WEBVTT - Listener Questions #12

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<v Speaker 1>Why are neutrons so complicated? And why is white chocolate

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<v Speaker 1>not more widely hated?

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<v Speaker 2>Are the bananas we eat all the same? Can we

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<v Speaker 2>save them from that fungal strain?

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<v Speaker 1>Is Jupiter really only made of gas? It's definitely got

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<v Speaker 1>a lot of.

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<v Speaker 2>Mess biology, physics, archaeology, forestry. Thanks for not asking about chemistry.

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<v Speaker 1>What diseases do you get from your cat? Well, we'll

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<v Speaker 1>find the answers to all of that.

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<v Speaker 2>Whatever questions keep you up at night, Daniel and Kelly's

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<v Speaker 2>answers will make it right.

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<v Speaker 1>Welcome to another Listener Questions episode on Daniel and Kelly's

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<v Speaker 1>Extraordinary Universe.

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<v Speaker 2>Hello, I'm Kelly Waitersmith.

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<v Speaker 1>I study parasites and s and you are surprisingly good

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<v Speaker 1>at limericks.

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<v Speaker 2>Well, I don't know about that. I gave a talk

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<v Speaker 2>in Kentucky and a woman who is a poet was invited,

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<v Speaker 2>and she gave a poem about our book, and she

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<v Speaker 2>encouraged me to be bolder about poetry and not so

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<v Speaker 2>self conscious. And I know it's not good my rhymes,

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<v Speaker 2>but I have so much fun, and I'm like, that's

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<v Speaker 2>kind of the point for me. For me, that's the point.

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<v Speaker 1>Well, I'm Daniel I'm a particle physicist. I don't pretend

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<v Speaker 1>to be a poet, but I think the universe is

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<v Speaker 1>kind of poetic.

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<v Speaker 2>Ah See, I think you're a poet in your own

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<v Speaker 2>way because you say very poetic things.

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<v Speaker 1>Well, if being corny and curious about the universe counts

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<v Speaker 1>as being poetic, then put me on that list.

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<v Speaker 2>It's a dad kind of poetry.

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<v Speaker 1>Dad poetry. Oh my gosh, science dad poetry. That is

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<v Speaker 1>a new genre we are pioneering here, science parent poetry. Really.

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<v Speaker 2>Yes, Well, you might ask yourself why would Kelly make

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<v Speaker 2>her poems public. I don't really know. I have a

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<v Speaker 2>confidence beyond what I ought to. But you know, there

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<v Speaker 2>are other questions out there, and our listeners have loads

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<v Speaker 2>of them.

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<v Speaker 1>Questions deeper than Kelly's ability to rhyme. We love hearing

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<v Speaker 1>your questions about the universe. How did it begin? How

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<v Speaker 1>is it going to end? What does it all mean?

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<v Speaker 1>How does it come together to explain everything we are

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<v Speaker 1>and everything we eat and all the poems we listen to.

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<v Speaker 1>If you have questions about the nature of the universe

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<v Speaker 1>and you can't find answers, you've been googling, you've been

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<v Speaker 1>asking your neighbors, you don't know any physicists or parasitologists yourself.

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<v Speaker 1>Please write into us to questions at Danielankelly dot org.

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<v Speaker 1>We love, love, love to hear from you, and you

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<v Speaker 1>will definitely hear from us.

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<v Speaker 2>And everybody should have a parasitologist and a physicist in

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<v Speaker 2>their lives, and we are here for you.

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<v Speaker 1>That's right. We are feeling that whole you didn't know

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<v Speaker 1>you had in your life exactly. And so today we

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<v Speaker 1>have a bunch of really fun questions about neutrons, about bananas,

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<v Speaker 1>and about Jupiter, and there's a theme that's going to

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<v Speaker 1>tie them all together. We'll reveal it at the end.

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<v Speaker 2>Oh, Daniel's going to be revealing this to Kelly too,

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<v Speaker 2>because I didn't see a theme well, I was reading

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<v Speaker 2>our outline. Can't wait to find out.

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<v Speaker 1>This first question is from Scott Lewis, who thought that

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<v Speaker 1>neutrons also needed some Daniel and Kelly love after hearing

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<v Speaker 1>our episode about protons.

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<v Speaker 3>Hi, Kelly and Daniel. There have been a number of

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<v Speaker 3>articles lately discussing the internal complexity of the proton and

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<v Speaker 3>everything we are learning about it. One article went so

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<v Speaker 3>far as to describe it as the most complicated thing

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<v Speaker 3>you can possibly imagine. I've read of unusual tetri quark

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<v Speaker 3>configurations and other weird things that show up in the

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<v Speaker 3>colliders from time to time. Is the internal structure of

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<v Speaker 3>a neutron similarly complex? Do we know less about the

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<v Speaker 3>guts of a neutron? And if so, is there a

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<v Speaker 3>reason why they are perhaps more difficult to study? Thank

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<v Speaker 3>you for everything you guys do great job on the program.

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<v Speaker 2>This is a great question. And you know, Daniel, whenever

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<v Speaker 2>I hear about neutrons, I think about one of those

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<v Speaker 2>disaster movies with John Cusack in it, where the world

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<v Speaker 2>was like falling apart because the neutrons had mutated. Yeah,

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<v Speaker 2>I know, I almost walked out of that movie. I

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<v Speaker 2>loved John Cusack as a child of the eighties.

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<v Speaker 1>You know, you can say anything, but don't say anything

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<v Speaker 1>about neutrons mutating.

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<v Speaker 2>That's right, That's a line for me, a line. But

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<v Speaker 2>I gotta say, I don't really understand neutrons very well.

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<v Speaker 2>So let's start at the beginning. What are neutrons? And

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<v Speaker 2>hopefully by the end I'll be convinced that they won't

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<v Speaker 2>mutate and I don't have to worry about the world

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<v Speaker 2>being destroyed.

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<v Speaker 1>Well, I agree with Scott. Neutrons are just as fascinating,

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<v Speaker 1>if not more so, than protons, and they don't get

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<v Speaker 1>as much attention because we don't think of them as

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<v Speaker 1>the building blocks of matter, but they really are. They're essential.

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<v Speaker 1>Without neutrons, we wouldn't have big, complicated atoms that you

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<v Speaker 1>need for biology and chemistry and bananas for example. But

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<v Speaker 1>protons and neutrons are very closely related. Both of them

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<v Speaker 1>are made of the same fundamental objects, just different amounts

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<v Speaker 1>of them. So a proton is made of two upcorks

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<v Speaker 1>and a down cork, and so the upcork is charged

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<v Speaker 1>two thirds and then down cork is charged minus one third.

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<v Speaker 1>So you add two upquarks and a down cork you

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<v Speaker 1>get a total charge of one. That's the proton. If

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<v Speaker 1>you switch one of those upcorks for a down cork,

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<v Speaker 1>and they have one upcork with charge two thirds and

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<v Speaker 1>two down corks with charge minus one third each, you

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<v Speaker 1>get a neutron because it's neutral as zero electric charge.

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<v Speaker 1>So two downs and an up neutron, two ups and

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<v Speaker 1>a down.

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<v Speaker 2>Proton got it. So usually on this show you hear

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<v Speaker 2>me complain about how bad physicists are at naming things

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<v Speaker 2>because we are exactly Yeah, I'm making an accurate observation,

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<v Speaker 2>but I love that y'all have named the thing that

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<v Speaker 2>holds it all together gluons, and I'm assuming that's because

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<v Speaker 2>it sounds like glue, right.

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<v Speaker 1>Well, the gluons aren't very sticky. Yes, yeah, they do

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<v Speaker 1>hold these things together. And so upquarks and down quarks

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<v Speaker 1>are super fascinating because they are similar to other particles

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<v Speaker 1>we know, like electrons, but they also feel another force,

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<v Speaker 1>the strong nuclear force, So they are charged. We talked

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<v Speaker 1>about them having two thirds or negative one third charge,

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<v Speaker 1>so they feel electromagnetism. They can shoot off photons, they

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<v Speaker 1>feel electric fields, but there's another field in the universe

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<v Speaker 1>that they feel that electrons ignore, and that's the color

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<v Speaker 1>field of the strong nuclear force and vibrations of that field.

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<v Speaker 1>They're actually eight different ones are called gluons, and so

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<v Speaker 1>gluons are the mediator of the strong force, the way

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<v Speaker 1>photons are the mediator of the electromagnetic force. It's just

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<v Speaker 1>one of the things the universe can do. And electrons

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<v Speaker 1>have zero color charge, so they just fly through and

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<v Speaker 1>ignore it the way neutrinos, for example, ignore electric fields.

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<v Speaker 1>But quarks they feel all of the fields. The weak feel,

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<v Speaker 1>the strong field, the electromagnetic field, they feel all of them,

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<v Speaker 1>and the strong field is the strongest one, and so

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<v Speaker 1>it binds these particles together very very tightly. So the

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<v Speaker 1>proton and the neutron are both bound together using gluon.

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<v Speaker 2>And is there a history behind gluons that's going to

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<v Speaker 2>like make me think y'all aren't clever or was it

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<v Speaker 2>called gluons because it like seems to glue things together.

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<v Speaker 1>No, we're called the gluons because they glue the nucleus

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<v Speaker 1>together exactly. And there's a whole fascinating history about the

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<v Speaker 1>discovery of gluons and the personalities involved. It was really

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<v Speaker 1>interesting moment with fascinating history. But basically every discovery in

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<v Speaker 1>particle physics has like cool personalities and controversies.

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<v Speaker 2>You would say that as a prominent member of that community.

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<v Speaker 1>They're not always positive stories. You know, there's like arguments

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<v Speaker 1>and people peeing on other people's experiments, and like, you know,

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<v Speaker 1>these are human stories, because hey, physicists are people, you know,

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<v Speaker 1>we're just curious about the universe, and there are Nobel

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<v Speaker 1>prizes at stake, so you don't always get the best

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<v Speaker 1>side of everybody.

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<v Speaker 2>They sure smell like people. You walk up to them,

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<v Speaker 2>you're like, yeah, you're a person. But anyway, okay, one

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<v Speaker 2>day we should get the great story behind gluons. But

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<v Speaker 2>let's talk about how neutrons decay.

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<v Speaker 1>Yeah, so the fascinating thing that neutrons can do that

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<v Speaker 1>protons do not do is that they decay. They don't

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<v Speaker 1>last forever. You have a neutron out there in the universe,

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<v Speaker 1>just by itself, it's gonna turn into a proton. And

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<v Speaker 1>the way it does this is that one of those quarks,

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<v Speaker 1>the dcork, turns into an upcork, so it goes from

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<v Speaker 1>D to up. Now it starts out as a D cork,

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<v Speaker 1>which is charged negative one third, and becomes an upcork,

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<v Speaker 1>which is charged two thirds. So to conserve electric charge,

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<v Speaker 1>it has to emit a negatively charged particle, so it

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<v Speaker 1>emits a W minus which has charged negative one So

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<v Speaker 1>all the charges balance out. So this dcork emits a

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<v Speaker 1>W minus and turns into an upcork, turning the neutron

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<v Speaker 1>into a proton, and then shooting off this W minus particle.

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<v Speaker 2>Okay, so neutron, when it becomes a proton, you get

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<v Speaker 2>a proton and an electron that shoots off.

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<v Speaker 1>You get a W minus, not an electron, but you're close.

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<v Speaker 1>Because the W minus doesn't live for very long. It

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<v Speaker 1>turns into an electron and an anti neutrino, and so

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<v Speaker 1>that's basically the process is the neutron turns into a

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<v Speaker 1>proton in order to balance the charge it has to

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<v Speaker 1>carry along an electron eventually, right, because you start with

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<v Speaker 1>a neutron it's zero charge, you end up with a

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<v Speaker 1>proton with plus one, and you need the electron with

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<v Speaker 1>minus one to balance the electric charges. But the universe

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<v Speaker 1>is not happy with that because the universe also conserves

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<v Speaker 1>the number of electrons. Like, you can't just create electrons

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<v Speaker 1>willy nilly. The universe keeps tabs on that. So if

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<v Speaker 1>you create an electron, you also have to create an

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<v Speaker 1>anti electron or it turns out electron neutrinos also count.

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<v Speaker 1>So if you create an electron and an anti electron

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<v Speaker 1>neutrino at the same time, then everything balances out. You've

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<v Speaker 1>accounted for everything the universe cares about.

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<v Speaker 2>I think the up down quarks give me this maybe

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<v Speaker 2>false sense of understanding what's going on, because I just

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<v Speaker 2>imagine an up arrow and a down arrow and I'm like, oh,

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<v Speaker 2>I got it. You just flip the down arrow. Now

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<v Speaker 2>it's pointing up. But what does it mean to say

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<v Speaker 2>it emits a W minus? Is it just like the

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<v Speaker 2>change in energy gets expelled, and that's what it means

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<v Speaker 2>to say emitting a W minus.

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<v Speaker 1>We really do think about these things as a pair,

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<v Speaker 1>or the up on the top and the D on

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<v Speaker 1>the bottom, And the way we think about it from

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<v Speaker 1>a sort of theoretical point of view is that the

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<v Speaker 1>W is the way to go up or down. So

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<v Speaker 1>there's actually two w's, the W plus and the W minus.

