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Hello! And welcome you have downloaded
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the podcast version of Inside Science
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first broadcast on the twenty First
0:55
of March. Twenty Twenty Four. This.
0:58
Week our focus is the widest
1:00
aperture out there are solar system
1:02
and beyond. Because I'm pleased to
1:04
say we're joined by Chris Lintott
1:06
professor of Astrophysics at the University
1:08
of Oxford, Gresham Professor of Astronomy
1:10
probably best known to many of
1:12
our listeners as a presenter of
1:14
the Sky at Night or two
1:16
radio purists you don't dabble in
1:18
Tv is that bloke off the
1:20
monkey cage astronomy specials. You can
1:22
answer any question about space at
1:24
Welcome to Inside. So as Chris.
1:26
Thinks it's it's good to be not argued start
1:28
know it's been around long enough. It's it's an
1:30
honorary radio program. Or yeah, yeah, you know what?
1:32
Yes for you've got the budgets of a radio
1:34
program. Right? And something I bought. Your
1:37
with me for the next half hour
1:39
for a good rummage through both the
1:41
history and the very latest discoveries in
1:43
a space themed show. Shall I tell
1:45
you what we got coming out? Yeah,
1:47
sure! We zooming in on Saturn's moon,
1:49
Titan to solve the mystery of what
1:51
created the massive genes that cover almost
1:53
a fifth of it surface to. Dial
1:55
or Love Titan. It's my favorite place.
1:58
rk and our moon,
2:00
talky of moons, commodity or communally
2:03
owned companion. We raise an eyebrow
2:05
at efforts to mine it. A
2:07
bit of space politics maybe. Yep, yep.
2:10
And we'll also be looking at twin
2:12
stars. They're born in the same cosmic
2:14
nursery and they ought to be identical.
2:16
We'll be hearing why some pairs aren't.
2:18
This just came out this morning. I was reading
2:20
this on the train, so it's good that that's
2:23
come up. Great, it's hot off the press. So
2:26
these topics are all within the scope
2:28
of your latest book and you've chosen
2:30
to write about the happy accidents that
2:32
help us discover so much about space
2:34
and what we know about it. It's
2:36
called Our Accidental Universe.
2:39
What grabbed you about the stories?
2:41
I think the thing that unites them and
2:43
it is really a set of stories of
2:45
discovery is that they're all fun. And
2:47
I think one of the things I really wanted to write
2:50
about was that discovering things in
2:52
the universe is a lot more fun than
2:54
I think we often talk about. We're often
2:56
quite serious when we talk about this. There's
2:58
the moment of revelation where we suddenly understood
3:00
the deep mysteries of the universe. Or there's
3:02
a film shot of people sitting
3:04
around a table worrying about an asteroid. And
3:06
actually a lot of astronomy is arguing with
3:08
friends, being confused, not knowing what the thing
3:10
that's appeared in the image that you've got
3:12
from the Hubble Space Telescope is. And so
3:14
I wanted to tell those stories. And as
3:16
I dug deeper, you discover that all
3:18
over the place that the best
3:20
discoveries, the most important discoveries, come from
3:22
the most interesting people having fun. And
3:24
so really that was the thing that
3:26
unites the book that talks about the
3:29
distant universe, nearby asteroids, things traveling through
3:31
the solar system. And as you said
3:33
Saturn, it's just this sense of
3:35
being surprised by the universe as a way of
3:38
understanding the cosmos. I
3:40
wanted to talk to you about what
3:44
we think about when we think about
3:46
a telescope, because so
3:49
much of what I think about
3:51
as the tool that helps us discover
3:53
stuff in space is essentially a tube
3:55
and you look down one end of
3:58
it. But there's also... a
4:00
lot that you can tell by listening to
4:02
space. Oh,
4:09
that's very high-tech listening to space. That's
4:11
actually a sound I recognise from a
4:13
space probe called Cassini that flew around
4:16
the Saturn system. And just
4:18
before it plunged to its doom, it
4:20
was studying plasma waves, so waves in Saturn's
4:23
atmosphere, caused by interactions with a small moon
4:25
called Enceladus that maybe we'll get to in
4:27
effect. And what you're hearing there is sort
4:29
of an audio representation of those waves. But
4:31
you're right, we get data in all sorts
4:34
of ways. So we can still look through
4:36
telescopes, though these days we tend to use
4:38
cameras because they can add
4:40
up light. They can take images over many
4:42
hours instead of your eyeball, which is processing
4:45
all the time. We can also use radio
4:47
telescopes. We can detect x-rays. And actually now
4:49
in astronomy, we can detect ripples in space
4:51
and particles. So we use all of this
4:53
information to try and understand what's
4:56
going on in this quite confusing cosmos we
4:58
find ourselves in. Your book
5:00
is full of characters. And one of
5:02
the ones I think your favourite is
5:04
a guy called Reba, who was for
5:07
a while the only radio astronomer. Can
5:09
you tell me a bit more about
5:11
