Pratique du Shadowing: The Most Extreme Explosion in the Universe - Apprendre l'anglais à l'oral avec la vidéo

Création de la leçon...
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Supernovae are the most powerful explosions in the universe, unleashing enough energy to outshine galaxies.
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We have no real metaphor for their power.
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If the sun were to magically go supernova, it would feel like you were being hit by the energy of a nuclear explosion every second for weeks.
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While supernovae are the engines of creation, forging the elements that enable life, they also burn sterile whole regions of galaxies.
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So, what would happen if one hit Earth?
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There are, roughly speaking, two ways to make a supernova.
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Either the core of a massive star implodes, or, less common, a white dwarf gains mass to the point where it ignites explosive nuclear fusion.
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The outcome is the same.
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A supernova explosion explosion.
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When we think of an explosion on Earth, we think of something that happens fast and ends.
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But a supernova is more like a volcanic eruption followed by a tsunami.
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At first, there's a colorful ball of hot, expanding gas, creating a spectacular cloud that will shine for about a month.
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But then, it doesn't stop.
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Hot and dangerous gas rushes outwards at speeds of 10,000 kilometers a second through the near vacuum of space, sweeping up the sparse gas of the galaxy.
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This wall of gas expands for tens of thousands of years
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and will eventually span up to dozens of light years until it finally cools off
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and disperses its substance back into the galaxy.
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So what if this star tsunami hits us?
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Well, the damage depends on how far away it is.
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Stage 1, thousands of light years away.
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Humans have witnessed dozens of supernovae, but all of them were thousands of light years away.
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They appeared as new stars some out shining the moon twinkling for a few weeks and disappearing
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Aside from looking very pretty at this distance.
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They don't do much to us
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Stage two 300 light years away
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Things begin to get a bit icky once a supernova occurs around 300 light years away
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We can expect one this close to us every few million
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years a single star giving the night sky an eerie glow like twilight
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And while this is far enough away and dim enough to not do harm to us, they can affect the Earth.
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At these distances, it's like being hit by the last weak waves of the star tsunami.
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Not strong enough to do real damage, but still noticeable.
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In fact, we know that over the past 10 million years, multiple supernovae have struck Earth from these distances
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because we can find radioactive isotopes of iron deep in the rocks and sediments at the bottom of the ocean.
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Amazingly, these supernovae around the solar system have cleared a 1,000 light-year wide pocket of space that's called the local bubble.
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They blew away the interstellar gas and dust, creating a lumpy wall of gas that's now a cradle for star formation.
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Stage 3, 150 light-years away.
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Once a supernova happens much closer than 300 light-years, we're approaching the zone where it does real damage.
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Stars have extremely powerful magnetic fields.
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When they die, the tsunami of Dead Star actually retains a lot of this magnetic energy, woven through the shockwave that expands outwards.
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In this highly magnetized cloud, we get conditions like in a huge particle accelerator that's accelerating charged particles like protons, nuclei and electrons to immense speeds.
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which means we have an expanding cloud
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that is shooting deadly radiation in all directions long after the bright light from the initial explosion has faded away.
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If a supernova happens too close by, waves of these cosmic rays will wash over the solar system for thousands of years.
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While we are mostly protected on Earth's surface by the atmosphere and ozone layer, the influx of extra radiation will still increase cancer and mutation rates.
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Not enough to cause a mass extinction, but it will be noticeable.
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Spaceflight would become impossible in the solar system as astronauts wouldn't survive the waves of radiation for long.
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We don't know exactly how bad this would be, but a supernova that is close enough may trap our species on Earth for generations, maybe thousands of years.
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It only gets worse from here.
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Stage 4, closer than 100 light years.
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Within 100 light years, things get bad as a supernova disrupts our climate in ways that we don't fully understand yet.
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there are a few unpleasant things happening all one after another.
