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Will the Sun ever burn out? 00:00
We Asked a NASA Scientist. 00:03
Well, the Sun, just like the stars we see at night, 00:05
is a star. 00:08
It's a giant ball of super hot hydrogen. 00:09
Gravity squeezes it in and it creates energy, 00:13
which is what makes the Sun shine. 00:17
Eventually, it will use up all of that hydrogen. 00:20
But in the process, it's creating helium. 00:23
So it will then use the helium. 00:26
And it will continue to use 00:29
larger and larger elements 00:30
until it can't do this anymore. 00:32
And when that happens, 00:35
it will start to expand 00:36
into a red giant 00:37
about the size of the inner planets. 00:39
Then it will shrink back down 00:42
into a very strange star called a white dwarf — 00:45
super hot, 00:49
but not very bright 00:51
and about the size of the Earth. 00:52
But our Sun has a pretty long lifetime. 00:55
It's halfway 00:58
through its 10-billion-year lifetime. 00:59
So the Sun will never really burn out, 01:02
but it will change and be a very, very different 01:06
dim kind of star 01:09
when it reaches the end of its normal life. 01:11
We Asked a NASA Scientist. 01:13
NASA. A NASA 360 Production. 01:15

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Lyrics & Translation

[English]
Will the Sun ever burn out?
We Asked a NASA Scientist.
Well, the Sun, just like the stars we see at night,
is a star.
It's a giant ball of super hot hydrogen.
Gravity squeezes it in and it creates energy,
which is what makes the Sun shine.
Eventually, it will use up all of that hydrogen.
But in the process, it's creating helium.
So it will then use the helium.
And it will continue to use
larger and larger elements
until it can't do this anymore.
And when that happens,
it will start to expand
into a red giant
about the size of the inner planets.
Then it will shrink back down
into a very strange star called a white dwarf —
super hot,
but not very bright
and about the size of the Earth.
But our Sun has a pretty long lifetime.
It's halfway
through its 10-billion-year lifetime.
So the Sun will never really burn out,
but it will change and be a very, very different
dim kind of star
when it reaches the end of its normal life.
We Asked a NASA Scientist.
NASA. A NASA 360 Production.

Key Vocabulary

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Vocabulary Meanings

Sun

/sʌn/

A2
  • noun
  • - the star at the center of the solar system

star

/stɑːr/

A2
  • noun
  • - a luminous celestial body

hydrogen

/ˈhaɪdrədʒən/

B2
  • noun
  • - the lightest chemical element; a gas that forms most of the universe

helium

/ˈhiːliɛm/

B2
  • noun
  • - a chemical element; a light inert gas

energy

/ˈɛnərdʒi/

B1
  • noun
  • - the capacity to do work or cause change

gravity

/ˈɡrævɪti/

B2
  • noun
  • - the force of attraction that pulls objects toward each other

create

/kriˈeɪt/

B1
  • verb
  • - to bring something into existence

shine

/ʃaɪn/

A2
  • verb
  • - to emit light; to glow

use

/juːz/

A1
  • verb
  • - to employ for a purpose

expand

/ɪkˈspænd/

B2
  • verb
  • - to become larger or wider; to spread out

shrink

/ʃrɪŋk/

B2
  • verb
  • - to become smaller in size

planets

/ˈplænɪts/

B1
  • noun
  • - celestial bodies orbiting a star

Earth

/ɜːrθ/

A2
  • noun
  • - the third planet from the Sun; our world

lifetime

/ˈlaɪftaɪm/

B1
  • noun
  • - the duration of a life; the period during which something lives

red

/rɛd/

A1
  • adjective
  • - the color red

giant

/ˈdʒaɪənt/

A2
  • adjective
  • - very large in size

white

/waɪt/

A1
  • adjective
  • - the color white

dwarf

/dwɔːrf/

B1
  • noun
  • - a small person or creature; in astronomy, a type of star

NASA

/ˈnæsə/

B1
  • noun
  • - the U.S. National Aeronautics and Space Administration

scientist

/ˈsaɪənˌtɪst/

B1
  • noun
  • - a person who studies or works in science

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