him? Yeah, he was a radio engineer working in Chicago
5:13
in the 30s and early 1940s. And he'd heard some
5:19
star noise on the radio from a
5:22
previous astronomer called Karl Jansky,
5:24
who was also a distracted radio engineer who'd
5:26
worked out that you his antennae were picking
5:29
up signals from space or or founds from
5:31
space, I suppose. And Reba wanted to investigate
5:33
these, wrote to Jansky and said, Can I
5:35
have a job with you? And Jansky essentially
5:38
said, No, my bosses would rather I studied
5:40
interference and things on Earth. He
5:42
wrote to all the astronomers in the country
5:44
at the time in the US and was told that
5:46
this was not proper science and that astronomers use telescopes,
5:49
as you said, and looked through them and mapped the
5:51
sky. And so he built
5:53
the world's first radio telescope in his back
5:55
garden in Wheaton, which is in about 50
5:57
miles outside Chicago, he'd get to work. during
6:00
the day, he'd come back, he'd remove the
6:02
washing that his mother tended to hang on
6:04
the radio telescope, and then overnight he would
6:06
map the Milky Way. And he
6:08
was the person who discovered our galaxy. The Milky
6:11
Way is a spiral galaxy. He found radio emission
6:13
coming from its centre, which we now know is
6:15
associated with a black hole. And
6:17
essentially no one took him seriously. He tried
6:19
to publish these results and he was basically
6:21
pursued by the establishment, despite
6:24
the fact he'd invented this means of
6:26
doing radio astronomy. And radio
6:28
astronomy you can do during the day
6:30
because it doesn't need the darkness. You
6:32
can. He had, as well as
6:34
having a day job, which was problematic,
6:36
he also realised that cars
6:38
of the time, their starter motors, emitted radio
6:41
waves. And so he needed to wait for
6:43
everyone else to stop driving around. And he
6:45
eventually got a job after the war, as
6:47
radio astronomy took off in this
6:49
country with Jodrell Bank and elsewhere. He did
6:51
get a job thinking about new radio telescopes,
6:53
but decided he'd rather be his own man,
6:56
move to Hawaii and then Tasmania, and essentially
6:58
spent the rest of his life building his
7:00
own telescopes. At one point he
7:02
did try to get hold of an ICBM,
7:05
a missile, to fly above the telescope and
7:07
alter the Earth's atmosphere, but
7:09
was refused permission, probably for the best. I
7:12
think he's a really interesting example of
7:14
what happens when you're trying to go
7:16
against the establishment. So to kind of
7:18
move things forward in a way that
7:21
creates a new picture or something incredibly
7:23
new. There's a lot of pushback. That's
7:25
right. And he also invented his own theory. So
7:27
he also was very rude about astronomers like me
7:29
who believe in such theories, such as the Big
7:31
Bang. And so he spent a lot of his
7:34
time trying to prove his own cosmological theories, but it
7:36
doesn't take away from his invention
7:38
of radio astronomy as a science. And lots
7:41
of what we do now, he would have
7:43
recognised using telescopes to map the sky. And
7:46
so radio astronomy is in the book as a big
7:49
example of a surprise. None of the
7:51
astronomers of the time at places like
7:53
Yerkes, the big national well-funded observatories,
7:55
were wondering about how to use radio to
7:57
look at the cosmos. It all came from...
7:59
people trying to understand how to use
8:02
radio to communicate. I just want
8:04
to read in your book, I
8:07
mean, you've mentioned Reba made up
8:09
his own series. He didn't believe in the Big
8:11
Bang. And he
8:14
thought of astronomers like you who
8:16
followed the cosmological status quo as
8:19
doing so not out of malice
8:21
or corruption, but simply due to
8:23
narrow-minded incompetence. See, I think that's quite generous. I've
8:25
definitely been called a lot worse, but I like that. And
8:28
it gives you a bit of a flavor of the man,
8:30
I think. He also discovered
8:32
Tasmanian parrots are right clawed and built his
8:34
own electric car in the 70s. So he's
8:36
clearly a forward thinker. Now,
8:39
when space missions are
8:42
decided to try and
8:44
explore the solar system, one
8:47
of the pools when deciding a destination is
8:50
the tantalizing prospect of finding life
8:52
off this planet. And the
8:54
European Space Agency currently has a mission
8:56
called JUICE. And that's to
8:58
Europa, right? Yeah, one of the moons
9:01
of Jupiter, one of the big moons of
9:03
Jupiter, with an ocean underneath a water ice
9:06
surface. This is going to
9:08
orbit Europa and give us more
9:10
data about whether there's possible life
9:12
there. Yeah, it will fly by. And really,
9:14
it's looking for habitats for life. So we
9:16
know, we think, that like many of the
9:18
moons in the outer solar system, Europa has
9:20
an ocean within it. But we don't know
9:22
how deep the ocean is. So therefore, we
9:24
don't know how big it is. We don't
9:26
know how long-lived it is. And those are
9:28
the questions that JUICE, and then there's an
9:31
American mission launching later this year called Europa
9:33
Clipper that will go into orbit around Europa.
