Episode Transcript
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0:00
The. Hello a explorer. Or.
0:02
Well come along to the club. We
0:04
going on an adventure to try and
0:06
search out the secrets laying around the
0:08
solar system. It's a brand new fun
0:11
kid sign sweetly. My
0:15
name is Dan. Thank you so much
0:17
for being that this is the only
0:19
place where we discover all the signs
0:21
that no one else bothers about. We.
0:24
Learn what's really out there. This week
0:26
you can hear all about a brand
0:28
new gallery that saw a museum. It's
0:31
filled with loads of hands on stuff
0:33
to explain energy and how it's changing
0:35
in the future. Were
0:38
showing some of these technologies from
0:40
solar panels to big wind farm
0:42
generators and. The exciting thing
0:45
for for me I think is to get
0:47
up close and personal to some of these
0:49
technologies and see them for yourself and appreciate
0:51
that those. Can help us in in
0:53
our our future to be more responsible on
0:55
this planet. Oh
0:58
so I've got some of your questions to
1:00
answer and this week one will take us
1:03
into space to take a look at baby
1:05
stars. Fusion
1:07
of hydrogen into helium and that's
1:09
the point that it becomes a
1:12
star, So essentially a protest or
1:14
becomes a stop when it's gathered
1:16
enough mass and when that cool
1:18
gets to ten million degrees. And.
1:23
We will hear about one of
1:25
the rarest animals on the planet.
1:27
It's a creature that's not really
1:29
been spotted fifteen years. it's all
1:31
coming up it a brandy. Fun
1:34
kid science weekly. Let's.
1:41
Kick things off with your science
1:43
in the news. And we start
1:45
with some sad news: sewage spills
1:48
into England's rivers and sees by
1:50
water companies more than doubled last
1:52
year. According to the Environment Agency,
1:55
there were three point six million
1:57
hours it spills compared to one
1:59
point. Than five million hours
2:01
the year before. So.
2:03
All those millions of hours think
2:05
of how much water, how much sewage
2:08
is being pumped into our rivers are
2:10
sees also Uk The industry bodies the
2:12
series companies said it was unacceptable that
2:15
record levels were down to heavy
2:17
rain. so we that a lot of
2:19
rain and that's flooding places where sewage
2:21
is cats he called help but over
2:24
slow But you can understand why some
2:26
people are frustrated with the water companies
2:28
because all of this much is being
2:31
pumped into rivers, seas and other
2:33
places. That we consume Posada sweet
2:35
say Starship Kiss made a big
2:37
broke it it's third test flight.
2:39
The to stage vehicle had a
2:41
clean get away from it's launch
2:44
site over in Texas. It said
2:46
it's up a bit around the
2:48
globe which reinstated over the Indian
2:50
Ocean. No radio contact with last
2:52
towards the end with Spacex say
2:55
it was incredible to see how
2:57
far he got this time around.
2:59
Need an amazing isn't it? We've
3:01
been following us Space X, Ceylon,
3:03
Musk and Space Company. We've been
3:05
following their attempts to ask rockets
3:07
into the atmosphere and they they
3:10
do get better and better each
3:12
time. I wonder where they might
3:14
be in the years from now.
3:16
Final story this week: Upper New
3:18
Gallery the expose the past that
3:20
the prison and the Future Energy
3:22
has opened at the Science Easy
3:24
it is Who'd Energy revolution, the
3:27
A Danny Green Energy Gallery and
3:29
examines how the world can limit
3:31
climate change. This week a very.
3:33
Keen to talk about sluts on that
3:35
lot with a gallery to rates at
3:37
the switch on. As a cop in,
3:40
there are so many different ideas that
3:42
we can about. Climate. Change
3:44
Ways to save the world and Ways
3:46
to present climate change. When you were
3:49
coming up with a new gallery, how
3:51
did you stop? I guess it starts
3:53
from. We. All know that. Burning.
3:56
saying such as: coal
3:58
oil gas religious. Generating
4:01
electricity to power the things that
4:03
we need such as our lights
4:05
off, Tv up posters are also
4:08
things such as you know petrol
4:10
and diesel can be burned power
4:12
cause you know passes big. Sits.
