WEBVTT - Astronomy On Ice

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<v Speaker 1>Get in test with technology with text stuff from stuff

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<v Speaker 1>coming either everyone, and welcome to tech stuff. I'm Jonathan

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<v Speaker 1>Strickland and today's topic comes to us courtesy of a listener.

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<v Speaker 1>Actually I had blogged about this topic. It's the ice

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<v Speaker 1>cube neutrino telescope, and I wrote a little Twitter message about, Hey,

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<v Speaker 1>I got to write about this telescope that's buried a

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<v Speaker 1>mile beneath the ice, And immediately Nick on Twitter said

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<v Speaker 1>you should do a podcast about that, And I thought

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<v Speaker 1>I should do a podcast about that because I've already

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<v Speaker 1>done the research for that thing. That's why you got

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<v Speaker 1>this research out so quickly. Well, you know, repurposing. No, No,

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<v Speaker 1>it's actually here's the thing. Well one, it's buried under

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<v Speaker 1>the ice, so already it's super cool. But I'm sorry

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<v Speaker 1>it's already started. But I genuinely find this absolutely fascinating.

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<v Speaker 1>I mean, it's it's the world's largest neutrino detector, it's

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<v Speaker 1>buried a mile under the ice. It's this is something

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<v Speaker 1>that if you had told me was in a science

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<v Speaker 1>fiction story, I would have said, that's just silly, that's

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<v Speaker 1>a that's a lame bond villain's layer. Yeah, there's no

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<v Speaker 1>way that would really exist, and it totally exists. So

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<v Speaker 1>what is it looking for. It's looking for evidence of neutrinos,

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<v Speaker 1>which are these massless or nearly massless particles with no

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<v Speaker 1>electrical charge. And we'll talk more about them a little

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<v Speaker 1>bit later. Yeah, because specifically it's looking for for interactions

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<v Speaker 1>of neutrinos with stuff. But but well, yes, yeah, because

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<v Speaker 1>as it turns out, neutrinos are a little tricky. But

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<v Speaker 1>they It is at the South Pole, or really it's

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<v Speaker 1>underneath it. It's in Antarctica, and specifically, like I said,

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<v Speaker 1>it's about a mile beneath the surface of the ice,

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<v Speaker 1>between between one and two thousand meters or one to

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<v Speaker 1>one point five miles. Yeah, it's pretty incredible. That's and

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<v Speaker 1>it takes up about a cubic kilometer of ice, which

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<v Speaker 1>is about two thirds of a mile on each side.

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<v Speaker 1>So just imagine an area underneath the surface of the

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<v Speaker 1>ice and Antarctica that is this kilometer by a kilometer

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<v Speaker 1>by a kilometer in in in proportions, and that is

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<v Speaker 1>a telescope. And the reason why it's there is because well,

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<v Speaker 1>there's a couple of reasons. One is that the ice

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<v Speaker 1>provides a medium through which the neutrinos travel, and an

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<v Speaker 1>exceptionally clear medium at that the pressure of the ice

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<v Speaker 1>that deep has has pushed all the air bubbles out, right,

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<v Speaker 1>so it's incredibly clear. And also when you get to

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<v Speaker 1>be about a mile down below the surface, things get

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<v Speaker 1>a little dark, especially when sunlight isn't hitting you for

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<v Speaker 1>what seven or eight months out of the year, right, Right,

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<v Speaker 1>So it's already in a part of the world where, yeah,

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<v Speaker 1>for eight months of the or you have no sun

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<v Speaker 1>and it's a mile down and so it's really really dark.

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<v Speaker 1>The medium it's in is really clear. And both of

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<v Speaker 1>those things are incredibly important. So when was this thing

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<v Speaker 1>actually built? Well, it was proposed in yeah, but um,

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<v Speaker 1>it wasn't actually approved as a project until May first,

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<v Speaker 1>two thousand four. Right, They began building it in December

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<v Speaker 1>two thousand four. They started melting the holes they would

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<v Speaker 1>need to drill down to put the various censors that

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<v Speaker 1>are part of this telescope. Uh, they started drilling those

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<v Speaker 1>on on December one, two thousand four. The very last

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<v Speaker 1>censor was placed in a December, Yes, so six years

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<v Speaker 1>to do a complete telescope. Now they had already started

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<v Speaker 1>to gather information from the censors they had placed up

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<v Speaker 1>to that point, but it wasn't until they did that

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<v Speaker 1>last row in two thousand ten for it to be

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<v Speaker 1>a completed project. So pretty cool. And um, we cost

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<v Speaker 1>you know, a couple of bucks, right, easily two seventy

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<v Speaker 1>one million, as we would say in the old days

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<v Speaker 1>of tech stuff, a princely some most of that money

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<v Speaker 1>was provided by the National Science Foundation. They footed the

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<v Speaker 1>bill for a tune of two forty two million, and

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<v Speaker 1>the rest came from funders from all well, all around

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<v Speaker 1>the world. Really, so it's truly an international effort. It's

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<v Speaker 1>not something that is controlled by one entity. Uh. There's

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<v Speaker 1>a kind of a consortium called the ice Cube Collaboration

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<v Speaker 1>that sort of represents all the different parties involved. Right.

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<v Speaker 1>It has a total staff of about two hundred and

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<v Speaker 1>fifty people from forty one institutions in twelve countries overall. Um,

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<v Speaker 1>it's all led out of the University of Wisconsin Madison, right,

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<v Speaker 1>and some of the institutions that are part of this

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<v Speaker 1>include the University of Delaware. Uh. They designed some of

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<v Speaker 1>the key elements for the project, the Lawrence Berkeley National Lab,

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<v Speaker 1>Clark Atlanta University. Shout out to a low cool school. Hey,

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<v Speaker 1>how about my rival college, Georgia Tech. Uh I of

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<v Speaker 1>course went to the University of Georgia. Georgia Tech are

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<v Speaker 1>are hated enemies. They were part of this as well.

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<v Speaker 1>So we could actually we could literally go down the

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<v Speaker 1>street and probably find someone who works work on the project,

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<v Speaker 1>works on this project, which is kind of exciting. The

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<v Speaker 1>Neils Bore Institute. You might have heard of us talking

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<v Speaker 1>about that when we did our Heisenberg episode. There's also

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<v Speaker 1>Ohio State University, Pennsylvania State University, Stockholm University, University of Alberta, Edmonton,

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<v Speaker 1>University of Canterbury in New Zealand, and Oxford, so among

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<v Speaker 1>lots of others. So, I mean, it's a it's it's

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<v Speaker 1>a really big project and it's something that a lot

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<v Speaker 1>of people, you know, physicists and engineers and computer science

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<v Speaker 1>kids have been really excited to get in on exactly

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<v Speaker 1>and when you start looking into what this telescope does

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<v Speaker 1>and the hesitated used the word, but the scope of

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<v Speaker 1>the project, it's it's you know, it's understandable why people

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<v Speaker 1>are so eager to be part of it. Lauren is

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<v Speaker 1>judging me and grinning and shaking your head. Uh So,

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<v Speaker 1>let's talk about what it is they're looking for. Let's

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<v Speaker 1>talk about these neutrinos, these nearly massless particles. So there's

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<v Speaker 1>sub atomic particles, meaning that they're smaller than actual atoms.

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<v Speaker 1>And what's really interesting about them is is that they're

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<v Speaker 1>they're electrically neutral, yeah, which means that they aren't affected

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<v Speaker 1>by electro magnetic fields or forces exactly. They they So

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<v Speaker 1>if you were to have, say, a positively charged particle

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<v Speaker 1>and ion flying through space, and it happened to come

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<v Speaker 1>either close to another positively charged body, it would be

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<v Speaker 1>repulsed by that and its direction would change, or if

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<v Speaker 1>it came close to a negatively charged body, would be

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<v Speaker 1>attracted to that, and again its course would change, meaning

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<v Speaker 1>that there'd be no way for you to tell where

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<v Speaker 1>that particle originated from because they bounce around. Yeah, they

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<v Speaker 1>could have been moving all over the place. It would

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<v Speaker 1>look kind of like the old Family Circus cartoons where

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<v Speaker 1>Billy's pathway does the little dotted line over the entire neighborhood.