9:35
Those two missions will sort of map the
9:37
geography. Of course, the place in the solar
9:39
system where we've got a bit further already
9:41
is Saturn's moon Enceladus, which is
9:43
a tiny thing. It's about the size of the British Isles. And
9:46
because it's being squeezed by Saturn's gravity
9:48
as it orbits, then it's got a
9:50
liquid ocean in the center. And
9:53
we know that it's a salty ocean. And
9:55
salt means that there must be an ocean floor. So
9:58
that's the place where I think we've got the... Best
10:00
habitat for nice and. The.
10:03
Ocean of In Salad Us was discovered
10:05
by accident by the Cassini probe which
10:07
was supposed to be looking at Saturn
10:09
and it's magnificent. rings and maybe some
10:11
of the large amounts flew past and
10:13
Xeloda, Son and one of the team
10:15
led by Michelle doctor year Imperial College
10:17
down the road discovered that there was
10:19
some disturbance in the magnetic field. dissuaded
10:21
the team to get back. Took pictures
10:23
are discovered there are fountains of water
10:25
shooting into space from the South Pole.
10:27
It's a it's an absolutely amazing discoveries
10:29
made completely by accident. Or they just
10:32
pointed the camera accident in my place.
10:34
Will that when they went back I knew
10:36
something odd was happening around the moon. So
10:38
they look to the moon and they followed
10:40
over the South Pole. I I think sometimes
10:42
maps if that first fly by had been
10:44
over the North Pole. weather isn't Morticia Dame
10:46
Spice Cassini may never have gone back to
10:48
insult us. say we might not know that
10:50
as this place where who knows their a
10:52
squid or bacteria or at least the potential
10:54
for life swimming around dumber and. Not just
10:56
more sense as he will. Test. Fizzy water
10:58
yet say I said it was salty
11:00
but guess is also and it's sort
11:02
of about the fish. You get off
11:04
a decent bottle of champagne to see
11:06
Fisa rather wonderful analogy that one of
11:08
the scientists gave me say say and
11:10
that means that there's chemistry happening down
11:12
there so it's beginning to look like
11:14
the kind of dynamic place where we
11:16
think on earth my my of got
11:18
started in the deep ocean around and
11:20
and volcanic vents or something like that
11:22
sites and some of this as I
11:24
think the most intriguing place and it
11:26
has the advantage. That you can
11:28
get back there if we send a probe
11:31
back and you can sample the water by
11:33
flying for it. So one day soon I
11:35
hope we'll send a chemistry set essentially to
11:37
go in and collect. Some of the city
11:39
will turn and might. My personal idea is
11:41
that we should fund this mission by bring
11:43
it back and Selling is the most expensive
11:45
mineral water ever obtained. I think people would
11:47
buy that. I think they would you
11:50
say subsidize their the science with sent
11:52
by selling the that's. Right? Yeah yeah you're
11:54
doing you're You're very rare and sell it and
11:56
mortar with Amy and by it's are included to
11:58
school to have health and. I'm sure
12:00
if. You were ideas as a flogging
12:03
men who reported to believe and
12:05
as I'm. Typing. Quite
12:07
nicely with one of today's stories,
12:09
Because taking resources from heavenly bodies
12:11
and bringing them back to earth
12:14
could be big business in the
12:16
future, and an isotope with helium
12:18
Helium three is one such commodity.
12:20
Seattle based Startup Interludes has recently
12:22
announced that it intends to harvest
12:25
this gas from our own main.
12:27
Now I called Sarah Russell, cosmic
12:29
Mineralogist at the Natural History Museum
12:31
in London to find out what
12:34
Helium Three even is. So.
12:36
Helium three is one neutron
12:38
with to protons so it's
12:40
the baby siblings of helium
12:42
for which is as you
12:44
protons and to neutrons and
12:47
which is much more abundant
12:49
so Helium three isn't that
12:51
much rarer isotope of the
12:53
to. A guy and
12:55
helium for is the one we
12:57
know with helium that guys in
12:59
party blades exactly most of those
13:01
stuff and possibly insists his helium
13:03
for so. Helium three is
13:05
it is it to. We use it
13:07
for anything. It doesn't even exist on
13:09
us. It doesn't exist on earth but
13:11
it's very very ras. I must say
13:13
Helium three on earth is the helium
13:16
three that the Earth was born with
13:18
which is not very much at all
13:20
plus a little bit that was formed
13:22
during things like ten nuclear testing said
13:24
the some human and pull into their
13:26
as well. but it does have some
13:28
uses say some cool it down to
13:30
very very low temperatures plus the absolute
13:32
zero up. For that reason it's used
13:34
in quantum. Computers to a cool
13:36
the components of them. it's also
13:38
used and medical imaging fit presumably
13:41
only in small amounts and quite
13:43
expensive, exactly. is incredibly expensive and
13:45
only use and very small amounts.