4:15
Across the oceans are unfortunately.
4:18
A when Japan things this release is
4:20
queued greenhouse gases into the air which
4:22
come on the planet and can cause
4:24
more kind of extreme weather such as
4:26
but heavy rains or floods or in
4:29
some places less rain or or fires.
4:31
So if we kind of wanted to
4:33
avoid the worst effects of climate change
4:35
we really need to. Change
4:37
the way we do energy or energy
4:39
sources to ones that don't release these
4:42
greenhouse gases. And that's what's called the
4:44
low carbon energy transition. And this is
4:46
what the gallery, the size museum is
4:48
all about. That's what's it about. So
4:50
what's in it? and what can we
4:53
find if we wander around? Yeah, well,
4:55
we've got a whole range of potential
4:57
options for the seek to of energy,
4:59
and we're displaying many of these inventions
5:01
or technologies together in our gallery province.
5:04
Discovered experience for themselves. So for example,
5:06
we've got. Probably the oldest
5:08
electric car certainly in the country,
5:11
your listeners, My family's my own
5:13
electric car on the quite modern
5:15
technologies for this one's from. The.
5:18
Eighty Nineties is over hundred and twenty years
5:20
old so as to gonna say the some
5:22
of the technology for the. Delay.
5:24
For this energy transition we've had for
5:26
a long time and it's just about how
5:29
we use the more effectively in the future.
5:31
That's one really cool thing is a
5:33
bright yellow and black electric taxi. It was
5:35
nicknamed the Bumble Bees him and it drove
5:38
around the streets of London in a
5:40
eighteen nineties already like afford to pay put
5:42
com I have a a close look at
5:44
this electric taxi it do we know
5:46
anything about. Why it was made
5:48
in them? Why we didn't make more?
5:50
Yes so it was invented by a
5:52
man quarterback. It's called the Bears Electric
5:54
Taxi Cab and he was really competing
5:56
with the horse. It was a company
5:59
called the Great Horseless Carriage Anthony and
6:01
it really does look like a carriage
6:03
but not without a horse. and so
6:05
he. He was trying to kind of
6:07
clean up the streets of London and
6:09
away because they wouldn't be any horse
6:11
manure or horses wouldn't get tired. And
6:13
the batteries on this electric taxicab you
6:15
could just take out and replaced with
6:17
charged batteries and then go off and
6:19
take passengers around around the city and
6:21
know for as long as the the
6:23
batteries last it and this gallery elixir
6:25
the past, the prison and the future
6:27
of energy in your. Time.
6:29
What you learn about how our knowledge
6:32
of energy. How it's changed
6:34
through the is well really I
6:36
suppose our know this is changes
6:38
that getting a better appreciation of
6:41
the effects of or energy choices
6:43
and so you know. Now.
6:46
We know. Stop. Burning.
6:48
A lot of fossil fuels can be
6:50
damaging to the planet and. We've.
6:52
Got so many exciting technologies to
6:54
use to help us move away
6:56
from biting and were showing some
6:59
of these technologies from solar panels
7:01
to big wind farms, generators and.
7:04
Exciting thing for up to me I think
7:06
is to get up close and personal to
7:08
some of these technologies and see them for
7:11
yourself and appreciate that those can help us
7:13
and and all our future to be more
7:15
responsible on this planet. You say get Up
7:18
close. One of the things the Science Museum
7:20
always does really well. We get hands on
7:22
in a way that we are able to
7:24
do other museums and other galleries. What? What
7:27
can we do? What we can walk me
7:29
touch. What can we play with at the
7:31
Adelante Green Energy Gallery. One thing I think's
7:33
quite cool. Is that we all know about. Batteries.