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<v Speaker 1>If you want to go from the D to the U,

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<v Speaker 1>you emit a W minus. If you want to go

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<v Speaker 1>from the U to the D, you emit a W plus.

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<v Speaker 1>So these are sort of like stair steps in order

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<v Speaker 1>to go from one to the other. That's sort of

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<v Speaker 1>the same way around an atom. An electron can go

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<v Speaker 1>up and down energy levels, and to do so, it

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<v Speaker 1>either emits or absorbs a photon. These ws change the

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<v Speaker 1>state from a D to a U, and there is

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<v Speaker 1>a connection to the sort of underlying theoretical structure which

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<v Speaker 1>we usually represent using these things called groups, where you

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<v Speaker 1>can transform an object, but it stays within a little

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<v Speaker 1>pre defined set that's called a group, and so it's

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<v Speaker 1>deeply connected to the sort of group theory structure, which

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<v Speaker 1>I think we should dig into sometime on the podcast.

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<v Speaker 1>But the basic version is that the up is sort

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<v Speaker 1>of the higher state and the down is the lower state.

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<v Speaker 1>But you can move between them using these ws.

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<v Speaker 2>Okay, awesome, all right, I think I get that. Thank you.

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<v Speaker 2>So you can go from neutron to proton. But protons

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<v Speaker 2>don't decay into neutrons. Why do neutrons decay?

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<v Speaker 1>Yeah, great question. Why do neutrons decay and protons don't. Well,

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<v Speaker 1>neutrons have a higher mass than protons, and so when

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<v Speaker 1>a neutron decays, it gives off a little bit of

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<v Speaker 1>energy and turns into a proton. Why does a neutron

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<v Speaker 1>have a higher mass than a proton. Well, remember, the

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<v Speaker 1>mass of these guys comes from the bonds between the quarks.

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<v Speaker 1>It's not because the neutron is made of heavier stuff

0:11:31.640 --> 0:11:34.080
<v Speaker 1>than the protons. These up and down quarks have almost

0:11:34.200 --> 0:11:37.000
<v Speaker 1>no mass, basically zero compared to the mass of the

0:11:37.000 --> 0:11:39.640
<v Speaker 1>proton and the neutron. All of the mass of these

0:11:39.720 --> 0:11:43.120
<v Speaker 1>guys comes from the gluons, the arrangements of the particles,

0:11:43.320 --> 0:11:46.240
<v Speaker 1>and so the neutron state up down down is a

0:11:46.320 --> 0:11:49.880
<v Speaker 1>higher energy configuration than the up, up down proton state,

0:11:50.280 --> 0:11:52.360
<v Speaker 1>and so it's just like a higher energy level the

0:11:52.400 --> 0:11:54.320
<v Speaker 1>way like around an atom. You know, there's like the

0:11:54.360 --> 0:11:57.000
<v Speaker 1>five two S state is a higher energy level than

0:11:57.040 --> 0:11:59.280
<v Speaker 1>like the two P or whatever. There's all these different

0:11:59.400 --> 0:12:01.480
<v Speaker 1>energy levels, and they have to do with the arrangements

0:12:01.480 --> 0:12:05.000
<v Speaker 1>between the particles, the configurations, and so the strong nuclear

0:12:05.000 --> 0:12:08.960
<v Speaker 1>force super duper complicated. But this neutron state, the UDD state,

0:12:09.360 --> 0:12:12.400
<v Speaker 1>is higher energy than the UUD and so it can

0:12:12.440 --> 0:12:14.640
<v Speaker 1>decay down. And that's what the universe does. It always

0:12:14.800 --> 0:12:18.040
<v Speaker 1>starts with massive particles which decay down into lighter particles.

0:12:18.480 --> 0:12:22.080
<v Speaker 1>The proton can't decay because there's nothing lighter than the proton.

0:12:22.800 --> 0:12:25.560
<v Speaker 1>Like you can't find a state that's lighter than the proton.

0:12:25.559 --> 0:12:27.920
<v Speaker 1>If you turned that other D into a U for example,

0:12:28.040 --> 0:12:31.120
<v Speaker 1>it actually would be a higher energy state than the proton.

0:12:31.520 --> 0:12:33.040
<v Speaker 1>So the proton is sort of like the bottom of

0:12:33.080 --> 0:12:35.800
<v Speaker 1>the ladder, the same way the electron is. The muon

0:12:35.880 --> 0:12:38.280
<v Speaker 1>can decay into an electron and other stuff. Why doesn't

0:12:38.320 --> 0:12:40.920
<v Speaker 1>the electron decay because there's nothing for it to decay into.

0:12:41.040 --> 0:12:44.040
<v Speaker 1>It's the lightest particle, and therefore it's stable. Now, we

0:12:44.080 --> 0:12:46.520
<v Speaker 1>don't know that the proton is actually stable, we've just

0:12:46.600 --> 0:12:49.680
<v Speaker 1>never seen it decay, and so we can estimate that

0:12:49.720 --> 0:12:52.720
<v Speaker 1>its lifetime is super duper long because we've watched a

0:12:52.760 --> 0:12:54.440
<v Speaker 1>bunch of protons for a long time to see if

0:12:54.440 --> 0:12:56.720
<v Speaker 1>any of them decay and never seen a single one decay,

0:12:56.720 --> 0:12:59.880
<v Speaker 1>which means either they're totally stable, like they live forever,

0:13:00.679 --> 0:13:02.960
<v Speaker 1>or they live for such a long time that we

0:13:03.040 --> 0:13:05.440
<v Speaker 1>just haven't seen one yet, and that lifetime would be

0:13:05.480 --> 0:13:08.200
<v Speaker 1>like billions and billions of years. So neutrons are super

0:13:08.200 --> 0:13:11.240
<v Speaker 1>fascinating because they actually do decay, so we can learn

0:13:11.280 --> 0:13:13.400
<v Speaker 1>something about what's going on inside them.

0:13:13.720 --> 0:13:16.120
<v Speaker 2>So, in the nucleus of an atom, you have the

0:13:16.120 --> 0:13:18.800
<v Speaker 2>same number of protons and neutrons, but the number of

0:13:18.800 --> 0:13:22.440
<v Speaker 2>protons isn't changing over time, but neutrons are decaying into protons.

0:13:22.920 --> 0:13:26.360
<v Speaker 2>What's gonna happen? Are we eventually not gonna have enough

0:13:26.360 --> 0:13:27.520
<v Speaker 2>neutrons for everything?

0:13:28.240 --> 0:13:30.840
<v Speaker 1>Yeah, this is really amazing because remember we were talking

0:13:30.880 --> 0:13:33.640
<v Speaker 1>about neutrons by themselves. A single neutron in the middle

0:13:33.679 --> 0:13:37.120
<v Speaker 1>of space will decay in about eleven to twelve minutes,

0:13:37.679 --> 0:13:40.120
<v Speaker 1>So you might be wondering, why isn't everything inside me?

0:13:40.160 --> 0:13:42.400
<v Speaker 1>Why aren't all my neutrons turning into protons? And then

0:13:42.480 --> 0:13:46.360
<v Speaker 1>like you know, everything's going haywire because the neutron is stable.

0:13:46.520 --> 0:13:49.440
<v Speaker 1>If it's inside the atom, it's unstable and will decay

0:13:49.440 --> 0:13:52.920
<v Speaker 1>into a proton when it's outside by itself, but inside

0:13:52.920 --> 0:13:55.439
<v Speaker 1>the atom, all of its other neutron and proton buddies

0:13:55.520 --> 0:13:59.000
<v Speaker 1>stabilize it. That's really weird, right, what's going on was

0:13:59.080 --> 0:14:02.360
<v Speaker 1>some really interesting stuff is happening there because when the

0:14:02.400 --> 0:14:05.400
<v Speaker 1>neutrons and the protons are together in the nucleus, they're

0:14:05.440 --> 0:14:08.359
<v Speaker 1>not just like packed in like tennis balls. They're interacting

0:14:08.360 --> 0:14:11.600
<v Speaker 1>with each other. Right, These things are quarks with gluons

0:14:11.600 --> 0:14:14.199
<v Speaker 1>holding them together, but they're not completely sealed off from

0:14:14.200 --> 0:14:16.679
<v Speaker 1>anything else. If you're like on one side of the gluon,

0:14:16.720 --> 0:14:18.280
<v Speaker 1>you might be closer to one of the quarks or

0:14:18.400 --> 0:14:20.680
<v Speaker 1>closer to one of the other quarks. So you can

0:14:20.720 --> 0:14:24.640
<v Speaker 1>actually feel the quarks inside the neutron if you're nearby it.

0:14:25.000 --> 0:14:26.600
<v Speaker 1>And so the atom is not just like a bunch

0:14:26.640 --> 0:14:29.680
<v Speaker 1>of tennis balls totally sealed off. They're interacting with each other.

0:14:29.880 --> 0:14:33.080
<v Speaker 1>There's this little residual strong force that's actually what holds

0:14:33.080 --> 0:14:34.080
<v Speaker 1>the nucleus together.

0:14:34.400 --> 0:14:36.480
<v Speaker 2>Friends help you hold everything together.

0:14:36.600 --> 0:14:40.360
<v Speaker 1>Yes, exactly, And so inside of the nucleus, neutrons can

0:14:40.400 --> 0:14:43.080
<v Speaker 1>live a long long time. Sometimes they can live forever.

0:14:43.600 --> 0:14:45.840
<v Speaker 1>Like take a carbon atom. Carbon has a bunch of

0:14:45.880 --> 0:14:49.480
<v Speaker 1>neutrons in the nuclei. Those neutrons will live forever. You

0:14:49.520 --> 0:14:51.120
<v Speaker 1>have a carbon atom, we think it could just sit

0:14:51.200 --> 0:14:54.600
<v Speaker 1>in space for a zillion zillion zillion years. Other elements

0:14:54.600 --> 0:14:57.600
<v Speaker 1>are not as stable, like uranium, for example, will break down,

0:14:58.000 --> 0:14:59.760
<v Speaker 1>and one of the ways it does is through these

0:14:59.800 --> 0:15:03.240
<v Speaker 1>kind of decays. And so neutrons can either crack open

0:15:03.280 --> 0:15:06.200
<v Speaker 1>your nucleus if they're not quite stable enough, or they

0:15:06.240 --> 0:15:09.080
<v Speaker 1>can help it stay together. Like the reason the nucleus

0:15:09.080 --> 0:15:11.640
<v Speaker 1>stays together all these protons which otherwise are pushing each

0:15:11.680 --> 0:15:14.320
<v Speaker 1>other apart, is because the neutrons are there in between

0:15:14.360 --> 0:15:16.840
<v Speaker 1>you to help stabilize it, to pull them together with

0:15:16.920 --> 0:15:19.080
<v Speaker 1>the strong force, and to keep the protons from pulling

0:15:19.160 --> 0:15:22.440
<v Speaker 1>themselves apart. So neutrons are really the glue that holds

0:15:22.440 --> 0:15:23.560
<v Speaker 1>the whole universe together.

0:15:23.680 --> 0:15:26.800
<v Speaker 2>I feel like you could write nerdy Hallmark cards.

0:15:28.520 --> 0:15:30.040
<v Speaker 1>I love you and your neutrons.

0:15:30.120 --> 0:15:36.280
<v Speaker 2>That's right. You hold me together, you're my proton, you

0:15:36.400 --> 0:15:38.560
<v Speaker 2>keep me from decay. That's right.

0:15:41.120 --> 0:15:44.000
<v Speaker 1>But there's also still a bunch of mysteries about the neutron,

0:15:44.080 --> 0:15:47.200
<v Speaker 1>Like we think we understand the basic story here, but

0:15:47.480 --> 0:15:50.440
<v Speaker 1>you know, particle physicist nerds always want to drill down

0:15:50.440 --> 0:15:52.320
<v Speaker 1>and said, do we really understand it. Let's make a

0:15:52.360 --> 0:15:55.200
<v Speaker 1>bunch of really precise measurements in different ways and see

0:15:55.200 --> 0:15:58.520
<v Speaker 1>if there's anything surprising. So there's this mystery right now

0:15:58.560 --> 0:16:01.520
<v Speaker 1>in exactly how long the neutron does live?

0:16:01.920 --> 0:16:03.480
<v Speaker 2>How do we ask that question?

0:16:03.720 --> 0:16:06.040
<v Speaker 1>So people came up with two very different ways to measure,

0:16:06.120 --> 0:16:09.080
<v Speaker 1>like how long does a neutron take to decay? There's

0:16:09.120 --> 0:16:12.120
<v Speaker 1>the bottle method and the beam method. And the bottle

0:16:12.160 --> 0:16:14.840
<v Speaker 1>method is pretty simple. It says, take a bunch of neutrons,

0:16:15.160 --> 0:16:17.560
<v Speaker 1>cool them down so they're not flying around everywhere, put

0:16:17.560 --> 0:16:20.360
<v Speaker 1>them in a bottle, and then just wait and see

0:16:20.360 --> 0:16:23.200
<v Speaker 1>how many you have, like you know, plot them over time.

