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  • So in 1781, an English composer,

    1781 年,一位英國作家、 工程師兼天文學家

  • technologist and astronomer called William Herschel

    名叫威廉•赫歇爾,

  • noticed an object on the sky that

    在浩瀚的夜空中觀測到一個天體,

  • didn't quite move the way the rest of the stars did.

    其運行方式與其他恒星大相徑庭。

  • And Herschel's recognition that something was different,

    赫歇爾覺得這個天體不同尋常,

  • that something wasn't quite right,

    有些不太對勁,

  • was the discovery of a planet,

    事實上他發現的是一顆行星,

  • the planet Uranus,

    也就是我們熟知的天王星。

  • a name that has entertained

    天王星這個名字

  • countless generations of children,

    讓一代又一代年輕人興趣盎然,

  • but a planet that overnight

    然而,這顆高懸於天際的行星

  • doubled the size of our known solar system.

    一經發現便讓人類已知的 太陽系範圍整整擴大了一倍。

  • Just last month, NASA announced the discovery

    就在上個月,美國太空總署 (NASA) 宣佈其又發現了

  • of 517 new planets

    517 顆環繞近地恒星

  • in orbit around nearby stars,

    運行的行星,

  • almost doubling overnight the number of planets

    幾乎在一夜間使銀河系中

  • we know about within our galaxy.

    已知的行星數量翻了一倍。

  • So astronomy is constantly being transformed by this

    人類收集的資料資訊 為天文學的不斷進步

  • capacity to collect data,

    注入了源源不斷的動力,

  • and with data almost doubling every year,

    而這些資料資訊幾乎 以每年翻一倍的速度增長,

  • within the next two decades, me may even

    未來二十年內,人類甚至可以

  • reach the point for the first time in history

    首次實現有史以來的一個夢想:

  • where we've discovered the majority of the galaxies

    探索浩瀚宇宙中

  • within the universe.

    的大部分星系。

  • But as we enter this era of big data,

    但是,人類開闢的是一個大資料資訊的時代,

  • what we're beginning to find is there's a difference

    我們開始探究的是

  • between more data being just better

    資料資訊越多越好

  • and more data being different,

    與資料資訊越多差別越大, 兩者之間有何差異,

  • capable of changing the questions we want to ask,

    這足以改變我們想問的一些問題,

  • and this difference is not about how much data we collect,

    這個差異並不在於我們收集多少資料資訊,

  • it's whether those data open new windows

    而是,那些資料資訊是否可以 為人類開啟一扇通往深邃宇宙的窗戶,

  • into our universe,

    那些資料資訊是否有助於 改變人類對觀測天空的方式。

  • whether they change the way we view the sky.

    下一扇通往宇宙的窗戶會有何奧秘呢?

  • So what is the next window into our universe?

    人類將如何譜寫天文學的下一個篇章?

  • What is the next chapter for astronomy?

    好,我會向諸位介紹一下

  • Well, I'm going to show you some of the tools and the technologies

    未來十年內人類將開發的一些工具與技術,

  • that we're going to develop over the next decade,

    這些先進技術,連同人類

  • and how these technologies,

    在運用資料資訊上展現的聰明才智,

  • together with the smart use of data,

    將再一次開啟一扇通往宇宙的窗戶

  • may once again transform astronomy

    使天文學發生革命性的變化,

  • by opening up a window into our universe,

    時間之窗。

  • the window of time.

    為什麼是時間?好,時間與起源

  • Why time? Well, time is about origins,

    和進化息息相關。

  • and it's about evolution.

    太陽系的起源、

  • The origins of our solar system,

    太陽系是如何形成的、

  • how our solar system came into being,

    有什麼不同尋常或獨特之處嗎?

  • is it unusual or special in any way?

    關於宇宙的演化。

  • About the evolution of our universe.

    為什麼宇宙處於不斷的膨脹中?

  • Why our universe is continuing to expand,

    促使宇宙膨脹的

  • and what is this mysterious dark energy

    神秘暗能量是什麼呢?

