Listener Questions #12

Daniel and Kelly answer questions about neutrons, bananas and Jupiter and find a secret theme that links them all!

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Episode Transcript

Speaker 1 (00:06):
Why are neutrons so complicated? And why is white chocolate
not more widely hated?

Speaker 2 (00:11):
Are the bananas we eat all the same? Can we
save them from that fungal strain?

Speaker 1 (00:17):
Is Jupiter really only made of gas? It's definitely got
a lot of.

Speaker 2 (00:21):
Mess biology, physics, archaeology, forestry. Thanks for not asking about chemistry.

Speaker 1 (00:28):
What diseases do you get from your cat? Well, we'll
find the answers to all of that.

Speaker 2 (00:33):
Whatever questions keep you up at night, Daniel and Kelly's
answers will make it right.

Speaker 1 (00:37):
Welcome to another Listener Questions episode on Daniel and Kelly's
Extraordinary Universe.

Speaker 2 (00:56):
Hello, I'm Kelly Waitersmith.

Speaker 1 (00:58):
I study parasites and s and you are surprisingly good
at limericks.

Speaker 2 (01:02):
Well, I don't know about that. I gave a talk
in Kentucky and a woman who is a poet was invited,
and she gave a poem about our book, and she
encouraged me to be bolder about poetry and not so
self conscious. And I know it's not good my rhymes,
but I have so much fun, and I'm like, that's

(01:24):
kind of the point for me. For me, that's the point.

Speaker 1 (01:27):
Well, I'm Daniel I'm a particle physicist. I don't pretend
to be a poet, but I think the universe is
kind of poetic.

Speaker 2 (01:33):
Ah See, I think you're a poet in your own
way because you say very poetic things.

Speaker 1 (01:39):
Well, if being corny and curious about the universe counts
as being poetic, then put me on that list.

Speaker 2 (01:45):
It's a dad kind of poetry.

Speaker 1 (01:48):
Dad poetry. Oh my gosh, science dad poetry. That is
a new genre we are pioneering here, science parent poetry. Really.

Speaker 2 (01:56):
Yes, Well, you might ask yourself why would Kelly make
her poems public. I don't really know. I have a
confidence beyond what I ought to. But you know, there
are other questions out there, and our listeners have loads
of them.

Speaker 1 (02:10):
Questions deeper than Kelly's ability to rhyme. We love hearing
your questions about the universe. How did it begin? How
is it going to end? What does it all mean?
How does it come together to explain everything we are
and everything we eat and all the poems we listen to.
If you have questions about the nature of the universe
and you can't find answers, you've been googling, you've been
asking your neighbors, you don't know any physicists or parasitologists yourself.

(02:34):
Please write into us to questions at Danielankelly dot org.
We love, love, love to hear from you, and you
will definitely hear from us.

Speaker 2 (02:43):
And everybody should have a parasitologist and a physicist in
their lives, and we are here for you.

Speaker 1 (02:48):
That's right. We are feeling that whole you didn't know
you had in your life exactly. And so today we
have a bunch of really fun questions about neutrons, about bananas,
and about Jupiter, and there's a theme that's going to
tie them all together. We'll reveal it at the end.

Speaker 2 (03:04):
Oh, Daniel's going to be revealing this to Kelly too,
because I didn't see a theme well, I was reading
our outline. Can't wait to find out.

Speaker 1 (03:11):
This first question is from Scott Lewis, who thought that
neutrons also needed some Daniel and Kelly love after hearing
our episode about protons.

Speaker 3 (03:19):
Hi, Kelly and Daniel. There have been a number of
articles lately discussing the internal complexity of the proton and
everything we are learning about it. One article went so
far as to describe it as the most complicated thing
you can possibly imagine. I've read of unusual tetri quark
configurations and other weird things that show up in the

(03:42):
colliders from time to time. Is the internal structure of
a neutron similarly complex? Do we know less about the
guts of a neutron? And if so, is there a
reason why they are perhaps more difficult to study? Thank
you for everything you guys do great job on the program.

Speaker 2 (04:02):
This is a great question. And you know, Daniel, whenever
I hear about neutrons, I think about one of those
disaster movies with John Cusack in it, where the world
was like falling apart because the neutrons had mutated. Yeah,
I know, I almost walked out of that movie. I
loved John Cusack as a child of the eighties.

Speaker 1 (04:21):
You know, you can say anything, but don't say anything
about neutrons mutating.

Speaker 2 (04:25):
That's right, That's a line for me, a line. But
I gotta say, I don't really understand neutrons very well.
So let's start at the beginning. What are neutrons? And
hopefully by the end I'll be convinced that they won't
mutate and I don't have to worry about the world
being destroyed.

Speaker 1 (04:39):
Well, I agree with Scott. Neutrons are just as fascinating,
if not more so, than protons, and they don't get
as much attention because we don't think of them as
the building blocks of matter, but they really are. They're essential.
Without neutrons, we wouldn't have big, complicated atoms that you
need for biology and chemistry and bananas for example. But
protons and neutrons are very closely related. Both of them

(05:00):
are made of the same fundamental objects, just different amounts
of them. So a proton is made of two upcorks
and a down cork, and so the upcork is charged
two thirds and then down cork is charged minus one third.
So you add two upquarks and a down cork you
get a total charge of one. That's the proton. If
you switch one of those upcorks for a down cork,

(05:20):
and they have one upcork with charge two thirds and
two down corks with charge minus one third each, you
get a neutron because it's neutral as zero electric charge.
So two downs and an up neutron, two ups and
a down.

Speaker 2 (05:34):
Proton got it. So usually on this show you hear
me complain about how bad physicists are at naming things
because we are exactly Yeah, I'm making an accurate observation,
but I love that y'all have named the thing that
holds it all together gluons, and I'm assuming that's because
it sounds like glue, right.

Speaker 1 (05:53):
Well, the gluons aren't very sticky. Yes, yeah, they do
hold these things together. And so upquarks and down quarks
are super fascinating because they are similar to other particles
we know, like electrons, but they also feel another force,
the strong nuclear force, So they are charged. We talked
about them having two thirds or negative one third charge,
so they feel electromagnetism. They can shoot off photons, they

(06:15):
feel electric fields, but there's another field in the universe
that they feel that electrons ignore, and that's the color
field of the strong nuclear force and vibrations of that field.
They're actually eight different ones are called gluons, and so
gluons are the mediator of the strong force, the way
photons are the mediator of the electromagnetic force. It's just

(06:36):
one of the things the universe can do. And electrons
have zero color charge, so they just fly through and
ignore it the way neutrinos, for example, ignore electric fields.
But quarks they feel all of the fields. The weak feel,
the strong field, the electromagnetic field, they feel all of them,
and the strong field is the strongest one, and so
it binds these particles together very very tightly. So the

(06:57):
proton and the neutron are both bound together using gluon.

