シャドーイング練習: How to Terraform Mars - WITH LASERS - 動画で英語スピーキングを学ぶ

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Mars is a disappointing hellhole lacking practically everything we need to stay alive.
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It looks like we'll only ever have small crews spend a miserable time hidden underground.
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Except we could terraform it into a green, new world.
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But to solve the planet's problems, we first need to make it worse and turn it into oceans of lava with gigantic lasers.
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This isn't a far -fetched science fiction tale.
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If humanity solves some of its pressing problems and ventures into space to expand into the solar system, this may not be that far off.
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Okay, so how do we terraform Mars quickly?
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Well, it's complicated.
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Mars is dry and has no soil to grow anything.
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Its atmosphere is too thin to breathe or protect us from radiation, giving you a high risk of cancer.
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So to turn it into a new home for humanity, we have to give it a proper atmosphere similar to Earth's.
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It should be made of 21 % oxygen, 79 % nitrogen and a tiny bit of CO2, as an average temperature of 14 degrees Celsius and under one bar of pressure.
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fertile soil to host living things.
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Then we need to install a biosphere on the surface, and prevent it all from being undone by installing protective measures that can stand the test of time.
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It is difficult, but a big laser makes it a lot easier.
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Challenge 1: The atmosphere.
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Some 4 billion years ago, Mars had a nice oxygen -rich atmosphere and was home to vast oceans and rivers.
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It held onto it for several hundred million years before it got blown away.
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Ultraviolet rays broke down the atmospheric gases and then the oceans until they were swept away by solar wind.
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Today, Mars is a dry, barren wasteland.
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Luckily, a sizeable portion of the water is frozen in deep reservoirs and in the polar ice caps,
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And enormous amounts of oxygen are bound as minerals in the Martian rocks, like the oxygen in the iron oxides that give the planet its rust red color,
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as well as carbon dioxide in carbonates.
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To free these gases, we need to reverse the reactions that lock them away by using thermolysis, which occurs at temperatures as high as on the surface of the Sun.
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In short, we want to melt the surface of Mars.
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The best way to do that would be to put lasers in orbit, aiming their beams down on Mars.
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is the ELI -NP, able to produce beams of 10 petawatts of power for a trillionth of a second.
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To melt Mars we need a laser twice as powerful that runs continuously.
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The easiest way is to use a solar -pumped laser that can be powered directly with sunlight.
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At its core are metal -infused glass rods that absorb energy and release it as a laser beam.
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If we build an array of mirrors in space about 11 times the size of the United States, we can focus enough sunlight Let's do it!
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As the lasers hit the surface, about 750 kilograms of oxygen and some carbon dioxide emerge from every cubic meter of rock melted.
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If we are efficient, our lasers only need to melt through the top 8 meters of the surface to get enough oxygen.
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It would look terrifying.
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The skies would be shrouded in storms, while the ground would glow red -hot, criss -crossed by currents of lava.
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Tireless laser beams sweep over the landscape, leaving trails too bright to look at.
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After they pass, the ground cools quickly.
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A strange snow falls.
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The ashes from all the elements that solidify as they cool down, like silicon and iron.
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Mars is still a cold planet at this point.
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A happy side effect of this inferno is
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that all the water in the polar ice caps and even deep underground rises into the sky as hot steam, forming clouds that rain down over the entire planet.
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They would wash out the nastier gases from the atmosphere like chlorine, and carry away harmful elements that accumulated on the surface.
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In the end, they would form shallow oceans, saltier than on Earth.
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We might need to do an extra clean -up afterwards.
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It would take about 50 years of continuous lasering to create our oxygen atmosphere.
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We could use this opportunity to dig deeper in some places to create the basins for salty oceans
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or rivers and spare some landmark features like Olympus Mons and Valles Marineris.
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We're not done though.
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The resulting atmosphere is nearly 100 % oxygen and only 0 .2 bar.
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It's hard to breathe and very flammable.
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To make it similar to Earth and a lot safer, which Mars is sadly lacking.
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We have to import it.
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The ideal source is Titan, a large moon of Saturn, covered in a thick atmosphere that's almost entirely nitrogen.
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We just have to move 3 ,000 trillion tons from the outer solar system to Mars.
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While that's not easy, it is doable.
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To process that much of Titan's atmosphere, we have to construct giant automated factories on its surface, powered by our lasers, to suck in the atmosphere and compress it into a liquid.
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This gets bullet -shaped tanks, which a mass driver shoots all the way to the red planet, where they explode and mix with the oxygen.
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We've already been able to send individual missions to Saturn in just a few years.
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With enough resources, it should be possible to complete the task within two generations.
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Of course, it would be much more convenient to have nitrogen left over from terraforming Venus on the site.
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We explained this in detail in another video.
