쉐도잉 연습: The Last Star in the Universe – Red Dwarfs Explained - 영상으로 영어 말하기 배우기

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One day the last star will die and the universe will turn dark forever.
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It will probably be a red dwarf, a tiny kind of star that's also one of our best bets to find alien life
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and might be the last home of humanity before the universe becomes uninhabitable.
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So what do we know about them and why are they our last hope?
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At least 70% of stars in the universe are red dwarfs.
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They are the tiniest stars out there, with only about 7-50% of the mass of our Sun.
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Not that much bigger than our planet Jupiter, which is still huge though.
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They are also very dim.
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It's impossible to see them with the naked eye.
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You've never seen one in the night sky.
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Even with all our technology, we can only clearly observe red dwarfs in our neighborhood.
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Approximately 20 of the 30 stars close to Earth are red dwarfs.
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Like all stars, red dwarfs fuse hydrogen into helium.
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But while more massive stars accumulate all the fuse helium in their cores, red dwarfs stay convective, meaning that the helium and hydrogen constantly mix.
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So they use up their fuel incredibly slowly before they're extinguished.
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Red dwarfs burn so slowly that their average lifespan is between 1 and 10 trillion years.
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By comparison, the Sun will survive for another 5 billion years.
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Because the universe is only 13.75 billion years old, not a single red dwarf has reached later development stages.
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Every single one of the trillions that exist is still a baby.
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Speaking of babies, the smallest star in the entire universe is also a red dwarf, because small red dwarfs are right on the verge of being a star at all,
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just a tiny bit less hydrogen, and they are mere brown dwarfs, failed stars that cannot sustain a fusion reaction for long.
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So what about aliens, or a new home for humanity?
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Since our sun will die one day, we'll eventually need to look for a new home.
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And where there are habitable planets, there might also be aliens.
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The Kepler Space Observatory found
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that at least half of all red dwarfs host rock planets between half and four times the mass of our Earth.
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Many of them are in the habitable zone, the area around a star where water can be liquid.
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But since red dwarfs burn at relatively cold temperatures, a planet would need to be really close to be hospitable, probably as close as Mercury to our Sun, or even closer.
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Which brings with it all kinds of problems.
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For example, a planet this close to a star would probably be tidally locked, meaning the same side would always face it.
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This side would be incredibly hot, while the shadow side would be frozen, which makes it hard for life to develop.
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Although a planet with a big enough ocean might be able to distribute the star's energy and create some kind of stability.
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All the gravitational forces of the red dwarf could squeeze the planet
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and heat it up so much that it might lose all its water over time.
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These planets could end up like Venus, a hot, burning hell.
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Another problem is that many red dwarfs vary in their energy output.
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They can be covered in star spots that can dim their emitted light by up to 40% for months, which would cause oceans on planets to freeze over.
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At other times they can emit powerful solar flares, sudden outbursts of energy incredibly powerful.
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These red dwarfs can double their brightness in minutes, which could strip away sizeable portions of a planet's atmosphere and burn it, rendering it sterile.
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On the other hand, their extremely long lifespan is a big plus.
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A red dwarf with just moderate levels of activity could be an amazing place for a planet that hosts life.
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Life on Earth has existed for about 4 billion years, and we have about a billion years left before the Sun becomes so hot that complex life on Earth will become impossible.
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We will either die out or leave Earth and look for a new home.
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We could build a civilization for potentially trillions of years around a red dwarf with the right conditions.
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About 5% of the red dwarfs in the Milky Way may host habitable, roughly Earth-sized planets.
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That would be more than 4 billion in total.
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But life may not even need a planet like Earth.
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Candidates for life around a red dwarf may be the moons of gas giants or so called super earths, really massive rocky planets.
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All in all there are an estimated 60 billion potentially habitable planets around red dwarfs and that's in the Milky Way alone.
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So red dwarfs might become really important for our survival in the future.
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But everything has to die at some point, even red dwarfs.
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When in trillions of years the life of the last red dwarf in the universe is about to end, it will not be a very spectacular event.
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As its hydrogen runs out it shrinks, becoming a blue dwarf burning out completely.
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After its fuel is spent, it's transformed into a white dwarf, an object about as small as Earth,
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packed very densely and made of degenerate gases, mostly of helium-4 nuclei.
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no more source of energy, it will cool extremely slowly over trillions of years until it becomes its final form, a cold, black dwarf.
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White and black dwarfs are so fascinating that they deserve their own video.
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Anyway, it's going to be a long time before the last stars in the universe vanish.
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It's kind of uplifting to know that if humanity succeeds in venturing into space, we have plenty of time before the universe turns out the lights.
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Our videos are made thanks to your support on Patreon.com.
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If you want to help us make more of them, we really appreciate your support.