Speaker 2 (07:00):
And is there a history behind gluons that's going to
like make me think y'all aren't clever or was it
called gluons because it like seems to glue things together.

Speaker 1 (07:10):
No, we're called the gluons because they glue the nucleus
together exactly. And there's a whole fascinating history about the
discovery of gluons and the personalities involved. It was really
interesting moment with fascinating history. But basically every discovery in
particle physics has like cool personalities and controversies.

Speaker 2 (07:25):
You would say that as a prominent member of that community.

Speaker 1 (07:30):
They're not always positive stories. You know, there's like arguments
and people peeing on other people's experiments, and like, you know,
these are human stories, because hey, physicists are people, you know,
we're just curious about the universe, and there are Nobel
prizes at stake, so you don't always get the best
side of everybody.

Speaker 2 (07:46):
They sure smell like people. You walk up to them,
you're like, yeah, you're a person. But anyway, okay, one
day we should get the great story behind gluons. But
let's talk about how neutrons decay.

Speaker 1 (07:56):
Yeah, so the fascinating thing that neutrons can do that
protons do not do is that they decay. They don't
last forever. You have a neutron out there in the universe,
just by itself, it's gonna turn into a proton. And
the way it does this is that one of those quarks,
the dcork, turns into an upcork, so it goes from
D to up. Now it starts out as a D cork,

(08:18):
which is charged negative one third, and becomes an upcork,
which is charged two thirds. So to conserve electric charge,
it has to emit a negatively charged particle, so it
emits a W minus which has charged negative one So
all the charges balance out. So this dcork emits a
W minus and turns into an upcork, turning the neutron

(08:38):
into a proton, and then shooting off this W minus particle.

Speaker 2 (08:42):
Okay, so neutron, when it becomes a proton, you get
a proton and an electron that shoots off.

Speaker 1 (08:48):
You get a W minus, not an electron, but you're close.
Because the W minus doesn't live for very long. It
turns into an electron and an anti neutrino, and so
that's basically the process is the neutron turns into a
proton in order to balance the charge it has to
carry along an electron eventually, right, because you start with
a neutron it's zero charge, you end up with a

(09:09):
proton with plus one, and you need the electron with
minus one to balance the electric charges. But the universe
is not happy with that because the universe also conserves
the number of electrons. Like, you can't just create electrons
willy nilly. The universe keeps tabs on that. So if
you create an electron, you also have to create an
anti electron or it turns out electron neutrinos also count.

(09:31):
So if you create an electron and an anti electron
neutrino at the same time, then everything balances out. You've
accounted for everything the universe cares about.

Speaker 2 (09:40):
I think the up down quarks give me this maybe
false sense of understanding what's going on, because I just
imagine an up arrow and a down arrow and I'm like, oh,
I got it. You just flip the down arrow. Now
it's pointing up. But what does it mean to say
it emits a W minus? Is it just like the
change in energy gets expelled, and that's what it means
to say emitting a W minus.

Speaker 1 (10:00):
We really do think about these things as a pair,
or the up on the top and the D on
the bottom, And the way we think about it from
a sort of theoretical point of view is that the
W is the way to go up or down. So
there's actually two w's, the W plus and the W minus.
If you want to go from the D to the U,
you emit a W minus. If you want to go
from the U to the D, you emit a W plus.

(10:21):
So these are sort of like stair steps in order
to go from one to the other. That's sort of
the same way around an atom. An electron can go
up and down energy levels, and to do so, it
either emits or absorbs a photon. These ws change the
state from a D to a U, and there is
a connection to the sort of underlying theoretical structure which
we usually represent using these things called groups, where you

(10:44):
can transform an object, but it stays within a little
pre defined set that's called a group, and so it's
deeply connected to the sort of group theory structure, which
I think we should dig into sometime on the podcast.
But the basic version is that the up is sort
of the higher state and the down is the lower state.
But you can move between them using these ws.

Speaker 2 (11:01):
Okay, awesome, all right, I think I get that. Thank you.
So you can go from neutron to proton. But protons
don't decay into neutrons. Why do neutrons decay?

Speaker 1 (11:11):
Yeah, great question. Why do neutrons decay and protons don't. Well,
neutrons have a higher mass than protons, and so when
a neutron decays, it gives off a little bit of
energy and turns into a proton. Why does a neutron
have a higher mass than a proton. Well, remember, the
mass of these guys comes from the bonds between the quarks.
It's not because the neutron is made of heavier stuff

(11:31):
than the protons. These up and down quarks have almost
no mass, basically zero compared to the mass of the
proton and the neutron. All of the mass of these
guys comes from the gluons, the arrangements of the particles,
and so the neutron state up down down is a
higher energy configuration than the up, up down proton state,
and so it's just like a higher energy level the

(11:52):
way like around an atom. You know, there's like the
five two S state is a higher energy level than
like the two P or whatever. There's all these different
energy levels, and they have to do with the arrangements
between the particles, the configurations, and so the strong nuclear
force super duper complicated. But this neutron state, the UDD state,
is higher energy than the UUD and so it can

(12:12):
decay down. And that's what the universe does. It always
starts with massive particles which decay down into lighter particles.
The proton can't decay because there's nothing lighter than the proton.
Like you can't find a state that's lighter than the proton.
If you turned that other D into a U for example,
it actually would be a higher energy state than the proton.
So the proton is sort of like the bottom of

(12:33):
the ladder, the same way the electron is. The muon
can decay into an electron and other stuff. Why doesn't
the electron decay because there's nothing for it to decay into.
It's the lightest particle, and therefore it's stable. Now, we
don't know that the proton is actually stable, we've just
never seen it decay, and so we can estimate that
its lifetime is super duper long because we've watched a
bunch of protons for a long time to see if

(12:54):
any of them decay and never seen a single one decay,
which means either they're totally stable, like they live forever,
or they live for such a long time that we
just haven't seen one yet, and that lifetime would be
like billions and billions of years. So neutrons are super
fascinating because they actually do decay, so we can learn
something about what's going on inside them.

Speaker 2 (13:13):
So, in the nucleus of an atom, you have the
same number of protons and neutrons, but the number of
protons isn't changing over time, but neutrons are decaying into protons.
What's gonna happen? Are we eventually not gonna have enough
neutrons for everything?

