The story of 'Oumuamua, the first visitor from another star system | Karen J. Meech | TED

7,246,629 views ・ 2018-07-19

TED


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譯者: Helen Chang 審譯者: SF Huang
00:13
NASA's always on the lookout for possible asteroid collision hazards,
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美國太空總署一直小心觀察著 潛在小行星碰撞的危險,
00:18
so the Pan-STARRS telescope is scanning the sky every night.
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所以泛星計畫的望遠鏡 每晚都在掃描天空。
00:23
Each morning, candidate objects are examined by Pan-STARRS staff
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每天早上,泛星計畫的工作人員 會檢查候選的對象,
00:27
and usually discovered to be no big deal.
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通常沒發現什麼大不了的狀況。
00:30
But on October 19, 2017,
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但是在 2017 年 10 月 19 日,
00:33
Pan-STARRS spotted an object moving rapidly between the stars,
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泛星計畫發現一顆 在恆星之間快速移動的物體,
00:38
and this time the usual follow-up measurements of position and speed
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而這次例行的後續追蹤 所測量出的位置和速度,
00:42
showed something completely different.
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顯示出完全不同的東西。
00:45
By October 22nd, we had enough data
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到 10 月 22 日,我們有足夠的數據
00:47
to realize that this object wasn't from our solar system.
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瞭解到這物體並非來自我們太陽系。
00:51
Holy cow.
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天啊。
00:53
That's when I got the phone call,
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我接到電話,
00:55
the phone call that all solar system astronomers are waiting for.
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是所有太陽系的天文學家 都在等待的電話。
00:59
Let me tell you how exciting this was.
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讓我告訴你這多麼令人興奮。
01:01
(Laughter)
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(笑聲)
01:02
NASA's been expecting to see an interstellar comet
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美國太空總署一直期待看到 穿過太陽系的星際彗星,
01:05
pass through the solar system since the 1970s,
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但自 20 世紀 70 年代 以來直到現在,
01:08
but until now, we'd never seen anything.
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我們未曾見過任何東西。
01:11
Our own solar system is huge,
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我們自己的太陽系很巨大,
01:14
so even getting a package from the nearest star system
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即使從距離 4.4 光年的 最近星系接收包裹
01:17
4.4 light years away
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01:19
would take over 50,000 years.
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也需要 5 萬年。
01:22
So this is a really big deal.
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所以這事至關重要。
01:24
The interstellar visitor entered our solar system
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星際訪客從黃道面的上方
01:27
from above the plane of the planets,
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進入我們的太陽系,
01:29
coming from the direction of the constellation Lyra,
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來自天琴座(Lyra)的方向,
01:32
and it passed closest to the Sun on September 9th,
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於 9 月 9 日經過近日點,
01:35
passing inside the orbit of Mercury.
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經水星軌道內側穿越。
01:38
Now this isn't a particularly close approach or unusual distance.
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這距離不算特別接近, 也不算非比尋常,
01:42
It's just much easier to see objects close by.
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只是近距離觀察物體要容易得多。
01:47
On October 14th,
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在我們發現它之前,
01:48
before we discovered it, it made its closest approach to the Earth,
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它在 10 月 14 日最接近地球,
01:52
within about 15 million miles.
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距離約在 1500 萬英里內。
01:55
This is really close by astronomical standards.
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以天文的標準而言,是非常近的。
01:59
Now rather than call this by its unwieldy catalog name,
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我們不用難懂的目錄名稱來稱呼它,
02:03
we briefly called it "Rama,"
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我們簡稱它為「拉瑪」,
02:06
after the cylindrical spacecraft that passed through the solar system
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那是亞瑟·查理斯·克拉克 1973 年的經典科幻小說裡
02:10
in Arthur C. Clarke's classic science fiction story in 1973.