13:47
So there's little on us that
13:49
there's more of it on the
13:52
moon. Cell count. Yes, yes. So
13:54
in some ways the earth and
13:56
the moon are very similar to
13:58
a chemically to each other, but
14:00
there are some. really. the difference
14:02
is one of them is that
14:05
the earth has got an atmosphere
14:07
on has a magnetic fields and
14:09
that shields it from all sorts
14:11
of cosmic rays. the Saw in
14:13
space and in particular the earth.
14:16
Solar Winds produces this stream of
14:18
items into space and these hit
14:20
the surface of the moon ah
14:22
on implants into the rock. So
14:24
the Solar Winds includes hydrogen and
14:26
helium, including helium three as well.
14:29
Okay, so this. Company that's announce
14:31
that they're putting sixteen million towards
14:33
getting helium three off. The mean:
14:35
how would they go about extracting
14:37
it? So they've made their own
14:39
special instruments that's like going to
14:42
put on the moon to try
14:44
to strip the helium out so
14:46
that the big problem with Helium
14:48
three on the moon is that
14:50
although the sun is kind of
14:52
spray painting the entire surface of
14:55
the moon with helium three, it
14:57
says so in a super super
14:59
thin layer. That a mates
15:01
and sake or less. So it's an
15:03
incredibly thin layer across the surface of
15:06
the moon. And so us.
15:08
The extra thing that from the rock
15:10
is going to be really really difficult
15:12
to have the process. It's huge amounts
15:14
of broke and in the end zone
15:16
he gets tiny amounts of helium three
15:18
outfits and return it to us and
15:20
then return. It's worth yes, Says a
15:22
lot of difficult steps in this whole
15:24
process. that feels like an awful lot
15:26
of effort. Sara Yes, Wouldn't it be
15:28
easier just to make kids on Earth?
15:31
Can you make it on us? Well,
15:33
it has been made on earth by
15:35
humans during and nuclear weapons tests. but.
15:37
I guess I also make the whole live other stuff
15:39
as well. That you might not or
15:41
once assuming. Ah, that's
15:43
they do manage to
15:45
successfully and via Bleed
15:47
Mine. Helium. Three from the
15:49
moon. And bring. It back. How
15:52
significant could that be? So. Industry
15:55
What could change it would be.
15:57
a real sort of milestones because
16:00
it would be the first time
16:03
that we have exploited material from
16:05
space commercially. So it throws up
16:07
an awful lot of legal and
16:10
ethical issues but it
16:12
would be a massive massive deal and
16:14
yeah so the companies think
16:16
that if they manage to get the helium-3
16:18
back to earth it might potentially
16:21
open up new ways of
16:23
using helium-3 so it might inspire
16:25
new industries to form that can
16:27
use this new resource. Like what?
16:30
Well the sort of great dream
16:32
of helium-3 has always been to
16:34
use it for nuclear fusion so
16:37
this is something that's been talked about
16:39
for decades and decades but so far
16:42
we haven't been able to make
16:45
nuclear fusion work and even if we did
16:47
then I'm not sure that helium-3 would be
16:49
the best type of fuel for it so
16:51
that dream is still quite a long
16:53
way away. Lovely point there from
16:55
Sarah Russell. This is Inside Science and
16:57
I'm Marnie Chesterton. Today I'm joined in
16:59
studio by Astro Physicist and presenter Professor
17:01
Chris Lintott. Chris, it feels daft to
17:04
even point out what a source of
17:06
wonder the moon has been to us
17:08
all. Where does that leave mining
17:10
the moon? Well I think you
17:12
heard it there as Sarah was finishing that
17:14
interview which is that it's
17:17
very strange to talk about using moon for
17:19
commercial purposes. I think those of us who
17:21
want to see more space exploration have been
17:23
used to cheerleading this stuff because it's a
17:25
reason to get companies to pay to go back
17:27
to the moon you know we'll go we'll all
17:29
go helium-3 mining that would be great even if
17:32
the economics works out this is strip mining the
17:34
moon and the moon should the
17:36
UN say belong to all of us
17:38
it's in space so I think we've
17:40
got some serious problems to work out
17:42
about who gets to exploit what. It's
17:45
this weird catch-ready too. Friends of mine are talking
17:47
about putting a radio telescope on the far side
17:49
of the moon shielded from all the noise of
17:52
Earth but the technology that's making it cheap enough
17:54
that we might be able to do that is
17:56
also causing noise around the moon so we're struggling
17:58
we may only have a of years
18:00
to use the far side of the
18:02
Moon before it becomes as commercial as
18:04
the rest of low Earth orbit and
18:07
near Earth space. So I think we
18:09
need to think hard about why we're
18:11
using celestial bodies and who
18:14
gets to make those decisions. I'm
18:17
also not sure about some of the stuff we've
18:19
already littered the Moon with. So
18:22
you know 96 bags of poo and
18:24
an old camera. That's true, some interesting
18:26
art as well, some tardigrades crashed. There's
18:28
all sorts of things there but those
18:31
are small scale. This would be large
18:33
scale. Thanks Chris. We started off
18:35
talking about one of Saturn's moons and
18:37
now let's move to its largest, Titan,
18:39
which is bigger than Mercury. But that's
18:41
not the only thing that makes it
18:43
special. It's the only
18:45
known Moon with an atmosphere which
18:48
means it has wind and rain,
18:50
lakes and oceans. It also has
18:52
these mysterious giant dunes, about 100
18:54
meters high. So that's on a
18:56
par with the tallest ones here
18:58
on Earth which I believe are
19:00
in the United Arab Emirates where
19:03
the film Dune was recently shot.
