Pratique du Shadowing: Introduction to Astronomy: Crash Course Astronomy #1 - Apprendre l'anglais à l'oral avec la vidéo
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Hello, and welcome to Crash Course Astronomy.
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I'm your host, Phil Plait, and I'll be taking you on a guided tour of the entire universe.
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You might want to pack a lunch.
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Over the course of this series, we'll explore planets, stars, black holes, galaxies, subatomic particles, and even the eventual fate of the universe itself.
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But before we step into space, let's take a step back.
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I want to talk to you about science.
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There are lots of definitions of science, but I'll say that it's a body of knowledge and a method of how we learned that knowledge.
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Science tells us that stuff we think we know may not be perfectly known.
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It may be partly or entirely wrong.
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We need to watch the universe, see how it behaves, make guesses about why it's doing what it's doing,
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and then try to think of ways to support or disprove those ideas.
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That last part is important.
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Science must be, above all else, honest if we really want to get to the bottom of things.
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Understanding that our understanding might be wrong is essential, and trying to figure out the ways we may be mistaken is the only way
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that science can help us find our way to the truth .
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Science learns.
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We meander a bit as we use it, but in the long run we get closer and closer to understanding reality,
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and that That is the strength of science, and it's all around us.
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Whether you know it or not, you're soaking in science.
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You're a primate, you have mass, mitochondria in your cells are generating energy, presumably you're breathing oxygen.
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But astronomy is different.
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It's still science, of course, but astronomy puts you in your place.
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Because of astronomy, I know we're standing on a sphere of mostly molten rock and metal 13 ,000 kilometers across,
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with a fuzzy atmosphere about 100 kilometers high,
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surrounded by a magnetic field that protects us from the onslaught of subatomic particles from the Sun 150 million kilometers away.
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Which is also flooding space with light that reaches across space to illuminate the planets, asteroids, dust, and comets, racing out past the Kuiper Belt,
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through the Oort Cloud, into interstellar space, past the nearest stars, which orbit along with gas clouds and dust lanes,
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in a gigantic spiral galaxy we call the Milky Way, that has a supermassive black hole in its center,
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and is surrounded by 150 globular clusters and a halo of dark matter and dwarf galaxies, some of which it's eating,
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all of which can be seen by other galaxies in our local group, like Andromeda and Triangulum.
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And our group is on the outskirts of the Virgo Galaxy Cluster, which is part of the Virgo Super Cluster,
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which is just one of many other gigantic structures that stretch most of the way across the visible universe,
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which is 90 billion light -years across and expanding every day, even faster today than yesterday, day due to mysterious dark energy,
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and even all that might be part of an infinitely larger multiverse that extends forever both in time and space.
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See?
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Astronomy puts you in your place.
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But what exactly is astronomy?
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This isn't necessarily an obvious thing to ask.
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When I was a kid, it was easy.
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Astronomy is the study of things in the sky — the Sun, Moon, stars, galaxies, and stuff like that.
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But it's not so easy to pigeonhole these days.
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Take, for example, Mars.
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When I haul my scope out to the end of my driveway and look at Mars, that's astronomy, right? Of course!
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But what about the rovers there?
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Those machines aren't doing astronomy, surely.
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They're doing chemistry, geology, hydrology, petrology.
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Everything but astronomy.
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So nowadays, what's astronomy?
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I'd say it's still studying stuff in the sky, but it's branched out quite a bit from there.
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Borders between it and other fields of science are fuzzy, a theme I'll be hitting on several times over this series.
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Humans might like firm, delineated boundaries between things, but nature isn't so picky.
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And that brings us to our first edition of Focus On.
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This week's topic, astronomers.
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Who are we?
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What do we do?
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I used to look through telescopes for a living, or at least study the data that came from detectors strapped onto them.
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But now I talk and write about astronomy, and relegate my viewing to my personal backyard telescope.
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But I still consider myself an astronomer.
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So that should give you an idea that there's a lot of wiggle room in the profession.
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In fact, when I worked on Hubble Space Telescope, I was actually hired as a programmer.
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I coded in the language used by the folks helping to build
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and calibrate a camera that was due to launch into space and be installed onto Hubble by an astronaut.
