请双击下面的英文字幕来播放视频。
翻译人员: Hong Li
校对人员: wenli liu
00:12
I am in search of another planet
in the universe where life exists.
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我正在宇宙中寻找另一颗有生命的行星。
00:18
I can't see this planet
with my naked eyes
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靠肉眼肯定看不到,
00:21
or even with the most powerful telescopes
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即使借助如今最强大的望远镜
00:23
we currently possess.
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也看不到。
00:25
But I know that it's there.
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但我坚信它的存在。
00:27
And understanding contradictions
that occur in nature
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了解自然界的矛盾法则,
00:31
will help us find it.
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能帮助我们找到它。
00:33
On our planet,
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在我们地球上,
00:34
where there's water, there's life.
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哪里有水,哪里就有生命。
00:36
So we look for planets that orbit
at just the right distance
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因此我们将目光锁定在
那些与恒星的距离
00:39
from their stars.
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正合适的行星。
00:42
At this distance,
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这一距离,
00:43
shown in blue on this diagram
for stars of different temperatures,
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在这张示意图中以蓝色表示,
根据恒星温度的高低而不同,
00:47
planets could be warm enough
for water to flow on their surfaces
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能保证行星足够温暖,
使水保持液态,
00:50
as lakes and oceans
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形成湖泊和海洋,
00:52
where life might reside.
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就有可能孕育生命。
00:54
Some astronomers focus their time
and energy on finding planets
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一些天文学家将时间和精力
投入到搜寻那些
00:58
at these distances from their stars.
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与其所围绕恒星的距离
在这一范围内的行星。
01:00
What I do picks up where their job ends.
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而我的工作紧随其后。
01:03
I model the possible
climates of exoplanets.
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我建立这些系外行星的气候模型。
01:07
And here's why that's important:
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这项工作很重要:
01:09
there are many factors
besides distance from its star
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因为要决定行星上是否有生命存在,
01:12
that control whether
a planet can support life.
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除了与恒星的距离外,
还有许多其他因素。
01:16
Take the planet Venus.
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以金星为例。
01:18
It's named after the Roman goddess
of love and beauty,
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它以罗马(神话中)
爱和美之女神的名字命名,
01:22
because of its benign,
ethereal appearance in the sky.
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因为它看起来如此优雅而美丽。
01:26
But spacecraft measurements
revealed a different story.
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然而宇宙飞船测量的结果
完全不是这么回事。
01:30
The surface temperature is close
to 900 degrees Fahrenheit,
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金星表面的温度接近900华氏度,
01:34
500 Celsius.
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也就是500摄氏度。
01:36
That's hot enough to melt lead.
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这温度足以融化铅。
01:39
Its thick atmosphere, not its distance
from the sun, is the reason.
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原因并不在于它与太阳的距离,
而在于它厚厚的大气层。
01:42
It causes a greenhouse effect on steroids,
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金星的大气层引发的温室效应,
01:46
trapping heat from the sun
and scorching the planet's surface.
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将来自太阳的热量牢牢锁住,
将金星地表变成一片焦土。
01:50
The reality totally contradicted
initial perceptions of this planet.
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这与我们之前对金星的想象
完全不一样。
01:55
From these lessons
from our own solar system,
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我们太阳系的这个例子告诉我们,
01:58
we've learned that a planet's atmosphere
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行星的大气层
02:00
is crucial to its climate
and potential to host life.
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对于其气候特点和
能否孕育生命至关重要。
02:04
We don't know what the atmospheres
of these planets are like
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我们无法了解那些(可能孕育生命的)
行星的大气情况,
02:07
because the planets are so small
and dim compared to their stars
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因为跟它们围绕的恒星相比,
它们又小又暗,
02:12
and so far away from us.
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而且离我们非常遥远。
02:14
For example, one of the closest planets
that could support surface water --
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比如,离我们最近的,
可能有液态水存在的行星之一,
02:18
it's called Gliese 667 Cc --
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叫做“格利泽667Cc”——
02:22
such a glamorous name, right,
nice phone number for a name --
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多美的名字啊,对吧,
做电话号码应该不错——
02:26
it's 23 light years away.
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离我们23光年。
02:29
So that's more than 100 trillion miles.
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也就是超过100万亿英里。
02:32
Trying to measure
the atmospheric composition
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想要在一颗系外行星
从它的主恒星前经过时,
02:35
of an exoplanet passing
in front of its host star is hard.
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测量它的大气成分太难了。
02:39
It's like trying to see a fruit fly
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就好比要看清一只
02:41
passing in front of a car's headlight.