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穿過太陽系的圓柱形太空船的名字。
02:15
But this wasn't quite right either,
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但這也不那麼合適,
02:17
so in honor of it being discovered by a telescope in Hawaii,
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所以為了紀念夏威夷的望遠鏡發現它,
02:21
we consulted two experts on Hawaiian culture --
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我們諮詢了兩位夏威夷文化專家,
02:24
a Hawaiian navigator and a linguist --
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他們是夏威夷航海家和語言學家,
02:27
to propose a name.
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提出一個名字。
02:28
And they suggested "'Oumuamua,"
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他們建議「斥侯星」,
02:31
which means scout or messenger from the distant past reaching out to us.
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意思是來自遙遠的過去, 向我們伸手的偵察員或使者。
02:37
Now this discovery was important for many reasons,
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這個發現很重要的原因相當多,
02:41
but to me the most significant is for what 'Oumuamua can tell us
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但對我而言,最重要的是
斥侯星可以告訴我們太陽系的過去。
02:45
about the past of our solar system.
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02:48
The process of the birth of a new solar system and the growth of planets
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新太陽系的誕生和行星生成的過程
02:52
can be a violent and messy business.
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可能很猛烈、很混亂。
02:55
Leftover icy and rocky debris gets ejected from the new solar system
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當巨大的行星穿過 形成它們的塵埃盤時,
02:59
as the giant planets migrate through the dusty disk
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殘餘的冰冷岩石碎片
便被逐出這個新生的太陽系。
03:03
out of which they're formed.
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03:06
Now have you ever felt an emotional chill,
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你有沒有感受到一種情緒的寒意?
03:10
something that's so exciting that a shiver runs up and down your spine?
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一種令人興奮的東西 讓你的脊椎上下顫抖?
03:16
Or something that's very emotionally moving?
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或是某種情緒激動?
03:19
Well this was it for me.
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對我來說就是這樣。
03:21
This was my wow moment.
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這是我的驚嘆時刻。
03:23
We actually had a piece of material from another solar system
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我們實際上有一塊 來自另一個太陽系的物質
03:27
coming close enough for us to observe.
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近到讓我們能夠觀察它。
03:31
So what would you like to know about 'Oumuamua,
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你想了解斥侯星
03:34
the very first visitor from another star system?
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這另一星系的首位訪客那些事呢?
03:38
Well, I could think of a million things,
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我可以想到一百萬件事,
03:41
but there's what you want and what you can have,
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但是想要的和得到的是兩碼事,
03:44
and 'Oumuamua was moving away and fading very rapidly.
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而斥侯星正迅速、逐漸地消失。
03:49
In the span of about a week,
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在大約一周的時間內,
03:51
it had dropped in brightness by a factor of [10].
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它的亮度下降到十分之一。
03:54
So this is about all the time we were going to have
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一個星期就是我們能便於 研究它的全部時間。
03:57
to study it easily.
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03:59
So we had to distill the process of getting telescope time --
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因此我們必須快馬加鞭 取得使用望遠鏡的時間,
04:04
normally a very competitive, peer-reviewed proposal process
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這個由同行評審的提案流程 通常競爭激烈,
04:08
that can take up to months --
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審核期可能長達數個月,
04:10
down to less than a few days.
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被縮減到短短幾天。
04:12
So began a "polite" competition for resources.
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一場「禮貌」的資源競爭開始了。
04:17
OK, let me not mince words. It was a fierce battle.
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好吧,我不再矯言了。 這是一場激烈的戰鬥。
04:20
We dropped everything,
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我們擱下所有的工作,
04:22
working around the clock,
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不分晝夜地
04:23
trying to craft perfectly crafted proposal words
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試圖趕製出完美的提案,
04:27
to send to the observatory directors.
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送交給天文台的主管們。
04:30
Well, good news. We got the time.
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好消息。我們獲得了使用的時間。
04:34
Now, from a perfectly selfish point of view,
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從一個完全自私的角度來看,
04:37
the first thing we might like to know is how massive 'Oumuamua is.