7:36
and you know if this a battery on on your
7:39
your your game we all that type device and can
7:41
it can run out and you can lead to recharge
7:43
it. Bought. An we've got a
7:45
hands on experience of a gravity
7:47
battery. so no batteries use chemicals
7:49
to store energy. So if you've
7:51
gotten access in in energy and
7:54
say on a really windy day
7:56
when is so much wind and
7:58
that generates electricity from wind. You
8:00
could store that electricity by wincing up
8:03
a wait inside a very deep hole
8:05
such as an old mine shaft And
8:07
them. You. Can use that energy
8:09
later on when you need it by releasing
8:11
the weight. Gravity take the weight down and
8:13
then electricity is generated from a tab on
8:15
motor there. So we've got a hands on
8:17
exhibit where you can. Win. Shots you
8:20
gravity battery press a button and then that
8:22
releases the weight and studied up to the
8:24
ground and and generates electricity. And.
8:26
To that's the kind of hands on
8:28
one. We've also got a couple of
8:30
games where you can step inside the
8:32
shoes of an engineer working on different
8:34
problems such as balancing a national grid
8:36
to help keep it running with all
8:38
these renewable and sometimes variable energy sources
8:40
for placing solar energy in different parts
8:42
of the world where it's needed the
8:44
most. So there's plenty on offer to
8:46
get hands on as well as up
8:48
place to the historic or new objects
8:50
in the gallery. The So Energy revolution
8:52
the A Danny Green Energy Gallery is
8:54
is looking at the past. The Prison
8:56
and the future. And because you've been. Looking.
9:00
And researching that. if you had to
9:02
make this gallery getting like fifty years,
9:04
what might you put in it? What
9:06
are we doing now that might become
9:08
incredible and world saving a in a
9:10
few years' time. One of the kind
9:13
of technologies that really excited me and
9:15
you know if it sees. Could
9:17
be a real exciting prospect for the
9:19
future is fusion power and this is
9:21
the reaction that powers the sun and
9:24
all the stars in the universe and
9:26
if we could he have recreate those
9:28
reactions down on us and we might
9:30
have potential unlimited energy to power on
9:32
Aids and if is good enough for
9:34
the sun's shown is good enough for
9:37
us will listen to the new exhibition
9:39
is Energy Revolution the A Danny Green
9:41
Energy Gallery it's on at the Science
9:43
museum on of a top into. As.
9:45
Been involved into in it Together. Thank you so much
9:48
for joining us Oliver No problem Thanks very much having
9:50
me. I'm. james stewart and
9:52
inside the planet earth onto the be
9:54
joined by some of the world's top
9:56
scientists introduce you to some the weed
9:59
out the full ideas being trialled
10:01
to try and save our planet.
10:03
Led of course by your questions.
10:05
Hi James I know that climate change is
10:08
affecting our oceans. Is there anything that's being
10:10
done to look after it? Our
10:12
other solutions involve some simpoo.
10:15
This is Saving Planet First, available
10:17
wherever you get your podcasts. Let's
10:20
get to your questions then. We have
10:22
one which will take us across the
10:25
universe in just a second to look
10:27
at ittle-biddle baby stars. Now
10:29
if you have a question that you
10:31
really want answered, make sure you send
10:33
it to us best ways by leaving
10:35
it as a voice though on the
10:37
free Fun Kids app or you can
10:39
do it to funkidslive.com too. This one
10:41
has been sent in as a message
10:43
to me from Raffi. Thank you Raff.
10:45
Raffi asks why when you see someone
10:47
yawn do you want to yawn?
10:50
Do you know what's amazing about this?
10:52
It's something that we do all
10:55
the time. That everyone knows
10:58
what happens. You
11:00
don't have to be Albert Einstein to know
11:02
if you see someone yawn it's
11:05
quite contagious. You're likely yawn
11:07
yourself. Even with
11:09
all that experts don't exactly
11:11
know. They think it
11:13
might have evolved. So over
11:16
hundreds and thousands of years
11:19
we have evolved that ability
11:21
that we yawn when other people do. Maybe to keep
11:23
us on our toes or on our toes. If you're
11:25
aware if you need to be on guard and you
11:27
see someone yawning it might make you
11:30
yawn and help you realise that hang on
11:32
you maybe you're a bit tired. You should
11:34
be extra vigilant and aware because other people
11:36
feel tired. Maybe it snaps you into action.
11:38
That would have been really helpful in times
11:41
when we were cavemen right? If you saw
11:43
someone probably hairy with a huge
11:45
club in his hand. If you saw them yawning
11:47
you'd think oh hang on they're a bit tired.