Speaker 1 (13:28):
Yeah, this is really amazing because remember we were talking
about neutrons by themselves. A single neutron in the middle
of space will decay in about eleven to twelve minutes,
So you might be wondering, why isn't everything inside me?
Why aren't all my neutrons turning into protons? And then
like you know, everything's going haywire because the neutron is stable.
If it's inside the atom, it's unstable and will decay

(13:49):
into a proton when it's outside by itself, but inside
the atom, all of its other neutron and proton buddies
stabilize it. That's really weird, right, what's going on was
some really interesting stuff is happening there because when the
neutrons and the protons are together in the nucleus, they're
not just like packed in like tennis balls. They're interacting
with each other. Right, These things are quarks with gluons

(14:11):
holding them together, but they're not completely sealed off from
anything else. If you're like on one side of the gluon,
you might be closer to one of the quarks or
closer to one of the other quarks. So you can
actually feel the quarks inside the neutron if you're nearby it.
And so the atom is not just like a bunch
of tennis balls totally sealed off. They're interacting with each other.
There's this little residual strong force that's actually what holds

(14:33):
the nucleus together.

Speaker 2 (14:34):
Friends help you hold everything together.

Speaker 1 (14:36):
Yes, exactly, And so inside of the nucleus, neutrons can
live a long long time. Sometimes they can live forever.
Like take a carbon atom. Carbon has a bunch of
neutrons in the nuclei. Those neutrons will live forever. You
have a carbon atom, we think it could just sit
in space for a zillion zillion zillion years. Other elements
are not as stable, like uranium, for example, will break down,

(14:58):
and one of the ways it does is through these
kind of decays. And so neutrons can either crack open
your nucleus if they're not quite stable enough, or they
can help it stay together. Like the reason the nucleus
stays together all these protons which otherwise are pushing each
other apart, is because the neutrons are there in between
you to help stabilize it, to pull them together with
the strong force, and to keep the protons from pulling

(15:19):
themselves apart. So neutrons are really the glue that holds
the whole universe together.

Speaker 2 (15:23):
I feel like you could write nerdy Hallmark cards.

Speaker 1 (15:28):
I love you and your neutrons.

Speaker 2 (15:30):
That's right. You hold me together, you're my proton, you
keep me from decay. That's right.

Speaker 1 (15:41):
But there's also still a bunch of mysteries about the neutron,
Like we think we understand the basic story here, but
you know, particle physicist nerds always want to drill down
and said, do we really understand it. Let's make a
bunch of really precise measurements in different ways and see
if there's anything surprising. So there's this mystery right now
in exactly how long the neutron does live?

Speaker 2 (16:01):
How do we ask that question?

Speaker 1 (16:03):
So people came up with two very different ways to measure,
like how long does a neutron take to decay? There's
the bottle method and the beam method. And the bottle
method is pretty simple. It says, take a bunch of neutrons,
cool them down so they're not flying around everywhere, put
them in a bottle, and then just wait and see
how many you have, like you know, plot them over time.

(16:23):
The way we study radioactive decay or any kind of
random process is you start with a bunch of them
and you wait to see how long does it take
until you have half as many and that's the characteristic lifetime.
And so that's what they do, and they get a number.
It's like fourteen minutes and thirty nine seconds. It's the
characteristic lifetime of a neutron. This is a really cool
experiment they do in Los Alamos, New Mexico, actually my hometown,

(16:45):
and they have these ultra cold neutrons. They've chilled them
down to like milli kelvin inside this container they call
the bathtub. It's like one meter in diameter. They just
like fill it with neutrons and count them and then
wait to see what happens. And so they get their number.
And you know, these are serious dudes. They take it
very seriously. They've account for all sorts of uncertainty, they
have cross checks whatever. They're very confident in their number.

(17:07):
But there's another experiment, the beam experiment, and they don't
get the same answer.

Speaker 2 (17:11):
What how much does it differ by the.

Speaker 1 (17:13):
Beam experiment makes a neutron beam? And you know we
said that neutrons decay into protons, right, So they had
this clever idea like, oh, neutrons are actually really hard
to count. The other guys have this complicated, sophisticated equipment
to count neutrons. They're hard. Let's just count the protons.
If neutrons are decaying into protons, let's just count the protons.
And so they fly it through an electromagnetic field, filter
out the protons and count those and they get a

(17:36):
different answer. They get a slightly longer answer by nine seconds.
So instead of fourteen minutes and thirty nine seconds, they
get fourteen minutes and forty eight seconds. So they think
neutrons live a little bit longer than the bathtub.

Speaker 2 (17:48):
Guys, but don't you have to at least know how
many neutrons you're starting with, because if you get ten protons,
but you don't know how many neutrons you started with,
how do you know the rate of decay?

Speaker 1 (17:58):
Yeah, good question. They know how many neutrons they've started
with because they know how they produce the neutrons, Okay,
and so they think they've accounted for that. But you
know something is going on here, like it's the same process.
They should get the same answer. So either somebody's made
a subtle air totally possible, right, and they both work
really really hard to reduce these uncertainties. Often in this scenario,

(18:19):
you get two experiments. They get different measurements, but they
both have large uncertainties and they overlap, and then they
both work really really hard to refine their experiments, and
usually as the uncertainty shrink, the results converge into one answer.
You're like, Okay, cool, the universe is coherent. But what's
happening here is that the uncertainties are shrinking, but the
answers are not getting closer together, so they're getting more

(18:39):
and more confident in their discrepancy, which means, hey, maybe
there's some new interesting physics. Maybe the neutron, like the
boring vanilla particle most people aren't excited about, is actually
the portal to discovering the nature of the universe. You
all are pros at Silver Linings, Well, this is really
fun idea that maybe neutrons don't just decay to protons.

(19:02):
Maybe sometimes neutrons decay into something else, like dark matter,
and so in the neutron beam, what's happening is these
neutrons are just disappearing into dark matter, and those guys
are not measuring it. So maybe the bathtub guys are
right because they're actually measuring the neutrons, whereas the guys
who are assuming they turn into protons. They're the ones
getting the wrong answer because it's not always going to protons.

(19:24):
Sometimes it's going to dark matter.

Speaker 2 (19:25):
And we can't measure dark matter right.

Speaker 1 (19:28):
We do not have ways to measure dark matter is
certainly not in these beams, and so this is really
interesting and really important because it could be an indication
of something that's happening. And it's also important because it
helps us understand the early universe. You know, in the
very early universe, we had like quarks and gluons flying
around and things cool down into hydrogen and briefly also
forming some helium. And that ratio of hydrogen helium is

(19:52):
super important because it tells us something about the density
of quarks at that time and what the early universe
was really like. And we need neutrons in order to
form helium, Like you can't form helium without neutrons. You
can just squeeze protons together. You have to have those
neutrons to facilitate. But if the neutrons decay a little
bit faster than they aren't around as long to make helium.