  • that drives that expansion?

    首先,我要向諸位介紹科學技術

  • But first, I want to show you how technology

    將有望改變人類對觀測天空的方式。

  • is going to change the way we view the sky.

    不妨設想一下,如果你在

  • So imagine if you were sitting

    智利北部山區

  • in the mountains of northern Chile

    仰望西天,

  • looking out to the west

    面向太平洋方向,

  • towards the Pacific Ocean

    就在日出前幾個小時。

  • a few hours before sunrise.

    這便是你將親眼目睹的夜空,

  • This is the view of the night sky that you would see,

    景色美麗動人,

  • and it's a beautiful view,

    銀河懸掛於天際。

  • with the Milky Way just peeking out over the horizon.

    但眼前是一幅靜止的美景,

  • but it's also a static view,

    而很多時候這也正是 我們腦海中勾勒出的宇宙:

  • and in many ways, this is the way we think of our universe:

    永恆不滅且一成不變。

  • eternal and unchanging.

    但宇宙絕不是靜止的。

  • But the universe is anything but static.

    宇宙處於永恆的變化中, 變化時間各不相同

  • It constantly changes on timescales of seconds

    有短短幾秒,也有幾十億年。

  • to billions of years.

    不同的星系

  • Galaxies merge, they collide

    在以幾十萬英里的時速融合、碰撞。

  • at hundreds of thousands of miles per hour.

    恒星不斷誕生,也不斷消亡,

  • Stars are born, they die,

    這些絢麗多彩的畫面展示了恒星的爆炸。

  • they explode in these extravagant displays.

    事實上,如果可以回到

  • In fact, if we could go back

    智利遙望寧靜的夜空,

  • to our tranquil skies above Chile,

    我們讓時間長河向前流淌

  • and we allow time to move forward

    一覽未來十年的天空, 會呈現出什麼模樣,

  • to see how the sky might change over the next year,

    你會觀察到宇宙的脈動

  • the pulsations that you see

    正是超新星,恒星在消亡中留下的殘餘,

  • are supernovae, the final remnants of a dying star

    爆炸、發出耀眼的光芒, 然後逐漸消失在視野中,

  • exploding, brightening and then fading from view,

    任何一顆超新星

  • each one of these supernovae

    都比太陽亮上五十億倍,

  • five billion times the brightness of our sun,

    因此,人類在相當遙遠的地方 就能發現它們的蹤跡

  • so we can see them to great distances

    但其光芒轉瞬即逝。

  • but only for a short amount of time.

    宇宙中每一秒都會 有十顆超新星發生爆炸。

  • Ten supernova per second explode somewhere

    如果我們可以聽見爆炸聲,

  • in our universe.

    會同一袋爆米花爆開的聲音一樣。

  • If we could hear it,

    超新星的光芒逐漸暗淡,

  • it would be popping like a bag of popcorn.

    這不只是亮度的變化。

  • Now, if we fade out the supernovae,

    天空處於永恆的運動之中。

  • it's not just brightness that changes.

    你會看到大量天體源源不斷地掠過天空

  • Our sky is in constant motion.

    這些是環繞太陽運行的小行星,

  • This swarm of objects you see streaming across the sky

    正是這些變化與運動

  • are asteroids as they orbit our sun,

    以及天體系統的動態變化

  • and it's these changes and the motion

    讓我們得以創建宇宙的模型,

  • and it's the dynamics of the system

    便於我們解讀過去,展望未來。

  • that allow us to build our models for our universe,

    然而,過去十年裡,我們使用的望遠鏡

  • to predict its future and to explain its past.

    其設計初衷並非用於 收集如此大規模的資料資訊。

  • But the telescopes we've used over the last decade

    哈伯太空望遠鏡:

  • are not designed to capture the data at this scale.