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Once the data from that camera are taken and analyzed, you have to know what to do with them.
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Do the observations fit the physical model of how stars blow up, or how galaxies form, or the way gas flows through space?
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Well, you better know your math and physics, because that's how we test our hypotheses.
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And someone who does that is generally called an astrophysicist.
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Of course, those telescopes and detectors don't create themselves.
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We need engineers to design and build them, and technicians to use them.
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Most astronomers don't actually use the telescopes themselves anymore.
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Someone who's trained in their specific use does that for them.
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Some of those instruments go into space, and some go to other worlds like the Moon and Mars.
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We need astronomers and engineers and software programmers who can build those, too.
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And then, at the end of all this, we need people to tell you all about it — teachers, professors, writers, video makers, even artists.
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So I'll tell you what.
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If you have an interest in the universe, if you love to look up at the stars,
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if you crave to understand what's going on literally over your head, then who am I to say you're not an astronomer?
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However you define astronomy, humans have been looking up at the sky for as long as we've been human.
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Certainly, ancient people noticed the big, glowy ball in the sky, and how it lit everything up while it was up,
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and how it got dark when it was gone.
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The other, fainter, glowy thing tried, but wasn't quite as good at lighting up the night.
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They probably took that sort of thing pretty seriously.
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They probably also noticed that when certain stars appeared in the sky, the weather started getting warmer and the days longer,
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and when other stars were seen, the weather would get colder and daytime shortened.
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And when humans settled down, discovered agriculture, and started farming, noticing those patterns in the sky would have had an even greater impact.
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It told them when to plant seeds and when to harvest.
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The cycles in the sky became pretty important.
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So important that it wasn't hard to imagine gods up there looking down on us weak
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and ridiculous humans interfering with our lives.
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Surely if the stars tell us when to plant and control the weather, seasons, and the length of the day, they control our lives, too.
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And astrology was born.
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Astrology literally means study of the stars.
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As a word, it's been used before science became a formal method of studying nature.
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It irks me a bit, since it got the good name and now we're stuck with astronomy, which means law or culture of the stars,
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and that's not really what we do.
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But what the heck?
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Words change meaning over time, and now it's pretty well understood that astronomy is science and astrology.. isn't.
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Millennia ago, astrology was as close to science as you got.
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It had some of the flavors of science.
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Astrologers observed the skies, made predictions about how it would affect people,
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and then those people would provide evidence for it by swearing up and down it worked.
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The thing is, it really didn't.
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The fault of astrology lies in ourselves and not our stars.
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People tend to remember the hits and forget the misses when predictions are made, which is why they sometimes sit in casinos pumping nickels into machines
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that are proven to be nothing more than a method for reducing the number of nickels you have.
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But astrology led people to really study the sky and find the patterns there,
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which led to a more rigorous understanding of how things really worked in the heavenly vault.
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It wasn't overnight, of course.
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This took centuries.
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Before the invention of the telescope, keen observers built all sorts of odd and wonderful devices to measure the heavens.
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And in fact, it was before the telescope was first turned to the sky that a huge revolution in astronomy took place.
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It is patently obvious that the ground you stand on is fixed, rooted if you will, and the skies turn above us.
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The sun rises, the sun sets.
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The moon rises and sets.
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The stars themselves wheel around the sky at night.
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Clearly the Earth is motionless and the sky is what is actually moving.
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In fact, if you think about it, geocentrism makes perfect sense, that all the objects in the sky revolve about the Earth
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and are fixed to a series of nested spheres, some of which are transparent, maybe made of crystal, which spin once per day.
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The stars may just be holes in otherwise opaque spheres letting sunlight through.
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Sounds silly to you, doesn't it?
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Well, here's the thing.
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If you don't have today's modern understanding of how the cosmos works, this whole multiple shells of things in the sky thing actually does make sense.
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It explains a lot of what's going on over your head.
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And if it was good enough for Plato, Aristotle and Ptolemy, then by God it was good enough for you.
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And speaking of which, it was endorsed by the major religions of the time,
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so maybe it's better if you just nod and agree and don't think about it too hard.
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But a few centuries ago, things changed.
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Although he wasn't the first, the Polish mathematician and astronomer Copernicus came up with the idea that the Sun was the center of the solar system,
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not the Earth.
