分是氮气,
还有一点点甲烷和乙烷——
09:18
and it's mostly大多 nitrogen
with a little methane甲烷 and ethane乙烷 --
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所以你需要用雷达来观测它。
09:23
that you have to peer窥视
through通过 it with radar雷达.
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在它的表面,
卡西尼号发现了液态水。
09:25
And on the surface表面,
Cassini卡西尼 has found发现 liquid液体.
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09:29
We see lakes湖泊 ...
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我们看到了湖泊——
09:32
actually其实 almost几乎 the size尺寸
of our Black黑色 Sea in some places地方.
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实际上,某些地方的湖几乎
跟我们的黑海一样大。
然而这块地方并不是液态水;
09:36
And this area is not liquid液体 water;
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它实际上是甲烷(译注:沼气)。
09:39
it's methane甲烷.
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09:41
If there's any place地点 in the solar太阳能 system系统
where life is not like us,
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如果在太阳系里存在这样一个地方,
那里的生命与我们不同,
09:47
where the substitute替代 of water
is another另一个 solvent溶剂 --
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那里水的代替物是另一种溶剂——
可以是甲烷——
09:50
and it could be methane甲烷 --
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那个地方就可以是土卫六。
09:52
it could be Titan泰坦.
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09:54
Well, is there life beyond Earth地球
in the solar太阳能 system系统?
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回到这个问题:
在地球以外,在太阳系中有生命么?
我们还不知道,
09:58
We don't know yet然而,
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但我们正在努力寻求答案。
10:00
but we're hot on the pursuit追求.
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我们现在接收到的信息非常让人激动,
10:02
The data数据 that we're receiving接收
is really exciting扣人心弦
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它告诉我们——
10:04
and telling告诉 us --
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并迫使我们以新的
令人激动的方式去思考这个问题。
10:06
forcing迫使 us to think about this
in new and exciting扣人心弦 ways方法.
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10:10
I believe we're on the right track跟踪.
205
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我相信我们正朝着正确的方向努力。
在接下来的10年内,
我们将能够回答这个问题。
10:13
That in the next下一个 10 years年份,
we will answer回答 that question.
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如果我们做出了解答,
10:17
And if we answer回答 it,
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并且结果是积极的,
10:19
and it's positive,
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那么太阳系中的生命将会无所不在。
10:21
then life is everywhere到处
in the solar太阳能 system系统.
209
609000
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10:25
Just think about that.
210
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1856
想想看吧。
我们也许并不孤单。
10:27
We may可能 not be alone单独.
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10:30
Thank you.
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谢谢。
(掌声)
10:31
(Applause掌声)
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Translated by Xiaoya Zhou

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ABOUT THE SPEAKER
James Green - Space physicist
James Green leads NASA's solar system exploration and astrobiology research.

Why you should listen

Dr. James Green began his career at NASA 35 years ago at the Marshall Space Flight Center, where he developed and managed the Space Physics Analysis Network. It provided scientists all over the world rapid access to data and resources. As NASA's Director of Planetary Science he leads NASA's solar system exploration and astrobiology research.

Green received his Ph.D. in Space Physics from the University of Iowa in 1979 and began working in the Magnetospheric Physics Branch at NASA's Marshall Space Flight Center (MSFC) in 1980. At Marshall, Green developed and managed the Space Physics Analysis Network that provided scientists all over the world with rapid access to data, to other scientists, and to specific NASA computer and information resources. In addition, Green was a Safety Diver in the Neutral Buoyancy tank making over 150 dives until left MSFC in 1985.

From 1985 to 1992 Green was the head of the National Space Science Data Center (NSSDC) at Goddard Space Flight Center (GSFC). The NSSDC is NASA's largest space science data archive. In 1992, he became the Chief of the Space Science Data Operations Office until 2005, when he became the Chief of the Science Proposal Support Office. While at GSFC, Green was a co-investigator and the Deputy Project Scientist on the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) mission. He has written over 100 scientific articles in refereed journals involving various aspects of the Earth's and Jupiter's magnetospheres and over 50 technical articles on various aspects of data systems and networks.

In August 2006, Green became the Director of the Planetary Science Division at NASA Headquarters. Over his career, Green has received numerous awards. In 1988, he received the Arthur S. Flemming award given for outstanding individual performance in the federal government and was awarded Japan's Kotani Prize in 1996 in recognition of his international science data management activities.

More profile about the speaker
James Green | Speaker | TED.com

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