    在過去二十五年內,

  • The Hubble Space Telescope:

    已為人類生成了部分宇宙深處

  • for the last 25 years it's been producing

    最生動具體的畫面,

  • some of the most detailed views

    不過,若要使用哈伯太空望遠鏡 去還原一幅天空全景圖,

  • of our distant universe,

    則需要彙聚 1300 萬個獨立的景象,

  • but if you tried to use the Hubble to create an image

    即使一次也得歷時 120 年之久。

  • of the sky, it would take 13 million individual images,

    面對這一形勢,我們必須開發新技術

  • about 120 years to do this just once.

    並建造全新的望遠鏡,

  • So this is driving us to new technologies

    這些望遠鏡不僅觀測距離更遠,

  • and new telescopes,

    讓人類深入宇宙腹地。

  • telescopes that can go faint

    而且觀測視野更寬,

  • to look at the distant universe

    可迅速拍攝天空中的一舉一動,

  • but also telescopes that can go wide

    像大口徑全景巡天望遠鏡之類的望遠鏡

  • to capture the sky as rapidly as possible,

    又稱為 LSST。

  • telescopes like the Large Synoptic Survey Telescope,

    縱觀天文學歷史,

  • or the LSST,

    在所有最有趣的科學實驗中

  • possibly the most boring name ever

    這個名稱算是最最無聊的,

  • for one of the most fascinating experiments

    事實上,你如果非得有個名稱,

  • in the history of astronomy,

    那千萬別讓科學家或工程師來命名,

  • in fact proof, if you should need it,

    甚至不要讓他們為你的孩子起名字。(笑聲)

  • that you should never allow a scientist or an engineer

    LSST 工程已開工建設。

  • to name anything, not even your children. (Laughter)

    有望於2020年年底前開始收集資料資訊。

  • We're building the LSST.

    我將為諸位解讀一下我們的思維方式

  • We expect it to start taking data by the end of this decade.

    這將轉變我們對宇宙的認識,

  • I'm going to show you how we think

    因為 LSST 拍攝的每個圖像

  • it's going to transform our views of the universe,

    相當於哈伯太空望遠鏡拍攝的 3000 個圖像,

  • because one image from the LSST

    LSST 的每個圖像覆蓋了天空中 3.5 度的區域,

  • is equivalent to 3,000 images

    相當於七個滿月的寬度。

  • from the Hubble Space Telescope,

    如何拍攝這麼大的圖像呢?

  • each image three and a half degrees on the sky,

    那就得製造有史以來最大的數位相機,

  • seven times the width of the full moon.

    採用的技術與你的手機鏡頭

  • Well, how do you capture an image at this scale?

    或在大街上購買的數位相機 採用的技術完全相同,

  • Well, you build the largest digital camera in history,

    而眼下這個數位相機的鏡頭 足足寬5.5英尺,

  • using the same technology you find in the cameras in your cell phone

    相當於一輛福斯金龜車的長度,

  • or in the digital cameras you can buy in the High Street,

    這個鏡頭拍攝的每個圖像 有30億個圖元。

  • but now at a scale that is five and a half feet across,

    因此,如果你想一睹 LSST 全解析度圖像的風采,

  • about the size of a Volkswagen Beetle,

    哪怕只是一個圖像,

  • where one image is three billion pixels.

    也得用 1500 個高清電視螢幕。

  • So if you wanted to look at an image

    這台相機將用於拍攝天空的全景,

  • in its full resolution, just a single LSST image,

    每隔 20 秒鐘拍攝一張照片,

  • it would take about 1,500 high-definition TV screens.

    永不停息地掃描天空。

  • And this camera will image the sky,

    這樣只要三個夜晚, 我們就能掃描一次天空,

  • taking a new picture every 20 seconds,

    重新繪製一幅智利上空的天空全景圖。

  • constantly scanning the sky

    這台望遠鏡會在其生命週期內

  • so every three nights, we'll get a completely new view

    探測 400 億恒星與星系,

  • of the skies above Chile.