19:05
But how did the ones on Titan get there?
19:08
That's always been a bit of a mystery. Over
19:11
at Southwest Research Institute in Boulder,
19:13
Colorado, planetary scientist Bill Bopka has
19:15
a new theory and I asked
19:17
him first to describe these dunes.
19:20
Think about your coffee you have in the
19:22
morning and now imagine sort of giant
19:24
mountains of coffee grounds that exist on Titan.
19:27
And some of these might be the order
19:29
of like 100 meters high. They're very large
19:32
and they cover about 17% of
19:34
the entire surface of Titan. So it's
19:37
a lot of stuff spread over this
19:39
really large area on this Moon. Okay
19:42
so I've got a mental picture
19:44
of Middle Eastern desert but
19:46
I'm just trying to make all the dunes a bit
19:48
darker so the colour of coffee grounds. Do you know
19:50
what they're made of? Are they sand? Well
19:53
this is the big mystery. Okay so
19:55
for a long time we thought they
19:58
might be organics that formed high-end. the
20:00
atmosphere. The current thinking was that
20:02
when the sun interacts with Titan's
20:04
atmosphere, it makes small little organic
20:06
particles, little carbon rich particles that
20:08
eventually fall out of the atmosphere.
20:11
And then the problem is, is the things that fall in
20:13
the atmosphere are too small, so they have to grow to
20:15
much larger sizes on the surface. Eventually
20:17
they would break free of the ground ice, and
20:20
then the wind would blow them around. And what happens
20:22
is that in order to get dunes, you have to
20:24
have the wind sort of blow you, and you jump
20:26
a little bit, and then when you strike the surface
20:28
again, you knock off over dune particles, within
20:30
undergo these little hops. And these hops are
20:32
called saltation. But the trick is, how can
20:34
the atmosphere make the particles that are the
20:37
right size for Titan's dunes? Okay,
20:39
and can it?
20:42
Well, they need to be about 200 microns
20:44
in size. That's about 0.2 millimeters.
20:47
This doesn't sound like very much, but that's a
20:49
very big particle to make in the atmosphere. And
20:51
making it on the ground, no one really understands
20:54
how you can make it on the ground. So
20:56
that's a problem. The other thing is they've looked
20:58
at particles not identical to Titan's dune particles, but
21:00
they've looked at particles in the laboratory that they
21:02
think might be like Titan's dune particles, and they
21:05
find that they're very weak, and they're very easy
21:07
to break apart. You need something that's stronger than
21:09
that, so we may need a different hypothesis. Okay,
21:12
and this is where you come in with a
21:14
different theory. That's right. So one
21:16
other thing that's always sort of interested me
21:19
is comets and comet particles. And these objects
21:21
are not only fairly strong, but they have
21:23
about the right sizes to saltate on Titan's
21:25
atmosphere. The question is, when it's a hypothesis
21:27
to make sense, is that where could you
21:29
get this huge amount of comet material? Where
21:31
could it come from? That's a lot of comets, yeah,
21:33
I was going to say. It's a lot
21:36
of comets, right? We probably can't get them just
21:38
from comets passing by. If you
21:40
go beyond Titan, so even more distant
21:42
from Saturn's orbit, what you find is
21:44
you eventually get to the realm of
21:46
where there's objects that look a lot
21:48
like big comets, or sometimes what we
21:50
call Kuiperball objects. And these are called
21:52
the irregular satellites. Some go
21:54
clockwise around, others go counterclockwise around.
21:57
We think that early on solar system history, a
22:00
lot of these objects were actually captured from
22:02
the processes that were happening at that time.
22:05
And because they were captured in these
22:07
strange orbits, they like to collide. And
22:09
so collusally, they're hitting each other and
22:11
they're breaking themselves down. And
22:13
when you look at the numbers on this, you can
22:15
get a lot of small particles that are created here.