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<v Speaker 1>You just don't know where it came from. But neutrinos

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<v Speaker 1>don't have that charge, so they're not affected by positive

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<v Speaker 1>or negative charges. That won't change the pathway. So to

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<v Speaker 1>you know that they're traveling in a straight line, and

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<v Speaker 1>they're traveling extremely fast. Because they are massless or near massless,

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<v Speaker 1>they can travel right up nosing up to the to

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<v Speaker 1>the speed of light right now. Obviously, if they were

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<v Speaker 1>to travel to the speed of light, that would be

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<v Speaker 1>a problem. According to the theory of relativity, anything with

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<v Speaker 1>mass would require infinite energy to get to the speed

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<v Speaker 1>of light. So it's close but not quite the speed

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<v Speaker 1>of light. And uh, depending upon the medium, it can

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<v Speaker 1>actually travel faster than light within that media, not within

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<v Speaker 1>the vacuum of space, but within the medium of say,

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<v Speaker 1>I don't know ice. This will be important later on. Um.

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<v Speaker 1>But but back to the basics here. Okay, So, so

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<v Speaker 1>we think that they're the second most common particle in

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<v Speaker 1>the entire universe, the first being photons. Right, So the

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<v Speaker 1>fundamental unit of light is more there's more of that

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<v Speaker 1>than neutrinos. But that's the only thing out there besides

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<v Speaker 1>the stuff we can't identify, like dark matter, but we'll

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<v Speaker 1>get into that too, yes, um. And and there's there's

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<v Speaker 1>three basic types of neutrinos or um or flavors as

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<v Speaker 1>they are legitimately called in physics, right, which makes me

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<v Speaker 1>just so excited. So it's vanilla chocolate and rocky road.

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<v Speaker 1>Is that it U close electron, muon, and taw neutrinos alright,

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<v Speaker 1>So electrons, muans and taw are all negatively charged particles.

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<v Speaker 1>Electrons are subatomic particles, thank you. Uh they are the

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<v Speaker 1>electrons I would say are the most familiar to people.

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<v Speaker 1>Everyone who has taken basic science knows the electrons the

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<v Speaker 1>negatively charged particle that you find in atoms. They have

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<v Speaker 1>uh energy shells that they stay in and orbit around

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<v Speaker 1>a eight an atomic nucleus um. So you know those

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<v Speaker 1>were familiar with. Muans and taw are a little more exotic.

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<v Speaker 1>They are actually heavier than electrons, but they also have

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<v Speaker 1>a negative charge. Right, Mulons have about twice the mass

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<v Speaker 1>of electrons, and how have almost four times the massive electrons.

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<v Speaker 1>And now most of what we know about neutrinos really

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<v Speaker 1>only comes from research done in the past couple of decades.

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<v Speaker 1>But we will get to that. Yeah, well you've got

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<v Speaker 1>a whole timeline that was actually really fascinating to me too.

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<v Speaker 1>Once again, it's one of those examples how people way

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<v Speaker 1>smarter than I am are able to figure out things

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<v Speaker 1>about the universe without ever actually seeing any proof of it,

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<v Speaker 1>which is phenomenal with with answers to questions that we

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<v Speaker 1>have not even thought of. Yeah, I would just think

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<v Speaker 1>my equations must be wrong because things aren't equaling out.

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<v Speaker 1>These are people are saying, my equations can't be wrong.

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<v Speaker 1>So something's going on that I don't know about. I

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<v Speaker 1>need to invent a new particle to explain it exactly.

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<v Speaker 1>And it turned out it works. So where do they

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<v Speaker 1>come from? Well, from from a bunch of different places.

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<v Speaker 1>They can come from lots of cosmological events like um

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<v Speaker 1>like like supernova more or even the Sun. Okay, so

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<v Speaker 1>so you know weak stuff, right, this little low power

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<v Speaker 1>now obviously black holes, no big yeah, exactly, little stuff,

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<v Speaker 1>you know, just the things that can rip a galaxy apart. Yeah.

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<v Speaker 1>It turns out that neutrinos can be generated lots of

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<v Speaker 1>different ways. But the ones that we are particularly interested

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<v Speaker 1>in are these high energy neutrinos that would be so

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<v Speaker 1>high energy as to be it would be impossible for

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<v Speaker 1>them to have originated in our solar system, right, because

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<v Speaker 1>we can detect the neutrinos that come to us courtesy

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<v Speaker 1>of the Sun or the ones that are formed within

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<v Speaker 1>the Earth's atmosphere, but the more elusive ones are neutrinos

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<v Speaker 1>that might come from a cosmological event that happened on

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<v Speaker 1>the other side of the galaxy millions of years ago.

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<v Speaker 1>Well and and those those larger events create vastly more

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<v Speaker 1>neutrinos than say, the Sun would create on any given day.

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<v Speaker 1>But since the Sun is so much closer to us,

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<v Speaker 1>we're basically in and did with with neutrinos from the Sun,

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<v Speaker 1>Electron neutrinos specifically um as a byproduct of the nuclear

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<v Speaker 1>fusion that goes on in in the sun where uh

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<v Speaker 1>you know, if you if you hold up your hand

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<v Speaker 1>to sunlight, billions of neutrinos passed through it in a

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<v Speaker 1>single second. Yeah. Now, remember, because these are sub atomic

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<v Speaker 1>particles and they have no mass, these things, they're so

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<v Speaker 1>small and they're moving so quickly, they can pass right

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<v Speaker 1>through what would appear to be completely solid matter. Because

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<v Speaker 1>I don't know if you know this or not, solid

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<v Speaker 1>matter still has gaps in it at the atomic level,

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<v Speaker 1>and so a neutrino can pass right through that, right

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<v Speaker 1>through the Earth, and in fact, billions do every single day.

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<v Speaker 1>So being able to detect these these neutrinos that came

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<v Speaker 1>from cosmological events would tell us more about our universe,

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<v Speaker 1>which is why we're so interested in them. All Right,

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<v Speaker 1>So we've already talked a little bit about how neutrinos

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<v Speaker 1>behave They aren't affected by electrical charge, they move nearly

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<v Speaker 1>at the speed of light. And the nice thing is

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<v Speaker 1>is that if we detect a neutrino and we're able

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<v Speaker 1>to observe the effects that the neutrino has had on

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<v Speaker 1>other atomic particles, then we can draw some information about

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<v Speaker 1>that neutrino, for example, where it may have come from

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<v Speaker 1>and how powerful it was. And so that is why

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<v Speaker 1>we're looking at the cosmological ones versus the ones that

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<v Speaker 1>we would say are emanating from our son um because

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<v Speaker 1>they are so they're they're nearly massless. They're also barely

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<v Speaker 1>affected by gravity, so because that's one thing that things

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<v Speaker 1>with mass do get affected by his gravity. But gravity,

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<v Speaker 1>out of the four fundamental forces of the universe, is

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<v Speaker 1>the weakest, right, So the only real force that tends

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<v Speaker 1>to affect neutrinos is the weak atomic force, but that

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<v Speaker 1>only takes effect at incredibly short distances. We're talking on

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<v Speaker 1>the atomic scale. So this is the kind of stuff

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<v Speaker 1>that holds atoms together. And so unless you're unless you're

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<v Speaker 1>is close to and I forget the exact distances that

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<v Speaker 1>we're that we're talking about here, but it's it's it's like, yeah,

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<v Speaker 1>as close as you can possibly get without being the

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<v Speaker 1>same thing pretty much plunk is what we're talking about here. Uh,

0:13:09.800 --> 0:13:13.400
<v Speaker 1>incredibly short distances. So you know, otherwise they just like

0:13:13.440 --> 0:13:17.160
<v Speaker 1>I said, our fly through uh uninhibited. They just go

0:13:17.320 --> 0:13:20.240
<v Speaker 1>straight in a straight line. So by seeing the direction

0:13:20.280 --> 0:13:22.960
<v Speaker 1>that they traveled in through the evidence they leave, which

0:13:23.000 --> 0:13:25.720
<v Speaker 1>we'll talk about in a second, then we can determine

0:13:25.800 --> 0:13:28.520
<v Speaker 1>where they came from. And and if we are able

0:13:28.559 --> 0:13:31.400
<v Speaker 1>to measure how much energy there was in that neutrino,

0:13:32.000 --> 0:13:34.920
<v Speaker 1>then that can give us an idea of what might

0:13:35.040 --> 0:13:37.400
<v Speaker 1>have eventually spawned it. For example, if we are able

0:13:37.440 --> 0:13:39.080
<v Speaker 1>to see what direction it came from and we figure

0:13:39.120 --> 0:13:42.280
<v Speaker 1>it was pretty powerful and we end up kind of

0:13:42.320 --> 0:13:45.560
<v Speaker 1>tracing back that pathway and we see that that pathway

0:13:45.640 --> 0:13:48.079
<v Speaker 1>takes it through to what used to be a supernova,

0:13:48.520 --> 0:13:53.959
<v Speaker 1>you could potentially say, hey, this neutrino was uh, it

0:13:54.080 --> 0:13:57.280
<v Speaker 1>came to us from that supernova. That's pretty phenomenal stuff.