    這也會是我們首次

  • Over the mission lifetime of this telescope,

    能探索的宇宙天體數量

  • it will detect 40 billion stars and galaxies,

    超過地球上的人口數。

  • and that will be for the first time

    目前,我們可以按

  • we'll have detected more objects in our universe

    百萬位元組與十億位元組, 通過研究數十億個天體

  • than people on the Earth.

    來解讀宇宙,

  • Now, we can talk about this

    但如果想要親身感受一下

  • in terms of terabytes and petabytes

    這款相機收集的訊息量,

  • and billions of objects,

    好比同時播放已錄製的每一個 TED 演講,

  • but a way to get a sense of the amount of data

    一天二十四小時,

  • that will come off this camera

    一周七天不停地播放,可以長達連續十年。

  • is that it's like playing every TED Talk ever recorded

    若要處理這些資料資訊,則如同

  • simultaneously, 24 hours a day,

    在所有訪談節目中搜索

  • seven days a week, for 10 years.

    每一個全新的觀點與理念,

  • And to process this data means

    關注影片中的每個細節。

  • searching through all of those talks

    查看每一幀內容

  • for every new idea and every new concept,

    有何變化。

  • looking at each part of the video

    我們正在開闢一個科學研究的新紀元,

  • to see how one frame may have changed

    顛覆天文學研究的傳統模式,

  • from the next.

    在全新的模式下人們 將運用軟體技術與演算法則

  • And this is changing the way that we do science,

    挖掘隱藏在資料資訊中的無窮奧秘,

  • changing the way that we do astronomy,

    屆時軟體技術對科學研究至關重要,

  • to a place where software and algorithms

    其重要性並不亞於這些 尚未問世的望遠鏡與相機。

  • have to mine through this data,

    目前,這個專案將為人類

  • where the software is as critical to the science

    開啟成千上萬的探索發現之門,

  • as the telescopes and the cameras that we've built.

    但我今天只向諸位講述

  • Now, thousands of discoveries

    有關起源與進化的兩個理念

  • will come from this project,

    這兩個理念也會隨著人們

  • but I'm just going to tell you about two

    對大規模資料資訊的研究而不斷發展。

  • of the ideas about origins and evolution

    過去五年內,NASA 已在近地恒星

  • that may be transformed by our access

    附近發現了 1000 多個行星系,

  • to data at this scale.

    但我們力求探尋的這些行星系

  • In the last five years, NASA has discovered

    並不十分類似於我們的太陽系。

  • over 1,000 planetary systems

    我們面臨的一個問題是

  • around nearby stars,

    究竟是人類對宇宙的觀測還不夠全面,

  • but the systems we're finding

    還是我們太陽系的起源

  • aren't much like our own solar system,

    本來就與眾不同?

  • and one of the questions we face is

    如果我們要解答這一問題,

  • is it just that we haven't been looking hard enough

    就得深入瞭解

  • or is there something special or unusual

    太陽系的前世與今生,

  • about how our solar system formed?

    這些具體資訊十分重要。

  • And if we want to answer that question,

    因此,時下當我們仰望星空,

  • we have to know and understand

    無數小行星掠過天際,

  • the history of our solar system in detail,

    彷彿是太陽系中遺落的殘骸。

  • and it's the details that are crucial.

    小行星所處的位置

  • So now, if we look back at the sky,

    就像海王星與木星早期運行軌道,

  • at our asteroids that were streaming across the sky,

    離太陽更近的時候在

  • these asteroids are like the debris of our solar system.

    宇宙中留下的指紋,

  • The positions of the asteroids

    這些體積巨大的行星在太陽系中遷徙,

  • are like a fingerprint of an earlier time

    一路遺落不計其數的小行星。

  • when the orbits of Neptune and Jupiter

    因此,探究小行星就像

  • were much closer to the sun,

    在進行法醫鑒定,

  • and as these giant planets migrated through our solar system,

    對整個太陽系的法醫鑒定。

  • they were scattering the asteroids in their wake.