0:16:23.840 --> 0:16:26.120
<v Speaker 1>The way we study radioactive decay or any kind of

0:16:26.240 --> 0:16:28.360
<v Speaker 1>random process is you start with a bunch of them

0:16:28.360 --> 0:16:29.680
<v Speaker 1>and you wait to see how long does it take

0:16:29.760 --> 0:16:32.720
<v Speaker 1>until you have half as many and that's the characteristic lifetime.

0:16:33.320 --> 0:16:35.000
<v Speaker 1>And so that's what they do, and they get a number.

0:16:35.040 --> 0:16:37.920
<v Speaker 1>It's like fourteen minutes and thirty nine seconds. It's the

0:16:38.000 --> 0:16:41.160
<v Speaker 1>characteristic lifetime of a neutron. This is a really cool

0:16:41.160 --> 0:16:44.440
<v Speaker 1>experiment they do in Los Alamos, New Mexico, actually my hometown,

0:16:45.120 --> 0:16:48.080
<v Speaker 1>and they have these ultra cold neutrons. They've chilled them

0:16:48.080 --> 0:16:51.520
<v Speaker 1>down to like milli kelvin inside this container they call

0:16:51.760 --> 0:16:54.800
<v Speaker 1>the bathtub. It's like one meter in diameter. They just

0:16:54.840 --> 0:16:57.080
<v Speaker 1>like fill it with neutrons and count them and then

0:16:57.160 --> 0:16:59.560
<v Speaker 1>wait to see what happens. And so they get their number.

0:16:59.640 --> 0:17:01.840
<v Speaker 1>And you know, these are serious dudes. They take it

0:17:01.920 --> 0:17:04.159
<v Speaker 1>very seriously. They've account for all sorts of uncertainty, they

0:17:04.160 --> 0:17:06.960
<v Speaker 1>have cross checks whatever. They're very confident in their number.

0:17:07.200 --> 0:17:10.400
<v Speaker 1>But there's another experiment, the beam experiment, and they don't

0:17:10.440 --> 0:17:11.359
<v Speaker 1>get the same answer.

0:17:11.640 --> 0:17:13.760
<v Speaker 2>What how much does it differ by the.

0:17:13.640 --> 0:17:16.919
<v Speaker 1>Beam experiment makes a neutron beam? And you know we

0:17:16.920 --> 0:17:19.359
<v Speaker 1>said that neutrons decay into protons, right, So they had

0:17:19.359 --> 0:17:22.000
<v Speaker 1>this clever idea like, oh, neutrons are actually really hard

0:17:22.000 --> 0:17:24.600
<v Speaker 1>to count. The other guys have this complicated, sophisticated equipment

0:17:24.640 --> 0:17:27.560
<v Speaker 1>to count neutrons. They're hard. Let's just count the protons.

0:17:27.600 --> 0:17:30.440
<v Speaker 1>If neutrons are decaying into protons, let's just count the protons.

0:17:30.640 --> 0:17:33.200
<v Speaker 1>And so they fly it through an electromagnetic field, filter

0:17:33.280 --> 0:17:36.040
<v Speaker 1>out the protons and count those and they get a

0:17:36.040 --> 0:17:39.600
<v Speaker 1>different answer. They get a slightly longer answer by nine seconds.

0:17:39.880 --> 0:17:42.280
<v Speaker 1>So instead of fourteen minutes and thirty nine seconds, they

0:17:42.280 --> 0:17:45.120
<v Speaker 1>get fourteen minutes and forty eight seconds. So they think

0:17:45.200 --> 0:17:47.960
<v Speaker 1>neutrons live a little bit longer than the bathtub.

0:17:48.080 --> 0:17:49.879
<v Speaker 2>Guys, but don't you have to at least know how

0:17:49.880 --> 0:17:53.240
<v Speaker 2>many neutrons you're starting with, because if you get ten protons,

0:17:53.840 --> 0:17:55.760
<v Speaker 2>but you don't know how many neutrons you started with,

0:17:55.960 --> 0:17:58.159
<v Speaker 2>how do you know the rate of decay?

0:17:58.440 --> 0:18:01.200
<v Speaker 1>Yeah, good question. They know how many neutrons they've started

0:18:01.200 --> 0:18:03.800
<v Speaker 1>with because they know how they produce the neutrons, Okay,

0:18:03.800 --> 0:18:06.000
<v Speaker 1>and so they think they've accounted for that. But you

0:18:06.040 --> 0:18:09.280
<v Speaker 1>know something is going on here, like it's the same process.

0:18:09.280 --> 0:18:11.880
<v Speaker 1>They should get the same answer. So either somebody's made

0:18:11.880 --> 0:18:15.760
<v Speaker 1>a subtle air totally possible, right, and they both work

0:18:15.880 --> 0:18:19.400
<v Speaker 1>really really hard to reduce these uncertainties. Often in this scenario,

0:18:19.440 --> 0:18:21.960
<v Speaker 1>you get two experiments. They get different measurements, but they

0:18:22.000 --> 0:18:24.119
<v Speaker 1>both have large uncertainties and they overlap, and then they

0:18:24.160 --> 0:18:27.040
<v Speaker 1>both work really really hard to refine their experiments, and

0:18:27.119 --> 0:18:30.560
<v Speaker 1>usually as the uncertainty shrink, the results converge into one answer.

0:18:30.560 --> 0:18:33.920
<v Speaker 1>You're like, Okay, cool, the universe is coherent. But what's

0:18:33.920 --> 0:18:36.840
<v Speaker 1>happening here is that the uncertainties are shrinking, but the

0:18:36.880 --> 0:18:39.520
<v Speaker 1>answers are not getting closer together, so they're getting more

0:18:39.560 --> 0:18:43.360
<v Speaker 1>and more confident in their discrepancy, which means, hey, maybe

0:18:43.359 --> 0:18:46.840
<v Speaker 1>there's some new interesting physics. Maybe the neutron, like the

0:18:46.880 --> 0:18:50.320
<v Speaker 1>boring vanilla particle most people aren't excited about, is actually

0:18:50.320 --> 0:18:53.800
<v Speaker 1>the portal to discovering the nature of the universe. You

0:18:53.880 --> 0:18:58.240
<v Speaker 1>all are pros at Silver Linings, Well, this is really

0:18:58.280 --> 0:19:01.760
<v Speaker 1>fun idea that maybe neutrons don't just decay to protons.

0:19:02.080 --> 0:19:06.440
<v Speaker 1>Maybe sometimes neutrons decay into something else, like dark matter,

0:19:06.920 --> 0:19:09.520
<v Speaker 1>and so in the neutron beam, what's happening is these

0:19:09.560 --> 0:19:12.320
<v Speaker 1>neutrons are just disappearing into dark matter, and those guys

0:19:12.320 --> 0:19:14.919
<v Speaker 1>are not measuring it. So maybe the bathtub guys are

0:19:15.000 --> 0:19:18.000
<v Speaker 1>right because they're actually measuring the neutrons, whereas the guys

0:19:18.000 --> 0:19:20.600
<v Speaker 1>who are assuming they turn into protons. They're the ones

0:19:20.640 --> 0:19:24.240
<v Speaker 1>getting the wrong answer because it's not always going to protons.

0:19:24.240 --> 0:19:25.639
<v Speaker 1>Sometimes it's going to dark matter.

0:19:25.840 --> 0:19:28.280
<v Speaker 2>And we can't measure dark matter right.

0:19:28.240 --> 0:19:30.080
<v Speaker 1>We do not have ways to measure dark matter is

0:19:30.119 --> 0:19:32.400
<v Speaker 1>certainly not in these beams, and so this is really

0:19:32.400 --> 0:19:35.240
<v Speaker 1>interesting and really important because it could be an indication

0:19:35.359 --> 0:19:38.080
<v Speaker 1>of something that's happening. And it's also important because it

0:19:38.080 --> 0:19:40.960
<v Speaker 1>helps us understand the early universe. You know, in the

0:19:41.080 --> 0:19:43.840
<v Speaker 1>very early universe, we had like quarks and gluons flying

0:19:43.880 --> 0:19:47.920
<v Speaker 1>around and things cool down into hydrogen and briefly also

0:19:48.080 --> 0:19:52.000
<v Speaker 1>forming some helium. And that ratio of hydrogen helium is

0:19:52.040 --> 0:19:55.000
<v Speaker 1>super important because it tells us something about the density

0:19:55.040 --> 0:19:57.640
<v Speaker 1>of quarks at that time and what the early universe

0:19:57.760 --> 0:20:00.560
<v Speaker 1>was really like. And we need neutrons in order to

0:20:00.640 --> 0:20:03.000
<v Speaker 1>form helium, Like you can't form helium without neutrons. You

0:20:03.000 --> 0:20:05.800
<v Speaker 1>can just squeeze protons together. You have to have those

0:20:05.840 --> 0:20:08.840
<v Speaker 1>neutrons to facilitate. But if the neutrons decay a little

0:20:08.840 --> 0:20:12.440
<v Speaker 1>bit faster than they aren't around as long to make helium.

0:20:12.520 --> 0:20:15.040
<v Speaker 1>If neutrons decay slower, there are more of them to

0:20:15.280 --> 0:20:19.119
<v Speaker 1>stick around and make helium. More helium means smaller, longer

0:20:19.200 --> 0:20:21.960
<v Speaker 1>lasting stars, so it has this cascading effect on the

0:20:22.000 --> 0:20:27.320
<v Speaker 1>whole history of the universe. Super fascinating anyway, neutrons really amazing.

0:20:27.440 --> 0:20:30.479
<v Speaker 1>Thank you very much Scott for asking about this, and

0:20:30.560 --> 0:20:32.879
<v Speaker 1>I hope that we've answered all of your questions about

0:20:32.920 --> 0:20:36.720
<v Speaker 1>neutrons and inspired new ones. Let's hear what Scott has

0:20:36.760 --> 0:20:39.440
<v Speaker 1>to say about our story of neutrons.

0:20:40.480 --> 0:20:43.000
<v Speaker 3>Hi, Daniel and Kelly, thank you for the thoughtful answer.

0:20:43.720 --> 0:20:46.119
<v Speaker 3>It seems like the neutron has a pr problem and

0:20:46.320 --> 0:20:47.400
<v Speaker 3>I'm just not.

0:20:47.440 --> 0:20:49.080
<v Speaker 1>Okay with that state of affairs.

0:20:49.760 --> 0:20:52.960
<v Speaker 3>Neutrons do some very cool and rather important things and

0:20:53.000 --> 0:20:56.679
<v Speaker 3>the world really needs to know. As a follow up question,

0:20:56.960 --> 0:20:59.919
<v Speaker 3>if a free neutron decays in a matter of minutes,

0:21:00.400 --> 0:21:03.280
<v Speaker 3>does that imply that the study of neutron guts is

0:21:03.560 --> 0:21:08.000
<v Speaker 3>practically more difficult than the study of proton guts. Thanks

0:21:08.040 --> 0:21:09.399
<v Speaker 3>again for everything you guys do.

0:21:09.800 --> 0:21:13.280
<v Speaker 1>Great question. Well, we can study neutrons because there are

0:21:13.359 --> 0:21:16.000
<v Speaker 1>lots of them, but seeing them fall apart is actually

0:21:16.119 --> 0:21:19.320
<v Speaker 1>useful because it gives us something to measure, to predict,

0:21:19.400 --> 0:21:22.600
<v Speaker 1>to calculate. Protons, on the other hand, just sit there,

0:21:22.640 --> 0:21:24.439
<v Speaker 1>so we have to do some work to smash them

0:21:24.520 --> 0:21:27.280
<v Speaker 1>or poke them to learn anything. So neutrons are actually

0:21:27.320 --> 0:21:45.080
<v Speaker 1>being helpful, all right.

0:21:45.080 --> 0:21:46.720
<v Speaker 2>So I gotta tell you, I'm on the edge of

0:21:46.760 --> 0:21:49.280
<v Speaker 2>my seat trying to figure out what ties together all

0:21:49.320 --> 0:21:51.359
<v Speaker 2>of the three questions that we got today. It's still

0:21:51.400 --> 0:21:53.720
<v Speaker 2>not clear to me other than the fact that, like,

0:21:53.760 --> 0:21:55.879
<v Speaker 2>bananas are made of protons and neutrons.

0:21:55.960 --> 0:21:56.400
<v Speaker 1>Hmmmm?

0:21:57.080 --> 0:21:58.520
<v Speaker 2>Is that it was it that simple?

0:21:58.760 --> 0:22:00.439
<v Speaker 1>No more than that.

0:22:00.560 --> 0:22:03.280
<v Speaker 2>It's gotta be more than that, Okay, So our next

0:22:03.320 --> 0:22:07.439
<v Speaker 2>question is about bananas. Matt from Discord had this question.

0:22:08.080 --> 0:22:10.919
<v Speaker 4>Hi, Danielle Kelly, this is Matt from Indiana. I was

0:22:10.960 --> 0:22:13.800
<v Speaker 4>walking through the grocery store and notice there are all

0:22:13.840 --> 0:22:19.240
<v Speaker 4>sorts of varieties of peppers, red green, tiny, big yellow orange,

0:22:19.480 --> 0:22:24.199
<v Speaker 4>tons of apple varieties, red delicious, Granny Smith. And then

0:22:24.240 --> 0:22:28.159
<v Speaker 4>I got to the bananas, just bananas, plain bananas, no

0:22:28.280 --> 0:22:30.959
<v Speaker 4>matter where I go. And then I found out that

0:22:31.000 --> 0:22:35.200
<v Speaker 4>most bananas we eat are banana clones. So why banana

0:22:35.200 --> 0:22:37.879
<v Speaker 4>clones and not from seeds is what I'm curious of.