0:13:57.280 --> 0:14:01.040
<v Speaker 1>That means we can learn more about a thing that

0:14:01.080 --> 0:14:03.520
<v Speaker 1>happens in our universe that otherwise we would never be

0:14:03.559 --> 0:14:07.120
<v Speaker 1>close enough to observe. Pretty mysterious. Yeah, you know, Unfortunately,

0:14:07.240 --> 0:14:11.080
<v Speaker 1>since they don't interact with matter all that much. You know,

0:14:11.160 --> 0:14:13.960
<v Speaker 1>you know, there's for for about every hundred billion neutrinos

0:14:14.000 --> 0:14:17.040
<v Speaker 1>that paths of the Earth, only one or so is

0:14:17.080 --> 0:14:20.240
<v Speaker 1>going to interact with anything. And since it's really the

0:14:20.320 --> 0:14:24.080
<v Speaker 1>interactions with stuff that we're looking for, not the neutrinos themselves,

0:14:24.600 --> 0:14:26.360
<v Speaker 1>that that is part of why they are a so

0:14:26.520 --> 0:14:30.360
<v Speaker 1>elusive and be so attractive as a field of scientific study.

0:14:30.400 --> 0:14:33.480
<v Speaker 1>And exactly, and that's also an explanation of why the

0:14:33.520 --> 0:14:36.920
<v Speaker 1>ice cube telescope is so enormous. If you were to

0:14:36.960 --> 0:14:40.680
<v Speaker 1>create a human sized neutrino detector, it would take you

0:14:40.720 --> 0:14:44.720
<v Speaker 1>a century before you would be likely to detect a neutrino,

0:14:44.760 --> 0:14:48.400
<v Speaker 1>Whereas if you make it a cubic kilometer, you have

0:14:48.520 --> 0:14:51.840
<v Speaker 1>increased your odds of that happening, uh like, quite a bit,

0:14:51.880 --> 0:14:54.160
<v Speaker 1>as it turns out, yea, by more than two. So

0:14:54.440 --> 0:14:57.120
<v Speaker 1>when did we first figure out that there were these things,

0:14:57.160 --> 0:15:00.360
<v Speaker 1>or at least suspect that they existed that That first

0:15:00.360 --> 0:15:05.560
<v Speaker 1>suspicion was in nineteen one. Um. That was theorist Wolfgang Polly. Yeah,

0:15:06.000 --> 0:15:10.880
<v Speaker 1>he was looking at some radioactive decay equations and saw

0:15:10.920 --> 0:15:13.520
<v Speaker 1>that there was some missing energy and energy k be

0:15:13.560 --> 0:15:16.760
<v Speaker 1>created or destroyed. Right, So he figured there has to

0:15:16.800 --> 0:15:20.720
<v Speaker 1>be something responsible for this, and and therefore there there

0:15:20.720 --> 0:15:25.440
<v Speaker 1>has to be a particle that's being given off. There's

0:15:25.480 --> 0:15:28.440
<v Speaker 1>some undetectable particle that is making off with some of

0:15:28.480 --> 0:15:34.480
<v Speaker 1>this energy. It must be an electrically neutral right and yeah,

0:15:34.560 --> 0:15:37.400
<v Speaker 1>so he figured out the basics of what must have

0:15:37.440 --> 0:15:41.360
<v Speaker 1>been there, but had no way of detecting it. And uh,

0:15:41.440 --> 0:15:44.120
<v Speaker 1>you know, this is again something that sounds phenomenal to me.

0:15:44.160 --> 0:15:47.200
<v Speaker 1>I can't imagine coming up with this conclusion. But if

0:15:47.200 --> 0:15:49.280
<v Speaker 1>you look at particle physics, this is a story that

0:15:49.320 --> 0:15:52.120
<v Speaker 1>we see happen over and over again, where people see something,

0:15:52.560 --> 0:15:57.000
<v Speaker 1>they theorize or hypothesize what must be happening, and then

0:15:57.560 --> 0:16:01.520
<v Speaker 1>future experiments end up bearing that out right. Um. Now,

0:16:01.640 --> 0:16:05.360
<v Speaker 1>the term neutrino wasn't coined until ninety four by by

0:16:05.480 --> 0:16:09.400
<v Speaker 1>Enrico Fermi. Oh for me, we've talked about for me before. Yeah,

0:16:09.560 --> 0:16:13.280
<v Speaker 1>so neutrino is an Italian word, and I think it

0:16:13.360 --> 0:16:18.120
<v Speaker 1>means enormous pasta dish, little neutral one, I think is

0:16:18.160 --> 0:16:22.000
<v Speaker 1>the more common translation. Well, I was using poetic license.

0:16:22.600 --> 0:16:26.280
<v Speaker 1>Uh yeah, so it's you know, it was it still

0:16:26.320 --> 0:16:30.200
<v Speaker 1>had not been actually seen or observed, right right, Um,

0:16:30.240 --> 0:16:33.320
<v Speaker 1>but this this was just a kind of formal equation

0:16:33.440 --> 0:16:37.480
<v Speaker 1>that he was using that incorporated Polly's ideas. Right, So

0:16:37.920 --> 0:16:40.040
<v Speaker 1>you have to skip from nineteen thirty four all the

0:16:40.080 --> 0:16:42.640
<v Speaker 1>way to nineteen fifty nine before you get to some

0:16:42.800 --> 0:16:46.240
<v Speaker 1>scientists who observed a new trino, and that would be

0:16:46.280 --> 0:16:50.360
<v Speaker 1>Clyde Cowen and Fred Rens, who discovered a particle that

0:16:50.480 --> 0:16:54.280
<v Speaker 1>fit all the expected characteristics of what was being called

0:16:54.640 --> 0:16:57.800
<v Speaker 1>the new trino. So now it was no longer hypothetical.

0:16:57.880 --> 0:16:59.920
<v Speaker 1>Now they actually had a particle they could point to

0:17:00.040 --> 0:17:02.560
<v Speaker 1>and say, that's it. This thing that we found in

0:17:02.560 --> 0:17:05.960
<v Speaker 1>the lab, that thing is probably a neutrino UM. And

0:17:06.000 --> 0:17:08.920
<v Speaker 1>specifically what they found was an electron neutrino, which is UM.

0:17:09.400 --> 0:17:12.120
<v Speaker 1>And I think that we forgot to explain this part earlier.

0:17:12.119 --> 0:17:14.720
<v Speaker 1>But the three different kinds of neutrinos pair with three

0:17:14.720 --> 0:17:17.880
<v Speaker 1>different kinds of particles, so it's the electron neutrinos pair

0:17:17.880 --> 0:17:21.280
<v Speaker 1>with electrons, right, and muon neutrinos pair with muan, so

0:17:21.320 --> 0:17:23.879
<v Speaker 1>they're heavier, they have more mass. You guys tell us

0:17:24.320 --> 0:17:26.800
<v Speaker 1>the tal neutrinos are a little heavier than the muans.

0:17:26.960 --> 0:17:30.280
<v Speaker 1>So yeah, each new trino has a mass that is equivalent,

0:17:30.640 --> 0:17:34.719
<v Speaker 1>well not not equivalent. It matches in a sense the

0:17:34.840 --> 0:17:38.239
<v Speaker 1>size of the other subatomic particle, because actually a an

0:17:38.240 --> 0:17:41.680
<v Speaker 1>electron new trino has less mass than an electronic way

0:17:41.760 --> 0:17:45.760
<v Speaker 1>less mass, but but they scale up as the negatively

0:17:45.840 --> 0:17:48.960
<v Speaker 1>charged subatomic particles scale up as well. So I don't

0:17:48.960 --> 0:17:51.480
<v Speaker 1>mean to suggest that an electron and electron new trino

0:17:51.600 --> 0:17:54.479
<v Speaker 1>are equivalent in the sense of mass. They are not.