    但為此,我們需要距離,

  • So studying the asteroids

    通過天體的運行,可以得知距離,

  • is like performing forensics,

    而由於對時間掌握, 我們才瞭解了天體的運行。

  • performing forensics on our solar system,

    我們可以從中得到什麼啟示呢?

  • but to do this, we need distance,

    你是否注意到一些黃色小行星

  • and we get the distance from the motion,

    匆匆掠過螢幕,

  • and we get the motion because of our access to time.

    這些小行星的運行速度很快,

  • So what does this tell us?

    是因為它們距離地球最近。

  • Well, if you look at the little yellow asteroids

    有朝一日人類或許會派 太空船造訪這些行星

  • flitting across the screen,

    開發上面的礦產資源,

  • these are the asteroids that are moving fastest,

    但這些小行星或許會在未來的某一天

  • because they're closest to us, closest to Earth.

    撞擊地球,

  • These are the asteroids we may one day

    就像 6000 萬年前的那次撞擊

  • send spacecraft to, to mine them for minerals,

    造成了恐龍的滅絕,

  • but they're also the asteroids that may one day

    也像上世紀初葉

  • impact the Earth,

    一顆小行星徑直墜落於西伯利亞,

  • like happened 60 million years ago

    1000 平方英里的森林頓時化為烏有,

  • with the extinction of the dinosaurs,

    甚至就在去年,有一顆小行星 在俄羅斯上空的大氣層內燒毀,

  • or just at the beginning of the last century,

    釋放的能量相當於一個小型核彈。

  • when an asteroid wiped out

    因此,對太陽系進行法醫鑒定

  • almost 1,000 square miles of Siberian forest,

    不只能讓我們瞭解過去,

  • or even just last year, as one burnt up over Russia,

    更可以展望未來,包括人類自身的未來。

  • releasing the energy of a small nuclear bomb.

    眼下只要我們得知距離,

  • So studying the forensics of our solar system

    就能觀察到小行星以其自然的方式,

  • doesn't just tell us about the past,

    環繞太陽運行。

  • it can also predict the future, including our future.

    所以,諸位在這幅景象中 看到的每一個亮點

  • Now when we get distance,

    都是一顆真實的小行星。

  • we get to see the asteroids in their natural habitat,

    憑藉這顆小行星在空中的運行狀況, 就能計算出其運行軌跡。

  • in orbit around the sun.

    這些小行星的顏色顯示了其組成物質,

  • So every point in this visualization that you can see

    中心部分是乾燥的岩石,

  • is a real asteroid.

    而表面卻粗糙不平,富含水分,

  • Its orbit has been calculated from its motion across the sky.

    含水量較高的小新星上可能會有

  • The colors reflect the composition of these asteroids,

    和地球上一模一樣的海洋,

  • dry and stony in the center,

    地球上的海洋正是小行星 早年撞擊地球後留下的。

  • water-rich and primitive towards the edge,

    由於 LSST 不僅觀察視野更寬,

  • water-rich asteroids which may have seeded

    而且探測距離更遠。

  • the oceans and the seas that we find on our planet

    我們將在遠離太陽系中心的區域

  • when they bombarded the Earth at an earlier time.

    一窺這些小行星的身影,

  • Because the LSST will be able to go faint

    觀察木星與火星軌道之外的小行星,

  • and not just wide,

    跟蹤距離太陽

  • we will be able to see these asteroids

    幾乎一光年之遙的彗星與小行星。

  • far beyond the inner part of our solar system,

    我們會更加詳細地解讀這些照片

  • to asteroids beyond the orbits of Neptune and Mars,

    將解讀細節從 10 個提高到 100 個,

  • to comets and asteroids that may exist

    就能找到一些問題的答案,例如

  • almost a light year from our sun.