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从车头灯前飞过的果蝇一样。
02:44
OK, now imagine that car
is 100 trillion miles away,
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而且,这辆车还远在100万亿英里之外,
02:47
and you want to know
the precise color of that fly.
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你还想看清这只果蝇的颜色。
02:52
So I use computer models
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因此我用计算机建模,
02:54
to calculate the kind of atmosphere
a planet would need
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来计算一颗行星要形成
适宜水和生命存在的气候,
02:57
to have a suitable climate
for water and life.
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需要何种大气类型。
03:01
Here's an artist's concept
of the planet Kepler-62f,
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这是一张“开普勒62f”行星的概念图,
03:05
with the Earth for reference.
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旁边是用来做对比的地球。
03:07
It's 1,200 light years away,
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它距离我们1200光年,
03:09
and just 40 percent larger than Earth.
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体积只比地球大40%。
03:12
Our NSF-funded work found that it
could be warm enough for open water
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我们的研究——由国家科学基金会资助——
发现它温度适宜,可能存在液态水,
03:16
from many types of atmospheres
and orientations of its orbit.
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它的大气拥有多种成分,
还有它的公转轨道(都可能证明这一点)。
03:20
So I'd like future telescopes
to follow up on this planet
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因此我希望未来的望远镜
能继续观测这颗行星,
03:23
to look for signs of life.
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寻找生命存在的迹象。
03:26
Ice on a planet's surface
is also important for climate.
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行星表面的冰层对于气候同样重要。
03:29
Ice absorbs longer,
redder wavelengths of light,
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冰能吸收波长较长、更靠近红端的光,
03:33
and reflects shorter, bluer light.
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反射波长较短、更靠近蓝端的光。
03:35
That's why the iceberg
in this photo looks so blue.
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这就是为什么这张照片里的
冰山看起来这么蓝。
03:39
The redder light from the sun
is absorbed on its way through the ice.
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阳光里偏红的光在穿过冰层时被吸收。
03:42
Only the blue light
makes it all the way to the bottom.
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只有蓝色的光一路走到底。
03:45
Then it gets reflected
back to up to our eyes
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然后反射到我们的眼睛里,
03:48
and we see blue ice.
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我们就看到了蓝色的冰。
03:50
My models show that planets
orbiting cooler stars
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我的模型显示,恒星温度越低,
其行星反而更温暖,
03:53
could actually be warmer
than planets orbiting hotter stars.
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恒星温度越高,
其行星反而更寒冷。
03:56
There's another contradiction --
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这又是一个矛盾之处——
03:58
that ice absorbs the longer
wavelength light from cooler stars,
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冰层吸收来自温度较低恒星
发出的波长较长的光,
04:02
and that light, that energy,
heats the ice.
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而这些光,这些能量,又加热了冰层。
04:06
Using climate models to explore
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运用气候模型
04:09
how these contradictions
can affect planetary climate
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来研究这些矛盾,
看它们如何影响行星的气候,
04:12
is vital to the search for life elsewhere.
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对于寻找地外生命至关重要。
04:16
And it's no surprise
that this is my specialty.
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而我命中注定要从事这个行业。
04:19
I'm an African-American female astronomer
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我是一名非裔美籍女天文学家,
04:22
and a classically trained actor
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也是受过古典艺术训练的演员,
04:24
who loves to wear makeup
and read fashion magazines,
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我喜欢化妆,喜欢时尚杂志,
04:28
so I am uniquely positioned to appreciate
contradictions in nature --
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所以上帝派我来理解这些矛盾——
04:33
(Laughter)
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(笑声)
04:34
(Applause)
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(掌声)
04:38
... and how they can inform our search
for the next planet where life exists.
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并利用它们来寻找
下一个有生命的行星。
04:42
My organization, Rising Stargirls,
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我成立的“新星女孩”组织,
04:45
teaches astronomy
to middle-school girls of color,
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通过戏剧、写作和视觉艺术的方式,
04:48
using theater, writing and visual art.
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向非白人女中学生传授天文学知识。
04:52
That's another contradiction --
science and art don't often go together,
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这也是一对矛盾——
科技和艺术看起来不同路,
04:56
but interweaving them can help
these girls bring their whole selves
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但两者的交融可以
帮助这些姑娘们实现自我,
05:00
to what they learn,
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学有所成,
05:01
and maybe one day join
the ranks of astronomers
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也许有一天她们也能成为
那些充满矛盾的
05:05
who are full of contradictions,
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天文学家中的一员,
05:06
and use their backgrounds
to discover, once and for all,
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运用自身所学,彻底证明
05:10
that we are truly not alone
in the universe.
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我们在茫茫宇宙中并不孤独。
05:14
Thank you.
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谢谢大家。
05:15
(Applause)
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(掌声)
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