0:17:55.119 --> 0:17:58.160
<v Speaker 1>But now we get up to nineteen sixty two when

0:17:58.480 --> 0:18:03.040
<v Speaker 1>another UH organization we're familiar with CERN along with the

0:18:03.119 --> 0:18:07.440
<v Speaker 1>Brookhaven National Laboratory. Yet they independently conducted experiments and discovered

0:18:07.440 --> 0:18:10.720
<v Speaker 1>a second type of neutrino, which was the muon neutrino,

0:18:11.200 --> 0:18:13.800
<v Speaker 1>and it behaved differently from the electron neutrino. That's what

0:18:13.960 --> 0:18:16.480
<v Speaker 1>first gave them a little bit of confusion, in fact,

0:18:16.480 --> 0:18:19.520
<v Speaker 1>to a point where they would expect to observe a

0:18:19.520 --> 0:18:23.160
<v Speaker 1>certain number of neutrinos coming from the Sun on any

0:18:23.240 --> 0:18:25.840
<v Speaker 1>given day, and they had a certain number that they

0:18:25.840 --> 0:18:29.119
<v Speaker 1>expected for electron neutrinos and a certain number for muon neutrinos,

0:18:29.440 --> 0:18:31.720
<v Speaker 1>and for some reason that wasn't working out, and they

0:18:31.720 --> 0:18:34.600
<v Speaker 1>could not figure out why that was, and they couldn't

0:18:34.600 --> 0:18:37.200
<v Speaker 1>figure out why that was for a long time, very

0:18:37.280 --> 0:18:42.600
<v Speaker 1>long time. So you have the Stanford Linear Accelerator Center,

0:18:42.920 --> 0:18:46.720
<v Speaker 1>and they discovered the twel subatomic particle, which was the

0:18:46.840 --> 0:18:50.480
<v Speaker 1>negatively charged sub atomic particle that's heavier than electron or muan,

0:18:51.200 --> 0:18:53.760
<v Speaker 1>and that led the scientist to hypothesize that perhaps there

0:18:53.840 --> 0:18:57.000
<v Speaker 1>was in fact a third type of neutrino, because there

0:18:57.040 --> 0:19:00.119
<v Speaker 1>already were neutrino counterparts for the other two negative lee

0:19:00.200 --> 0:19:03.320
<v Speaker 1>charged particles. So now they had the new the tow

0:19:03.520 --> 0:19:06.879
<v Speaker 1>new trino um, but they could not directly observe it.

0:19:07.760 --> 0:19:10.280
<v Speaker 1>And at that point they were still kind of wondering

0:19:10.400 --> 0:19:13.159
<v Speaker 1>why there seems to be this new trino shortage, you know,

0:19:13.200 --> 0:19:16.240
<v Speaker 1>based upon their calculations, there should be more than what

0:19:16.320 --> 0:19:19.960
<v Speaker 1>they were detecting. Yeah, like like twice again as much, right,

0:19:20.520 --> 0:19:24.320
<v Speaker 1>And then we get up to in nine seven, an

0:19:24.520 --> 0:19:29.080
<v Speaker 1>enormous newtrino detector is built, the Cameo conde, and I'm

0:19:29.200 --> 0:19:32.520
<v Speaker 1>sure I'm mispronouncing that newtrino detector. It was a large

0:19:32.520 --> 0:19:35.240
<v Speaker 1>water detector, not meaning that I don't mean that it

0:19:35.280 --> 0:19:37.679
<v Speaker 1>was detecting large amounts of water. I meant that it

0:19:37.760 --> 0:19:39.920
<v Speaker 1>had a large amount of water and that used as

0:19:39.960 --> 0:19:45.399
<v Speaker 1>the detector. Now, this water was incredibly pure and incredibly clear,

0:19:46.160 --> 0:19:50.000
<v Speaker 1>so clear that sunlight could pass through it without slowing

0:19:50.080 --> 0:19:54.840
<v Speaker 1>down for something like seventy meters, which is far longer

0:19:54.880 --> 0:19:56.560
<v Speaker 1>than it could if it were passing through the water

0:19:56.640 --> 0:20:01.840
<v Speaker 1>of say, your typical swimming pool. Yeah, in in your

0:20:01.880 --> 0:20:04.199
<v Speaker 1>typical swimming pool, you might get a couple of meters

0:20:04.200 --> 0:20:07.800
<v Speaker 1>if you're lucky, right, So it was very very clear,

0:20:07.840 --> 0:20:11.120
<v Speaker 1>and that was important to detect these tiny little reactions

0:20:11.119 --> 0:20:14.000
<v Speaker 1>that the neutrino would cause if it collided with another

0:20:14.040 --> 0:20:16.880
<v Speaker 1>sub atomic particle. And it also had more than eleven

0:20:16.920 --> 0:20:21.359
<v Speaker 1>thousand light collectors that were called photo multiplier tubes in

0:20:21.440 --> 0:20:24.040
<v Speaker 1>the water itself, and those were what we're looking for,

0:20:24.080 --> 0:20:26.359
<v Speaker 1>these these reactions that we're going to talk about in

0:20:26.359 --> 0:20:30.040
<v Speaker 1>the second So that was a huge advance. It was

0:20:30.080 --> 0:20:33.760
<v Speaker 1>an enormous neutrino detector, one of the largest until the

0:20:33.800 --> 0:20:38.800
<v Speaker 1>ice cube one comes along. Certain starts to experiment and

0:20:38.840 --> 0:20:41.680
<v Speaker 1>determine that no other types of neutrinos beyond the three

0:20:41.800 --> 0:20:45.080
<v Speaker 1>types that already been identified could exist based upon what

0:20:45.160 --> 0:20:48.240
<v Speaker 1>we know. So maybe one day we'll find out we're

0:20:48.240 --> 0:20:51.080
<v Speaker 1>wrong about that, but based upon everything we know right now,

0:20:51.119 --> 0:20:54.680
<v Speaker 1>it appears that only those three types of neutrinos, the electron, muan,

0:20:54.800 --> 0:20:58.080
<v Speaker 1>and tao, are the ones that exist. UM now in

0:20:58.119 --> 0:21:01.439
<v Speaker 1>two thousand one was that was when we finally solved

0:21:01.480 --> 0:21:04.439
<v Speaker 1>that solar neutrino problem that we were talking about earlier.

0:21:04.600 --> 0:21:08.320
<v Speaker 1>UM experiments that were conducted at the Canadian Solar Neutrino

0:21:08.400 --> 0:21:13.200
<v Speaker 1>Observatory or snow UM showed because it's in Canada, there's

0:21:13.640 --> 0:21:16.440
<v Speaker 1>anyway showed that it could be solved with the explanation

0:21:16.520 --> 0:21:19.600
<v Speaker 1>that okay, So so even though the Sun releases only

0:21:19.680 --> 0:21:24.000
<v Speaker 1>electron neutrinos, they oscillate sometimes while they travel through space

0:21:24.040 --> 0:21:26.840
<v Speaker 1>to become a pretty even mix of muan, tao, and

0:21:27.040 --> 0:21:31.680
<v Speaker 1>electron neutrinos, So that that explains like if they're oscillating

0:21:31.760 --> 0:21:34.040
<v Speaker 1>and some of them are town neutrinos, which we have

0:21:34.160 --> 0:21:36.720
<v Speaker 1>not been able to observe directly, that would that would

0:21:36.720 --> 0:21:41.800
<v Speaker 1>explain the apparent shortage of neutrinos right, previous experiments. Most

0:21:41.840 --> 0:21:45.760
<v Speaker 1>previous experiments were really only looking for electron neutrinos, especially

0:21:45.760 --> 0:21:49.400
<v Speaker 1>coming from the Sun, and the instruments were not calibrated

0:21:49.440 --> 0:21:53.200
<v Speaker 1>to be detecting Muon and tao. So, and that's because

0:21:53.280 --> 0:21:55.919
<v Speaker 1>if it's if it's oscillating, it has to have mass.

0:21:55.960 --> 0:22:00.719
<v Speaker 1>It's one of those things fundamental nature. Yeah, so you know,

0:22:01.960 --> 0:22:05.320
<v Speaker 1>they're still really tiny. An electron neutrino would be about

0:22:05.400 --> 0:22:08.720
<v Speaker 1>one one million the mass of an electron. Yeah, that's

0:22:08.760 --> 0:22:13.359
<v Speaker 1>that's incredibly that's inconceivably tiny, at least in my mind.