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이 레슨의 어휘와 말하기 포인트

이 C1 수준 말하기 레슨은 영상 “The Last Star in the Universe – Red Dwarfs Explained”을(를) 바탕으로 합니다. 가장 자주 반복되는 단어는 다음과 같습니다: dwarf, planet, star, Earth, universe. 이 영상에는 섀도잉할 문장 61개와 단어 976개가 있습니다. 말하는 구간의 길이는 5:45입니다. 화자는 분당 약 170단어로, 일상 대화에 가까운 자연스러운 속도로 말합니다. 단어의 82%가 영어에서 가장 많이 쓰이는 3,000단어에 속합니다. 나머지는 연습 전에 미리 확인해 두세요.

이 영상의 핵심 어휘

영상에서 가장 어려운 단어 13개를 발음, 뜻과 함께 정리했습니다.

단어발음뜻
helium 명사/ˈhiː.li.əm/헬륨
hydrogen 명사/ˈhaɪdɹəd͡ʒ(ə)n/수소
fuse 명사/fjuːz/도화선
accumulate 동사/əˈkjuːmjʊˌleɪt/모으다, 축적하다
vanish 동사/ˈvænɪʃ/사라지다
nucleus 명사/ˈnuː.kli.əs/핵심, 핵
render 동사/ˈɹɛn.dɚ/일어나게 하다, 하게하다
squeeze 동사/skwiːz/짜다
civilization 명사/ˌsɪv.ɪ.laɪˈzeɪ.ʃən/문명
fusion 명사/ˈfjuː.ʒən/핵융합
transform 동사/tɹænsˈfɔɹm/변형시키다, 변형하다
spectacular 형용사/spɛkˈtæk.jə.lɚ/눈부신
observe 동사/əbˈzɜːv/관찰하다

이 영상의 문법

화자가 가장 많이 쓰는 문형을 영상 속 실제 표현과 함께 정리했습니다.

문형영상 속 표현
수동태 be + 과거분사 — 누가 하는지보다 무슨 일이 일어나는지에 초점would be frozen · can be covered · is spent
현재완료 have/has + 과거분사 — 과거의 일이 지금도 관련이 있을 때You've never seen · has reached · has existed
관계절 who / which + 절 — 사람이나 사물에 대한 추가 정보Jupiter, which is · frozen, which makes

주의할 발음

화자는 they're, we'll, you've 같은 축약형과 약화된 형태를 3번 사용합니다. 들리는 대로 짧게 발음하세요.

  • “sh”와 “zh” 소리: extinguish /ɪkˈstɪŋ.ɡwɪʃ/, gravitational /ˌɡɹævɪˈteɪʃənəl/, vanish /ˈvænɪʃ/, civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, fusion /ˈfjuː.ʒən/
  • 긴 단어 — 강세 위치에 주의: habitable /ˈhæbɪtəbəl/, accumulate /əˈkjuːmjʊˌleɪt/, degenerate /dɪˈd͡ʒɛnəɹɪt/, gravitational /ˌɡɹævɪˈteɪʃənəl/, uninhabitable /ˌʌnɪnˈhæbɪtəbəl/

한국어 화자가 어려워하는 소리:

  • /f/ — ㅍ(/p/)으로 바꾸지 말고 윗니를 아랫입술에 대기: lifespan /ˈlaɪf.spæn/, fuse /fjuːz/, fascinate /ˈfæsɪneɪt/, flare /flɛɚ̯/, fusion /ˈfjuː.ʒən/
  • /v/ — ㅂ(/b/)과 구별하기: convective /kənˈvɛk.tɪv/, gravitational /ˌɡɹævɪˈteɪʃənəl/, vanish /ˈvænɪʃ/, verge /vɜːd͡ʒ/, civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/
  • /z/ — ㅈ이 아니라 성대를 울리는 /s/: fuse /fjuːz/, squeeze /skwiːz/, civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, observe /əbˈzɜːv/

이 영상으로 연습하는 방법

  1. 먼저 말하지 않고 영상을 끝까지 듣고 모르는 단어를 적어 둡니다.
  2. 0.75배속으로 한 문장씩 섀도잉을 시작하고, 익숙해지면 보통 속도로 돌아갑니다.
  3. 자신의 목소리를 녹음해 원본과 비교하고, helium, hydrogen, fuse 같은 단어에 특히 주의합니다.

쉐도잉이란? 영어 실력을 빠르게 키우는 과학적 방법

쉐도잉(Shadowing)은 원래 전문 통역사 훈련을 위해 개발된 언어 학습 기법으로, 다언어 학자인 Dr. Alexander Arguelles에 의해 대중화된 방법입니다. 핵심 원리는 간단하지만 매우 강력합니다: 원어민의 영어를 들으면서 1~2초의 짧은 지연으로 즉시 소리 내어 따라 말하는 것——마치 '그림자(shadow)'처럼 화자를 따라가는 것입니다. 문법 공부나 수동적인 청취와 달리, 쉐도잉은 뇌와 입 근육이 동시에 실시간으로 영어를 처리하고 재현하도록 훈련합니다. 연구에 따르면 이 방법은 발음 정확도, 억양, 리듬, 연음, 청취력, 말하기 유창성을 크게 향상시킵니다. IELTS 스피킹 준비와 자연스러운 영어 소통을 원하는 분들에게 특히 효과적입니다.

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