11:49
Maybe I need to snap to attention. Maybe I
11:52
need to get to it. And
11:54
The reason that we yawn really isn't
11:56
to do with us being tired. It's
11:58
because we've not taken in enough. Oxygen
12:00
when we're breathing so you have one massive
12:02
breath and that saw your knees. Experts also
12:04
think it might be to do with social
12:06
mirroring. When you see someone do something your
12:08
brain thinks it might be a good thing.
12:10
Today the other had that when you see
12:12
some on scratch their face and some legal
12:15
was gets of the a cheat it's your
12:17
brain that constantly almost makes you want us
12:19
to in it's always looking for different cues
12:21
and ways that you can improve and figure
12:23
out what to do so well See that's
12:25
why. We. Think that we your own
12:27
and why we think that we your and
12:29
when we see other people your and but
12:32
we don't exact month. Anti much that
12:34
costs and let's get on another one. This is
12:36
a voice nice and into the freeze on kids
12:38
out the by Danny. Island. Danny
12:44
thank you for your question. All
12:47
about prose host star turning into
12:49
a proper star I guess about
12:51
go some help him whenever we
12:53
and travel across the galaxy. says.
12:55
One person I turned to first because
12:57
they know everything Dora Patel from the
13:00
National space and to joins us Dora
13:02
Thank you for being that cillizza of
13:04
what what is a proton star. Yes
13:07
it really depressed and set the prices.
13:09
Thought is basically. Just a very
13:11
very young star was haven't started
13:13
what we call nuclear fusion said
13:16
his post have club my style
13:18
skin off my own what's insult
13:20
sexist, really young and it still
13:22
growing interesting material or less. Than.
13:25
A really young in style turns of
13:27
you know it's not a we go
13:29
to see how how old are these
13:32
really young stars? Yeah, Honestly speaking when
13:34
we talk about. Time. It's Martha kind
13:36
of the time we used to say when
13:38
we're talking about a better to be swiftly.
13:41
Talking just a few hundred thousand
13:43
years and the bare minimum levy
13:45
star start to go and it
13:47
may take you know a few
13:49
million years for them to become
13:52
a fully self star. So with
13:54
humans. We. Have very clear
13:56
boundaries on. A Huge He's
13:58
right when you're upset of. year old,
14:00
then you're a baby, then you become
14:02
a toddler, then you become a kid,
14:04
then you become a teenager, then you're
14:07
an adult, right? Is it similar with
14:09
stars? Do we have defined names for
14:11
ages? Yeah, in a sense we do
14:13
but they're not necessarily a particular
14:15
and defined age. So it's more a
14:17
broad range of sort of ages. So
14:20
a proto star is anywhere from I guess
14:23
a few like we said, hundreds of
14:25
thousands of years and they're collecting material
14:27
up to a few tens of millions
14:29
of years, perhaps when they become a
14:31
nuclear fusing star or what we call
14:33
a proper star, but then
14:35
stars can live for many more millions
14:37
of years. Stars like
14:40
our son will live for billions of
14:42
years and there are even very small
14:44
stars which actually use their fuel very
14:46
slowly that can live for trillions of
14:48
years. So when we think
14:50
about stars and their ages, it doesn't really
14:52
give us an idea of their true age but
14:54
thinking about our son, it's about four and a
14:56
half billion years old and we consider it to
14:58
be like a middle-aged adult. It's about halfway through
15:01
its life. So we know what a
15:03
proto star is, the question,
15:05
how does it turn into a star? So
15:08
what has to happen for it to decide
15:10
to make nuclear fusion?