0:22:13.600 --> 0:22:17.639
<v Speaker 1>But but something so inconceivably tiny is very important on

0:22:17.680 --> 0:22:22.199
<v Speaker 1>a universal level because this could possibly explain why, uh,

0:22:23.040 --> 0:22:26.240
<v Speaker 1>why the universe contains more matter than antimatter. Why we

0:22:26.280 --> 0:22:29.879
<v Speaker 1>think that this could explain dark matter basically exactly. It

0:22:29.880 --> 0:22:32.760
<v Speaker 1>could well, when you get to why more matter than

0:22:32.800 --> 0:22:35.840
<v Speaker 1>antimatter that explained. That would explain why the universe is

0:22:35.880 --> 0:22:37.439
<v Speaker 1>the way it is, because if there had been an

0:22:37.440 --> 0:22:39.560
<v Speaker 1>equal amount of matter and antimatter, it would have all

0:22:39.560 --> 0:22:42.440
<v Speaker 1>annihilated itself and we wouldn't have a universe, which would

0:22:42.480 --> 0:22:45.399
<v Speaker 1>be terrible because that's where I keep all my stuff. Now,

0:22:45.720 --> 0:22:49.159
<v Speaker 1>how do we actually create neutrinos ourselves. Well, it's mostly

0:22:49.200 --> 0:22:52.280
<v Speaker 1>through particle accelerators. You know, you moved some subatomic particles

0:22:52.320 --> 0:22:54.840
<v Speaker 1>fast enough and smash them to see what happens. And

0:22:54.880 --> 0:22:56.879
<v Speaker 1>some of the stuff that gets spun off tends to

0:22:56.960 --> 0:23:01.600
<v Speaker 1>be these other subatomic particles and energy that we would

0:23:01.640 --> 0:23:05.080
<v Speaker 1>otherwise not have been able to observe, and neutrinos are

0:23:05.080 --> 0:23:08.399
<v Speaker 1>one of those. Although again we don't directly observe the neutrinos,

0:23:08.480 --> 0:23:12.320
<v Speaker 1>we observe the reactions that they have with other stuff, right,

0:23:12.400 --> 0:23:14.520
<v Speaker 1>And these neutrinos that we can create here on Earth

0:23:14.560 --> 0:23:16.600
<v Speaker 1>are much lower in energy than most of the ones

0:23:16.680 --> 0:23:19.920
<v Speaker 1>that we're seeing from from from the Sun, and way

0:23:20.040 --> 0:23:23.720
<v Speaker 1>lower than anything that would be produced from a cosmological event.

0:23:23.840 --> 0:23:28.320
<v Speaker 1>So yeah, if you compare the neutrinos from the ones

0:23:28.359 --> 0:23:31.520
<v Speaker 1>that have been detected at the ice cube detector versus

0:23:31.560 --> 0:23:33.560
<v Speaker 1>the ones that have been created in the lab, it's

0:23:33.800 --> 0:23:36.639
<v Speaker 1>worlds of difference. So we've got a lot more we

0:23:36.720 --> 0:23:39.760
<v Speaker 1>want to talk about with the ice cube detector, including

0:23:39.800 --> 0:23:42.720
<v Speaker 1>how it actually detects these new trinos, or at least

0:23:42.760 --> 0:23:45.920
<v Speaker 1>the interactions and the neutrinos are having with other particles.

0:23:45.960 --> 0:23:48.639
<v Speaker 1>But before we do that, let's take a quick break

0:23:48.680 --> 0:23:52.359
<v Speaker 1>to thank our sponsor. All right, let's get back into

0:23:52.440 --> 0:23:56.200
<v Speaker 1>the discussion about as cube. What is this thing actually

0:23:56.280 --> 0:23:58.080
<v Speaker 1>made of? Okay, so we've talked about there are these

0:23:58.080 --> 0:24:01.199
<v Speaker 1>sensors that are buried a mile beneath the ice, but

0:24:01.359 --> 0:24:03.879
<v Speaker 1>what are the sensors actually Well, first of all, I

0:24:03.920 --> 0:24:06.120
<v Speaker 1>like your verbal suggestion that we are talking in fact

0:24:06.160 --> 0:24:10.359
<v Speaker 1>about the rapper ice cube. Well, but what was that?

0:24:10.400 --> 0:24:13.040
<v Speaker 1>Not it? Man? The second half of this episode is

0:24:13.080 --> 0:24:17.800
<v Speaker 1>going to be so confusing. Okay, that the main components

0:24:17.880 --> 0:24:21.639
<v Speaker 1>of of ice cube are these these digital optical modules

0:24:21.760 --> 0:24:24.840
<v Speaker 1>or doms, and each one is about the size of

0:24:24.840 --> 0:24:29.560
<v Speaker 1>a basketball and they are specifically looking for a very

0:24:29.920 --> 0:24:33.560
<v Speaker 1>um peculiar kind of light. And I'll talk more about

0:24:33.640 --> 0:24:35.880
<v Speaker 1>that in the second but you know now they are

0:24:36.880 --> 0:24:40.960
<v Speaker 1>deep within the ice. That means that we can't really

0:24:41.359 --> 0:24:43.600
<v Speaker 1>fix them if something goes wrong. Yeah, there's really no

0:24:43.720 --> 0:24:47.560
<v Speaker 1>diving down into a mile of ice to fix the

0:24:48.080 --> 0:24:50.639
<v Speaker 1>wet dom. Number four hundred and seventy three is on

0:24:50.680 --> 0:24:54.520
<v Speaker 1>the fritz. C oll. We can actually we being the

0:24:54.520 --> 0:24:58.080
<v Speaker 1>people who are actually working on and no, we're not

0:24:58.160 --> 0:25:00.800
<v Speaker 1>giving access to this sort of thing but they can

0:25:00.880 --> 0:25:03.600
<v Speaker 1>make software updates and firmware updates. Each one of those

0:25:03.640 --> 0:25:06.040
<v Speaker 1>doms is wired to the headquarters, which is at the

0:25:06.040 --> 0:25:09.280
<v Speaker 1>South Pole. Uh. The South Pole headquarters houses lots of

0:25:09.320 --> 0:25:12.280
<v Speaker 1>different stuff, not just the ice cube project. There are

0:25:12.320 --> 0:25:15.119
<v Speaker 1>other projects that are at the South Pole as well,

0:25:15.520 --> 0:25:17.800
<v Speaker 1>but that's one of the ones, and they're all wired

0:25:17.800 --> 0:25:21.280
<v Speaker 1>in there so that you can administer commands to the

0:25:21.320 --> 0:25:26.240
<v Speaker 1>doms and update their software as needed. So there are

0:25:26.320 --> 0:25:31.399
<v Speaker 1>a few of them. There's actually sixty uh doms per hole,

0:25:31.680 --> 0:25:35.359
<v Speaker 1>and there are holes if we do a little bit

0:25:35.400 --> 0:25:37.639
<v Speaker 1>of math, that comes up with about five thousand, one

0:25:37.680 --> 0:25:41.280
<v Speaker 1>hundred sixty of these things. Uh. These holes were drilled

0:25:41.359 --> 0:25:45.040
<v Speaker 1>by UM by shooting hot, pressurized water down into the ice,

0:25:45.080 --> 0:25:48.399
<v Speaker 1>which then froze back over UM through a very careful

0:25:48.440 --> 0:25:50.919
<v Speaker 1>engineering process, into that very clear ice that we were

0:25:51.000 --> 0:25:53.399
<v Speaker 1>looking for. Right. Yeah, I'll have to, uh see if

0:25:53.440 --> 0:25:55.439
<v Speaker 1>I can find some photos that we can link to,

0:25:55.560 --> 0:25:58.480
<v Speaker 1>because the photos of these holes where they just they

0:25:58.480 --> 0:26:00.760
<v Speaker 1>shot a picture straight down the whole after it was drilled,

0:26:01.280 --> 0:26:04.480
<v Speaker 1>is vertigo inducing. It's pretty amazing stuff to be looking

0:26:04.520 --> 0:26:07.920
<v Speaker 1>down a a you know, a perfect circle that goes

0:26:08.000 --> 0:26:10.480
<v Speaker 1>down a mile. It reminded me very much of all

0:26:10.520 --> 0:26:12.280
<v Speaker 1>the things that I didn't want to jump down into

0:26:12.320 --> 0:26:15.679
<v Speaker 1>in silent hill too, that having to jump down into.