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首先我們想知道斥侯星有多大。
04:42
Because after all, it passed very close to the Earth,
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因為它畢竟曾非常接近地球,
04:45
and we didn't know about it until afterwards.
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這是事後我們才知道的。
04:48
How bad would this have been had it not missed the Earth?
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如果它擊中地球會多糟糕?
04:53
Well, the impact energy
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衝擊的能量取決於 速度的平方乘以質量,
04:55
depends on the square of the velocity times its mass,
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04:59
and the mass depends on how big it is and what it's made of.
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質量取決於它的大小和組成。
05:03
So how big is 'Oumuamua, and what's its shape?
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那麼斥侯星有多大,是什麼形狀?
05:07
Well, we can get this from its brightness.
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我們可從它的亮度得知。
05:10
Now, if you don't believe me, think of comparing the brightness
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如果你不相信我,
可以比較後院的螢火蟲亮度
05:13
of a firefly in your backyard
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05:14
to the navigation lights on a distant airplane.
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與遙遠飛機上的導航燈亮度。
05:18
You know the airplane is much brighter --
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你知道飛機比較亮,
05:20
it just appears faint because it's so far away.
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它的亮度顯得微弱只因為距離遠。
05:24
We're also going to need to know
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我們還需要知道
05:26
how reflective the surface of 'Oumuamua is,
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斥侯星表面的反射程度。
05:29
and we don't have any clue,
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我們沒有任何線索,
05:31
but it's reasonable to assume it's very similar to small asteroids
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但我們認為它與太陽系中的
小行星和彗星非常相似,
05:35
and comets in our solar system,
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05:37
or in technical terms,
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或以技術用詞來說,
05:39
something between the reflectivity of charcoal and wet sand.
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它的反射率類似介於木炭和濕沙之間。
05:44
Nowadays, most of the big telescopes are used in what's called a service mode,
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如今,大多數大型望遠鏡 採用所謂的服務模式,
05:50
meaning we have to carefully develop all the instructions
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意思是我們必須仔細闡述所有的指令,
05:54
and send them to the telescope operator,
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並將它們發送給望遠鏡操作員,
05:56
and then anxiously wait for the data to come back,
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然後焦急地等待收回數據,
05:59
praying to the weather gods.
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向天氣之神祈禱。
06:01
Now I bet most of you don't have careers
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我敢打賭,你們大多數人的職涯
06:04
that critically depend on whether or not it's cloudy last night.
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不取決於昨晚是不是陰天。
06:08
Well, we weren't going to get any second chances here.
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我們不會有任何第二次機會。
06:12
Because the weather was great, 'Oumuamua decided not to be.
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天氣很好,而斥侯星則否。
06:16
Its brightness wasn't constant.
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它的亮度不恆定。
06:18
Now here we see 'Oumuamua racing between the stars.
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我們看到斥侯星在星星間急駛。
06:21
It's centered in the middle.
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中間就是它。
06:23
The stars are trailed out because the telescope is following its motion.
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星星拖出尾巴, 因為望遠鏡追著斥侯星移動。
06:28
It started faint and then it got brighter, fainter, brighter, and fainter again,
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它的亮度轉弱,再次變亮, 變暗,變亮,又變暗。
06:33
as sunlight is reflected off of four sides of an oblong object.
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由於陽光從長方形物體的四面反射。
06:39
The extreme brightness change
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極端的亮度變化使我們對其形狀
06:41
led us to an unbelievable conclusion about its shape.
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產生了令人難以置信的結論。
06:46
As shown in this artist's impression,
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正如這位藝術家的圖象所示,
06:48
'Oumuamua is apparently very long and narrow,
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斥侯星顯然非常長而窄,
06:51
with an axis ratio of about 10 to one.
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軸比約為 10 比 1。
06:55
Assuming it's dark, this means it's about half a mile long.