22:18
And then what happens is that they
22:20
start to evolve inward towards Saturn by
22:23
interaction with solar radiation forces. And many of
22:25
those particles go to Titan. So
22:28
it could be on the end, Titan's
22:30
particles are actually from ground up of
22:32
regular satellites of Saturn. Is
22:34
there any way of testing whether you're right? NASA's
22:37
Dragonfly mission. This mission is
22:40
going to be launched in 2028. It
22:42
will get there in 2032. And
22:44
they have a special device which is called a mass
22:46
spectrometer that they're going to use
22:48
to analyze the molecules and the rest that
22:50
exist on the surface. And they're actually going
22:52
to fly into the dunes. And so using
22:54
that instrument, it's very possible we'll be able
22:57
to tell whether my hypothesis is right or
22:59
whether the existing hypothesis is right. If
23:01
you're right, when would you get an
23:03
answer? Probably 2032, when Dragonfly goes
23:05
there, or at
23:07
least a little bit afterwards. They're going to be
23:10
landing on Titan. And then eventually they're going
23:12
to fly into the dunes. And I think the
23:14
dune passage will probably happen, let's say,
23:16
within a year or so about landing on the surface. I
23:19
guess I keep your fingers crossed. And
23:22
yeah, we'll have you back on in a
23:24
decade. I
23:26
would greatly enjoy coming back. And we
23:28
can see if I'm right or wrong. And you guys
23:31
can be the judge. Bill Bocker there.
23:33
Professor Chris Lintott is with me in
23:35
the studio. Chris, what I love about
23:37
this is the timing. So Bill wanted
23:39
to flag this theory now so that
23:41
the next NASA mission flies with the
23:43
right equipment in order to test it.
23:46
Yeah, this next mission is, I think, the
23:48
coolest that we've flown in a long while.
23:51
It's called Dragonfly, good name. Great name. And
23:53
it's essentially a little chemistry lab attached to
23:55
a robocopter. So it can hop around the
23:57
surface of Titan, land in many different places.
24:00
We've been to Titan once already with the
24:02
Huygens probe, but Huygens touchdown lasted for half
24:04
an hour Gave us one picture and sampled
24:06
one place. Dragonfly is going to be a
24:09
proper mission of exploration And it probably
24:11
can test this it may be able to
24:13
tell us if those dunes are made of
24:15
distant comet stuff Or whether they're something a
24:17
bit more local and and it's just I
24:19
mean you go online look at the video
24:22
of it It's just cool. I can just
24:24
this is radio but a huge smile on
24:26
Chris's face right now. This is clearly exciting
24:28
Yeah, I think it's this sense of exploration
24:30
of Titan is a world.
24:32
It's a place that has different landscapes It
24:35
has oceans it has rivers It has strange
24:37
islands that appear and disappear which may
24:39
be something to do with bubbles in
24:41
the oceans It's got polar regions and the
24:43
idea of hopping around and exploring a new
24:45
world. That's really exciting Now
24:48
moving on all over the universe.
24:50
There are stars that originate from
24:53
the same molecular clouds That travel
24:55
together as a pair and should
24:57
be identical. They're called twin stars
25:00
But researchers in Australia recently
25:02
found something very odd something
25:04
that might have significant consequences
25:07
beyond the stars themselves What's
25:09
going on? I
25:11
spoke to Yoon Seung Ting from
25:13
the Australian National University Twin
25:16
stars are the star that were
25:18
born together And
25:20
they're also of the same mass.
25:23
So that should be identical
25:25
to each other And
25:27
what we did in the study is to
25:29
use the twin star to try to figure
25:32
out if one of the twins are
25:34
More odd than the other because
25:36
we know that by nature that
25:38
should be identical So if there's
25:40
anything strange in one star, we
25:43
know that it's by nurture not
25:45
the nature Oh, love
25:47
it. So exactly the same as twin
25:49
studies in in epidemiology
25:51
in genetics You're
25:53
looking for nature versus nurture but in
25:56
the cosmos Yes,
25:58
exactly got twin stars,
26:01
I mean how far away would they be
26:03
orbiting from each other? Yeah,
26:05
so they can be quite far away. So we are
26:07
talking about 10,000 to a million times the
26:11
distance of the Earth to
26:14
the Sun. So they are quite far apart,
26:16
but of course by a cosmic standard it's
26:18
not that far. Yeah, the space is
26:20
vast. So we study
26:22
91 pairs of twin
26:24
stars and we find that about
26:27
8% of them do
26:29
show chemical peculiarity, meaning that
26:31
out of the 91 pairs,
26:33
7 pairs of
26:35
twins do not look exactly the same. And
26:38
we dug deeper into the differences between
26:40
the two stars and confirmed
26:43
that some of them might have
26:45
created a planet or
26:47
some planetary material to change
26:49
the composition of the stars.
26:52
So they're born identical and
26:55
then one of the
26:57
pair starts swallowing planets? One
27:00
of the stars of the pair has
27:02
swallowed a planet. Looking at the
27:04
Earth and the Sun, the Earth
27:06
has more heavy elements than
27:08
the Sun, more iron
27:10
than carbon compared to the Sun. So
27:13
if the Earth were to drop into
27:15
the Sun, that will
27:17
elevate the iron to carbon
27:19
ratio a little bit. And this is
27:22
also what we detect from these
27:24
seven pairs of twins. So one
27:26
of them seems to have slightly
27:28
elevated heavy elements from
27:31
which we can tell that they must have engulfed
27:34
some planets. Can I just
27:36
check at this point, given that this
27:39
is about stars swallowing up
27:41
Earth-like planets, that's unlikely to happen
27:43
with our solar system, right? It could
27:46
happen. I was talking to
27:48
a theorist yesterday on the
27:51
stability of the solar system. It could
27:54
be the solar system in the past
27:56
has more than eight planets and
27:58
some of them might be by the
28:00
Sun. But this is still like
28:02
happening on a timescale of billions
28:04
of years. So when we talk
28:07
about either the solar system
28:09
is stable or not, we are
28:11
really talking about in the long timescale.