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His idea had problems, which we'll get to in a later episode, but but it did an incrementally better job than geocentrism.
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And then along came Tycho Brahe and Johannes Kepler, who modified that system, making it even better.
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Then, Isaac Newton.
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Oh, Newton.
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He invented calculus, partly to help him understand the way objects moved in space.
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Over time, our math got better, our physics got better, and our understanding grew.
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Applied math was a revolution in astronomy, and then the use of telescopes was another.
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Galileo didn't invent the telescope, by the way, but made them better.
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Newton invented a new kind that was even better than that, and we've run with the idea from there.
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Then, about a century ago, came another revolution—photography.
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We could capture much fainter objects on glass plates sprayed with light -sensitive chemicals, which revealed stars otherwise invisible to us.
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Details in galaxies, beautiful clouds of gas and dust in space.
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And then, in the latter half of the last century, Digital detectors were invented, which were even more sensitive than film.
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We could use computers to directly analyze observations, and our knowledge leaped again.
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When these were coupled with telescopes sent into orbit around the Earth, where our roiling and boiling atmosphere doesn't blur out observations,
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we began yet another revolution.
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And where are we now?
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We've come such a long way.
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What questions can we routinely ask that our ancestors would not have dared?
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What statements made with a pretty good degree of certainty?
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Think on this.
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The lights in the sky are stars.
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There are other worlds.
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We take the idea of looking for life on alien planets seriously and spend billions of dollars doing it.
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Our galaxy is one of a hundred billion others.
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We can only directly see 4 % of the universe.
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Stars explode.
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And when they do, they create the stuff of life.
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The iron in our blood, the calcium in our bones, the phosphorus that is the backbone of our DNA.
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The most common kind of star in the universe is so faint you can't even see it without a telescope.
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Our solar system is filled to overflowing, with worlds more bizarre than we could have dreamed.
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Nature has more imagination than we do.
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It comes up with some nutty stuff.
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We're clever too, we big -brained apes.
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We've learned a lot.
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But there's still a long way to go.
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So with that, I think we're ready.
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Let's explore the universe.
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Today, you learned what astronomy is, and that astronomers aren't just people who operate telescopes, but include mathematicians, engineers, technicians, programmers, and even artists.
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We also wrapped up with a quick history of the origins and development of astronomy, from ancient observers to the Hubble Space Telescope.
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Crash Course is produced in association with PBS Digital Studios.
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This episode was written by me, Phil Plait.
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The script was edited by Blake DePastino, and our consultant is Dr. Michelle Thaller.
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It was co -directed by Nicholas Jenkins and Michael Aranda, and the graphics is Thought Cafe.
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Vocabulaire et conseils d’expression pour cette leçon
Cette leçon d’expression orale s’appuie sur la vidéo « Introduction to Astronomy: Crash Course Astronomy ». Les mots qui reviennent le plus souvent : astronomy, star, sky, science, telescope. Cette vidéo contient 53 phrases et 2244 mots à répéter en shadowing. La partie parlée dure 11:59. Le locuteur parle vite, environ 187 mots par minute : attendez-vous à des liaisons et à des sons réduits. Seuls 80 % des mots font partie des 3 000 mots les plus courants en anglais, le vocabulaire est donc exigeant. 12 de ses 53 phrases sont des questions : un bon entraînement pour l’intonation interrogative et les réponses courtes.