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So, about a century after the start of the terraforming process, we have a breathable atmosphere that has the right gases.
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If the liberated CO2 isn't enough to warm it up to temperatures we can stand, we just add some super greenhouse gases.
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Mars at this point resembles a black marble from all the cooling lava, spotted with growing oceans and red patches where the old surface remains untouched.
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It's still a wasteland, no better than a desert on Earth.
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to fill it with life.
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Challenge 2: Biosphere.
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Installing a biosphere on a new planet is very difficult.
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Unexpected interactions between species or sudden diseases can destabilize it to the point of collapse.
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We would probably begin by seeding our young oceans with phytoplankton.
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Without competition, it would bloom rapidly, filling up the oceans to become the bottom of an aquatic food chain.
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Life on land is harder.
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Plants need nutrient -filled ground to sink their roots into, but most of the surface is the congealed remains of lava and ash.
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We could wait for thousands of years for water and wind to grind it down into finer sands, or try to do it manually.
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But we want to be quick, and we have a big laser.
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Turning the beam on and off in rapid succession would cause the ground to quickly heat up and contract, which breaks it into smaller and smaller pieces.
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and you get a sort of dark mud.
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Into this mud we can mix fungi and nitrogen fixing bacteria.
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They're able to absorb nitrogen and convert it into nitrate compounds to feed plants.
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The first plants we want to bring are native to volcanic
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islands on Earth since they're perfectly suited to the laser -blasted Martian landscape.
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Eventually the enriched mud becomes the foundation for grasslands and forests.
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In Mars's lower gravity trees can become very tall very fast.
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Their roots gather the nutrients they need and then dig deeper to turn more rocks into soil, forming a self -sustaining ecosystem.
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At this point, we can slowly introduce more plant varieties, insects and animals.
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Not mosquitoes, though.
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The new biosphere needs to be maintained to prevent it from falling out of balance.
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If plants grow too quickly and absorb too much carbon dioxide, the planet cools down too much.
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If key species die out, we could see Other species would move in to fill the void,
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but our Martian biosphere is not as flexible.
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It takes hundreds if not thousands of years before Mars becomes a stable environment.
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But eventually the planet will have the potential to sustain large human colonies.
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With air, water and food available, we can finally call Mars, black, blue and green, our home.
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A giant volcanic island in space.
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Will it last though?
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See? the long -term future.
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There is a problem we haven't addressed.
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Mars' core does not produce a magnetic field, so it doesn't have enough protection from solar radiation or cosmic rays.
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This becomes dangerous for the long -term health of Martian populations.
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So, as a final step, we need an artificial magnetic field.
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It doesn't have to be huge like Earth's, it just needs to deflect the solar wind enough so that it doesn't touch Mars.
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solar wind to the sides.
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A big superconducting ring powered by nuclear facilities is all it takes.
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It would orbit at the Mars Sun L1 point, keeping it constantly in between the Sun and Mars, and protect the new atmosphere.
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And that's it.
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Terraforming Mars would take some work, hefty resources, and probably a century or ten,
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but it would be the first time we've lived in a home designed and shaped solely by us and for us.
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A first step towards our future among the stars.
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Welcome to the Kurzgesagt Lab.
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Let's conduct a few stellar experiments.
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We'll first add some more mass to this protostar.
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More.
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A bit more.
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Wow, we've just created a blue giant, a star with ten times the mass of our Sun.
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Let's now add a couple of million years and see what happens.
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A supernova.
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Breathtaking.
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And look, it leaves behind a black hole.
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Fascinating stuff.
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Record our findings.
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Be careful to preserve the sparkle.
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It's now time for Duck's final inspection.
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This one is always a nail -biter.
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He has incredibly high standards.
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Lucky for us our work is scientifically accurate, offers an overview of important astrophysical processes, and is a real stunner.
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Duck approves.
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Looks like it's ready to be shared with the world as a poster.
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A very special piece of Kurzgesagt you can take home and touch.
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You can get this very special poster along with many other sciencey
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and spacey things created with love and care from our shop.
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Every Kurzgesagt product you buy directly funds another moment we get to spend working on our videos.
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Thank you so much for being a part of our story and for making this channel possible you -
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なぜこの動画で話す練習をするべきか？