(20:12):
If neutrons decay slower, there are more of them to
stick around and make helium. More helium means smaller, longer
lasting stars, so it has this cascading effect on the
whole history of the universe. Super fascinating anyway, neutrons really amazing.
Thank you very much Scott for asking about this, and
I hope that we've answered all of your questions about

(20:32):
neutrons and inspired new ones. Let's hear what Scott has
to say about our story of neutrons.

Speaker 3 (20:40):
Hi, Daniel and Kelly, thank you for the thoughtful answer.
It seems like the neutron has a pr problem and
I'm just not.

Speaker 1 (20:47):
Okay with that state of affairs.

Speaker 3 (20:49):
Neutrons do some very cool and rather important things and
the world really needs to know. As a follow up question,
if a free neutron decays in a matter of minutes,
does that imply that the study of neutron guts is
practically more difficult than the study of proton guts. Thanks
again for everything you guys do.

Speaker 1 (21:09):
Great question. Well, we can study neutrons because there are
lots of them, but seeing them fall apart is actually
useful because it gives us something to measure, to predict,
to calculate. Protons, on the other hand, just sit there,
so we have to do some work to smash them
or poke them to learn anything. So neutrons are actually
being helpful, all right.

Speaker 2 (21:45):
So I gotta tell you, I'm on the edge of
my seat trying to figure out what ties together all
of the three questions that we got today. It's still
not clear to me other than the fact that, like,
bananas are made of protons and neutrons.

Speaker 1 (21:55):
Hmmmm?

Speaker 2 (21:57):
Is that it was it that simple?

Speaker 1 (21:58):
No more than that.

Speaker 2 (22:00):
It's gotta be more than that, Okay, So our next
question is about bananas. Matt from Discord had this question.

Speaker 4 (22:08):
Hi, Danielle Kelly, this is Matt from Indiana. I was
walking through the grocery store and notice there are all
sorts of varieties of peppers, red green, tiny, big yellow orange,
tons of apple varieties, red delicious, Granny Smith. And then
I got to the bananas, just bananas, plain bananas, no

(22:28):
matter where I go. And then I found out that
most bananas we eat are banana clones. So why banana
clones and not from seeds is what I'm curious of.
Thanks at advance, and thanks for giving me an excuse
to say bananas way too many times.

Speaker 2 (22:43):
Oh man. So I was excited to have an opportunity
to read more about bananas. So let's start with banana reproduction.
Bananas can reproduce in two different ways. They reproduce sexually
by making seeds, and they reproduce asexually by producing suckers.

Speaker 1 (23:01):
Hold on, wait, I have a question already. Okay, great,
First of all, bananas reproduce or banana trees reproduced, right,
because the bananas themselves are just part of the banana tree.

Speaker 2 (23:09):
Right, Yeah, yeah, yes, you're right. You're right. I was
being lazy with my words, although I'm gonna call you
on it, because bananas aren't really trees. I think technically
they're curves.

Speaker 1 (23:18):
Really, do you remember one of.

Speaker 2 (23:20):
Our other episodes we were talking about the anatomy of
the tree and how it forms rings. Bananas are just
taxonomically distantly related. They don't form that way. They just
kind of have like a stalk that's really trunk and
tree like in the middle. But they're not like typical trees.

Speaker 1 (23:36):
Well, all right, so banana trees are not trees. I've
already learned something. And what part of the plant is
the banana? Is it fruit the way an apple? Is
this just something else weird? I remember strawberries or something
totally different. Which part of the plant are we actually
snacking on?

Speaker 2 (23:51):
It is the fruit?

Speaker 1 (23:51):
Okay?

Speaker 2 (23:52):
Yeah, yeah, what do you mean by strawberries aren't really
the fruit? I'm confused.

Speaker 1 (23:55):
Didn't we do an episode where like strawberries are actually
the seed or something? I don't remember I remember, I
mean something surprising about.

Speaker 2 (24:01):
Strawberry Strawberry seeds are on the outside, which is atypical.
But was that the whole fact?

Speaker 1 (24:06):
Anymore? Biology doesn't stay in my head as long as
physics stock.

Speaker 2 (24:10):
No, busted, Let's get away from this.

Speaker 1 (24:13):
So back to bananas. Bananas are the fruit, but they're
not technically growing on trees, because I thought fruit had
to grow on trees.

Speaker 2 (24:18):
No, I mean like strawberries aren't growing on trees.

Speaker 1 (24:21):
Hmmm, all right, cool.

Speaker 2 (24:22):
Although I guess maybe we're not quite sure if strawberries
are fruits. We're all confused today.

Speaker 1 (24:26):
I'm not sure. It doesn't mean people aren't show Okay,
got it, I got it. I'm far for an expert.
All right, So bananas can reproduce sexually or asexually.

Speaker 2 (24:34):
You were telling us yes, And so what happens with
the asexual reproduction is that the giant stalk that looks
like a trunk at the bottom underground. In addition to
its roots, it's producing what are called suckers. And these
suckers come out from the mother plant and pop up
along the sides, and they are essentially just clones of
the mom and they'll stay connected for a while, but
you can cut them off, move them somewhere else, and

(24:58):
now you've got a new banana plance.

Speaker 1 (25:00):
And why do biologists call them suckers? I mean that
makes me think of the things on an octopus's tentacle.
Are these like an octopus tentacles sticking out through the
ground or what's going on here? Do they suck in
some way?

Speaker 2 (25:11):
I don't know the history, but it's just a much
more fun name than any of you guys would have
come up with. I'm kidding. Glue ones is a great name.

Speaker 1 (25:18):
I wish we had called some particle the suckers. That
would have been really fun.

Speaker 2 (25:21):
You might discover a new particle, and I think that's
what you should name it.

Speaker 1 (25:24):
In the suckers beam, that's right. So they can basically
clone themselves, make mini versions, or they can actually get
it on with their neighbors.

Speaker 2 (25:32):
That's right. And there's something like a thousand species of
plant that could be called banana plants. Oh, so it's
a lot of diversity. But at some point in the past,
so like bananas don't fossilize, so it's hard to know
exactly when humans started eating bananas, but way before written
records were a thing for our species. What we think

(25:53):
happened was that a banana plant had a mutation and
it didn't produce seeds. And you would know if your
banana had seeds in it because the seeds produced by
lots of banana plants are big and hard, and it
would be very unpleasant to eat a banana with seeds
in it. And so bananas don't have seeds. And some
human must have found this tree and they were like, oh,

(26:14):
this is solid. There's nothing that cracks my teeth in
this plant, and so they took the suckers and that
got propagated.