    是否有證據顯示木星軌道之外還存在行星,

  • And as we increase the detail of this picture,

    在可能撞擊地球的小行星威脅地球之前很久

  • increasing the detail by factors of 10 to 100,

    便鎖定它們的行蹤,

  • we will be able to answer questions such as,

    並解答太陽只有一個

  • is there evidence for planets outside the orbit of Neptune,

    還是宇宙中存在一大把這樣的恒星,

  • to find Earth-impacting asteroids

    或許正是太陽的姊妹星

  • long before they're a danger,

    對太陽系的形成產生了巨大的影響,

  • and to find out whether, maybe,

    或許這正是太陽系在宇宙中 如此罕見的原因之一。

  • our sun formed on its own or in a cluster of stars,

    宇宙中的距離與變化,

  • and maybe it's this sun's stellar siblings

    距離等於時間,

  • that influenced the formation of our solar system,

    以及天空中的變化。

  • and maybe that's one of the reasons why solar systems like ours seem to be so rare.

    你的目光每延伸一英尺

  • Now, distance and changes in our universe

    或某一個天體運行每一英尺,

  • distance equates to time,

    其實在諸位眼睛中留下的景象 是之前十億分之一秒發生的事情,

  • as well as changes on the sky.

    眺望宇宙就是眺望過去的時光

  • Every foot of distance you look away,

    這個觀點或概念讓我們 對宇宙的認識發生了革命性的變化,

  • or every foot of distance an object is away,

    這種變化不止一次,而是多次。

  • you're looking back about a billionth of a second in time,

    第一次發生在 1929 年,

  • and this idea or this notion of looking back in time

    一位名叫愛德文·哈伯的天文學家

  • has revolutionized our ideas about the universe,

    指出宇宙處在不斷的膨脹中,

  • not once but multiple times.

    形成了宇宙大爆炸觀點。

  • The first time was in 1929,

    觀察結果非常簡單:

  • when an astronomer called Edwin Hubble

    只有 24 個星系

  • showed that the universe was expanding,

    和一張手工繪製的圖片。

  • leading to the ideas of the Big Bang.

    但星系的距離越遠,

  • And the observations were simple:

    它遠離我們的速度就越快,

  • just 24 galaxies

    這一觀點足以促成現代宇宙學的誕生。

  • and a hand-drawn picture.

    第二次革命發生在 70 年後,

  • But just the idea that the more distant a galaxy,

    兩組天文學家指出

  • the faster it was receding,

    宇宙不僅在不斷地膨脹,

  • was enough to give rise to modern cosmology.

    而且正在加速膨脹。

  • A second revolution happened 70 years later,

    這個觀點令人驚訝, 好比將一個球拋到空中,

  • when two groups of astronomers showed

    你會發現這個球離地面越高,

  • that the universe wasn't just expanding,

    飛行的速度也越快。

  • it was accelerating,

    他們展示研究結果的方法是

  • a surprise like throwing up a ball into the sky

    通過測量超新星的亮度,

  • and finding out the higher that it gets,

    和超新星的亮度

  • the faster it moves away.

    如何隨著距離增加而不斷減弱。

  • And they showed this

    這些觀察結果更加複雜。

  • by measuring the brightness of supernovae,

    於是新技術與全新的望遠鏡呼之欲出,

  • and how the brightness of the supernovae

    由於超新星存在於一些星系中

  • got fainter with distance.

    而這些星系比哈伯望遠鏡

  • And these observations were more complex.

    拍攝到的星系還要遠 2000 倍。

  • They required new technologies and new telescopes,

    經過三年鍥而不捨的觀察, 只發現了 42 顆超新星,

  • because the supernovae were in galaxies

    由於一個星系中的超新星

  • that were 2,000 times more distant

    幾百年中才爆炸一次。

  • than the ones used by Hubble.

    整整三年才發現了 42 顆超新星,

  • And it took three years to find just 42 supernovae,

    搜索了成千上萬個星系。

  • because a supernova only explodes

    收集了這些資料資訊,

  • once every hundred years within a galaxy.

    這是他們發現的。

  • Three years to find 42 supernovae

    這一研究成果可能看上去不起眼,

  • by searching through tens of thousands of galaxies.