0:22:38.320 --> 0:22:40.560
<v Speaker 4>Thanks at advance, and thanks for giving me an excuse

0:22:40.600 --> 0:22:42.600
<v Speaker 4>to say bananas way too many times.

0:22:43.000 --> 0:22:46.080
<v Speaker 2>Oh man. So I was excited to have an opportunity

0:22:46.119 --> 0:22:50.280
<v Speaker 2>to read more about bananas. So let's start with banana reproduction.

0:22:51.119 --> 0:22:55.480
<v Speaker 2>Bananas can reproduce in two different ways. They reproduce sexually

0:22:55.520 --> 0:23:01.000
<v Speaker 2>by making seeds, and they reproduce asexually by producing suckers.

0:23:01.040 --> 0:23:02.920
<v Speaker 1>Hold on, wait, I have a question already. Okay, great,

0:23:02.920 --> 0:23:06.840
<v Speaker 1>First of all, bananas reproduce or banana trees reproduced, right,

0:23:06.880 --> 0:23:09.480
<v Speaker 1>because the bananas themselves are just part of the banana tree.

0:23:09.560 --> 0:23:11.439
<v Speaker 2>Right, Yeah, yeah, yes, you're right. You're right. I was

0:23:11.480 --> 0:23:14.159
<v Speaker 2>being lazy with my words, although I'm gonna call you

0:23:14.240 --> 0:23:17.520
<v Speaker 2>on it, because bananas aren't really trees. I think technically

0:23:17.520 --> 0:23:18.200
<v Speaker 2>they're curves.

0:23:18.720 --> 0:23:20.080
<v Speaker 1>Really, do you remember one of.

0:23:20.080 --> 0:23:22.280
<v Speaker 2>Our other episodes we were talking about the anatomy of

0:23:22.320 --> 0:23:25.879
<v Speaker 2>the tree and how it forms rings. Bananas are just

0:23:26.119 --> 0:23:29.359
<v Speaker 2>taxonomically distantly related. They don't form that way. They just

0:23:29.480 --> 0:23:33.119
<v Speaker 2>kind of have like a stalk that's really trunk and

0:23:33.240 --> 0:23:36.240
<v Speaker 2>tree like in the middle. But they're not like typical trees.

0:23:36.359 --> 0:23:38.600
<v Speaker 1>Well, all right, so banana trees are not trees. I've

0:23:38.600 --> 0:23:41.760
<v Speaker 1>already learned something. And what part of the plant is

0:23:41.800 --> 0:23:44.679
<v Speaker 1>the banana? Is it fruit the way an apple? Is

0:23:44.760 --> 0:23:47.960
<v Speaker 1>this just something else weird? I remember strawberries or something

0:23:48.000 --> 0:23:50.320
<v Speaker 1>totally different. Which part of the plant are we actually

0:23:50.359 --> 0:23:50.760
<v Speaker 1>snacking on?

0:23:51.000 --> 0:23:51.720
<v Speaker 2>It is the fruit?

0:23:51.920 --> 0:23:52.160
<v Speaker 1>Okay?

0:23:52.200 --> 0:23:54.400
<v Speaker 2>Yeah, yeah, what do you mean by strawberries aren't really

0:23:54.400 --> 0:23:55.560
<v Speaker 2>the fruit? I'm confused.

0:23:55.640 --> 0:23:58.119
<v Speaker 1>Didn't we do an episode where like strawberries are actually

0:23:58.160 --> 0:24:00.080
<v Speaker 1>the seed or something? I don't remember I remember, I

0:24:00.080 --> 0:24:01.280
<v Speaker 1>mean something surprising about.

0:24:01.040 --> 0:24:03.960
<v Speaker 2>Strawberry Strawberry seeds are on the outside, which is atypical.

0:24:04.000 --> 0:24:06.119
<v Speaker 2>But was that the whole fact?

0:24:06.800 --> 0:24:09.360
<v Speaker 1>Anymore? Biology doesn't stay in my head as long as

0:24:09.359 --> 0:24:09.880
<v Speaker 1>physics stock.

0:24:10.000 --> 0:24:13.080
<v Speaker 2>No, busted, Let's get away from this.

0:24:13.200 --> 0:24:15.360
<v Speaker 1>So back to bananas. Bananas are the fruit, but they're

0:24:15.400 --> 0:24:18.000
<v Speaker 1>not technically growing on trees, because I thought fruit had

0:24:18.040 --> 0:24:18.720
<v Speaker 1>to grow on trees.

0:24:18.880 --> 0:24:20.800
<v Speaker 2>No, I mean like strawberries aren't growing on trees.

0:24:21.000 --> 0:24:22.879
<v Speaker 1>Hmmm, all right, cool.

0:24:22.640 --> 0:24:24.919
<v Speaker 2>Although I guess maybe we're not quite sure if strawberries

0:24:24.960 --> 0:24:26.760
<v Speaker 2>are fruits. We're all confused today.

0:24:26.920 --> 0:24:29.320
<v Speaker 1>I'm not sure. It doesn't mean people aren't show Okay,

0:24:29.359 --> 0:24:30.879
<v Speaker 1>got it, I got it. I'm far for an expert.

0:24:30.880 --> 0:24:34.359
<v Speaker 1>All right, So bananas can reproduce sexually or asexually.

0:24:34.359 --> 0:24:36.600
<v Speaker 2>You were telling us yes, And so what happens with

0:24:36.640 --> 0:24:39.680
<v Speaker 2>the asexual reproduction is that the giant stalk that looks

0:24:39.720 --> 0:24:42.840
<v Speaker 2>like a trunk at the bottom underground. In addition to

0:24:42.880 --> 0:24:46.080
<v Speaker 2>its roots, it's producing what are called suckers. And these

0:24:46.119 --> 0:24:48.840
<v Speaker 2>suckers come out from the mother plant and pop up

0:24:48.880 --> 0:24:52.320
<v Speaker 2>along the sides, and they are essentially just clones of

0:24:52.359 --> 0:24:54.320
<v Speaker 2>the mom and they'll stay connected for a while, but

0:24:54.359 --> 0:24:58.679
<v Speaker 2>you can cut them off, move them somewhere else, and

0:24:58.720 --> 0:25:00.000
<v Speaker 2>now you've got a new banana plance.

0:25:00.480 --> 0:25:02.879
<v Speaker 1>And why do biologists call them suckers? I mean that

0:25:02.920 --> 0:25:05.640
<v Speaker 1>makes me think of the things on an octopus's tentacle.

0:25:06.080 --> 0:25:08.480
<v Speaker 1>Are these like an octopus tentacles sticking out through the

0:25:08.480 --> 0:25:10.520
<v Speaker 1>ground or what's going on here? Do they suck in

0:25:10.520 --> 0:25:10.920
<v Speaker 1>some way?

0:25:11.160 --> 0:25:12.960
<v Speaker 2>I don't know the history, but it's just a much

0:25:13.200 --> 0:25:15.119
<v Speaker 2>more fun name than any of you guys would have

0:25:15.119 --> 0:25:17.880
<v Speaker 2>come up with. I'm kidding. Glue ones is a great name.

0:25:18.560 --> 0:25:20.440
<v Speaker 1>I wish we had called some particle the suckers. That

0:25:20.440 --> 0:25:21.320
<v Speaker 1>would have been really fun.

0:25:21.440 --> 0:25:23.680
<v Speaker 2>You might discover a new particle, and I think that's

0:25:23.680 --> 0:25:24.600
<v Speaker 2>what you should name it.

0:25:24.600 --> 0:25:27.280
<v Speaker 1>In the suckers beam, that's right. So they can basically

0:25:27.280 --> 0:25:31.040
<v Speaker 1>clone themselves, make mini versions, or they can actually get

0:25:31.040 --> 0:25:32.800
<v Speaker 1>it on with their neighbors.

0:25:32.480 --> 0:25:36.080
<v Speaker 2>That's right. And there's something like a thousand species of

0:25:36.200 --> 0:25:39.560
<v Speaker 2>plant that could be called banana plants. Oh, so it's

0:25:39.560 --> 0:25:43.080
<v Speaker 2>a lot of diversity. But at some point in the past,

0:25:43.119 --> 0:25:45.639
<v Speaker 2>so like bananas don't fossilize, so it's hard to know

0:25:45.680 --> 0:25:50.040
<v Speaker 2>exactly when humans started eating bananas, but way before written

0:25:50.080 --> 0:25:53.160
<v Speaker 2>records were a thing for our species. What we think

0:25:53.200 --> 0:25:56.439
<v Speaker 2>happened was that a banana plant had a mutation and

0:25:56.480 --> 0:25:59.479
<v Speaker 2>it didn't produce seeds. And you would know if your

0:25:59.520 --> 0:26:02.719
<v Speaker 2>banana had seeds in it because the seeds produced by

0:26:02.760 --> 0:26:05.240
<v Speaker 2>lots of banana plants are big and hard, and it

0:26:05.240 --> 0:26:07.760
<v Speaker 2>would be very unpleasant to eat a banana with seeds

0:26:07.800 --> 0:26:11.000
<v Speaker 2>in it. And so bananas don't have seeds. And some

0:26:11.400 --> 0:26:14.160
<v Speaker 2>human must have found this tree and they were like, oh,

0:26:14.200 --> 0:26:16.600
<v Speaker 2>this is solid. There's nothing that cracks my teeth in

0:26:16.640 --> 0:26:19.800
<v Speaker 2>this plant, and so they took the suckers and that

0:26:19.840 --> 0:26:20.760
<v Speaker 2>got propagated.

0:26:20.920 --> 0:26:23.200
<v Speaker 1>But this is like prehistory because we don't have records

0:26:23.240 --> 0:26:25.760
<v Speaker 1>of it. We don't know when this happened, that's right, Yeah,

0:26:25.800 --> 0:26:27.760
<v Speaker 1>So could it also have been the product of like

0:26:28.119 --> 0:26:31.080
<v Speaker 1>human breeding. We found like a plant with smaller seeds

0:26:31.080 --> 0:26:33.240
<v Speaker 1>and another one that crossbred them and pushed them in

0:26:33.280 --> 0:26:35.400
<v Speaker 1>that direction. Or do you think it's more likely it's

0:26:35.400 --> 0:26:36.760
<v Speaker 1>just like one random mutation.

0:26:37.119 --> 0:26:41.120
<v Speaker 2>Artificial selection could have helped it along. I believe our

0:26:41.240 --> 0:26:46.000
<v Speaker 2>understanding is that this happened before humans really had enough

0:26:46.000 --> 0:26:50.160
<v Speaker 2>of an understanding to engage an artificial selection on purpose.

0:26:50.400 --> 0:26:50.720
<v Speaker 1>Wow.

0:26:50.880 --> 0:26:53.600
<v Speaker 2>But it certainly could have been the case that Joe

0:26:53.680 --> 0:26:56.239
<v Speaker 2>had a plant that had two seeds in it and

0:26:56.280 --> 0:26:58.360
<v Speaker 2>Sally had a plant that only had one, and everybody

0:26:58.359 --> 0:27:01.080
<v Speaker 2>wanted the suckers from Sally's plant. That's way better, and

0:27:01.200 --> 0:27:03.560
<v Speaker 2>over time that process could have played out. But I

0:27:03.560 --> 0:27:05.800
<v Speaker 2>don't think it was purposeful initially.

0:27:06.000 --> 0:27:09.000
<v Speaker 1>And so that was the last sexual reproduction of these

0:27:09.040 --> 0:27:12.000
<v Speaker 1>bananas that were eating in every reproduction of banana trees

0:27:12.080 --> 0:27:14.280
<v Speaker 1>since that moment has been asexual.

0:27:14.480 --> 0:27:16.879
<v Speaker 2>So my understanding is that there have been strains that

0:27:16.920 --> 0:27:19.560
<v Speaker 2>have arisen through this process. So it didn't necessarily happen

0:27:19.640 --> 0:27:21.960
<v Speaker 2>just once. It could have happened in like five different

0:27:22.000 --> 0:27:24.880
<v Speaker 2>banana trees in different areas, and now you've got these

0:27:24.920 --> 0:27:28.240
<v Speaker 2>different clonal lineages. But there's still all of those wild

0:27:28.320 --> 0:27:30.520
<v Speaker 2>banana species out there that are still producing seeds.

0:27:30.720 --> 0:27:31.120
<v Speaker 1>I see.

0:27:31.160 --> 0:27:34.359
<v Speaker 2>Okay, So around the nineteen hundreds, there was a strain

0:27:34.440 --> 0:27:38.680
<v Speaker 2>of bananas called the gro Michelle, which means big mic.

0:27:39.640 --> 0:27:41.800
<v Speaker 1>It sounds so much fancier inference.