Speaker 1 (26:20):
But this is like prehistory because we don't have records
of it. We don't know when this happened, that's right, Yeah,
So could it also have been the product of like
human breeding. We found like a plant with smaller seeds
and another one that crossbred them and pushed them in
that direction. Or do you think it's more likely it's
just like one random mutation.

Speaker 2 (26:37):
Artificial selection could have helped it along. I believe our
understanding is that this happened before humans really had enough
of an understanding to engage an artificial selection on purpose.

Speaker 1 (26:50):
Wow.

Speaker 2 (26:50):
But it certainly could have been the case that Joe
had a plant that had two seeds in it and
Sally had a plant that only had one, and everybody
wanted the suckers from Sally's plant. That's way better, and
over time that process could have played out. But I
don't think it was purposeful initially.

Speaker 1 (27:06):
And so that was the last sexual reproduction of these
bananas that were eating in every reproduction of banana trees
since that moment has been asexual.

Speaker 2 (27:14):
So my understanding is that there have been strains that
have arisen through this process. So it didn't necessarily happen
just once. It could have happened in like five different
banana trees in different areas, and now you've got these
different clonal lineages. But there's still all of those wild
banana species out there that are still producing seeds.

Speaker 1 (27:30):
I see.

Speaker 2 (27:31):
Okay, So around the nineteen hundreds, there was a strain
of bananas called the gro Michelle, which means big mic.

Speaker 1 (27:39):
It sounds so much fancier inference.

Speaker 2 (27:42):
It does. But the big mic was everywhere, and I'm
gonna bum everybody out, which is exactly what everybody expects
from me. Apparently the grow michelle bananas tasted better than
the bananas we have now.

Speaker 1 (27:52):
Whoa.

Speaker 2 (27:53):
But they were all clones, and so these were being
grown all over the world. Bananas were getting huge, They're
being shipped all over the world, and a fungal infection
broke out, and because all of the gro michells were clones,
they were all susceptible and it decimated the bananas around
the world. Socker, blue Blue, We're sorry, French speakers.

Speaker 1 (28:17):
Wait, do you know what the kro Michelle tasted like?
Do we have like written records or living people who
have eaten them who can tell us about this banana
that none of us will ever eat.

Speaker 2 (28:26):
There probably are some people still alive who have eaten it.
I think it was just a sweeter tasting banana than
what we have now.

Speaker 1 (28:32):
I know, the lost bananas, I know.

Speaker 2 (28:35):
My gosh, it is said, it is said.

Speaker 1 (28:37):
Is there somebody out there who's like going to de
extinctify the Groa michelle. That sounds like a billion dollar
idea right there.

Speaker 2 (28:43):
Yeah, so there might be someone who's still maintaining the
suckers from the Groa michelle in some lab somewhere, but
it remains susceptible to Panama disease, which is what we
call this fungal disease that wiped out the bananas. So
somebody maybe could bring it back. But when the Gromychelle declined,
the Cavendish arose, and the Cavendish must have just been

(29:05):
a slightly different strain that happened to be resistant to
the dominant fungal strain at the time, and so Cavendish.
If you live in North America, this is the banana
that you find on your grocery shelf. So if you
go to Harris Teeter or you go to Target, or
you go to Kroger, or you go to Trader Joe's
or Whole Foods, those are all the same banana genotypes.

(29:26):
They're clones everywhere you go.

Speaker 1 (29:27):
They all have the same DNA you're saying.

Speaker 2 (29:29):
They all have the same code in their DNA. There
could be a couple mutations, but they are very similar.

Speaker 1 (29:34):
Wow.

Speaker 2 (29:35):
Amazing In countries like Africa and India, they have a
greater appreciation for other banana varieties. So there are other
parts of the world where you can get other kinds
of bananas, but in the US we get this one.

Speaker 1 (29:45):
I've traveled in Mexico and the grocery store is there.
They have lots of different kinds of bananas there, like
little dark red bananas that taste a little bit like strawberries. Whoa,
you know, big fat bananas, and all sorts of stuff.
It's a lot of fun.

Speaker 2 (29:56):
Yeah, And plantains are fairly popular in the and I
think that's another strain where there were no seeds that
were made and then that got propagated by suckers. But
in the nineteen nineties, bad news. Oh no, the Cavendish
gets affected by Panama disease. So this fungal disease has
continued to evolve while the Cavendish is staying still in

(30:19):
this evolutionary arms race, because it's just a clone that
we propagate over and over and over again. And there's
now a strain of Panama disease that is going after
the Cavendish bananas.

Speaker 1 (30:29):
Why do they hate us so much?

Speaker 2 (30:31):
I know, I know, fungus is the worst, except.

Speaker 1 (30:35):
When it's helping us make beer and bread and al sorts.

Speaker 2 (30:37):
Of Rather you get me things, you know, I guess
whenever you say a blanket statement, you're a most always
going to be wrong.

Speaker 1 (30:42):
Some of them are really fun guys.

Speaker 2 (30:43):
Actually, no, dad jokes, dead poetry. Okay. So now we've
got Panama disease and it is spreading, and so there's
some people who will be concerned what happens if the
Cavendish declines? Do we have something waiting to replace it?
And the answer is no, no, no, what?

Speaker 1 (31:04):
No? What are those people doing? Get on it? Food scientists.

Speaker 2 (31:07):
There is a lot of money in bananas, so there's
a lot of people working on it. The first thing
that they're doing to try to slow the decline is
biocontrol efforts. So if you go to a major banana
plantation and you want to go amongst the trees, you
have to suit up in sterilized clothes, you have to
put on boots and then walk through a sterilizing solution,

(31:28):
and you have to do that every time you walk
from like one plot of bananas to another. Because the
way the fungus transmits is in the soil. So if
you get like dirt in your boots and then you
walk in another area, you can transmit that.

Speaker 1 (31:41):
Wow.

Speaker 2 (31:41):
So it's a pain in the rear end. And like
every truck that comes in and out has to get sprayed.
But if they do find a tree that's infected, they
have to dump fungicides into the soil, kill everything in
that area, cover it with urea, which I think just
also changes soil chemistry, making it more likely to kill
the fungus, cover it with the tarp so that birds
don't walk on it, and then bring the fungus somewhere else.

