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B1 中級 英語 12:12 Educational

Introduction to Astronomy: Crash Course Astronomy #1

CrashCourse · 5,478,846 回視聴 · 追加日 3週間前

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00:03

Hello, and welcome to Crash Course Astronomy! I’m your host, Phil Plait, and I’ll be

00:06

taking you on a guided tour of the entire Universe. You might want to pack a lunch.

00:21

Over the course of this series we’ll explore planets, stars, black holes, galaxies, subatomic

00:27

particles, and even the eventual fate of the Universe itself.

00:31

But before we step into space, let’s take a step back. I wanna talk to you about science.

00:36

There are lots of definitions of science, but I’ll say that it’s a body of knowledge,

00:40

and a method of how we learned that knowledge.

00:42

Science tells us that stuff we know may not be perfectly known; it may be partly or entirely

00:47

wrong. We need to watch the Universe, see how it behaves, make guesses about why it’s

00:53

doing what it’s doing, and then try to think of ways to support or disprove those ideas.

00:57

That last part is important. Science must be, above all else, honest if we really want

01:03

to get to the bottom of things.

01:05

Understanding that our understanding might be wrong is essential, and trying to figure

01:09

out the ways we may be mistaken is the only way that science can help us find our way

01:14

to the truth, or at least the nearest approximation to it.

01:17

Science learns. We meander a bit as we use it, but in the long run we get ever closer

01:23

to understanding reality, and that is the strength of science. And it’s all around us!

01:28

Whether you know it or not, you’re soaking in science.

01:31

You’re a primate. You have mass. Mitochondria

01:34

in your cells are generating energy. Presumably, you’re breathing oxygen.

01:38

But astronomy is different. It’s still science, of course, but astronomy puts you in your place.

01:43

Because of astronomy, I know we’re standing on a sphere of mostly molten rock and metal

01:48

13,000 kilometers across, with a fuzzy atmosphere about 100 km high, surrounded by a magnetic

01:54

field that protects us from the onslaught of subatomic particles from the Sun 150 million

02:00

km away, which is also flooding space with light that reaches across space, to illuminate

02:05

the planets, asteroids, dust, and comets, racing out past the Kuiper Belt, through the

02:10

Oort Cloud, into interstellar space, past the nearest stars, which orbit along with

02:14

gas clouds and dust lanes in a gigantic spiral galaxy we call the Milky Way that has a supermassive

02:20

black hole in its center, and is surrounded by 150 globular clusters and a halo of dark

02:25

matter and dwarf galaxies, some of which it’s eating, all of which can be seen by other

02:29

galaxies in our Local Group like Andromeda and Triangulum, and our group is on the outskirts

02:34

of the Virgo galaxy cluster, which is part of the Virgo supercluster, which is just one

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