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First, the high-energy photons arrive from the explosion, followed by many decades of radiation from the radioactive tsunami, both of which seriously damage the ozone layer,
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Earth's shield against harmful radiation.
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The ozone layer absorbs ultraviolet radiation by breaking apart ozone, O3, into O2 and a free oxygen atom,
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which later reforms back into another ozone molecule.
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But the supernova radiation breaks up nitrogen molecules that gobble up the free oxygen, the cycle and depleting the ozone layer quickly.
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Without a radiation shield, everybody living on the surface is exposed to very high levels of UV radiation from our sun.
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Cancer rates would skyrocket and just going outside during the day could be life-threatening.
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The extra radiation would also kill a lot, if not most, of the plankton in the oceans
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that live near the surface and are the basis for the marine food chains, leading to a mass extinction.
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Worse still, supernova radiation would ionize gas in the atmosphere, which means that it would punch through molecules and knock electrons off nuclei, leaving them charged.
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These charged nuclei then act as seeds for water vapor to gather and form massive global clouds.
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In the worst case, they would reflect enough sunlight to trigger an ice age.
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In fact, it's thought that the ice age 2.5 million years ago was caused by a supernova.
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Some scientists even think
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that a supernova about 60 light-years away might have been the cause of the Devonian mass extinction 350 million years ago.
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But wait, there's more.
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The electrons punched free by the radiation form enormous electric avalanches, or in other words, lightning.
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Earth is hit by some of the worst thunderstorms in millions of years.
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The intense lightning causes global wildfires that consume forests and crops, devastate cities disrupt our electrical grids and global supply chains,
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all while a decimated ozone layer leaks deadly radiation.
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While in the past the ecosystem may have bounced back from a nearby supernova after a few thousand or million years, there's no guarantee modern civilization can take a hit of this magnitude.
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We would face food shortages, skyrocketing prices and wars as nations struggle to not be consumed by chaos.
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So a supernova this close would at the very least do significant damage for hundreds or thousands of years,
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if not end our modern civilization and with it millions or even billions of lives.
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Still, humanity would likely survive and could recover.
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Stage 5, closer than 25 light years.
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A supernova closer than 25 light years means that we're in its kill radius, where a mass extinction is all but guaranteed.
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Probably about half of the ozone layer would be destroyed, and massive climatic disruption on a scale we've never witnessed would ravage Earth.
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Entire ecosystems would swiftly be wiped out by radiation as global wildfires envelop the planet.
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All the things described before happen, but way more intensely and much faster.
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A few people might survive for years in bunkers if they have food supplies, but the world they return to will be devastated and hostile to life for hundreds of thousands of years.
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Human extinction is extremely likely.
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Final stage, four light years.
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Being any closer to a supernova is very unlikely because space is big, but the effects would be extreme.
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Even from four light-years away, the distance to Alpha Centauri, a supernova would be almost as bright as the sun in the sky.
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While casting two shadows could be fun for a few hours, within days the Earth's surface gets as hot as a sauna, baking the surface for weeks until the explosion fades.
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The surface of Earth burns, scared of life.
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Even the oceans aren't safe unsafe.
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The massive amount of radiation that follows burns away the ozone layer, killing everything that sees sunlight.
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It would be the largest extinction event in history, reducing life to a few survivors in the deep sea and critters in the deep soil.
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Life basically has to start over.
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How worried do you need to be?
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So, should you worry?
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No. Fortunately, there are only a handful of stars that may explode within 1000 light-years of Earth, and none are close enough to be a serious threat.
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Even better, these stars will probably not go supernova for many millions of years.
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So you are safe.
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But there's no guarantee for the far future.
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As stars orbit the galaxy, our descendants may find themselves dangerously close to a supernova,
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but by then, a far more advanced and wiser humanity will hopefully be able to just move out of the way.
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In any case, you can sleep well tonight under the beautiful night sky.