(32:03):
The next zone of plants also get like fungicides and
herbicides injected into the soil, and then the zone after
that you have to check, like every month, you have
to do like a survey to make sure none of
them have it. And so it's intense.

Speaker 1 (32:17):
Apology is just so hard to control. It's always wriggling
and squirming out of our control.

Speaker 2 (32:22):
Yes, well, man an invasive species. I feel like it's
such an interesting conversation about when do you just give up,
Like it's not worth trying to get starlings out of
the US anymore. They're not going anywhere.

Speaker 1 (32:32):
They're here anyway, Well, what about bananas? Is there anything
else we can do? Like, can't we somehow protect our
bananas or cross them with other wild species or something?

Speaker 2 (32:41):
Yeah, I can hear the panic building in your voice.
Don't worry. We have a couple options.

Speaker 1 (32:45):
I like banana bread.

Speaker 2 (32:46):
Okay, I know, me too, Me too. Zach makes a
good banana bread. I don't get in the kitchen, but
he does a great job. So genetic engineering is one solution,
and they have in fact added genes from other plants,
I think tomato to make the cavendish resist to Panama disease.
And this works, it is resistant. But in the European Union,
I believe, you're not allowed to sell genetically modified plants.

(33:08):
And in the United States there's a lot of people
who feel very squeamish about genetically modified plants, and so
the industry has decided that this can't be the solution.
It just would not be financially viable.

Speaker 1 (33:18):
Wow, so he could save the bananas, but still it's
not good enough.

Speaker 2 (33:22):
Not good enough, And so the last thing that they're
trying are breeding experiments. So apparently something like one in
ten thousand bananas will produce a seed. Sometimes it like
still slips through, so you can search bananas for that
seed and then cross the Cavendish with other species of
wild bananas, and so there are some efforts to cross breed.

(33:43):
But the problem is, like the Cavendish, it's actually an
absolute marble of a fruit. You know, it comes in
its own packaging that ripens over the course of a
week while it is in transit to you, so it
arrives to you mostly unbruised and now perfectly ready to eat.
And the various crosses that they've done have produced bananas

(34:05):
that are like, you know, maybe they're yellow, maybe they
still have a good you know, outer coating. But so
far they haven't been able to find anything that meets
all of their criteria and is delicious. I was reading
about one banana that looks like a Cavendish and tastes good,
but it's described as an acid banana, which doesn't sound delicious,
but it just doesn't taste like the Cavendish. And so

(34:26):
right now they haven't been able to find anything to
replace the Cavendish in what some people would say is
a more sort of natural method. So that's where we are.
Are we going to have a banana in one to
two decades. We'll have to wait and see.

Speaker 1 (34:39):
Oh my gosh, our children or our grandchildren might never
know the tastes of bananas the way we don't know
the taste of the groamy shell.

Speaker 2 (34:48):
I know it could be traged I mean, think of
how many babies had bananas as their very first food
or something like. It could be that my kid's first
foods were smushed up bananas. My memory is a sieve,
so I don't know exactly what I fed them the
first time, but a banana.

Speaker 1 (35:01):
And you know, there's something else fascinating about bananas, which
is that they are radioactive.

Speaker 2 (35:07):
Is that gonna be the connection?

Speaker 1 (35:09):
Don't give it away, Kelly. Yeah, but yes, inside bananas
there's naturally occurring potassium forty, which is unstable, and the
neutrons inside potassium forty decay, And so if you are
hanging around a banana, it will emit high energy electrons
and anti neutrinos. Wow, which is technically a radiation.

Speaker 2 (35:28):
Oh would we all be better off without bananas in
our life?

Speaker 1 (35:31):
I don't know. Bananas contribute to the natural radiation background,
which I'm sure affects the mutation rate so it's made
all of us who we are.

Speaker 2 (35:38):
Oh wow, Okay, on that deep dad poetry note. Let's
find out if Matt found this answer satisfactory. And we'd
also like to take this moment to thank Matt for
being an amazing moderator of our discord channel. And if
you want to join us on discord, go to Daniel
and Kelly dot org not dot com, although dot com
appears to be a dead link now because the other

(36:00):
duel and Kelly got married and their website is down.

Speaker 1 (36:03):
Which means either the wedding went wonderfully and they don't
care about it anymore, or maybe something didn't go so well.

Speaker 2 (36:08):
Oh man, I'm hoping for the former.

Speaker 1 (36:10):
Yes, good luck Daniel Kelly. Yes, but please do join
us on the discord with lots of people are asking
questions and having conversations about science and pizza and all
sorts of crazy stuff. Go to Danielankelly dot org to
find the link to join.

Speaker 2 (36:23):
The discord, and let's hear what Matt had to say.

Speaker 4 (36:25):
That answer was beautiful. Thank you so much.

Speaker 5 (36:28):
Now I know more about banana suckers than I've ever
wanted to know. And also thanks for giving me a
shout out on the discord for being an administrator there,
and we really do hope other people will join, just
like Daniel said, please join us. We'll answer any questions. Yeah,
have a wonderful day, guys.

Speaker 2 (36:42):
Thanks.

Speaker 1 (37:00):
All right, we're back and we are answering questions from listeners.
There's a special secret theme of today's podcast that's going
to tie all of these questions together. Let's see how
long it takes Kelly to figure it out?

Speaker 2 (37:10):
How many lifetimes?

Speaker 1 (37:14):
The next question is from Steve, who has a question
about the biggest gaseest planet in the Solar System.

Speaker 2 (37:20):
That isn't Uranus. Sorry I had to.

Speaker 6 (37:25):
Hi, Daniel and Kelly. This is Steve from BC Canada.
I have a controversial take here. Could it be said
that there is no such thing as a gas giant
because these planets have so much pressure that gas becomes liquefied.
So aren't they really liquid planets? Maybe liquid giants? Sure,

(37:46):
they are composed of liquid elements that are gaseous to
earthlings living in earthly pressures, but they are not earth
and they don't have earthly pressures, so we should be
calling them liquid giants. Don't you think? I think it's
about high time that we do a deep dive into
the inner workings of gas planets. What really are they?

Speaker 1 (38:09):
All right? So Steve is asking a question about the
science of Jupiter, but also about the name of the
category that Jupiter finds itself in gas giants. Are they
really gassy? Should we be calling them liquid giants? These
are good questions, Steve.

Speaker 2 (38:22):
These are great questions. Yeah, and you gotta tell Jupiter
and lay off the beans.

Speaker 1 (38:27):
No, No, we're pro beans, even if it makes you gassy.
Katrina would tell me that beans makes everything better.

Speaker 2 (38:33):
Nobody knows better than Katrina.