0:26:15.960 --> 0:26:18.760
<v Speaker 1>Now on top of the literally on top of these

0:26:18.800 --> 0:26:22.040
<v Speaker 1>five thousand one sixty doms on the surface of the

0:26:22.080 --> 0:26:27.399
<v Speaker 1>ice itself are an additional three twenty four digital operating modules,

0:26:27.480 --> 0:26:31.280
<v Speaker 1>and that is part of a second detector called ice top.

0:26:32.080 --> 0:26:35.600
<v Speaker 1>So you have the five thousand one or sixty underneath

0:26:35.600 --> 0:26:38.320
<v Speaker 1>the surface and three four on the surface, all of

0:26:38.320 --> 0:26:42.880
<v Speaker 1>which are looking for these new trino interactions. Okay, so

0:26:42.920 --> 0:26:46.280
<v Speaker 1>how exactly are are they looking for these interactions? All right?

0:26:46.359 --> 0:26:50.040
<v Speaker 1>So when a new trino meets another sub atomic particle

0:26:50.080 --> 0:26:53.919
<v Speaker 1>that really likes it's traveling at a pretty high amount

0:26:53.920 --> 0:26:58.800
<v Speaker 1>of energy, uh, you tend to have a mouon emitted

0:26:59.320 --> 0:27:02.760
<v Speaker 1>as part of this interaction, and it's going to be

0:27:02.800 --> 0:27:05.280
<v Speaker 1>moving in the same direction as the neutrino. So, when

0:27:05.280 --> 0:27:09.200
<v Speaker 1>a neutrino makes contact with a subatomic particle in the ice,

0:27:09.520 --> 0:27:13.200
<v Speaker 1>within an ice molecule, uh, a muan is given off

0:27:13.359 --> 0:27:17.800
<v Speaker 1>and that ends up producing something called cheren CoV radiation. Now,

0:27:17.880 --> 0:27:22.399
<v Speaker 1>cheren CoV radiation is emitted whenever a particle moves through

0:27:22.520 --> 0:27:26.840
<v Speaker 1>a medium faster than light. Could move through that same medium.

0:27:26.880 --> 0:27:28.919
<v Speaker 1>So in this case, the neutrino is moving through that

0:27:29.040 --> 0:27:32.480
<v Speaker 1>ice faster than light could travel through that ice, and

0:27:32.520 --> 0:27:35.919
<v Speaker 1>it makes contact with the subatomic particle. You end up

0:27:35.960 --> 0:27:39.080
<v Speaker 1>having this MoU on uh given off as a result,

0:27:39.400 --> 0:27:43.600
<v Speaker 1>and you get this light blue radiation. This is typical

0:27:43.840 --> 0:27:48.639
<v Speaker 1>of any kind of nuclear radioactive process. You get this

0:27:48.720 --> 0:27:52.479
<v Speaker 1>blue glow as a result. So what these detectors are

0:27:52.520 --> 0:27:56.120
<v Speaker 1>looking for is evidence of that blue glow, and when

0:27:56.160 --> 0:27:59.399
<v Speaker 1>they detect it, they record it and then it's measured,

0:27:59.480 --> 0:28:02.640
<v Speaker 1>so you can it an entire track of this through

0:28:02.720 --> 0:28:06.960
<v Speaker 1>the the kilometer of ice and find out where it

0:28:07.040 --> 0:28:10.280
<v Speaker 1>came from and get an idea from the intensity of

0:28:10.320 --> 0:28:13.840
<v Speaker 1>the light how much energy that neutrino had. So you're

0:28:13.880 --> 0:28:16.040
<v Speaker 1>looking at the direction of the light and the intensity

0:28:16.080 --> 0:28:19.680
<v Speaker 1>of it to infer the information about this subatomic particle,

0:28:20.080 --> 0:28:24.080
<v Speaker 1>which is awesome. I just think that's so amazing that

0:28:24.160 --> 0:28:28.359
<v Speaker 1>you can learn so much from just a pattern of light.

0:28:29.040 --> 0:28:32.119
<v Speaker 1>And uh, it really is a lot. It's a ton

0:28:32.440 --> 0:28:35.320
<v Speaker 1>of light uh and ton of information that they are

0:28:35.320 --> 0:28:39.320
<v Speaker 1>gathering each year, something like a terabyte of data per

0:28:39.480 --> 0:28:42.320
<v Speaker 1>day that they're gathering. Uh. The ends up being just

0:28:42.400 --> 0:28:44.440
<v Speaker 1>about a hundred gigabytes but all the time they're done

0:28:44.440 --> 0:28:48.920
<v Speaker 1>with this. Yeah it's tiny, tiny, but yeah, hundred gigabytes

0:28:48.960 --> 0:28:51.720
<v Speaker 1>once they filter through all the data. But uh, that's

0:28:51.760 --> 0:28:54.600
<v Speaker 1>exactly what they're looking for. And that's why these detectors

0:28:54.600 --> 0:28:58.000
<v Speaker 1>have to be so far underground in such dark, clear

0:28:58.200 --> 0:29:00.040
<v Speaker 1>conditions for it to be able to detect this of

0:29:00.080 --> 0:29:03.560
<v Speaker 1>these very small little packets of life that are just yeah,

0:29:03.560 --> 0:29:06.440
<v Speaker 1>it happens in an instant and they are so faint

0:29:06.480 --> 0:29:08.520
<v Speaker 1>that if it were not that dark, you would never

0:29:08.520 --> 0:29:11.600
<v Speaker 1>be able to detect it. So that's the that's the

0:29:11.640 --> 0:29:16.040
<v Speaker 1>whole purpose of this thing. And because neutrinos are given

0:29:16.080 --> 0:29:19.240
<v Speaker 1>off by lots of stuff besides just the Sun or

0:29:19.360 --> 0:29:23.240
<v Speaker 1>by particle accelerators, we can if we detect the right types,

0:29:23.480 --> 0:29:26.640
<v Speaker 1>learn more about stuff like cosmic rays, gamma ray bursts,

0:29:26.680 --> 0:29:30.600
<v Speaker 1>supernova um We might also be able to start to

0:29:31.120 --> 0:29:34.480
<v Speaker 1>infer things about dark matter and dark energy, things that

0:29:34.560 --> 0:29:37.400
<v Speaker 1>we do not We we know have to exist based

0:29:37.440 --> 0:29:40.560
<v Speaker 1>upon our understanding of our universe, but we have no evidence.

0:29:40.760 --> 0:29:44.360
<v Speaker 1>But again, yeah, right now, they're really just just mathematical placeholders, right, yeah,

0:29:44.400 --> 0:29:46.640
<v Speaker 1>Because when I say we have no evidence for it,

0:29:46.680 --> 0:29:49.280
<v Speaker 1>we have no direct evidence. We have lots of indirect

0:29:49.320 --> 0:29:52.360
<v Speaker 1>evidence by the way that the universe behaves, and the

0:29:52.360 --> 0:29:55.600
<v Speaker 1>way it behaves is different from how we would understand

0:29:55.600 --> 0:29:57.760
<v Speaker 1>it based upon the matter and energy we are able

0:29:57.840 --> 0:30:00.920
<v Speaker 1>to observe. So this might be able to give us

0:30:00.920 --> 0:30:04.320
<v Speaker 1>more clues about that and learn more about our our universe.

0:30:04.520 --> 0:30:08.360
<v Speaker 1>Pretty cool stuff. So, like we said, it's gathering lots

0:30:08.360 --> 0:30:13.360
<v Speaker 1>of information every single day. It's already detected several interesting neutrinos.

0:30:13.560 --> 0:30:17.000
<v Speaker 1>In May two thousand thirteen, they reported that they had

0:30:17.040 --> 0:30:20.760
<v Speaker 1>detected twenty eight neutrinos that had higher energy levels than

0:30:20.800 --> 0:30:23.400
<v Speaker 1>what they would expect from any neutrinos that would be

0:30:23.440 --> 0:30:28.480
<v Speaker 1>omitted by the Sun or any other nearby system within

0:30:28.520 --> 0:30:31.240
<v Speaker 1>our solar system. So it must be that these came

0:30:31.240 --> 0:30:35.360
<v Speaker 1>from outside the Solar system, assuming everything else is correct,

0:30:35.920 --> 0:30:39.120
<v Speaker 1>which is incredibly exciting. In fact, two of them had

0:30:39.160 --> 0:30:42.200
<v Speaker 1>so much high energy that they broke all records of

0:30:42.240 --> 0:30:45.400
<v Speaker 1>all neutrinos ever detected, and they got nicknames they got

0:30:45.520 --> 0:30:49.640
<v Speaker 1>They were nicknamed Bertie, Bert and Ernie. So yeah, I

0:30:49.720 --> 0:30:52.360
<v Speaker 1>assume one of them has an affinity for rubber duckies

0:30:52.880 --> 0:30:56.000
<v Speaker 1>and the other one is a neat freak, So yeah,

0:30:56.040 --> 0:30:59.280
<v Speaker 1>It's really exciting though, that these could possibly have come

0:30:59.320 --> 0:31:02.920
<v Speaker 1>from outside our solar system and could be evidence for

0:31:03.000 --> 0:31:07.040
<v Speaker 1>something that happened light years away, millions of years ago.