Vocabulaire clé de cette vidéo
15 mots de la vidéo à retenir, avec leur prononciation et leur sens :
| Mot | Prononciation | Sens |
|---|---|---|
| astronomy nom | /əˈstɹɑ.nə.mi/ | astronomie |
| telescope nom | /ˈtɛl.əˌskoʊp/ | lunette, télescope |
| galaxy nom | /ˈɡæl.ək.si/ | galaxie |
| invent verbe | /ɪnˈvɛnt/ | inventer |
| dust nom | /dʌst/ | poussière |
| mathematics nom | /mæθ(.ə)ˈmæt.ɪks/ | mathématiques |
| observation nom | /ˌɑbzɚˈveɪʃn̩/ | observation |
| faint adjectif | /feɪnt/ | faible, faire un malaise |
| detector nom | /dɪˈtɛktə(ɹ)/ | détecteur |
| programmer nom | /ˈpɹoʊɡɹæmɚ/ | programmeur, programmeuse |
| atmosphere nom | /ˈætməsˌfɪɹ/ | atmosphère |
| cloud nom | /ˈklaʊ̯d/ | nuage |
| sensitive adjectif | /ˈsɛn.sɪt.ɪv/ | sensible |
| physics nom | /ˈfɪz.ɪks/ | physique |
| explore verbe | /ɪkˈsploɹ/ | explorer |
Les verbes à particule que vous entendrez
| Mot | Sens |
|---|---|
| come up with verbe | inventer, imaginer |
| blow up verbe | faire sauter |
| figure out verbe | cerner |
| look down on verbe | mépriser, regarder de haut |
| settle down verbe | s'installer |
Des phrases à répéter
Des phrases courtes et complètes de la vidéo, à réutiliser dans la conversation de tous les jours :
- What do we do?
- Sounds silly to you, doesn’t it?
- We’ve come such a long way!
- We’re clever too, we big-brained apes.
La grammaire de cette vidéo
Les structures que le locuteur utilise le plus, avec les mots exacts de la vidéo :
| Structure | Dans la vidéo |
|---|---|
| Voix passive be + participe passé — l’accent est mis sur ce qui arrive, pas sur qui le fait | may not be perfectly known · may be mistaken · is surrounded |
| Propositions relatives who / which + proposition — une précision sur une personne ou une chose | Cluster, which is · someone who does · astronomy, which means |
| Present perfect have/has + participe passé — une action passée qui compte encore maintenant | we've been · it's been · we've run |
Prononciation à surveiller
Le locuteur utilise 40 contractions et formes réduites, comme don't, I'll, wasn't. Prononcez-les sous leur forme courte, telles que vous les entendez.
- Les sons « th »: mathematics /mæθ(.ə)ˈmæt.ɪks/, breathe /bɹiːð/, hypothesis /haɪˈpɒθɪsɪs/, mathematician /ˌmæθ.(ə.)məˈtɪʃ.ən/
- Les sons « sh » et « zh »: observation /ˌɑbzɚˈveɪʃn̩/, prediction /pɹɪˈdɪkʃən/, technician /tɛkˈnɪʃən/, capture /ˈkæp.(t)ʃɚ/, shell /ʃɛl/
- Mots longs — placez bien l’accent: astronomy /əˈstɹɑ.nə.mi/, mathematics /mæθ(.ə)ˈmæt.ɪks/, necessarily /ˌnɛs.əˈsɛɹ.ə.li/, ridiculous /ɹɪˈdɪk.jə.ləs/, photography /fəˈtɑ.ɡɹə.fi/
Les sons difficiles pour les francophones :
- /h/ — il se souffle, il n’est pas muet: hire /ˈhaɪɹ/, harvest /ˈhɑɹ.vəst/, heck /hɛk/, behave /bɪˈheɪv/, haul /hɔl/
- /tʃ/ et /dʒ/ — à ne pas adoucir en « ch » et « j »: gigantic /d͡ʒaɪˈɡæntɪk/, agriculture /ˈæɡ.ɹɪˌkʌl.t͡ʃɚ/, stretch /stɹɛt͡ʃ/, oxygen /ˈɑksɪd͡ʒən/, generate /ˈd͡ʒɛn.ə.ɹeɪt/
- /r/ anglais — langue recourbée, sans frotter la gorge: astronomy /əˈstɹɑ.nə.mi/, detector /dɪˈtɛktə(ɹ)/, programmer /ˈpɹoʊɡɹæmɚ/, atmosphere /ˈætməsˌfɪɹ/, explore /ɪkˈsploɹ/
Comment s’entraîner avec cette vidéo
- Écoutez la vidéo en entier une fois sans parler et notez les mots que vous ne connaissez pas.
- Commencez à la vitesse 0,75×, répétez phrase par phrase, puis revenez à la vitesse normale quand cela devient facile.
- Enregistrez-vous et comparez avec l’original, en faisant attention à des mots comme astronomy, telescope, galaxy.
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.