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假設它很暗, 意思是它大約半英里長。
06:59
Nothing else in our solar system looks like this.
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我們的太陽系中沒有像這樣的物體。
07:03
We only have a handful of objects that even have an axis ratio
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我們只有少數幾個
軸比大過 5 比 1 的物體。
07:07
bigger than five to one.
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07:09
So we don't know how this forms,
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因此我們不知道這是如何形成的,
07:11
but it may be part of its birth process in its home solar system.
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但可能是其太陽系 誕生過程中的一部分。
07:17
'Oumuamua was varying in brightness every 7.34 hours,
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斥侯星的亮度每 7.34 小時變化一次,
07:23
or so we thought.
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或者這是我們認為的數字。
07:24
As more data started to come in from other teams,
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隨著其他團隊的數據開始加了進來,
07:27
they were reporting different numbers.
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他們報告的數字不同。
07:29
Why is it the more we learn about something,
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為什麼我們越了解某事,
07:31
the harder it gets to interpret?
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就越難以解釋?
07:34
Well, it turns out that 'Oumuamua is not rotating in a simple way.
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原來斥侯星不以簡單的方式旋轉。
07:38
It's wobbling like a top.
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它像陀螺一樣搖擺不定。
07:40
So while it is rotating around its short axis,
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因此,它圍繞短軸旋轉,
07:43
it's also rolling around the long axis
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也圍繞長軸滾動,
07:46
and nodding up and down.
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並且上下搖擺。
07:48
This very energetic, excited motion
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這種充滿活力、活躍的運行方式,
07:51
is almost certainly the result of it being violently tossed
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幾乎可以肯定它是從自己的太陽系
07:55
out of its home solar system.
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被猛烈拋出的結果。
07:58
Now how we interpret the shape from its brightness
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我們如何從亮度解釋形狀
08:01
depends very critically on how it's spinning,
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關鍵取決於它是如何旋轉的,
08:04
so now we have to rethink what it may look like,
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所以我們必須重新思考它的外觀。
08:07
and as shown in this beautiful painting by space artist Bill Hartmann,
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正如空間藝術家比爾 · 哈特曼 這幅美麗的畫作所示,
08:10
we think that 'Oumuamua may be more of a flattened oval.
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我們認為斥侯星 更可能是個扁平的橢圓形。
08:15
So let's get back to the energetics.
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讓我們回到能量學。
08:17
What is it made of?
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它的組成是什麼?
08:19
Well, ideally we would love to have a piece of 'Oumuamua
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理想情況下,我們希望 帶塊斥侯星的碎片到實驗室,
08:22
into the laboratory, so we could study it in detail.
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讓我們可以詳細研究它。
08:26
But since even private industry can't manage to launch
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但是,由於在這情形下,
即使是私營企業
08:29
a spacecraft within a week
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也無法在一周內成功發射太空船,
08:31
to something like this,
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08:33
astronomers have to rely on remote observations.
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天文學家不得不仰賴遠程觀測。
08:36
So astronomers will look at how the light interacts with the surface.
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因此,天文學家研究 光線如何與表面相互作用。
08:40
Some colors may get absorbed, giving it a chemical fingerprint,
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有些顏色可能被吸收, 留下化學指紋,
08:44
whereas other colors may not.
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而其他顏色可能沒被吸收、沒指紋。
08:46
On the other hand, some substances may just reflect more blue
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另一方面,某些物質可能只是
更有效地反射藍光或紅光。
08:51
or red light efficiently.
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08:53
In the case of 'Oumuamua, it reflected more red light,
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斥侯星的情況是它反射更多的紅光,
08:57
making it look very much like the organic rich surface of the comet recently visited
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使它看起來非常像
羅塞塔號太空船最近訪問的彗星
09:02
by the Rosetta spacecraft.
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所遇到的富含有機物的表面。
09:04
But not everything that looks reddish has the same composition.