0:27:42.040 --> 0:27:44.760
<v Speaker 2>It does. But the big mic was everywhere, and I'm

0:27:44.800 --> 0:27:47.200
<v Speaker 2>gonna bum everybody out, which is exactly what everybody expects

0:27:47.240 --> 0:27:51.520
<v Speaker 2>from me. Apparently the grow michelle bananas tasted better than

0:27:51.560 --> 0:27:52.760
<v Speaker 2>the bananas we have now.

0:27:52.960 --> 0:27:53.320
<v Speaker 1>Whoa.

0:27:53.880 --> 0:27:57.320
<v Speaker 2>But they were all clones, and so these were being

0:27:57.320 --> 0:27:59.520
<v Speaker 2>grown all over the world. Bananas were getting huge, They're

0:27:59.520 --> 0:28:02.360
<v Speaker 2>being shipped all over the world, and a fungal infection

0:28:02.520 --> 0:28:06.640
<v Speaker 2>broke out, and because all of the gro michells were clones,

0:28:06.760 --> 0:28:11.040
<v Speaker 2>they were all susceptible and it decimated the bananas around

0:28:11.080 --> 0:28:16.480
<v Speaker 2>the world. Socker, blue Blue, We're sorry, French speakers.

0:28:17.160 --> 0:28:19.960
<v Speaker 1>Wait, do you know what the kro Michelle tasted like?

0:28:20.200 --> 0:28:22.479
<v Speaker 1>Do we have like written records or living people who

0:28:22.520 --> 0:28:24.600
<v Speaker 1>have eaten them who can tell us about this banana

0:28:24.720 --> 0:28:25.880
<v Speaker 1>that none of us will ever eat.

0:28:26.080 --> 0:28:28.919
<v Speaker 2>There probably are some people still alive who have eaten it.

0:28:29.000 --> 0:28:31.760
<v Speaker 2>I think it was just a sweeter tasting banana than

0:28:31.800 --> 0:28:32.520
<v Speaker 2>what we have now.

0:28:32.600 --> 0:28:34.960
<v Speaker 1>I know, the lost bananas, I know.

0:28:35.119 --> 0:28:37.320
<v Speaker 2>My gosh, it is said, it is said.

0:28:37.720 --> 0:28:39.680
<v Speaker 1>Is there somebody out there who's like going to de

0:28:39.800 --> 0:28:42.720
<v Speaker 1>extinctify the Groa michelle. That sounds like a billion dollar

0:28:42.760 --> 0:28:43.520
<v Speaker 1>idea right there.

0:28:43.720 --> 0:28:46.880
<v Speaker 2>Yeah, so there might be someone who's still maintaining the

0:28:46.960 --> 0:28:51.080
<v Speaker 2>suckers from the Groa michelle in some lab somewhere, but

0:28:51.160 --> 0:28:54.560
<v Speaker 2>it remains susceptible to Panama disease, which is what we

0:28:54.600 --> 0:28:57.040
<v Speaker 2>call this fungal disease that wiped out the bananas. So

0:28:57.080 --> 0:29:00.640
<v Speaker 2>somebody maybe could bring it back. But when the Gromychelle declined,

0:29:00.880 --> 0:29:05.000
<v Speaker 2>the Cavendish arose, and the Cavendish must have just been

0:29:05.080 --> 0:29:08.080
<v Speaker 2>a slightly different strain that happened to be resistant to

0:29:08.440 --> 0:29:12.520
<v Speaker 2>the dominant fungal strain at the time, and so Cavendish.

0:29:12.560 --> 0:29:15.560
<v Speaker 2>If you live in North America, this is the banana

0:29:15.600 --> 0:29:17.640
<v Speaker 2>that you find on your grocery shelf. So if you

0:29:17.640 --> 0:29:19.880
<v Speaker 2>go to Harris Teeter or you go to Target, or

0:29:19.920 --> 0:29:22.200
<v Speaker 2>you go to Kroger, or you go to Trader Joe's

0:29:22.280 --> 0:29:25.880
<v Speaker 2>or Whole Foods, those are all the same banana genotypes.

0:29:26.040 --> 0:29:27.440
<v Speaker 2>They're clones everywhere you go.

0:29:27.680 --> 0:29:29.760
<v Speaker 1>They all have the same DNA you're saying.

0:29:29.640 --> 0:29:31.600
<v Speaker 2>They all have the same code in their DNA. There

0:29:31.640 --> 0:29:34.600
<v Speaker 2>could be a couple mutations, but they are very similar.

0:29:34.680 --> 0:29:34.920
<v Speaker 1>Wow.

0:29:35.000 --> 0:29:38.000
<v Speaker 2>Amazing In countries like Africa and India, they have a

0:29:38.040 --> 0:29:41.800
<v Speaker 2>greater appreciation for other banana varieties. So there are other

0:29:41.840 --> 0:29:43.800
<v Speaker 2>parts of the world where you can get other kinds

0:29:43.840 --> 0:29:45.560
<v Speaker 2>of bananas, but in the US we get this one.

0:29:45.680 --> 0:29:48.000
<v Speaker 1>I've traveled in Mexico and the grocery store is there.

0:29:48.000 --> 0:29:50.080
<v Speaker 1>They have lots of different kinds of bananas there, like

0:29:50.320 --> 0:29:53.720
<v Speaker 1>little dark red bananas that taste a little bit like strawberries. Whoa,

0:29:53.960 --> 0:29:56.200
<v Speaker 1>you know, big fat bananas, and all sorts of stuff.

0:29:56.200 --> 0:29:56.800
<v Speaker 1>It's a lot of fun.

0:29:56.960 --> 0:30:00.720
<v Speaker 2>Yeah, And plantains are fairly popular in the and I

0:30:00.720 --> 0:30:03.560
<v Speaker 2>think that's another strain where there were no seeds that

0:30:03.600 --> 0:30:05.760
<v Speaker 2>were made and then that got propagated by suckers. But

0:30:05.840 --> 0:30:10.720
<v Speaker 2>in the nineteen nineties, bad news. Oh no, the Cavendish

0:30:11.120 --> 0:30:15.880
<v Speaker 2>gets affected by Panama disease. So this fungal disease has

0:30:15.920 --> 0:30:19.280
<v Speaker 2>continued to evolve while the Cavendish is staying still in

0:30:19.320 --> 0:30:21.800
<v Speaker 2>this evolutionary arms race, because it's just a clone that

0:30:21.840 --> 0:30:24.440
<v Speaker 2>we propagate over and over and over again. And there's

0:30:24.520 --> 0:30:27.680
<v Speaker 2>now a strain of Panama disease that is going after

0:30:28.280 --> 0:30:29.640
<v Speaker 2>the Cavendish bananas.

0:30:29.880 --> 0:30:31.200
<v Speaker 1>Why do they hate us so much?

0:30:31.400 --> 0:30:35.440
<v Speaker 2>I know, I know, fungus is the worst, except.

0:30:35.160 --> 0:30:37.920
<v Speaker 1>When it's helping us make beer and bread and al sorts.

0:30:37.720 --> 0:30:39.120
<v Speaker 2>Of Rather you get me things, you know, I guess

0:30:39.120 --> 0:30:41.280
<v Speaker 2>whenever you say a blanket statement, you're a most always

0:30:41.280 --> 0:30:41.920
<v Speaker 2>going to be wrong.

0:30:42.120 --> 0:30:43.360
<v Speaker 1>Some of them are really fun guys.

0:30:43.360 --> 0:30:49.840
<v Speaker 2>Actually, no, dad jokes, dead poetry. Okay. So now we've

0:30:49.840 --> 0:30:53.200
<v Speaker 2>got Panama disease and it is spreading, and so there's

0:30:53.240 --> 0:30:56.520
<v Speaker 2>some people who will be concerned what happens if the

0:30:56.520 --> 0:30:59.960
<v Speaker 2>Cavendish declines? Do we have something waiting to replace it?

0:31:00.760 --> 0:31:04.240
<v Speaker 2>And the answer is no, no, no, what?

0:31:04.520 --> 0:31:07.800
<v Speaker 1>No? What are those people doing? Get on it? Food scientists.

0:31:07.920 --> 0:31:10.040
<v Speaker 2>There is a lot of money in bananas, so there's

0:31:10.040 --> 0:31:12.400
<v Speaker 2>a lot of people working on it. The first thing

0:31:12.520 --> 0:31:15.360
<v Speaker 2>that they're doing to try to slow the decline is

0:31:15.360 --> 0:31:19.160
<v Speaker 2>biocontrol efforts. So if you go to a major banana

0:31:19.200 --> 0:31:22.480
<v Speaker 2>plantation and you want to go amongst the trees, you

0:31:22.560 --> 0:31:25.280
<v Speaker 2>have to suit up in sterilized clothes, you have to

0:31:25.280 --> 0:31:28.520
<v Speaker 2>put on boots and then walk through a sterilizing solution,

0:31:28.880 --> 0:31:30.560
<v Speaker 2>and you have to do that every time you walk

0:31:30.600 --> 0:31:33.160
<v Speaker 2>from like one plot of bananas to another. Because the

0:31:33.200 --> 0:31:36.440
<v Speaker 2>way the fungus transmits is in the soil. So if

0:31:36.480 --> 0:31:39.120
<v Speaker 2>you get like dirt in your boots and then you

0:31:39.160 --> 0:31:41.080
<v Speaker 2>walk in another area, you can transmit that.

0:31:41.360 --> 0:31:41.840
<v Speaker 1>Wow.

0:31:41.920 --> 0:31:43.920
<v Speaker 2>So it's a pain in the rear end. And like

0:31:43.960 --> 0:31:46.160
<v Speaker 2>every truck that comes in and out has to get sprayed.

0:31:46.440 --> 0:31:48.960
<v Speaker 2>But if they do find a tree that's infected, they

0:31:48.960 --> 0:31:52.720
<v Speaker 2>have to dump fungicides into the soil, kill everything in

0:31:52.760 --> 0:31:55.480
<v Speaker 2>that area, cover it with urea, which I think just

0:31:55.520 --> 0:31:57.960
<v Speaker 2>also changes soil chemistry, making it more likely to kill

0:31:57.960 --> 0:32:00.600
<v Speaker 2>the fungus, cover it with the tarp so that birds

0:32:00.640 --> 0:32:03.240
<v Speaker 2>don't walk on it, and then bring the fungus somewhere else.

0:32:03.600 --> 0:32:06.720
<v Speaker 2>The next zone of plants also get like fungicides and

0:32:06.760 --> 0:32:10.520
<v Speaker 2>herbicides injected into the soil, and then the zone after

0:32:10.600 --> 0:32:13.720
<v Speaker 2>that you have to check, like every month, you have

0:32:13.800 --> 0:32:15.360
<v Speaker 2>to do like a survey to make sure none of

0:32:15.440 --> 0:32:17.400
<v Speaker 2>them have it. And so it's intense.

0:32:17.520 --> 0:32:20.280
<v Speaker 1>Apology is just so hard to control. It's always wriggling

0:32:20.320 --> 0:32:22.160
<v Speaker 1>and squirming out of our control.

0:32:22.520 --> 0:32:25.160
<v Speaker 2>Yes, well, man an invasive species. I feel like it's

0:32:25.200 --> 0:32:27.880
<v Speaker 2>such an interesting conversation about when do you just give up,

0:32:28.080 --> 0:32:30.920
<v Speaker 2>Like it's not worth trying to get starlings out of

0:32:30.960 --> 0:32:32.680
<v Speaker 2>the US anymore. They're not going anywhere.

0:32:32.680 --> 0:32:35.520
<v Speaker 1>They're here anyway, Well, what about bananas? Is there anything

0:32:35.520 --> 0:32:38.040
<v Speaker 1>else we can do? Like, can't we somehow protect our

0:32:38.040 --> 0:32:41.200
<v Speaker 1>bananas or cross them with other wild species or something?

0:32:41.320 --> 0:32:43.240
<v Speaker 2>Yeah, I can hear the panic building in your voice.

0:32:43.240 --> 0:32:45.080
<v Speaker 2>Don't worry. We have a couple options.

0:32:45.560 --> 0:32:46.600
<v Speaker 1>I like banana bread.

0:32:46.600 --> 0:32:49.240
<v Speaker 2>Okay, I know, me too, Me too. Zach makes a

0:32:49.240 --> 0:32:50.800
<v Speaker 2>good banana bread. I don't get in the kitchen, but

0:32:50.840 --> 0:32:54.000
<v Speaker 2>he does a great job. So genetic engineering is one solution,

0:32:54.120 --> 0:32:56.960
<v Speaker 2>and they have in fact added genes from other plants,

0:32:57.000 --> 0:33:01.959
<v Speaker 2>I think tomato to make the cavendish resist to Panama disease.

0:33:02.160 --> 0:33:05.720
<v Speaker 2>And this works, it is resistant. But in the European Union,

0:33:05.880 --> 0:33:08.520
<v Speaker 2>I believe, you're not allowed to sell genetically modified plants.

0:33:08.840 --> 0:33:10.440
<v Speaker 2>And in the United States there's a lot of people

0:33:10.440 --> 0:33:13.440
<v Speaker 2>who feel very squeamish about genetically modified plants, and so

0:33:13.520 --> 0:33:16.360
<v Speaker 2>the industry has decided that this can't be the solution.

0:33:16.760 --> 0:33:18.480
<v Speaker 2>It just would not be financially viable.