Speaker 1 (38:36):
She certainly does. She certainly does, all right, So let's
dig into it. What in the end is Jupiter made
out of? Well, Jupiter, like Earth and the Sun, formed
from this big blob of stuff that the whole Solar
System was made out of. And you know, the Solar
system is mostly just the Sun. Like the Sun has
ninety nine points something percent of all the mass in
the Solar System. Basically, you have a much larger cloud

(38:58):
of stuff than our Solar system and others systems formed from.
But there was in there some seed, some gravitational over
density that pulled stuff together to form our Solar System,
and mostly that just collapsed into the center, and most
of it was hydrogen, because that's what the universe started
out at. As in fourteen billion years later, were still
mostly hydrogen, and so the Sun is mostly hydrogen. But

(39:20):
near the Sun there were also other little areas of
over density that managed to pull themselves together and hold
themselves together and resist the Sun's attraction, and that's how
the planets formed. So you get small rocky planets like
Earth and the Inner Solar System because the Sun then
blew away their atmospheres, but far enough out away from
the Sun, the Sun's radiation didn't blast away all the

(39:41):
helium and hydrogen, and there was ice out there. Things
were cold enough to form ice crystals, so you had
a little bit of an advantage to make bigger planets
that could grab a little bit more mass. So Jupiter
is just a scoop of the original protosolar system that
everything else is made out of.

Speaker 2 (39:56):
So it's a better representation of the protosolar system than Earth.

Speaker 1 (40:00):
Yeah, absolutely, Earth once had an atmosphere of hydrogen the
way that the Sun does and the way Jupiter does,
but it was blown away by the early Sun and
so the Earth is not a great representation of what
the Solar System is. And actually we're gonna do an
episode pretty soon about how we know what the universe
is made out of it And it was a big
shocker when we discovered that most of the universe is
not made of the same stuff as the Earth. The

(40:20):
Earth is an unusual helping of Solar System or universe material.

Speaker 2 (40:25):
Thankfully for us, Yes, exactly, thanks early for us.

Speaker 1 (40:28):
That's why we have bananas. No, that's not the secret theme.
So Jupiter is mostly hydrogen right by mass. The outside
is like seventy six percent hydrogen and then twenty four
percent helium and then just like trace tiny other stuff
like a little bit of carbon, a little bit oxygen,
and a little bit of salt for a little bit
of neon. But the atmosphere, which is just really an

(40:48):
artificial designation of like a certain layer within Jupiter, is
mostly hydrogen and helium.

Speaker 2 (40:54):
What would be the arbitrary divider for Jupiter? I do
think of Jupiter is being just gas all the way through,
and maybe that's just because it's called a gas giant.
So what is the dividing line or dividing criteria for
the atmosphere versus the interior yees.

Speaker 1 (41:11):
So it's a little bit arbitrary, but basically, you have
layers of stuff that get denser and denser as you
go in. So you start out the very outer layers
of Jupiter are cloud layers, and so these are like
ammonia crystals. There's really high winds, but it's mostly gaseous
hydrogen with these clouds of ammonia crystals. And that's what
you see when you look at Jupiter, you know, like

(41:31):
the rings and the red spot and all this stuff.
These are like weather patterns in those clouds in the
very very top layer of Jupiter's atmosphere. But then once
you penetrate through those layers of clouds, like fifty kilometers
of clouds or so, below that, there's liquid hydrogen, right,
And so hydrogen is an atom, but it also forms

(41:53):
H two, which is a molecule, and then it has
various phases and it depends on the temperature and depends
on the pressure. So you start out with gaseous hydrogen
and then you squeeze it down and you get liquid hydrogen.
And so this stuff flows, right, it's just denser, and
so you might say, all right, we're not really in
the atmosphere anymore, because now we have a liquid and
you know, here on Earth we consider the atmosphere of

(42:14):
the gaseous part, and then the surface is where you
have like solid rock and also liquid. But it's not
quite so simple on Jupiter because it's not as clear
and crisp like here on Earth. You know, you have
liquid and above it is gas, and like if you're
swimming in the ocean, you can very clearly tell the
crisp difference. But on Jupiter, they don't really have the
same distinct transition between liquid and gas, and so you

(42:37):
have this like gradual transition between gaseous hydrogen and liquid hydrogen.
What's really going on here is that molecular hydrogen, if
you look at its phase diagram, there are some pressures
and temperatures where it's gas and some pressures in temperatures
where it's liquid. But there's this critical point, this temperature
and pressure above which it's not really gas and not

(42:58):
really liquid, and this transition sort of therefore gradual. There's
this sort of super critical fluid. It's not really technically
a liquid, it's not really technically a gas that has
some similarity to both, And so the reason you can't
just say like, oh, this is the surface of Jupiter
is that as you descend, it just sort of gets
denser and denser till eventually it feels like liquid. And

(43:19):
if you rose back up, it would get less and
less dense, and then it would just sort of feel
like gas. But it's a gradual transition rather than an
abrupt one the way it is here on Earth.

Speaker 2 (43:28):
I see we have yet again accidentally foraid into chemistry,
but I understand it better now.

Speaker 1 (43:33):
And as you descend, the weather gets really really weird.
So you get this like helium neon rain. What. Yeah,
I know, it's really crazy and not something I think
you should dance and sing in, for example. But this
is sort of rain like droplets. And what's happening is
that you have helium and neon the and the upper atmosphere,
but they come together and form these drops, which then
sink and depleting the abundance of these elements in the

(43:55):
upper atmosphere, and they fall down to lower levels of
the atmosphere. And this is all very speculative. You know.
There are people who think, for example, like on Saturn,
there might be conditions that cause diamonds to rain, you know,
like formation of diamonds in the atmosphere because the intense
pressure which then fall below. But a lot of this
is speculative. This is like people running models and thinking

(44:16):
maybe this is what happens and it's super cool. But
you know, the big fixture story here is like, we
really don't understand this stuff. A lot of this is
just speculation.

Speaker 2 (44:25):
Which is why we need more money to go out
there and find out definitely do.

Speaker 1 (44:29):
And then things get even weirder as you squeeze it down.
As you go down further towards the center of Jupiter,
you're getting higher temperature and higher pressure. Then you reach
this region where the hydrogen is metallic, right, And metallic
is a really weird term to apply to hydrogen because
in astronomy usually they say, well you have helium and
you have hydrogen. Everything else they call them metal, right,

(44:52):
So if you talk about the metallicity of stars, it
means how much of the star is not hydrogen, how
much of it is not helium, everything else they call
a metal have a different meaning for what is a metal? Right.
They're thinking about things where the electrons are flowing because
the atoms are sort of linked together and the electrons
are not attached to individual atoms. And that's what we're
talking about here. This is like the chemical version of

(45:13):
a metal.