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但並非所有看起來偏紅的 東西,成分都相同。
09:09
In fact, minerals that have tiny little bits of iron in the surface
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事實上,表面上含有少量鐵的礦物質
09:13
can also look red,
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也可能看起來紅紅的,
09:15
as does the dark side of Saturn's moon Iapetus,
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土星的月亮「土衛八」的 黑暗面正是如此,
09:17
shown in these images from the Cassini spacecraft.
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這些圖像來自卡西尼號太空船。
09:21
Nickel-iron meteorites, in other words, metal,
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鎳鐵隕石,換句話說,金屬,
09:23
can also look red.
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看起來也紅紅的。
09:26
So while we don't know what's on the surface,
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因此,我們不知道表面是什麼,
09:28
we know even less about what's on the inside.
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對內部所知更少。
09:32
However, we do know that it must at least be strong enough
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然而,我們確實知道 它必須至少要夠堅固,
09:35
to not fly apart as it rotates,
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在旋轉時才不會分開,
09:37
so it probably has a density similar to that of rocky asteroids;
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所以它的密度可能 與岩石小行星的密度相似,
09:41
perhaps even denser, like metal.
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也許更密些,像金屬那樣。
09:45
Well, at the very least, I want to show you
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我至少想展示美麗的彩色圖像之一,
09:47
one of the beautiful color images that we got
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是我們的地面望遠鏡獲得的。
09:49
from one of the ground-based telescopes.
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09:52
All right, I admit, it's not all that spectacular.
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好吧,我承認,它不是那麼壯觀。
09:55
(Laughter)
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(笑聲)
09:56
We just don't have the resolution.
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只是解析度不夠。
09:59
Even Hubble Space Telescope
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甚至哈伯太空望遠鏡 也沒有更好的視野。
10:01
doesn't present a much better view.
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10:04
But the importance of the Hubble data was not because of the images,
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但哈伯數據的重要性不在於圖像,
10:07
but because it extended our observations out
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而是它將我們的觀察結果
10:10
to two and a half months from the discovery,
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延伸到發現它之後的兩個半月,
10:12
meaning we get more positions along the orbit,
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意思是我們獲得軌道上更多的位置,
10:15
which will hopefully let us figure out where 'Oumuamua came from.
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有望讓我們弄明白斥侯星來自哪裡。
10:21
So what exactly is 'Oumuamua?
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那麼斥侯星究竟是什麼?
10:25
We firmly believe it's likely to be a leftover archaeological remnant
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我們堅信,它可能是
另一個行星系統誕生過程中 剩餘的考古遺跡,
10:30
from the process of the birth of another planetary system,
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10:34
some celestial driftwood.
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是天體的漂流木。
10:36
Some scientists think that maybe 'Oumuamua formed
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一些科學家認為,也許斥侯星形成時
10:40
very close to a star that was much denser than our own,
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很靠近一顆比我們太陽 密度更大的恆星,
10:43
and the star's tidal forces shredded planetary material
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而那恆星的潮汐力
在它自己太陽系的歷史早期 就弄碎了行星物質。
10:47
early in the solar system's history.
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10:49
Still others suggest that maybe this is something that formed
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還有一些人認為
它可能是一顆恆星 在痛苦的死亡過程中形成的,
10:53
during the death throes of a star,
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10:55
perhaps during a supernova explosion,
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可能是在超新星爆炸的期間,
10:58
as planetary material got shredded.
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行星的物質被粉碎了。
11:02
Whatever it is, we believe it's a natural object,
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不管是什麼,我們相信 這是一個自然物體,
11:05
but we can't actually prove that it's not something artificial.
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但實際上我們無法證明 這不是人為的東西。
11:10
The color, the strange shape, the tumbling motion
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顏色、奇怪的形狀、翻滾動作
11:14
could all have other explanations.