Vocabulaire et conseils d’expression pour cette leçon

Cette leçon d’expression orale de niveau C1 s’appuie sur la vidéo « The Most Extreme Explosion in the Universe ». Les mots qui reviennent le plus souvent : supernova, radiation, star, ozone, Earth. Cette vidéo contient 101 phrases et 1507 mots à répéter en shadowing. La partie parlée dure 9:26. Le locuteur parle à un rythme naturel d’environ 160 mots par minute, proche d’une conversation courante. Seuls 76 % des mots font partie des 3 000 mots les plus courants en anglais, le vocabulaire est donc exigeant.

Vocabulaire clé de cette vidéo

Les 15 mots les plus avancés de la vidéo, avec leur prononciation et leur sens :

MotPrononciationSens
supernova nom/ˌsuː.pə(ɹ)ˈnəʊ.və/supernova
ozone nom/ˈoʊzoʊn/ozone
extinction nom/ɪkˈstɪŋkʃən/extinction
tsunami nom/(t)suːˈnɑːmi/tsunami, raz-de-marée
nucleus nom/ˈnuː.kli.əs/noyau
molecule nom/ˈmɑ.lɪ.kjul/molécule
skyrocket verbe/ˈskaɪˌɹɒk.ɪt/grimper en flèche, monter en flèche
wildfire nom/ˈwaɪldˌfaɪər/feu de forêt, FdF
disrupt verbe/dɪsˈɹʌpt/perturber, déranger
radioactive adjectif/ˌɹeɪdioʊˈæktɪv/radioactif
noticeable adjectif/ˈnəʊtɪsəbl̩/repérable, détectable
ecosystem nom/ˈikoʊˌsɪstəm/écosystème
sunlight nom/ˈsʌnˌlaɪt/lumière du soleil
fade verbe/feɪd/s'affadir, faner
consume verbe/kənˈsum/consommer

Les verbes à particule que vous entendrez

MotSens
blow away verbesouffler
break up verberompre, couper
start over verberecommencer
wipe out verbeanéantir

La grammaire de cette vidéo

Les structures que le locuteur utilise le plus, avec les mots exacts de la vidéo :

StructureDans la vidéo
Voix passive be + participe passé — l’accent est mis sur ce qui arrive, pas sur qui le faitbeing hit · is exposed · was caused
Present perfect have/has + participe passé — une action passée qui compte encore maintenanthave witnessed · have struck · have cleared

Prononciation à surveiller

Le locuteur utilise 9 contractions et formes réduites, comme don't, we're, aren't. Prononcez-les sous leur forme courte, telles que vous les entendez.

  • Les sons « th »: thunderstorm /ˈθʌn.dɚˌstɔɹm/, threaten /ˈθɹɛt.n̩/
  • Les sons « sh » et « zh »: extinction /ɪkˈstɪŋkʃən/, civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, avalanche /ˈævəlɑːnʃ/, outshine /aʊtˈʃaɪn/, unleash /ʌnˈliʃ/
  • Mots longs — placez bien l’accent: supernova /ˌsuː.pə(ɹ)ˈnəʊ.və/, radioactive /ˌɹeɪdioʊˈæktɪv/, ecosystem /ˈikoʊˌsɪstəm/, civilization /ˌsɪv.ɪ.laɪˈzeɪ.ʃən/, accelerator /əkˈsɛl.əˌɹeɪ.tɚ/

Les sons difficiles pour les francophones :

  • /h/ — il se souffle, il n’est pas muet: harmful /ˈhɑɹmfl̩/, hostile /ˈhɑstəl/
  • /tʃ/ et /dʒ/ — à ne pas adoucir en « ch » et « j »: magically /ˈmæd͡ʒ.ɪ.kli/, ravage /ˈɹævɪd͡ʒ/, nitrogen /ˈnaɪ.tɹə.d͡ʒən/, forge /fɔɹd͡ʒ/, shortage /ˈʃɔː(ɹ)tɪd͡ʒ/
  • /r/ anglais — langue recourbée, sans frotter la gorge: supernova /ˌsuː.pə(ɹ)ˈnəʊ.və/, skyrocket /ˈskaɪˌɹɒk.ɪt/, wildfire /ˈwaɪldˌfaɪər/, disrupt /dɪsˈɹʌpt/, radioactive /ˌɹeɪdioʊˈæktɪv/

Comment s’entraîner avec cette vidéo

  1. Écoutez la vidéo en entier une fois sans parler et notez les mots que vous ne connaissez pas.
  2. Commencez à la vitesse 0,75×, répétez phrase par phrase, puis revenez à la vitesse normale quand cela devient facile.
  3. Enregistrez-vous et comparez avec l’original, en faisant attention à des mots comme supernova, ozone, extinction.

Qu'est-ce que la technique du Shadowing ?

Le Shadowing est une technique d'apprentissage des langues fondée sur la science, développée à l'origine pour la formation des interprètes professionnels. Le principe est simple mais puissant : vous écoutez de l'anglais natif et le répétez immédiatement à voix haute — comme une ombre suivant le locuteur avec un décalage de 1 à 2 secondes. Les recherches montrent une amélioration significative de la précision de la prononciation, de l'intonation, du rythme, des liaisons, de la compréhension orale et de la fluidité.

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