15:12
Yeah, so stars are
15:14
basically born from what we call
15:16
molecular clouds or a pretty aware
15:18
nebula, so these big clouds of
15:20
gas and dust in space and
15:23
essentially something happens that causes this material
15:25
to be pulled together by gravity. So
15:27
that might be a shockwave
15:29
from a relatively nearby star that's
15:32
exploded or it might be
15:34
from something like two galaxies that are
15:36
colliding and then therefore the clouds within
15:38
them start to get closer together and
15:40
knock into each other. So when this
15:42
material comes together, gravity pulls it together
15:45
to form what we call a dense
15:47
core and then
15:49
eventually it's kind of a balancing act
15:51
between gravity pulling this material in and
15:54
then a bit like when you've got a
15:56
balloon and you fill it with air you
15:58
get pressure from the gas in inside the
16:00
balloon pushing back outwards and expanding the
16:02
balloon. So it's not just balancing it
16:05
between the star. Lots of material being
16:07
pulled in and that star trying to
16:09
hold itself up. But eventually gravity wins
16:11
and it pulls enough material together to
16:14
the point where that core gets to
16:16
10 million degrees Kelvin,
16:18
which is roughly 10 million degrees
16:21
Celsius. And that's the point
16:23
where it can undergo fusion of
16:25
hydrogen into helium and that's the
16:27
point that it becomes a star.
16:29
So essentially a protostar becomes a
16:31
star when it's gathered in
16:33
enough mass and when that core gets to
16:36
10 million degrees. We know
16:38
what stars look like.
16:40
These brilliant bright balls of
16:42
energy fusion happening all the
16:44
time. What do we know
16:46
about how protostars look? Yeah,
16:48
so protostars when they're very small
16:50
and they're just starting to pull that
16:52
material together, they're not going to be
16:54
very well visible. So we're not going
16:56
to be able to see them very
16:58
easily. And in fact, they're hiding within
17:00
these huge clouds of gas and dust,
17:02
which makes them tricky to spot anyway.
17:04
But as they gather more material, although
17:06
they're not giving it late by nuclear
17:08
fusion, they are getting warmer.
17:10
So just like when you pump air
17:13
into a bike tire, we know that
17:15
the tire gets hot, right? The air
17:17
in there is being squashed together and
17:19
therefore it gets a bit hotter. Similarly,
17:21
these protostars, once they start to gather
17:23
enough material, they will get hotter and
17:25
they will emit light in the form
17:27
of infrared. So some of you might have
17:30
heard of infrared light. We
17:32
have infrared cameras to see hot bodies
17:34
in the dark. And similarly, we
17:36
can use infrared telescopes to spot
17:39
these protostars in this huge cloudy
17:41
regions in space where they're starting
17:43
to form. How well have we
17:45
done with spotting them? We are
17:47
quite close to a star with
17:49
our sun. We know where other
17:51
ones are around us. What about
17:53
protostars? Do we have any idea of
17:56
where they are in the universe and how many we
17:58
might have? Yeah, so there are tele- all
18:00
over the world that are actually looking for protostars,
18:03
and we're starting to find more
18:05
and more evidence of protostars in
18:07
the earlier stages of their life.
18:10
So with things like the James Webb
18:12
Space Telescope that works with infrared light,
18:14
we're able to see these protostars forming
18:17
earlier than we've been able to see
18:19
them before. But of course,
18:21
we're still not yet at the stage
18:23
where we completely understand, perhaps, exactly
18:26
how protostars come to be and exactly
18:28
what they're like at the beginning of their lives. But
18:31
we're starting to put together a much better
18:33
picture in it. In fact, lots of stars
18:35
are actually born together from the same cloud
18:37
of gas and dust. And
18:39
so one of the big questions is, well,
18:42
if our sun were born in a similar
18:44
way, where are all the other stars that
18:46
our sun would have been born with? Like
18:48
star twins, star triplets, star quadruplets. Do we
18:51
know very quickly if they have any connection,
18:53
if the sun does have a twin that's
18:55
been born from the same kind of nebula?
18:58
Is there any link? Do we know? Yeah,
19:00
so this is one of the bigger questions
19:02
where we've not yet understood whether our sun
19:04
is a little bit of a deviant or
19:07
a little bit of an oddity that it
19:09
didn't quite form. Likely, you see many of these
19:11
other protostars forming. But if it did form in
19:13
a group, one of the questions is, okay, so
19:15
what happened to those stars? So it's still a
19:17
bit of a mystery. It's still a bit of
19:19
an unknown. And that is why,
19:21
when we got any question across the
19:24
galaxy, we head straight to the National
19:26
Space Centre. Dara Patel, thank you so
19:28
much for helping us with Danny's question. No worries. Let's
19:35
get to this week's Dangerous Dan.