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可能有其他的解釋。
11:16
Now while we don't believe this is alien technology,
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既然我們不相信這是外星人的技術,
11:20
why not do the obvious experiment and search for a radio signal?
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為什麼不做明顯的實驗, 蒐索無線電信號呢?
11:25
That's exactly what the Breakthrough Listen project did,
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這正是「突破聆聽」計劃所做的,
11:28
but so far, 'Oumuamua has remained completely quiet.
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但到目前為止,斥侯星仍然完全安靜。
11:33
Now could we send a spacecraft to 'Oumuamua
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我們現在可以將宇宙飛船送到斥侯星
11:35
and answer this question once and for all?
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並一勞永逸地回答這個問題嗎?
11:38
Yes, we do actually have the technology,
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是的,我們的確擁有這項技術,
11:40
but it would be a long and expensive voyage,
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但那將會是個既貴又長的旅程,
11:42
and we would get there so far from the Sun
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到達時,會離太陽那麼的遠,
11:45
that the final approach trajectory would be very difficult.
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最終的接近軌跡將會極端困難。
11:49
So I think 'Oumuamua probably has many more things to teach us,
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所以我認為斥侯星可能 還有很多東西要教我們。
11:54
and in fact there might be more surprises in store
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事實上,隨著像我這樣的科學家 繼續使用這些數據,
11:57
as scientists such as myself continue to work with the data.
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可能會有更多的驚喜。
12:02
More importantly, I think this visitor from afar
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更重要的是,我認為這位遠到的訪客
12:05
has really brought home the point that our solar system isn't isolated.
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確實帶回一個觀點:
那就是我們的太陽系並不孤立,
12:10
We're part of a much larger environment,
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我們是更寬廣宇宙的一部分,
12:13
and in fact, we may even be surrounded by interstellar visitors
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事實上,我們甚至可能 被星際訪客包圍著,
12:18
and not even know it.
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只是自己不知道。
12:20
This unexpected gift
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這個意想不到的禮物
12:22
has perhaps raised more questions than its provided answers,
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所衍生的提問 可能比帶來的答案還更多,
12:26
but we were the first to say hello to a visitor from another solar system.
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但我們首次
向另一個太陽系的訪客打招呼。
12:32
Thank you.
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謝謝。
12:33
(Applause)
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(掌聲)
12:42
Jedidah Isler: Thanks, Karen.
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吉迪達 · 伊斯勒:謝謝,凱倫。 我當然非常喜歡這個話題。謝謝。
12:44
I of course enjoyed that talk very much. Thank you.
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12:46
As I recall, we found it pretty late in its journey towards us.
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我記得你說到,我們在 它行經我們的旅程後期才發現它。
12:50
Will future technologies like the Large Synoptic Survey Telescope
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未來的大型天氣測量望遠鏡技術等等
12:54
help us detect these things sooner?
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能幫助我們更早發現這些事情嗎?
12:56
Karen Meech: Yeah. We're hoping that we'll start to see a lot of these things,
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凱倫 · 米區:是的。我們希望 之後會開始看到很多這類東西。
13:00
and ideally, you'd love to find one as it's approaching the Sun,
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理想的情況是 在它正接近太陽時找到它,
13:03
because you want to have time to do all the science,
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因為想爭取充裕的時間 做所有的科學研究。
13:07
or even more ideal,
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甚至更理想的是 準備好一艘太空船,
13:08
you'd get a spacecraft ready to go,
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13:10
parked somewhere in the L4 or L5 position,
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停在 L4 或 L5 位置的某個地方,
13:13
somewhere near Earth,
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停在靠近地球的某處,
13:14
so that when something comes by, you can chase it.
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這樣有東西進來時, 就可以去追蹤它了。
13:17
JI: Awesome, thanks so much. Let's thank Karen again.
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伊斯勒:太棒了,非常感謝。 讓我們再次感謝凱倫。
13:20
(Applause)
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(掌聲)
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