    但可以堪稱物理學上的一次革命:

  • And once they'd collected their data,

    這條直線預測距離地球 110 億光年之遙的超新星亮度,

  • this is what they found.

    一些小點與這條直線並不十分吻合。

  • Now, this may not look impressive,

    細微的變化往往會催生重大結果。

  • but this is what a revolution in physics looks like:

    細微的變化讓我們實現突破,探索發現,

  • a line predicting the brightness of a supernova

    就像赫歇爾當年發現天王星一樣。

  • 11 billion light years away,

    細微的變化顛覆了

  • and a handful of points that don't quite fit that line.

    我們對浩瀚宇宙的理解。

  • Small changes give rise to big consequences.

    因此,42 顆超新星,十分昏暗,

  • Small changes allow us to make discoveries,

    可見其距離地球稍遠,

  • like the planet found by Herschel.

    由此可推斷宇宙肯定不只是在膨脹,

  • Small changes turn our understanding

    而是在加速膨脹。

  • of the universe on its head.

    揭示了宇宙的一個組成部分

  • So 42 supernovae, slightly too faint,

    就是我們目前所稱的暗能量,

  • meaning slightly further away,

    正是暗能量在加速宇宙的膨脹,

  • requiring that a universe must not just be expanding,

    已知宇宙中的能量預計有68%為暗能量。

  • but this expansion must be accelerating,

    下一次革命可能會發生在哪個領域?

  • revealing a component of our universe

    暗能量是什麼,暗能量為什麼會存在?

  • which we now call dark energy,

    每一條直線為我們展現了

  • a component that drives this expansion

    一種不同的暗能量可能存在的模式

  • and makes up 68 percent of the energy budget

    揭示了暗能量的各種屬性。

  • of our universe today.

    已發現的 42 個亮點完全符合這些屬性,

  • So what is the next revolution likely to be?

    但隱藏在這些直線背後的理念

  • Well, what is dark energy and why does it exist?

    則截然不同。

  • Each of these lines shows a different model

    有人設想暗能量

  • for what dark energy might be,

    隨著時間的流逝而變化,

  • showing the properties of dark energy.

    或是暗能量的屬性是否不同,

  • They all are consistent with the 42 points,

    取決於你觀察天空時所處的地點。

  • but the ideas behind these lines

    其他人則在亞原子的層面

  • are dramatically different.

    釐定物理學上的差異與變化。

  • Some people think about a dark energy

    或者,他們關注

  • that changes with time,

    重力與廣義相對論作用的規模與變化,

  • or whether the properties of the dark energy

    或他們覺得我們的宇宙只是

  • are different depending on where you look on the sky.

    這個神秘莫測的多元宇宙中的一部分而已,

  • Others make differences and changes

    但是所有這些觀點、理論

  • to the physics at the sub-atomic level.

    非常不可思議,毋庸置疑 其中一些稍稍有些瘋狂,

  • Or, they look at large scales

    但所有這些觀點與理論 都於我們發現的 42 個亮點相互印證。

  • and change how gravity and general relativity work,

    因此,我們如何在未來十年內

  • or they say our universe is just one of many,

    理解其中的奧秘?

  • part of this mysterious multiverse,

    設想一下,如果給你兩個骰子,

  • but all of these ideas, all of these theories,

    我問你如何知道這兩個骰子

  • amazing and admittedly some of them a little crazy,

    是不是被人做了手腳。

  • but all of them consistent with our 42 points.

    只投一次骰子,你得不出什麼結論,

  • So how can we hope to make sense of this

    但多投幾次,

  • over the next decade?

    積攢起數據,

  • Well, imagine if I gave you a pair of dice,

    就會對自己更有信心,

  • and I said you wanted to see whether those dice

    不僅知道這些骰子 有沒有被人做過手腳,

  • were loaded or fair.