19:37
We're going into the mountains around Vietnam
19:39
to try and find the Saola. And
19:43
I really mean try and find it.
19:45
It's one of the rarest animals on
19:47
the planet. It was first discovered back
19:49
in 1992, so 30 years
19:52
ago, when forest scientists were
19:54
searching mountains for anything unusual.
19:57
That was 1992. The last time one was photographed... was
20:01
in 2013. It's
20:03
in the bovine family, the Saula, so
20:05
it's closely related to catals and goats
20:07
and antelopes. Here's the thing, it's known
20:10
as the Asian unicorn because
20:12
it's from Asia and a few other reasons. It's
20:14
rare just like a
20:16
unicorn, perhaps people think it's mystical, but
20:19
also it's got two huge horns
20:23
just like a unicorn. This
20:25
creature has two long slender horns
20:27
that can stretch back, they arch from
20:29
the top of its head to over
20:31
a meter tall. It's got a dark
20:33
brown coat with white markings on its
20:35
face and legs which make it incredibly
20:37
tough to spot in the wild. It
20:39
blends in with the snow or with
20:41
the rocks around the mountains where it
20:43
lives and because of this we don't
20:45
know how many there are really. It's
20:48
a pretty endangered species but there could
20:50
be loads, I don't know. Probably isn't
20:52
as experts from Vietnam would see it
20:54
more and more and would know more
20:56
about it you might think, but
20:58
who knows maybe they're there and just really
21:00
good at hiding. It's got hooves and thick
21:02
teeth and here's something
21:04
strange. In
21:06
the past when people have found them
21:09
they have captured them, taken them to
21:11
try and study them, but
21:13
sadly the animals don't last very long
21:15
in captivity. They die quite quickly, it's
21:18
sad, it's strange, no one really knows
21:20
why and it's one of
21:22
the rarest animals on the planet which is why
21:25
the Saola goes on to our dangerous down list.
21:31
Let's head back into space then shall
21:34
we and catch up with one
21:36
of our favorite geniuses Professor Pulsar
21:38
with Dara Patel. Earlier on we
21:41
heard all about protostars. What about
21:43
other types of stars? Well
21:45
Professor Pulsar is an expert on space and
21:48
he joins us to tell us
21:50
some of the other things that
21:52
move through the universe like shooting
21:54
stars and why some of them
21:56
twinkle. that
22:00
is, support from the UK Space Agency.
22:04
Somewhere between Polaris and Ursa Minor,
22:06
just a glint in the night
22:08
sky to the naked eye, it
22:10
looked a little closer, and you
22:12
will see it as Professor Pulsar's
22:14
exploration craft, the intrepid vibe
22:17
piloted by a trusted Captain
22:19
T. Torrey. While the pupils
22:21
of Deep Space High take their school
22:23
holidays, Pulsar is roaming
22:25
the universe to explore the most
22:28
dastardly difficult mysteries and
22:30
broadcasting his findings back to the planet.
22:33
It can only be another
22:35
episode of Professor Pulsar's case
22:37
explanation. Professor, I'm
22:40
picking up some incoming data on the
22:42
Medrange scanners. Stand by. It sounds like
22:44
another question. Hey. Oh,
22:48
she can call us what a good-less
22:50
me. I'm used to tricky questions, but
22:52
I can't understand what that even means.
22:54
Computer, replay that question. Accessing database, replay
22:57
last question. Hey. Professor,
23:01
I think that question may have got scrambled
23:03
up on its way from Earth. Computer, run
23:05
the descrambling program on it. Great
23:11
work, Captain T. Torrey. Right, let's get on
23:13
the case of solving this little mystery. Computer,
23:15
can you find me an expert, please? Searching?
23:18
This looks promising. Stevenage, England on
23:20
planet Earth, patching through to flight
23:22
decks. This is Captain T.