0:31:07.160 --> 0:31:11.920
<v Speaker 1>That's that's incredible. So we're still waiting to hear more

0:31:12.080 --> 0:31:15.040
<v Speaker 1>about that. As of the recording of this podcast, there

0:31:15.040 --> 0:31:18.640
<v Speaker 1>are plenty of scientists still poring over this information. Of course,

0:31:18.640 --> 0:31:23.200
<v Speaker 1>scientists are very careful before saying definitively whether or not

0:31:23.320 --> 0:31:26.520
<v Speaker 1>something came from outside the solar system. That seems to

0:31:26.560 --> 0:31:29.600
<v Speaker 1>be the indication, but they won't want to. I don't

0:31:29.600 --> 0:31:31.479
<v Speaker 1>want to jump to conclusions. You don't want to have

0:31:31.520 --> 0:31:34.200
<v Speaker 1>another Hey, the voyager left the solar system. No, wait,

0:31:34.240 --> 0:31:36.560
<v Speaker 1>no it didn't. No, no, it totally did. No it didn't. Okay,

0:31:36.560 --> 0:31:39.920
<v Speaker 1>it did, but it did it a year ago. We

0:31:39.920 --> 0:31:41.920
<v Speaker 1>don't want another one of those, right, No, no, no.

0:31:42.120 --> 0:31:44.520
<v Speaker 1>I I think it's much preferable in the scientific community

0:31:44.560 --> 0:31:46.640
<v Speaker 1>to be like, we're not sure about this thing, then

0:31:46.680 --> 0:31:50.320
<v Speaker 1>like we're sure. Oh we're wrong. Yeah. So this is

0:31:50.400 --> 0:31:53.840
<v Speaker 1>what we call exploratory science in the sense that there's

0:31:53.880 --> 0:31:57.800
<v Speaker 1>not like a specific practical application, there's no particular end goal.

0:31:57.920 --> 0:32:00.440
<v Speaker 1>It's just learning for the sake of learning, which is

0:32:01.320 --> 0:32:05.240
<v Speaker 1>invaluable because even though I mean there there are some

0:32:05.280 --> 0:32:09.040
<v Speaker 1>philosophies that say that science needs to be goal oriented,

0:32:09.040 --> 0:32:12.240
<v Speaker 1>like there needs to be an actual practical goal to

0:32:12.320 --> 0:32:16.680
<v Speaker 1>whatever scientific exploration you're doing. But that kind of puts

0:32:16.720 --> 0:32:19.800
<v Speaker 1>blinders on, right, because just by learning stuff, you never

0:32:19.880 --> 0:32:23.120
<v Speaker 1>know what kind of useful applications can come out of that. Yeah,

0:32:23.240 --> 0:32:25.840
<v Speaker 1>people hadn't been studying sub atomic particles, we would never

0:32:25.880 --> 0:32:29.640
<v Speaker 1>have come up with transistors, right, So, yeah, you can't

0:32:29.680 --> 0:32:34.480
<v Speaker 1>predict what sort of world changing discoveries can come out

0:32:34.520 --> 0:32:38.120
<v Speaker 1>of exploratory science. So personally, I find this to be

0:32:38.200 --> 0:32:42.480
<v Speaker 1>an absolutely fascinating use of resources to learn more about

0:32:42.520 --> 0:32:45.560
<v Speaker 1>our universe, and you never know how that information is

0:32:45.560 --> 0:32:47.560
<v Speaker 1>going to play out in ways that we just can't

0:32:47.600 --> 0:32:52.600
<v Speaker 1>anticipate right now, right, So I think it's pretty darn awesome.

0:32:52.880 --> 0:32:56.120
<v Speaker 1>But but more practically, what what exactly is it like

0:32:57.000 --> 0:33:02.440
<v Speaker 1>living and working? You know the South Pole. Yeah, there's

0:33:02.440 --> 0:33:05.640
<v Speaker 1>a great with a giant ice telescope. I have to

0:33:05.680 --> 0:33:08.760
<v Speaker 1>give a shout out. The ice cube website is fantastic.

0:33:08.800 --> 0:33:12.720
<v Speaker 1>It's tons of information and a lot of great video interviews.

0:33:12.760 --> 0:33:15.640
<v Speaker 1>Oh yeah, yes, so it is highly recommended. You'll have

0:33:15.720 --> 0:33:17.000
<v Speaker 1>to go and check it out. But one of the

0:33:17.040 --> 0:33:20.120
<v Speaker 1>sections is about what's it like at the South Pole?

0:33:20.480 --> 0:33:23.040
<v Speaker 1>So first of all, it describes what your experience would

0:33:23.040 --> 0:33:25.600
<v Speaker 1>be like just to get to the South Pole. Because first,

0:33:25.880 --> 0:33:30.560
<v Speaker 1>assuming you don't live in New Zealand or Australia, you've

0:33:30.560 --> 0:33:32.560
<v Speaker 1>got a little bit of a trip ahead of you. Yeah. Well,

0:33:32.600 --> 0:33:34.600
<v Speaker 1>I mean first you need to be issued some clothing

0:33:34.600 --> 0:33:36.680
<v Speaker 1>that will keep you from freezing to death. Yeah. That

0:33:36.680 --> 0:33:39.360
<v Speaker 1>that you can probably pick up somewhere in New Zealand.

0:33:39.400 --> 0:33:42.400
<v Speaker 1>Maybe you know, because they're the that's the only way

0:33:42.480 --> 0:33:46.880
<v Speaker 1>to get from UH at least by air to the

0:33:46.920 --> 0:33:49.920
<v Speaker 1>antar to the Antarctic. I mean you could go by boat,

0:33:50.160 --> 0:33:51.640
<v Speaker 1>but still you would have to pick up a lot

0:33:51.640 --> 0:33:55.560
<v Speaker 1>of clothing to keep you from freezing. Um. So yeah,

0:33:55.640 --> 0:33:58.200
<v Speaker 1>you would fly to Australia, fly to New Zealand get

0:33:58.200 --> 0:34:01.240
<v Speaker 1>all this clothing because you want to keep all your

0:34:01.360 --> 0:34:04.440
<v Speaker 1>fingers and toes and your nose, and I actually do.

0:34:04.520 --> 0:34:06.480
<v Speaker 1>I don't want to speak for all of humanity. Okay,

0:34:06.480 --> 0:34:09.959
<v Speaker 1>that's fair, that's fair, um, but so many of you

0:34:10.160 --> 0:34:12.800
<v Speaker 1>would like to keep your fingers and toes. From New Zealand,

0:34:12.960 --> 0:34:16.359
<v Speaker 1>you bought a military transport to the U S Station McMurdo. Oh,

0:34:16.440 --> 0:34:20.920
<v Speaker 1>not just a military transport, a Lockheed Hercules, Lauren, we

0:34:21.040 --> 0:34:24.560
<v Speaker 1>just talked about those, we did. Yeah, it's a Lockheed

0:34:24.600 --> 0:34:28.600
<v Speaker 1>Hercules military transport that you would board. Clearly not one

0:34:28.680 --> 0:34:33.120
<v Speaker 1>of the ones that the CIA is operating. Probably, yeah,

0:34:33.239 --> 0:34:36.640
<v Speaker 1>question as far as you know, uh if it if

0:34:36.680 --> 0:34:40.560
<v Speaker 1>it has you know, non standard Lockheed Hercules equipment on it,

0:34:40.640 --> 0:34:42.759
<v Speaker 1>maybe it's one of the CIA ones. But anyway, Yeah,

0:34:42.760 --> 0:34:45.560
<v Speaker 1>that takes you to to McMurdo, which is on the

0:34:45.600 --> 0:34:49.360
<v Speaker 1>coast of Antarctica, and from there you would have to