    而且還知道做了多少手腳, 而且怎麼做的。

  • One roll of the dice would tell you very little,

    我們歷時整整三年 才發現了 42 個超新星,

  • but the more times you rolled them,

    因為我們已建造的望遠鏡

  • the more data you collected,

    只能探索天空中的很小一部分。

  • the more confident you would become,

    有了 LSST,每三個夜晚我們就可以觀察到

  • not just whether they're loaded or fair,

    智利上空的一個全新景象。

  • but by how much, and in what way.

    觀測的第一個夜晚,

  • It took three years to find just 42 supernovae

    發現的超新星的數量, 就會是當初發現暗能量時

  • because the telescopes that we built

    所用的超新星數量的整整十倍。

  • could only survey a small part of the sky.

    最初的四個月內的觀測數字將提升 1000:

  • With the LSST, we get a completely new view

    這次觀察後會發現 150 萬顆超新星,

  • of the skies above Chile every three nights.

    每一顆超新星就像投一次骰子

  • In its first night of operation,

    每一個超新星測試哪些暗能量理論吻合,

  • it will find 10 times the number of supernovae

    哪些不吻合。

  • used in the discovery of dark energy.

    所以,這些超新星資料資訊會

  • This will increase by 1,000

    與宇宙學的其他措施相結合,

  • within the first four months:

    我們會逐步篩除

  • 1.5 million supernovae by the end of its survey,

    不同的暗能量觀點與理論,

  • each supernova a roll of the dice,

    此次觀察有望在 2030 年左右結束,

  • each supernova testing which theories of dark energy

    我們希望屆時發現

  • are consistent, and which ones are not.

    一種宇宙理論,

  • And so, by combining these supernova data

    一種宇宙物理的基本理論

  • with other measures of cosmology,

    漸漸顯出雛形。

  • we'll progressively rule out the different ideas

    我在許多領域提出過一些問題

  • and theories of dark energy

    實際上都是最簡單的問題。

  • until hopefully at the end of this survey around 2030,

    但答案至今無從知曉,

  • we would expect to hopefully see

    但我們至少知道該如何提問。

  • a theory for our universe,

    但是如果縱觀成千上萬個星系

  • a fundamental theory for the physics of our universe,

    結果只發現了 42 顆超新星,

  • to gradually emerge.

    足以轉變我們對茫茫宇宙的理解,

  • Now, in many ways, the questions that I posed

    當我們專注於研究數十億星系,

  • are in reality the simplest of questions.

    我們費盡周折只發現了 42 個亮點, 這顯然不符合我們的期望值,

  • We may not know the answers,

    但這樣事倍功半的事情還會發生多少次呢?

  • but we at least know how to ask the questions.

    就像赫歇爾發現天王星

  • But if looking through tens of thousands of galaxies

    或暗能量,

  • revealed 42 supernovae that turned

    或量子力學或廣義相對論,

  • our understanding of the universe on its head,

    這些理論的產生,都是因為資訊

  • when we're working with billions of galaxies,

    並不符合我們的期望,

  • how many more times are we going to find

    天文學資訊的下一個十年

  • 42 points that don't quite match what we expect?

    激動人心的一面正是

  • Like the planet found by Herschel

    我們甚至不知道會有多少問題

  • or dark energy

    等待著我們去解答,

  • or quantum mechanics or general relativity,

    這些解答關乎宇宙起源與演化。

  • all ideas that came because the data

    還有多少解答已經擺在面前,

  • didn't quite match what we expected.

    但我們甚至不知道

  • What's so exciting about the next decade of data

    要問些什麼?

  • in astronomy is,

    謝謝。

  • we don't even know how many answers

    (掌聲)

  • are out there waiting,

  • answers about our origins and our evolution.

  • How many answers are out there

  • that we don't even know the questions

  • that we want to ask?

  • Thank you.

  • (Applause)

So in 1781, an English composer,

1781 年,一位英國作家、 工程師兼天文學家

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    Max Lin 發佈於 2021 年 01 月 14 日
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