28:14
And therefore for the human race,
28:16
if we know the current solar
28:18
system is stable, it will
28:20
still be stable for the
28:22
human timescale, it should be like forever. This
28:26
is some quite clever research, you
28:28
know, looking at stars and working out
28:30
what they must have eaten and
28:33
noticing the difference between it
28:35
and its twin. Why
28:38
does it matter? What does it tell us about the universe?
28:40
So I think at the grander level,
28:42
it will give us a better appreciation
28:45
of how star and
28:47
planet are interact, right?
28:50
Because not too long ago, the
28:52
only planetary system that we know
28:54
is the solar system. But because
28:57
of modern day technology, we
28:59
can look into the planetary system outside
29:01
the solar system. But not only that,
29:03
like now we can even study some
29:06
of the fate of this planet.
29:08
So it really gives us a
29:11
perspective of ourselves and our position
29:13
in the universe. Joon
29:16
Seung Ting, talking about how studying
29:18
these very far off twin star
29:20
systems gives us insights into our
29:22
own solar system. Chris Lintock,
29:24
for people who don't care about anything
29:26
that happens outside our own planet, does
29:28
any of this matter? Well, I
29:31
think it matters if you care about
29:33
our existence here. One of the things
29:35
I took from this study is it's
29:37
telling us that these solar systems aren't
29:39
stable, that planets have been pingy around
29:41
and into the star, even when the
29:43
stars are mature. We thought that was
29:45
something that happened when stars were young,
29:47
but once you reach a nice stable
29:49
maturity, planetary systems shouldn't do this. And
29:51
so then you can ask the question,
29:53
will this happen here? Yeah, that's what
29:55
I did. Yeah. And we're
29:57
not sure, right? But also, I think it's
29:59
another way in which perhaps our solar system
30:01
is slightly unusual or at least we don't
30:03
live in one of these unstable systems so
30:06
it helps us understand our place in the
30:08
cosmos and it helps us understand and appreciate
30:10
maybe the planet that we're sitting on. Isn't
30:13
there that that threat, may you
30:15
live an interesting time? Yeah you definitely
30:17
don't want to live in an interesting solar
30:19
system, a nice boring one, stable planetary orbits,
30:22
less useful for physicists maybe but
30:24
we should stay here. There
30:26
was a time when people were predicting that
30:29
our solar system should be unstable and
30:31
that was disturbing but we now think that
30:34
we live in a peculiarly stable solar system
30:36
that the planets are interacting
30:38
with each other through gravity in such a way
30:40
that they they more or less are likely to
30:42
stay in their nice orbits and we get a
30:44
nice temperate earth to exist on for the
30:47
next few billion years or so. Now Radio
30:49
4 doesn't make a habit of
30:51
plugging rival podcasts but you have
30:53
one that fills a niche that
30:55
we haven't got to yet. Stargazing
30:57
with your dog. Is
30:59
your dog into astronomy? Well sort of.
31:02
I've always been a fan of lazy astronomy
31:04
of just going out and looking up and
31:06
I found having a quiet Mr. Max the
31:09
dog that I found myself outside most east things
31:12
looking at the sky and so I thought we'd
31:14
take some people with us on our walks and
31:16
experience what I see which is the sky and
31:18
a little bit of what Mr. Max sees which
31:21
is mostly whatever's on the ground and probably edible.
31:23
Let's have a little clip of you out with Max. Hello
31:26
and welcome to Dog Stars for Friday the
31:28
25th of... Hello Max. There's
31:31
an event happening in the next 10 days that I'm really excited
31:33
about which is the annual Perseid
31:35
meteor shower where we
31:37
get shooting stars. What's good
31:40
about this year is that the
31:42
moon for those peak nights is
31:44
out the way. Hello and welcome from Mr.
31:46
Max and I to... Don't leave it! Welcome.
31:50
If you haven't seen the space station it's fat.
31:53
It's just this bright star that travels across
31:56
the sky and then after a while it's
31:58
like somebody turns on a door... which
32:01
vanishes. It's quite disturbing
32:03
if you're thinking about the astronauts that are on board. Have
32:05
you found any more? No,
32:07
that's a dandelion. Okay,
32:10
you investigate that. That seems fine. Oh my god,
32:12
a whole lot of bread. No, no,
32:14
no. No, it's not the bread. That's
32:17
great. I love it. That's
32:20
pretty much my life at the minute. So, yeah. So
32:23
that's you and Rescue Lurch Max.