Speaker 2 (45:14):
Does it mean that the atoms are flowing or we're
using the chemistry definition.

Speaker 1 (45:17):
Now, yeah, we're using the chemistry definition. Because what happens
is you take those H two molecules, you squeeze them together,
and the hygen forms something like a lattice. Right, instead
of having individual H two molecules which have some interaction,
you know, because of the polarity of them, now you're
squeezing them together, so the electrons can just jump from
one hydrogen to another hydrogen to another one. It's like

(45:39):
a big crystal. It's not quite as tight, but it
conducts electricity. Right. Normally hydrogen does not conduct any electricity,
but you squeeze it together, you make it dense enough
it will conduct. And so it has this like bulk
lattice phase with delocalized electrons in it. And this is
something people have been thinking for decades and decades, and
only the last few years have they been able to

(46:01):
convincingly make this stuff in the lab by recreating these
conditions and seeing it actually conduct electricity. So this is
this huge chunk of Jupiter which is hydrogen squeeze so
tight that we think it's basically one enormous conductor.

Speaker 2 (46:16):
So when you touch metallic hydrogen, is it hard like
the metals that I am thinking of, or are we
still in a sort of like gassy liquidy kind of phase.

Speaker 1 (46:26):
Yeah, great question. Not something we understand super well. But
I don't recommend you lick it. If somebody has some
metallic hydrogen, it's hard to imagine what would be like
to touch it because you can't have it around unless
it's under very, very high pressure. So it's not like
somebody could hand you a chunk of metallic hydrogen that
you could like even consider licking. Okay, it's just going
to be like super duper dense material.

Speaker 2 (46:46):
Got it, Okay, I don't want to die for this podcast.

Speaker 1 (46:48):
Probably not tasty. I'd recommend a banana for a snack
instead of metallic hydrogen.

Speaker 2 (46:52):
Wait, hold on, what is the connection then? Is the
connection that there's a part of Jupiter that's solid like
a banana and the equipment we used to study neutrons
as solid too, Daniel, I just don't know.

Speaker 1 (47:03):
Well, Jupiter is active right the same way the Sun is.
It's a big hot thing and so it radiates. There's
no fusion going on inside Jupiter, but you know, the
pressure and the temperature are very high, and so there
is a lot of radiation being emitted. If you wanted to,
for example, establish a base on one of the moons
of Jupiter, you really have to worry about the Jupiter
win the Jovian winds, very high energy particles shooting at you.

(47:27):
So just like a banana and just like a neutron,
you have to worry about radiation if you're going to
live near any of these things.

Speaker 2 (47:34):
Radiation is the theme.

Speaker 1 (47:37):
It's a particle, of course, I'm not trying to be
tricky about it.

Speaker 2 (47:41):
Well I got it before the end of the episode almost,
so bravo Kelly.

Speaker 1 (47:45):
Congratulations. You get a banana. If I had a grow Michelle,
I would share it with you.

Speaker 2 (47:49):
Oh, thank you.

Speaker 1 (47:49):
So then we can dig down even deeper into Jupiter,
and eventually you get to stuff that's not hydrogen. So
we think there's a really thick atmosphere. Metallic hydrogen is
up to like maybe eighty percent of the radio is
if you go down to like thirty to fifty percent
of the radius of Jupiter. There is stuff down there
that's solid. It's like made of rock, the same kind
of stuff that the Earth is made out of. And
it's not small. It's like thirty to fifty percent of

(48:12):
the radius of Jupiter. It's a really big chunk of
ice and rock. But you know it's buried under an
incredibly thick layer of hydrogen. And so if you're really
hardcore about you could say, well, that's the surface because
everything else is a gas. It's hydrogen. But you know
it's not in a gas phase. It's in a metallic phase,
or it's in a super critical fluid phase. And so

(48:34):
you could, if you do really deep into Jupiter, stand
on a rocky quote unquote surface. But I don't think
you could still call Jupiter a rocky planet.

Speaker 2 (48:42):
All right, yep, I'm giving it to the astronomers. I
think gas giant is a reasonable name, and also it
gives many school kids lots of chuckles, and so I
think it's great.

Speaker 1 (48:51):
Yeah, but it is confusing, right because we call it
a gas giant because it's mostly made of hydrogen. But
hydrogen is not always in a gaseous state, and especially
in Jupiter. Most of the gas on Jupiter is metallic,
so you could also call it a metallic giant and
be like, kind.

Speaker 2 (49:05):
Of correct, that does sound cooler.

Speaker 1 (49:08):
It does sound more metal, right, that's right, that's right,
all right. So I think we've concluded that astronomy names
are very confusing and maybe there's no way to do
it right, but it's fun to dig into anyway. And
so Steve from BC let us know if we answered
your question about Jupiter.

Speaker 7 (49:23):
Thanks Daniel and Kelly for answering my question. That was
really insightful to know that Jupiter could be really a
metal giant. But it makes me think now about how
we've named Earth. You know, Earth has a lot of
gas and we depend on that gas. And you know
how much different is the amount of gas and rock
ratio than Jupiter. I mean, would it be correct to

(49:45):
say that Earth is a gas midget? Thanks again for
answering my question. You're still my favorite podcast. Keep the
great answers coming, and thank you for being such great
signs communicators.

Speaker 2 (49:57):
Well, thank you for all of the wonderful questions we
got today, and we hope to hear from you. Send
us your questions at Questions at Danielankelly dot org. We
answer every question, and some of the questions even end
up on the show.

Speaker 1 (50:09):
We do love to hear from you, and we'd love
to hear that you are curious that you share our
passion to understand the universe how it works, from the
bananas all the way out to the galaxies. So join
us on the discord. Write to us at questions at
danielan Kelly dot org. Let us know you're out there.

Speaker 2 (50:32):
Daniel and Kelly's Extraordinary Universe is produced by iHeartRadio. We
would love to hear from you, We really would.

Speaker 1 (50:39):
We want to know what questions you have about this
Extraordinary Universe.

Speaker 2 (50:43):
We want to know your thoughts on recent shows, suggestions
for future shows. If you contact us, we will get
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Speaker 1 (50:50):
We really mean it. We answer every message. Email us
at questions at Danielankelly.

Speaker 2 (50:56):
Dot org, or you can find us on social media.
We have accounts on x, Instagram, Blue Sky and on
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and K Universe.

Speaker 1 (51:06):
Don't be shy, write to us