この動画「How to Terraform Mars - WITH LASERS」は、宇宙探査と地球外の生活に関する大規模なプロジェクトについて説明しています。話し手は、火星をテラフォーミング（人間が住める環境に変えること）する過程を、科学的な観点から興味深く解説しています。このような内容は、IELTS スピーキング対策において非常に有益です。なぜなら、専門的な用語や概念を理解することで、より深い言語運用能力が養われます。また、実際の会話で科学や技術について話す自信がつき、自分の意見を述べる練習にもなります。さらに、視覚的な情報と音声を組み合わせることで、記憶の定着が促進されます。

文法と表現の文脈での分析

この動画では、いくつかの重要な文法構造と表現が用いられています。以下にその一部を示します：

  • 「create oceans and rivers」: このフレーズは「ocean」と「river」という名詞を用いて、具体的なアクションを示すことができます。動詞「create」によって、活動が強調されています。
  • 「we have to give it a proper atmosphere」: ここでは、義務を示す「have to」が使われており、計画の必要性が明確になっています。
  • 「Mars is a disappointing hellhole」: この表現は比喩的で、火星の状態を強調するために効果的です。また、強い形容詞「disappointing」が感情を引き出します。

これらの句やフレーズを用いることで、話し手は明確かつ興味深い説明を提供しています。英語を話す練習をする際には、これらの文法構造を意識して使うことが重要です。

一般的な発音の落とし穴

この動画には、視聴者にとって難しい発音やアクセントがいくつかあります。例えば、「terraform」と「atmosphere」という単語は特に注意が必要です。言葉の強弱やリズムが自然な会話には不可欠ですので、繰り返し発音練習を行うことをお勧めします。また、語尾の発音に気を付けることで、英語の発音を良くすることができます。

さらに、「radiation」や「solar wind」のような専門用語も発音しにくい場合があります。英語学習の一環として、YouTubeで英語学習しながらこれらの言葉を練習するのは非常に効果的です。

この動画を通じて、シンプルな英語の表現から専門的な言葉まで、幅広く学ぶことができるため、ぜひ積極的に話す練習を行いましょう。

この動画の文法

話し手がよく使っている文型を、動画の実際の表現とともに紹介します。

文型動画での表現
受動態 be + 過去分詞 — 誰がするかより、何が起きるかに焦点を当てるshould be made · were swept · is frozen
現在完了形 have/has + 過去分詞 — 過去の出来事が今も関係しているWe've already been · haven't addressed · we've lived

シャドーイングとは？英語上達に効果的な理由

シャドーイング（Shadowing）は、もともとプロの通訳者養成プログラムで開発された言語学習法で、多言語習得者として知られるDr. Alexander Arguelles によって広く普及されました。方法はシンプルですが非常に効果的：ネイティブスピーカーの英語を聞きながら、1〜2秒の遅延で声に出してすぐに繰り返す——まるで「影（shadow）」のように話者を追いかけます。文法ドリルや受動的なリスニングと異なり、シャドーイングは脳と口の筋肉が同時にリアルタイムで英語を処理・再現することを強制します。研究により、発音精度、抑揚、リズム、連音、リスニング力、そして会話の流暢さが大幅に向上することが確認されています。IELTSスピーキング対策や自然な英語コミュニケーションを目指す方に特におすすめです。

シャドーイングのやり方: ステップ別の完全ガイドを読む →