32:25
Yes, indeed. So dog-spouse wherever you
32:27
get your podcasts. Am I allowed
32:29
to plug it? Yes, sure, why
32:31
not? Chris,
32:34
will you stay with us for more
32:36
accidental science for the podcast version of
32:38
Inside Science? Of course, yes. Because I
32:40
want to talk about the possible alien
32:43
signal picked up by the Parkes Telescope
32:45
in 2020. Okay. Now,
32:47
because this is the podcast version of
32:49
Inside Science, we don't have to stick
32:52
to strict timings. And I've still got
32:54
Chris Lintock with me in the studio.
32:56
We can wang on for as long
32:58
as we like. Good stuff. So
33:01
in your book, you talk
33:03
about this strange alien signal
33:06
that the Parkes Telescope discovered.
33:09
Tell me about the Parkes Telescope and tell me
33:11
about the story. So the Parkes
33:13
Telescope, people will know as
33:15
the dish, which relayed
33:18
some of the Apollo landing footage back down
33:20
to Earth, but it's a working radio telescope.
33:22
It's sort of Australia's jodral bank. That's
33:25
probably offended everyone at Parkes and Jodrol, but nevermind.
33:27
You get the idea. It's a big radio telescope.
33:29
It does all sorts of sorts of science, but
33:31
it's particularly good at finding things that change in
33:33
the sky. And it's had a couple of adventures
33:35
that I talked about in the book. One was
33:38
something that the astronomers call peritons,
33:40
which are bursts of radio waves
33:43
that seem to come from all over the
33:45
sky. They're very mysterious and they couldn't be
33:47
seen by any other telescope. But, you
33:49
know, a bit of Australian pride. It's very good
33:51
at this. They thought, well, maybe our telescope is
33:53
just better at seeing these things until Somebody
33:56
made a crucial discovery, which is that they discovered
33:58
that these things, these peritons, Since
34:00
when you turn up around
34:02
lunchtime and. Whatever creating
34:05
radio waves in the universe doesn't know
34:07
about lumps time on earth we hope.
34:09
Ah as for a little bit more
34:11
investigation and see a help from a
34:13
citizen scientists to a retired engineer who
34:15
read some of the papers have recognized
34:17
the signals stand out. The door on
34:19
the microwave in the visitors center was
34:21
broken and so if you if you
34:23
impatient and opens the door before the
34:25
my wife went pings created a parrot
34:27
on and he had this is what's
34:29
known as a terrestrial signal study Also
34:31
illustrates how hard the job of radio
34:33
astronomers us we. Have to filter through
34:35
this noise and around the same
34:37
time. I'm they were
34:39
also during ah what we call Saturday
34:42
So actually you looking for signals that
34:44
might indicate the presence of Amy and
34:46
license? This has got easier in recent
34:49
years because we can look at stars
34:51
when we know that they were planets
34:53
and they looked at proximal center I
34:56
the nearest star to the sun. And
34:58
to their surprise they saw a signal.
35:00
I saw what appeared to be a.
35:03
Radio source attached to a moving as if
35:05
it was attached to a planet around the
35:08
star which they only saw when they pointed
35:10
the telescope at the stars say it was
35:12
there for for a few weeks When they
35:14
went back. Was. I found in the
35:16
data they went back it seem to have disappeared
35:18
but still very exciting and this was a product
35:20
called Breakthrough. Listen say that the. Things
35:23
could be Lc once and.
35:26
It. Leaked into the press that they might be
35:28
looking at aliens. The bills memory good about
35:30
same when we don't know I had the
35:32
for a while we have this candid at
35:34
signal from her near was planet that seem
35:36
to perhaps the at a signal of the
35:38
kind we'd expect from intention isis. It turns
35:40
out once they. Knew what they do look
35:42
like. They went and found it. All. over the
35:44
sky and some student quite know
35:46
when it was but it was
35:48
certainly something local it was a
35:50
malfunctioning not quite a mike wife
35:52
this died but satellite or something
35:54
like that sites know aliens i'm
35:56
and plenty of lunch but it
35:58
does illustrate that capable of looking
36:00
for signs of intelligence and I think
36:03
we're getting better at using telescopes like
36:06
parks to do their normal science but
36:08
at the same time listen along and
36:10
hope to be surprised. Okay
36:12
so one day one of the surprises is
36:14
going to be something that... I will
36:17
come on the Inside Science podcast and tell you the
36:19
moment it happens. Excellent! It's
36:22
a date. But for
36:24
now Chris Lin's our author of
36:27
Our Accidental Universe stories
36:29
of discovery from asteroids to aliens. Thank
36:31
you so much for coming on the
36:33
Inside Science podcast. My pleasure. This
36:36
was BBC Inside Science with me
36:38
Marnie Kesterton. The producers were Louise
36:41
Orchard and Florian Baugh and
36:43
Iman Moyn. Technical production was by Gareth
36:45
Tyrrell. The show was made in Cardiff
36:48
by BBC Wales and West in collaboration
36:50
with the Open University. BBC
36:54
Sounds, music radio podcast.
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