0:33:18.920 --> 0:33:21.800
<v Speaker 1>Wow, so he could save the bananas, but still it's

0:33:21.840 --> 0:33:22.840
<v Speaker 1>not good enough.

0:33:22.560 --> 0:33:24.240
<v Speaker 2>Not good enough, And so the last thing that they're

0:33:24.240 --> 0:33:28.440
<v Speaker 2>trying are breeding experiments. So apparently something like one in

0:33:28.520 --> 0:33:32.440
<v Speaker 2>ten thousand bananas will produce a seed. Sometimes it like

0:33:32.520 --> 0:33:35.680
<v Speaker 2>still slips through, so you can search bananas for that

0:33:35.840 --> 0:33:39.760
<v Speaker 2>seed and then cross the Cavendish with other species of

0:33:39.800 --> 0:33:43.360
<v Speaker 2>wild bananas, and so there are some efforts to cross breed.

0:33:43.800 --> 0:33:47.200
<v Speaker 2>But the problem is, like the Cavendish, it's actually an

0:33:47.200 --> 0:33:49.600
<v Speaker 2>absolute marble of a fruit. You know, it comes in

0:33:49.640 --> 0:33:53.200
<v Speaker 2>its own packaging that ripens over the course of a

0:33:53.200 --> 0:33:55.920
<v Speaker 2>week while it is in transit to you, so it

0:33:56.040 --> 0:34:00.480
<v Speaker 2>arrives to you mostly unbruised and now perfectly ready to eat.

0:34:01.160 --> 0:34:05.760
<v Speaker 2>And the various crosses that they've done have produced bananas

0:34:05.800 --> 0:34:07.440
<v Speaker 2>that are like, you know, maybe they're yellow, maybe they

0:34:07.480 --> 0:34:10.600
<v Speaker 2>still have a good you know, outer coating. But so

0:34:10.719 --> 0:34:13.040
<v Speaker 2>far they haven't been able to find anything that meets

0:34:13.080 --> 0:34:16.200
<v Speaker 2>all of their criteria and is delicious. I was reading

0:34:16.200 --> 0:34:20.080
<v Speaker 2>about one banana that looks like a Cavendish and tastes good,

0:34:20.440 --> 0:34:24.279
<v Speaker 2>but it's described as an acid banana, which doesn't sound delicious,

0:34:24.680 --> 0:34:26.600
<v Speaker 2>but it just doesn't taste like the Cavendish. And so

0:34:26.760 --> 0:34:29.200
<v Speaker 2>right now they haven't been able to find anything to

0:34:29.320 --> 0:34:31.719
<v Speaker 2>replace the Cavendish in what some people would say is

0:34:31.719 --> 0:34:35.440
<v Speaker 2>a more sort of natural method. So that's where we are.

0:34:35.480 --> 0:34:37.680
<v Speaker 2>Are we going to have a banana in one to

0:34:37.760 --> 0:34:39.680
<v Speaker 2>two decades. We'll have to wait and see.

0:34:39.800 --> 0:34:43.239
<v Speaker 1>Oh my gosh, our children or our grandchildren might never

0:34:43.360 --> 0:34:46.520
<v Speaker 1>know the tastes of bananas the way we don't know

0:34:46.600 --> 0:34:47.759
<v Speaker 1>the taste of the groamy shell.

0:34:48.040 --> 0:34:49.719
<v Speaker 2>I know it could be traged I mean, think of

0:34:49.719 --> 0:34:52.240
<v Speaker 2>how many babies had bananas as their very first food

0:34:52.320 --> 0:34:54.959
<v Speaker 2>or something like. It could be that my kid's first

0:34:54.960 --> 0:34:57.399
<v Speaker 2>foods were smushed up bananas. My memory is a sieve,

0:34:57.480 --> 0:34:59.080
<v Speaker 2>so I don't know exactly what I fed them the

0:34:59.080 --> 0:35:01.680
<v Speaker 2>first time, but a banana.

0:35:01.719 --> 0:35:05.200
<v Speaker 1>And you know, there's something else fascinating about bananas, which

0:35:05.239 --> 0:35:07.200
<v Speaker 1>is that they are radioactive.

0:35:07.440 --> 0:35:08.520
<v Speaker 2>Is that gonna be the connection?

0:35:09.200 --> 0:35:12.560
<v Speaker 1>Don't give it away, Kelly. Yeah, but yes, inside bananas

0:35:12.600 --> 0:35:16.520
<v Speaker 1>there's naturally occurring potassium forty, which is unstable, and the

0:35:16.600 --> 0:35:20.399
<v Speaker 1>neutrons inside potassium forty decay, And so if you are

0:35:20.400 --> 0:35:24.279
<v Speaker 1>hanging around a banana, it will emit high energy electrons

0:35:24.320 --> 0:35:28.520
<v Speaker 1>and anti neutrinos. Wow, which is technically a radiation.

0:35:28.280 --> 0:35:30.560
<v Speaker 2>Oh would we all be better off without bananas in

0:35:30.600 --> 0:35:31.200
<v Speaker 2>our life?

0:35:31.960 --> 0:35:34.680
<v Speaker 1>I don't know. Bananas contribute to the natural radiation background,

0:35:34.719 --> 0:35:37.520
<v Speaker 1>which I'm sure affects the mutation rate so it's made

0:35:37.560 --> 0:35:38.480
<v Speaker 1>all of us who we are.

0:35:38.640 --> 0:35:42.799
<v Speaker 2>Oh wow, Okay, on that deep dad poetry note. Let's

0:35:42.800 --> 0:35:46.359
<v Speaker 2>find out if Matt found this answer satisfactory. And we'd

0:35:46.360 --> 0:35:48.400
<v Speaker 2>also like to take this moment to thank Matt for

0:35:48.440 --> 0:35:51.600
<v Speaker 2>being an amazing moderator of our discord channel. And if

0:35:51.600 --> 0:35:53.840
<v Speaker 2>you want to join us on discord, go to Daniel

0:35:53.840 --> 0:35:57.879
<v Speaker 2>and Kelly dot org not dot com, although dot com

0:35:57.880 --> 0:35:59.759
<v Speaker 2>appears to be a dead link now because the other

0:36:00.040 --> 0:36:02.600
<v Speaker 2>duel and Kelly got married and their website is down.

0:36:03.280 --> 0:36:05.319
<v Speaker 1>Which means either the wedding went wonderfully and they don't

0:36:05.320 --> 0:36:08.200
<v Speaker 1>care about it anymore, or maybe something didn't go so well.

0:36:08.239 --> 0:36:09.640
<v Speaker 2>Oh man, I'm hoping for the former.

0:36:10.160 --> 0:36:12.680
<v Speaker 1>Yes, good luck Daniel Kelly. Yes, but please do join

0:36:12.760 --> 0:36:14.960
<v Speaker 1>us on the discord with lots of people are asking

0:36:15.080 --> 0:36:19.160
<v Speaker 1>questions and having conversations about science and pizza and all

0:36:19.200 --> 0:36:21.840
<v Speaker 1>sorts of crazy stuff. Go to Danielankelly dot org to

0:36:21.840 --> 0:36:23.040
<v Speaker 1>find the link to join.

0:36:23.000 --> 0:36:25.480
<v Speaker 2>The discord, and let's hear what Matt had to say.

0:36:25.840 --> 0:36:28.080
<v Speaker 4>That answer was beautiful. Thank you so much.

0:36:28.120 --> 0:36:30.319
<v Speaker 5>Now I know more about banana suckers than I've ever

0:36:30.400 --> 0:36:32.400
<v Speaker 5>wanted to know. And also thanks for giving me a

0:36:32.400 --> 0:36:34.879
<v Speaker 5>shout out on the discord for being an administrator there,

0:36:35.760 --> 0:36:38.239
<v Speaker 5>and we really do hope other people will join, just

0:36:38.239 --> 0:36:41.439
<v Speaker 5>like Daniel said, please join us. We'll answer any questions. Yeah,

0:36:41.840 --> 0:36:42.719
<v Speaker 5>have a wonderful day, guys.

0:36:42.760 --> 0:36:43.720
<v Speaker 2>Thanks.

0:37:00.000 --> 0:37:03.160
<v Speaker 1>All right, we're back and we are answering questions from listeners.

0:37:03.160 --> 0:37:06.440
<v Speaker 1>There's a special secret theme of today's podcast that's going

0:37:06.520 --> 0:37:08.680
<v Speaker 1>to tie all of these questions together. Let's see how

0:37:08.719 --> 0:37:10.479
<v Speaker 1>long it takes Kelly to figure it out?

0:37:10.600 --> 0:37:11.880
<v Speaker 2>How many lifetimes?

0:37:14.040 --> 0:37:16.600
<v Speaker 1>The next question is from Steve, who has a question

0:37:16.800 --> 0:37:20.680
<v Speaker 1>about the biggest gaseest planet in the Solar System.

0:37:20.280 --> 0:37:23.120
<v Speaker 2>That isn't Uranus. Sorry I had to.

0:37:25.640 --> 0:37:29.320
<v Speaker 6>Hi, Daniel and Kelly. This is Steve from BC Canada.

0:37:29.800 --> 0:37:33.400
<v Speaker 6>I have a controversial take here. Could it be said

0:37:33.520 --> 0:37:36.839
<v Speaker 6>that there is no such thing as a gas giant

0:37:37.120 --> 0:37:40.719
<v Speaker 6>because these planets have so much pressure that gas becomes liquefied.

0:37:41.000 --> 0:37:46.560
<v Speaker 6>So aren't they really liquid planets? Maybe liquid giants? Sure,

0:37:46.719 --> 0:37:50.400
<v Speaker 6>they are composed of liquid elements that are gaseous to

0:37:50.520 --> 0:37:55.160
<v Speaker 6>earthlings living in earthly pressures, but they are not earth

0:37:55.800 --> 0:37:59.239
<v Speaker 6>and they don't have earthly pressures, so we should be

0:37:59.239 --> 0:38:02.200
<v Speaker 6>calling them liquid giants. Don't you think? I think it's

0:38:02.520 --> 0:38:05.080
<v Speaker 6>about high time that we do a deep dive into

0:38:05.080 --> 0:38:09.080
<v Speaker 6>the inner workings of gas planets. What really are they?

0:38:09.680 --> 0:38:12.040
<v Speaker 1>All right? So Steve is asking a question about the

0:38:12.080 --> 0:38:14.239
<v Speaker 1>science of Jupiter, but also about the name of the

0:38:14.280 --> 0:38:18.399
<v Speaker 1>category that Jupiter finds itself in gas giants. Are they

0:38:18.440 --> 0:38:21.200
<v Speaker 1>really gassy? Should we be calling them liquid giants? These

0:38:21.200 --> 0:38:22.719
<v Speaker 1>are good questions, Steve.

0:38:22.560 --> 0:38:24.680
<v Speaker 2>These are great questions. Yeah, and you gotta tell Jupiter

0:38:24.719 --> 0:38:26.120
<v Speaker 2>and lay off the beans.

0:38:27.600 --> 0:38:30.920
<v Speaker 1>No, No, we're pro beans, even if it makes you gassy.

0:38:31.239 --> 0:38:33.640
<v Speaker 1>Katrina would tell me that beans makes everything better.

0:38:33.760 --> 0:38:36.680
<v Speaker 2>Nobody knows better than Katrina.

0:38:36.760 --> 0:38:39.319
<v Speaker 1>She certainly does. She certainly does, all right, So let's

0:38:39.320 --> 0:38:42.160
<v Speaker 1>dig into it. What in the end is Jupiter made

0:38:42.200 --> 0:38:45.120
<v Speaker 1>out of? Well, Jupiter, like Earth and the Sun, formed

0:38:45.160 --> 0:38:47.760
<v Speaker 1>from this big blob of stuff that the whole Solar

0:38:47.760 --> 0:38:49.840
<v Speaker 1>System was made out of. And you know, the Solar

0:38:49.840 --> 0:38:52.359
<v Speaker 1>system is mostly just the Sun. Like the Sun has

0:38:52.480 --> 0:38:54.719
<v Speaker 1>ninety nine points something percent of all the mass in

0:38:54.760 --> 0:38:58.160
<v Speaker 1>the Solar System. Basically, you have a much larger cloud

0:38:58.160 --> 0:39:01.200
<v Speaker 1>of stuff than our Solar system and others systems formed from.