23:24
Torrey of the Intrepid Five. Please identify
23:27
yourself. My name's Sharn, and I'm an
23:29
engineer at Airbus Defence and Space. Loading
23:31
file. As the world's second
23:33
largest aerospace company, Airbus Defence
23:35
and Space has expertise in a range
23:37
of disciplines, from aircraft to defence to
23:40
space. One of the projects it is working
23:42
on at the moment is the Solar Orbiter,
23:44
a satellite mission launching in 2017, which will
23:46
travel to the sun to
23:49
closely study areas which are difficult to view
23:51
from Earth. It is hoped it will help
23:53
us learn more about the complex workings of
23:55
the sun. Thanks, Computer. So, Sharn, we
23:57
have a bit of a cosmic conundrum. that
24:00
you might be able to help with,
24:02
can you explain what causes shooting stars?
24:04
Well in space there's lots of particles
24:06
and bits of rock floating around and
24:08
every now and then one of these usually quite
24:10
tiny pieces of rock enters the top
24:13
of the Earth's atmosphere and because
24:15
it's travelling so quickly it appears to burn
24:17
up in the upper atmosphere and that's what
24:19
we see as a shooting star. So it's
24:21
not actually a star, it's just a piece
24:24
of debris or rock that's coming into our
24:26
atmosphere. Most shooting stars come from pieces of
24:28
rock that are from the size of a
24:30
grain of sand so really really tiny up
24:33
to probably about a metre in diameter. So
24:35
they're not actually that big so it's quite
24:37
impressive that we can see them all the
24:39
way from the ground and they can streak
24:42
right across the sky. Thanks Sean, you're
24:44
a star. Professor, I have another star
24:46
related question flagged on the database. Perhaps
24:48
there's another expert at Airbus who can
24:51
help. That's
24:53
identified. Connecting. Well done T-Tory,
24:55
who are we speaking to? Hi I'm Kyle
24:57
Palmer, I've just finished university and I'm now
24:59
working at Airbus Defence in Space in future
25:01
missions which means I design all the future
25:03
missions that won't be launching till after 2020.
25:06
Good, good. Computer, please load up our
25:08
question for Kyle. Why
25:12
do some stars twinkle and
25:15
others do? So stars themselves are
25:17
basically suns like our own and are just
25:19
as bright if not a lot, lot brighter
25:22
but they're very very far away which means
25:24
that it takes a while for the star light to
25:26
reach us and when it does it then has to
25:29
pass through our very thick atmosphere so
25:31
that we can actually see them and when we see them they
25:33
appear to twinkle because of all the light rays
25:35
are hitting off all the stuff in the atmosphere
25:38
and they look really faint and they twinkle. The
25:40
stars which appear to not twinkle are
25:43
actually satellites and the International Space Station and
25:45
planets in our own solar system which are
25:47
a lot closer to us and therefore they're
25:49
a lot brighter in the sky and that
25:52
means that we don't quite see the twinkle
25:54
in quite as much. Well, a shining example
25:56
of a space mystery soul. And
26:13
I see for this week's episode of
26:16
The Fun Kids Science Weekly, thank you
26:18
so much for catching up with us.
26:20
If you have anything science-y that you
26:22
want answered next week on the podcast,
26:24
make sure you leave it as a
26:26
voice note for me on the FreeFunKids
26:28
app or at funkidslive.com. You heard Professor
26:30
Polsar a second ago. We've got loads
26:32
more brilliant podcasts and episodes for you
26:34
to listen to on Google, Apple, Spotify,
26:36
wherever you get your shows, and they're
26:38
at funkidslive.com too. And Fun Kids are
26:40
our children's radio station from the UK,
26:42
listen all over the country on the
26:44
app, on our website, and if you've got a smart
26:46
speaker, wake it up and ask it to play Fun
26:48
Kids. I'm
26:54
James Stewart and in Saving Planet Earth,
26:56
I'm going to be joined by some
26:58
of the world's top scientists to introduce
27:00
you to some of the weird and
27:03
wonderful ideas being trialled to try and
27:05
save our planet. Led, of course, by
27:07
your questions. Hi, James. I
27:09
know that climate change is affecting our oceans.
27:11
Is there anything that's being done to look
27:13
after it? And one of the
27:15
solutions involves some sim poo. This
27:18
is Saving Planet Earth, available wherever
27:21
you get your podcasts.
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