0:39:01.520 --> 0:39:04.600
<v Speaker 1>But there was in there some seed, some gravitational over

0:39:04.680 --> 0:39:07.960
<v Speaker 1>density that pulled stuff together to form our Solar System,

0:39:08.320 --> 0:39:11.319
<v Speaker 1>and mostly that just collapsed into the center, and most

0:39:11.400 --> 0:39:13.800
<v Speaker 1>of it was hydrogen, because that's what the universe started

0:39:13.840 --> 0:39:16.000
<v Speaker 1>out at. As in fourteen billion years later, were still

0:39:16.000 --> 0:39:19.680
<v Speaker 1>mostly hydrogen, and so the Sun is mostly hydrogen. But

0:39:20.400 --> 0:39:23.120
<v Speaker 1>near the Sun there were also other little areas of

0:39:23.120 --> 0:39:26.359
<v Speaker 1>over density that managed to pull themselves together and hold

0:39:26.360 --> 0:39:30.000
<v Speaker 1>themselves together and resist the Sun's attraction, and that's how

0:39:30.000 --> 0:39:32.799
<v Speaker 1>the planets formed. So you get small rocky planets like

0:39:32.840 --> 0:39:35.200
<v Speaker 1>Earth and the Inner Solar System because the Sun then

0:39:35.280 --> 0:39:38.719
<v Speaker 1>blew away their atmospheres, but far enough out away from

0:39:38.719 --> 0:39:41.719
<v Speaker 1>the Sun, the Sun's radiation didn't blast away all the

0:39:41.760 --> 0:39:44.480
<v Speaker 1>helium and hydrogen, and there was ice out there. Things

0:39:44.520 --> 0:39:46.840
<v Speaker 1>were cold enough to form ice crystals, so you had

0:39:46.840 --> 0:39:49.040
<v Speaker 1>a little bit of an advantage to make bigger planets

0:39:49.080 --> 0:39:51.560
<v Speaker 1>that could grab a little bit more mass. So Jupiter

0:39:51.640 --> 0:39:54.880
<v Speaker 1>is just a scoop of the original protosolar system that

0:39:54.920 --> 0:39:56.160
<v Speaker 1>everything else is made out of.

0:39:56.680 --> 0:40:00.360
<v Speaker 2>So it's a better representation of the protosolar system than Earth.

0:40:00.520 --> 0:40:03.640
<v Speaker 1>Yeah, absolutely, Earth once had an atmosphere of hydrogen the

0:40:03.680 --> 0:40:05.839
<v Speaker 1>way that the Sun does and the way Jupiter does,

0:40:05.960 --> 0:40:08.759
<v Speaker 1>but it was blown away by the early Sun and

0:40:08.840 --> 0:40:10.759
<v Speaker 1>so the Earth is not a great representation of what

0:40:10.880 --> 0:40:12.560
<v Speaker 1>the Solar System is. And actually we're gonna do an

0:40:12.600 --> 0:40:15.280
<v Speaker 1>episode pretty soon about how we know what the universe

0:40:15.320 --> 0:40:16.359
<v Speaker 1>is made out of it And it was a big

0:40:16.400 --> 0:40:19.000
<v Speaker 1>shocker when we discovered that most of the universe is

0:40:19.040 --> 0:40:20.719
<v Speaker 1>not made of the same stuff as the Earth. The

0:40:20.719 --> 0:40:25.200
<v Speaker 1>Earth is an unusual helping of Solar System or universe material.

0:40:25.440 --> 0:40:28.640
<v Speaker 2>Thankfully for us, Yes, exactly, thanks early for us.

0:40:28.719 --> 0:40:31.520
<v Speaker 1>That's why we have bananas. No, that's not the secret theme.

0:40:32.200 --> 0:40:35.759
<v Speaker 1>So Jupiter is mostly hydrogen right by mass. The outside

0:40:35.880 --> 0:40:38.759
<v Speaker 1>is like seventy six percent hydrogen and then twenty four

0:40:38.800 --> 0:40:42.320
<v Speaker 1>percent helium and then just like trace tiny other stuff

0:40:42.400 --> 0:40:44.640
<v Speaker 1>like a little bit of carbon, a little bit oxygen,

0:40:44.680 --> 0:40:45.759
<v Speaker 1>and a little bit of salt for a little bit

0:40:45.800 --> 0:40:48.839
<v Speaker 1>of neon. But the atmosphere, which is just really an

0:40:48.880 --> 0:40:52.719
<v Speaker 1>artificial designation of like a certain layer within Jupiter, is

0:40:52.800 --> 0:40:54.759
<v Speaker 1>mostly hydrogen and helium.

0:40:54.920 --> 0:40:59.360
<v Speaker 2>What would be the arbitrary divider for Jupiter? I do

0:40:59.400 --> 0:41:01.640
<v Speaker 2>think of Jupiter is being just gas all the way through,

0:41:01.840 --> 0:41:03.920
<v Speaker 2>and maybe that's just because it's called a gas giant.

0:41:04.239 --> 0:41:08.480
<v Speaker 2>So what is the dividing line or dividing criteria for

0:41:08.600 --> 0:41:10.960
<v Speaker 2>the atmosphere versus the interior yees.

0:41:11.000 --> 0:41:13.400
<v Speaker 1>So it's a little bit arbitrary, but basically, you have

0:41:13.719 --> 0:41:16.239
<v Speaker 1>layers of stuff that get denser and denser as you

0:41:16.320 --> 0:41:19.040
<v Speaker 1>go in. So you start out the very outer layers

0:41:19.280 --> 0:41:22.440
<v Speaker 1>of Jupiter are cloud layers, and so these are like

0:41:22.520 --> 0:41:25.960
<v Speaker 1>ammonia crystals. There's really high winds, but it's mostly gaseous

0:41:26.040 --> 0:41:29.160
<v Speaker 1>hydrogen with these clouds of ammonia crystals. And that's what

0:41:29.200 --> 0:41:31.319
<v Speaker 1>you see when you look at Jupiter, you know, like

0:41:31.480 --> 0:41:34.080
<v Speaker 1>the rings and the red spot and all this stuff.

0:41:34.200 --> 0:41:37.799
<v Speaker 1>These are like weather patterns in those clouds in the

0:41:37.920 --> 0:41:41.719
<v Speaker 1>very very top layer of Jupiter's atmosphere. But then once

0:41:41.760 --> 0:41:46.160
<v Speaker 1>you penetrate through those layers of clouds, like fifty kilometers

0:41:46.160 --> 0:41:50.319
<v Speaker 1>of clouds or so, below that, there's liquid hydrogen, right,

0:41:50.360 --> 0:41:53.280
<v Speaker 1>And so hydrogen is an atom, but it also forms

0:41:53.520 --> 0:41:55.960
<v Speaker 1>H two, which is a molecule, and then it has

0:41:56.040 --> 0:41:58.680
<v Speaker 1>various phases and it depends on the temperature and depends

0:41:58.680 --> 0:42:01.640
<v Speaker 1>on the pressure. So you start out with gaseous hydrogen

0:42:01.920 --> 0:42:04.920
<v Speaker 1>and then you squeeze it down and you get liquid hydrogen.

0:42:04.920 --> 0:42:07.560
<v Speaker 1>And so this stuff flows, right, it's just denser, and

0:42:07.640 --> 0:42:09.560
<v Speaker 1>so you might say, all right, we're not really in

0:42:09.600 --> 0:42:12.799
<v Speaker 1>the atmosphere anymore, because now we have a liquid and

0:42:12.880 --> 0:42:14.960
<v Speaker 1>you know, here on Earth we consider the atmosphere of

0:42:14.960 --> 0:42:17.400
<v Speaker 1>the gaseous part, and then the surface is where you

0:42:17.440 --> 0:42:20.440
<v Speaker 1>have like solid rock and also liquid. But it's not

0:42:20.520 --> 0:42:24.080
<v Speaker 1>quite so simple on Jupiter because it's not as clear

0:42:24.160 --> 0:42:26.120
<v Speaker 1>and crisp like here on Earth. You know, you have

0:42:26.200 --> 0:42:28.040
<v Speaker 1>liquid and above it is gas, and like if you're

0:42:28.040 --> 0:42:30.040
<v Speaker 1>swimming in the ocean, you can very clearly tell the

0:42:30.120 --> 0:42:33.759
<v Speaker 1>crisp difference. But on Jupiter, they don't really have the

0:42:33.840 --> 0:42:37.160
<v Speaker 1>same distinct transition between liquid and gas, and so you

0:42:37.200 --> 0:42:42.239
<v Speaker 1>have this like gradual transition between gaseous hydrogen and liquid hydrogen.

0:42:42.480 --> 0:42:45.480
<v Speaker 1>What's really going on here is that molecular hydrogen, if

0:42:45.520 --> 0:42:48.960
<v Speaker 1>you look at its phase diagram, there are some pressures

0:42:48.960 --> 0:42:51.799
<v Speaker 1>and temperatures where it's gas and some pressures in temperatures

0:42:51.880 --> 0:42:55.200
<v Speaker 1>where it's liquid. But there's this critical point, this temperature

0:42:55.239 --> 0:42:58.080
<v Speaker 1>and pressure above which it's not really gas and not

0:42:58.200 --> 0:43:02.480
<v Speaker 1>really liquid, and this transition sort of therefore gradual. There's

0:43:02.520 --> 0:43:06.080
<v Speaker 1>this sort of super critical fluid. It's not really technically

0:43:06.160 --> 0:43:08.319
<v Speaker 1>a liquid, it's not really technically a gas that has

0:43:08.320 --> 0:43:11.120
<v Speaker 1>some similarity to both, And so the reason you can't

0:43:11.160 --> 0:43:13.560
<v Speaker 1>just say like, oh, this is the surface of Jupiter

0:43:13.719 --> 0:43:15.600
<v Speaker 1>is that as you descend, it just sort of gets

0:43:15.640 --> 0:43:19.000
<v Speaker 1>denser and denser till eventually it feels like liquid. And

0:43:19.040 --> 0:43:21.120
<v Speaker 1>if you rose back up, it would get less and

0:43:21.160 --> 0:43:22.800
<v Speaker 1>less dense, and then it would just sort of feel

0:43:22.880 --> 0:43:25.640
<v Speaker 1>like gas. But it's a gradual transition rather than an

0:43:25.680 --> 0:43:27.920
<v Speaker 1>abrupt one the way it is here on Earth.

0:43:28.120 --> 0:43:31.280
<v Speaker 2>I see we have yet again accidentally foraid into chemistry,

0:43:32.360 --> 0:43:33.680
<v Speaker 2>but I understand it better now.

0:43:33.920 --> 0:43:36.680
<v Speaker 1>And as you descend, the weather gets really really weird.

0:43:36.719 --> 0:43:40.560
<v Speaker 1>So you get this like helium neon rain. What. Yeah,

0:43:40.560 --> 0:43:42.520
<v Speaker 1>I know, it's really crazy and not something I think

0:43:42.560 --> 0:43:44.880
<v Speaker 1>you should dance and sing in, for example. But this

0:43:45.040 --> 0:43:47.680
<v Speaker 1>is sort of rain like droplets. And what's happening is

0:43:47.719 --> 0:43:50.520
<v Speaker 1>that you have helium and neon the and the upper atmosphere,

0:43:50.880 --> 0:43:53.040
<v Speaker 1>but they come together and form these drops, which then

0:43:53.160 --> 0:43:55.880
<v Speaker 1>sink and depleting the abundance of these elements in the

0:43:55.920 --> 0:43:58.880
<v Speaker 1>upper atmosphere, and they fall down to lower levels of

0:43:58.920 --> 0:44:01.920
<v Speaker 1>the atmosphere. And this is all very speculative. You know.

0:44:01.960 --> 0:44:04.080
<v Speaker 1>There are people who think, for example, like on Saturn,

0:44:04.360 --> 0:44:08.440
<v Speaker 1>there might be conditions that cause diamonds to rain, you know,

0:44:08.520 --> 0:44:11.360
<v Speaker 1>like formation of diamonds in the atmosphere because the intense

0:44:11.400 --> 0:44:14.000
<v Speaker 1>pressure which then fall below. But a lot of this

0:44:14.080 --> 0:44:16.720
<v Speaker 1>is speculative. This is like people running models and thinking

0:44:16.760 --> 0:44:19.239
<v Speaker 1>maybe this is what happens and it's super cool. But

0:44:19.640 --> 0:44:21.799
<v Speaker 1>you know, the big fixture story here is like, we

0:44:21.880 --> 0:44:24.480
<v Speaker 1>really don't understand this stuff. A lot of this is

0:44:24.520 --> 0:44:25.919
<v Speaker 1>just speculation.

0:44:25.600 --> 0:44:27.279
<v Speaker 2>Which is why we need more money to go out

0:44:27.280 --> 0:44:29.680
<v Speaker 2>there and find out definitely do.

0:44:29.880 --> 0:44:33.080
<v Speaker 1>And then things get even weirder as you squeeze it down.

0:44:33.120 --> 0:44:35.800
<v Speaker 1>As you go down further towards the center of Jupiter,

0:44:36.120 --> 0:44:38.799
<v Speaker 1>you're getting higher temperature and higher pressure. Then you reach

0:44:38.840 --> 0:44:42.440
<v Speaker 1>this region where the hydrogen is metallic, right, And metallic

0:44:42.520 --> 0:44:45.760
<v Speaker 1>is a really weird term to apply to hydrogen because

0:44:46.120 --> 0:44:49.080
<v Speaker 1>in astronomy usually they say, well you have helium and

0:44:49.120 --> 0:44:52.120
<v Speaker 1>you have hydrogen. Everything else they call them metal, right,

0:44:52.120 --> 0:44:54.400
<v Speaker 1>So if you talk about the metallicity of stars, it

0:44:54.440 --> 0:44:56.799
<v Speaker 1>means how much of the star is not hydrogen, how

0:44:56.880 --> 0:44:59.120
<v Speaker 1>much of it is not helium, everything else they call

0:44:59.160 --> 0:45:02.560
<v Speaker 1>a metal have a different meaning for what is a metal? Right.

0:45:02.560 --> 0:45:05.520
<v Speaker 1>They're thinking about things where the electrons are flowing because

0:45:05.520 --> 0:45:08.000
<v Speaker 1>the atoms are sort of linked together and the electrons

0:45:08.000 --> 0:45:11.040
<v Speaker 1>are not attached to individual atoms. And that's what we're

0:45:11.080 --> 0:45:13.640
<v Speaker 1>talking about here. This is like the chemical version of

0:45:13.680 --> 0:45:14.120
<v Speaker 1>a metal.

0:45:14.480 --> 0:45:16.560
<v Speaker 2>Does it mean that the atoms are flowing or we're

0:45:16.640 --> 0:45:17.800
<v Speaker 2>using the chemistry definition.

0:45:17.880 --> 0:45:20.400
<v Speaker 1>Now, yeah, we're using the chemistry definition. Because what happens

0:45:20.440 --> 0:45:23.840
<v Speaker 1>is you take those H two molecules, you squeeze them together,

0:45:24.320 --> 0:45:27.560
<v Speaker 1>and the hygen forms something like a lattice. Right, instead

0:45:27.560 --> 0:45:30.880
<v Speaker 1>of having individual H two molecules which have some interaction,

0:45:31.040 --> 0:45:33.520
<v Speaker 1>you know, because of the polarity of them, now you're

0:45:33.560 --> 0:45:36.640
<v Speaker 1>squeezing them together, so the electrons can just jump from

0:45:36.640 --> 0:45:39.160
<v Speaker 1>one hydrogen to another hydrogen to another one. It's like

0:45:39.200 --> 0:45:41.799
<v Speaker 1>a big crystal. It's not quite as tight, but it

0:45:41.840 --> 0:45:46.480
<v Speaker 1>conducts electricity. Right. Normally hydrogen does not conduct any electricity,

0:45:46.719 --> 0:45:48.759
<v Speaker 1>but you squeeze it together, you make it dense enough

0:45:49.040 --> 0:45:52.240
<v Speaker 1>it will conduct. And so it has this like bulk

0:45:52.360 --> 0:45:56.600
<v Speaker 1>lattice phase with delocalized electrons in it. And this is

0:45:56.600 --> 0:45:58.880
<v Speaker 1>something people have been thinking for decades and decades, and

0:45:58.920 --> 0:46:00.920
<v Speaker 1>only the last few years have they been able to

0:46:01.160 --> 0:46:04.520
<v Speaker 1>convincingly make this stuff in the lab by recreating these

0:46:04.600 --> 0:46:09.000
<v Speaker 1>conditions and seeing it actually conduct electricity. So this is

0:46:09.000 --> 0:46:12.680
<v Speaker 1>this huge chunk of Jupiter which is hydrogen squeeze so

0:46:12.760 --> 0:46:16.320
<v Speaker 1>tight that we think it's basically one enormous conductor.

0:46:16.600 --> 0:46:20.799
<v Speaker 2>So when you touch metallic hydrogen, is it hard like

0:46:20.840 --> 0:46:23.880
<v Speaker 2>the metals that I am thinking of, or are we

0:46:23.960 --> 0:46:26.680
<v Speaker 2>still in a sort of like gassy liquidy kind of phase.

0:46:26.840 --> 0:46:29.279
<v Speaker 1>Yeah, great question. Not something we understand super well. But

0:46:29.320 --> 0:46:31.520
<v Speaker 1>I don't recommend you lick it. If somebody has some

0:46:31.600 --> 0:46:33.799
<v Speaker 1>metallic hydrogen, it's hard to imagine what would be like

0:46:33.840 --> 0:46:36.120
<v Speaker 1>to touch it because you can't have it around unless

0:46:36.120 --> 0:46:38.520
<v Speaker 1>it's under very, very high pressure. So it's not like

0:46:38.560 --> 0:46:41.400
<v Speaker 1>somebody could hand you a chunk of metallic hydrogen that

0:46:41.480 --> 0:46:43.960
<v Speaker 1>you could like even consider licking. Okay, it's just going

0:46:44.040 --> 0:46:46.320
<v Speaker 1>to be like super duper dense material.

0:46:46.040 --> 0:46:48.160
<v Speaker 2>Got it, Okay, I don't want to die for this podcast.

0:46:48.320 --> 0:46:51.000
<v Speaker 1>Probably not tasty. I'd recommend a banana for a snack

0:46:51.080 --> 0:46:52.400
<v Speaker 1>instead of metallic hydrogen.

0:46:52.520 --> 0:46:54.239
<v Speaker 2>Wait, hold on, what is the connection then? Is the

0:46:54.239 --> 0:46:57.799
<v Speaker 2>connection that there's a part of Jupiter that's solid like

0:46:57.840 --> 0:47:01.520
<v Speaker 2>a banana and the equipment we used to study neutrons

0:47:01.520 --> 0:47:03.720
<v Speaker 2>as solid too, Daniel, I just don't know.

0:47:03.960 --> 0:47:07.239
<v Speaker 1>Well, Jupiter is active right the same way the Sun is.

0:47:07.280 --> 0:47:10.319
<v Speaker 1>It's a big hot thing and so it radiates. There's

0:47:10.320 --> 0:47:12.960
<v Speaker 1>no fusion going on inside Jupiter, but you know, the

0:47:13.000 --> 0:47:15.480
<v Speaker 1>pressure and the temperature are very high, and so there

0:47:15.520 --> 0:47:17.600
<v Speaker 1>is a lot of radiation being emitted. If you wanted to,

0:47:17.680 --> 0:47:20.440
<v Speaker 1>for example, establish a base on one of the moons

0:47:20.440 --> 0:47:23.480
<v Speaker 1>of Jupiter, you really have to worry about the Jupiter

0:47:23.560 --> 0:47:27.440
<v Speaker 1>win the Jovian winds, very high energy particles shooting at you.

0:47:27.840 --> 0:47:30.719
<v Speaker 1>So just like a banana and just like a neutron,

0:47:30.800 --> 0:47:33.120
<v Speaker 1>you have to worry about radiation if you're going to

0:47:33.200 --> 0:47:34.240
<v Speaker 1>live near any of these things.

0:47:34.360 --> 0:47:35.880
<v Speaker 2>Radiation is the theme.

0:47:37.520 --> 0:47:40.040
<v Speaker 1>It's a particle, of course, I'm not trying to be

0:47:40.080 --> 0:47:40.960
<v Speaker 1>tricky about it.

0:47:41.640 --> 0:47:44.040
<v Speaker 2>Well I got it before the end of the episode almost,

0:47:44.160 --> 0:47:45.640
<v Speaker 2>so bravo Kelly.

0:47:45.760 --> 0:47:48.360
<v Speaker 1>Congratulations. You get a banana. If I had a grow Michelle,

0:47:48.360 --> 0:47:49.080
<v Speaker 1>I would share it with you.

0:47:49.120 --> 0:47:49.640
<v Speaker 2>Oh, thank you.

0:47:49.840 --> 0:47:52.040
<v Speaker 1>So then we can dig down even deeper into Jupiter,

0:47:52.160 --> 0:47:55.120
<v Speaker 1>and eventually you get to stuff that's not hydrogen. So

0:47:55.120 --> 0:47:58.040
<v Speaker 1>we think there's a really thick atmosphere. Metallic hydrogen is

0:47:58.120 --> 0:48:00.200
<v Speaker 1>up to like maybe eighty percent of the radio is

0:48:00.440 --> 0:48:02.600
<v Speaker 1>if you go down to like thirty to fifty percent

0:48:02.640 --> 0:48:05.279
<v Speaker 1>of the radius of Jupiter. There is stuff down there

0:48:05.400 --> 0:48:07.919
<v Speaker 1>that's solid. It's like made of rock, the same kind

0:48:07.920 --> 0:48:09.759
<v Speaker 1>of stuff that the Earth is made out of. And

0:48:09.800 --> 0:48:12.680
<v Speaker 1>it's not small. It's like thirty to fifty percent of

0:48:12.719 --> 0:48:15.520
<v Speaker 1>the radius of Jupiter. It's a really big chunk of

0:48:15.600 --> 0:48:18.200
<v Speaker 1>ice and rock. But you know it's buried under an

0:48:18.280 --> 0:48:22.319
<v Speaker 1>incredibly thick layer of hydrogen. And so if you're really

0:48:22.360 --> 0:48:24.600
<v Speaker 1>hardcore about you could say, well, that's the surface because

0:48:24.600 --> 0:48:27.640
<v Speaker 1>everything else is a gas. It's hydrogen. But you know

0:48:27.719 --> 0:48:30.440
<v Speaker 1>it's not in a gas phase. It's in a metallic phase,

0:48:30.560 --> 0:48:34.080
<v Speaker 1>or it's in a super critical fluid phase. And so

0:48:34.280 --> 0:48:37.240
<v Speaker 1>you could, if you do really deep into Jupiter, stand

0:48:37.320 --> 0:48:40.120
<v Speaker 1>on a rocky quote unquote surface. But I don't think

0:48:40.160 --> 0:48:42.240
<v Speaker 1>you could still call Jupiter a rocky planet.

0:48:42.360 --> 0:48:44.200
<v Speaker 2>All right, yep, I'm giving it to the astronomers. I

0:48:44.200 --> 0:48:46.920
<v Speaker 2>think gas giant is a reasonable name, and also it

0:48:46.960 --> 0:48:49.960
<v Speaker 2>gives many school kids lots of chuckles, and so I

0:48:49.960 --> 0:48:50.600
<v Speaker 2>think it's great.

0:48:51.600 --> 0:48:54.120
<v Speaker 1>Yeah, but it is confusing, right because we call it

0:48:54.120 --> 0:48:56.239
<v Speaker 1>a gas giant because it's mostly made of hydrogen. But

0:48:56.320 --> 0:48:58.960
<v Speaker 1>hydrogen is not always in a gaseous state, and especially

0:48:59.040 --> 0:49:02.240
<v Speaker 1>in Jupiter. Most of the gas on Jupiter is metallic,

0:49:02.480 --> 0:49:04.520
<v Speaker 1>so you could also call it a metallic giant and

0:49:04.560 --> 0:49:05.480
<v Speaker 1>be like, kind.

0:49:05.280 --> 0:49:07.640
<v Speaker 2>Of correct, that does sound cooler.

0:49:08.080 --> 0:49:10.560
<v Speaker 1>It does sound more metal, right, that's right, that's right,

0:49:10.680 --> 0:49:13.439
<v Speaker 1>all right. So I think we've concluded that astronomy names

0:49:13.440 --> 0:49:15.480
<v Speaker 1>are very confusing and maybe there's no way to do

0:49:15.520 --> 0:49:18.440
<v Speaker 1>it right, but it's fun to dig into anyway. And

0:49:18.480 --> 0:49:21.120
<v Speaker 1>so Steve from BC let us know if we answered

0:49:21.160 --> 0:49:22.840
<v Speaker 1>your question about Jupiter.

0:49:23.360 --> 0:49:26.719
<v Speaker 7>Thanks Daniel and Kelly for answering my question. That was

0:49:26.840 --> 0:49:30.279
<v Speaker 7>really insightful to know that Jupiter could be really a

0:49:30.440 --> 0:49:34.200
<v Speaker 7>metal giant. But it makes me think now about how

0:49:34.239 --> 0:49:37.000
<v Speaker 7>we've named Earth. You know, Earth has a lot of

0:49:37.040 --> 0:49:39.400
<v Speaker 7>gas and we depend on that gas. And you know

0:49:39.760 --> 0:49:42.360
<v Speaker 7>how much different is the amount of gas and rock

0:49:42.520 --> 0:49:45.799
<v Speaker 7>ratio than Jupiter. I mean, would it be correct to

0:49:45.880 --> 0:49:49.719
<v Speaker 7>say that Earth is a gas midget? Thanks again for

0:49:49.800 --> 0:49:53.040
<v Speaker 7>answering my question. You're still my favorite podcast. Keep the

0:49:53.080 --> 0:49:56.239
<v Speaker 7>great answers coming, and thank you for being such great

0:49:56.239 --> 0:49:57.160
<v Speaker 7>signs communicators.

0:49:57.520 --> 0:49:59.480
<v Speaker 2>Well, thank you for all of the wonderful questions we

0:49:59.560 --> 0:50:01.880
<v Speaker 2>got today, and we hope to hear from you. Send

0:50:01.960 --> 0:50:05.840
<v Speaker 2>us your questions at Questions at Danielankelly dot org. We

0:50:05.920 --> 0:50:08.480
<v Speaker 2>answer every question, and some of the questions even end

0:50:08.600 --> 0:50:09.200
<v Speaker 2>up on the show.

0:50:09.400 --> 0:50:10.799
<v Speaker 1>We do love to hear from you, and we'd love

0:50:10.800 --> 0:50:13.120
<v Speaker 1>to hear that you are curious that you share our

0:50:13.160 --> 0:50:16.520
<v Speaker 1>passion to understand the universe how it works, from the

0:50:16.520 --> 0:50:19.839
<v Speaker 1>bananas all the way out to the galaxies. So join

0:50:19.920 --> 0:50:22.440
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0:50:22.520 --> 0:50:25.680
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0:50:32.600 --> 0:50:36.400
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0:50:53.960 --> 0:50:57.160
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