0:34:49.480 --> 0:34:53.200
<v Speaker 1>wait for a while, um and get another flight out

0:34:53.280 --> 0:34:56.800
<v Speaker 1>to the South Pole where you would land, walk outside

0:34:56.920 --> 0:35:01.600
<v Speaker 1>and immediately shield your eyes on ski Yes, that's my

0:35:01.640 --> 0:35:05.040
<v Speaker 1>favorite part. Honestly. For some reason, landing on skis just

0:35:05.080 --> 0:35:08.000
<v Speaker 1>makes me incredibly happy. Yeah, this Hercules has skis instead

0:35:08.000 --> 0:35:10.360
<v Speaker 1>of wheels, because you know, you can not so useful

0:35:10.480 --> 0:35:14.399
<v Speaker 1>in the Antarctic. So that South Pole station has two

0:35:14.920 --> 0:35:18.080
<v Speaker 1>people in it, um, only only about fifty of those

0:35:18.080 --> 0:35:21.160
<v Speaker 1>would be during during the height of study. During any

0:35:21.160 --> 0:35:23.960
<v Speaker 1>given year through the winter, about fifty people are are

0:35:24.000 --> 0:35:27.120
<v Speaker 1>going to be stationed right right, and only a couple

0:35:27.239 --> 0:35:30.680
<v Speaker 1>are there year round. Like stay for the full year

0:35:31.920 --> 0:35:34.239
<v Speaker 1>and uh and so it has h it's got a

0:35:34.280 --> 0:35:36.960
<v Speaker 1>couple of amenities. It's got a kitchen, it's got a gym,

0:35:37.000 --> 0:35:41.760
<v Speaker 1>it's got greenhouse, dining room. Uh. So it's got actually

0:35:42.080 --> 0:35:44.080
<v Speaker 1>meeting rooms and things like that. They have a lot

0:35:44.120 --> 0:35:47.839
<v Speaker 1>of extracurricular activities for people, so they don't go snow crazy.

0:35:48.200 --> 0:35:51.399
<v Speaker 1>Is that is that the scientific term? I would call

0:35:51.440 --> 0:35:55.600
<v Speaker 1>it that. If you will watch the Shining, I would

0:35:55.640 --> 0:35:58.440
<v Speaker 1>call that snow crazy. They don't want any Jack torrans

0:35:58.480 --> 0:36:00.799
<v Speaker 1>is running around the South Pole, so so they don't

0:36:00.800 --> 0:36:03.680
<v Speaker 1>have a lot of topiary in the greens. I'm guessing

0:36:03.680 --> 0:36:06.400
<v Speaker 1>no hedge mazes over at the South Pole, but they do.

0:36:06.560 --> 0:36:08.920
<v Speaker 1>They do have lots of different lectures you can attend.

0:36:09.040 --> 0:36:12.319
<v Speaker 1>Apparently the people will show up and find out that

0:36:12.360 --> 0:36:15.520
<v Speaker 1>they have complementary musical skills and a lot of bands

0:36:15.600 --> 0:36:18.759
<v Speaker 1>end up forming at the South Pole. Um. You know,

0:36:18.840 --> 0:36:20.880
<v Speaker 1>it's it's kind of interesting stuff and there's I was.

0:36:21.080 --> 0:36:23.520
<v Speaker 1>I was actually very much entertained. I love the idea

0:36:23.960 --> 0:36:25.759
<v Speaker 1>one of the things that you could take classes and

0:36:26.120 --> 0:36:32.399
<v Speaker 1>totally nonrelated things like lately unscientific like Scottish dance that

0:36:33.000 --> 0:36:35.239
<v Speaker 1>I just love the idea of all these scientists doing

0:36:35.239 --> 0:36:40.320
<v Speaker 1>a Scottish Highland dance in the South Pole. Yeah, parkas

0:36:40.320 --> 0:36:44.279
<v Speaker 1>and lab coats. So it did say that things like

0:36:44.440 --> 0:36:47.000
<v Speaker 1>preparing food at the South Pole is a little different

0:36:47.040 --> 0:36:49.640
<v Speaker 1>from other places in the world because it can take

0:36:50.080 --> 0:36:52.959
<v Speaker 1>anywhere from several hours to like a couple of weeks. Yeah.

0:36:53.040 --> 0:36:55.800
<v Speaker 1>They said that if you wanted to, say, serve ice cream,

0:36:56.080 --> 0:36:58.319
<v Speaker 1>you would take it out of the freezer and let's

0:36:58.360 --> 0:37:01.120
<v Speaker 1>sit out for no half a day or else you

0:37:01.120 --> 0:37:04.440
<v Speaker 1>would need a hack saw to uh to make us serving.

0:37:04.520 --> 0:37:07.000
<v Speaker 1>So I thought that was pretty interesting too. They have

0:37:07.160 --> 0:37:10.799
<v Speaker 1>lots of educational outreach programs to various high schools and

0:37:10.880 --> 0:37:15.600
<v Speaker 1>colleges throughout the world, and uh, they have programs where

0:37:15.719 --> 0:37:19.120
<v Speaker 1>schools can have someone talk to them about the project

0:37:19.440 --> 0:37:22.080
<v Speaker 1>via webcast or even come in. Yeah. Yeah, because not

0:37:22.120 --> 0:37:24.080
<v Speaker 1>that all these scientists are working at the South Pole.

0:37:24.160 --> 0:37:26.360
<v Speaker 1>Some of them are working remotely. They get the data

0:37:26.480 --> 0:37:29.959
<v Speaker 1>sent up to them via satellite and then they work

0:37:30.000 --> 0:37:32.520
<v Speaker 1>on that. But they're still doing very important work in

0:37:32.520 --> 0:37:35.520
<v Speaker 1>in the whole experiment, and they can talk at length

0:37:35.560 --> 0:37:37.440
<v Speaker 1>about what it is they do and why it's important.

0:37:37.480 --> 0:37:39.360
<v Speaker 1>So lots of schools if your school is interested in

0:37:39.360 --> 0:37:41.080
<v Speaker 1>that sort of thing, go to the ice Cube website.

0:37:41.080 --> 0:37:44.560
<v Speaker 1>You can totally check it out there. And if your

0:37:44.560 --> 0:37:50.240
<v Speaker 1>school has high aspirations and and a high budget, yeah,

0:37:50.280 --> 0:37:53.359
<v Speaker 1>they can actually look into paying a visit to the

0:37:53.400 --> 0:37:56.480
<v Speaker 1>South Pole headquarters and finding out more about the ice

0:37:56.520 --> 0:37:59.520
<v Speaker 1>Cube detector. I think paying is probably the operative word,

0:37:59.520 --> 0:38:03.960
<v Speaker 1>because it is expensive to Antarctica, you know, I noticed

0:38:04.320 --> 0:38:07.359
<v Speaker 1>I saw that between for an average person, if you're

0:38:07.400 --> 0:38:09.760
<v Speaker 1>just talking about a tour, you're not even talking about

0:38:09.960 --> 0:38:12.440
<v Speaker 1>going down to the South Pole to see the headquarters,

0:38:12.520 --> 0:38:15.640
<v Speaker 1>just just to look at Antarctica, can be between four

0:38:15.680 --> 0:38:18.520
<v Speaker 1>thousand and eleven thousand dollars per person, so it is

0:38:18.560 --> 0:38:21.239
<v Speaker 1>a bit dear. However, I think you know, it's a

0:38:21.280 --> 0:38:24.200
<v Speaker 1>once in a lifetime kind of opportunity, right except for

0:38:24.239 --> 0:38:26.400
<v Speaker 1>the people who live there where it's every day. But

0:38:26.440 --> 0:38:28.240
<v Speaker 1>for most of us, it's a once in a lifetime

0:38:28.239 --> 0:38:31.640
<v Speaker 1>type thing. So I think it would be absolutely cool

0:38:31.960 --> 0:38:35.120
<v Speaker 1>to go visit it. To bring things back around again, Lauren,

0:38:35.560 --> 0:38:38.200
<v Speaker 1>you can't really start or endo tech stuff episode without

0:38:38.239 --> 0:38:41.480
<v Speaker 1>having you judge me, so we have to you already,

0:38:42.000 --> 0:38:43.680
<v Speaker 1>you already did that pun. You should come up with

0:38:43.719 --> 0:38:50.640
<v Speaker 1>some fresh new puns. Flash freeze waters, look, stop, collaborate

0:38:50.680 --> 0:38:54.200
<v Speaker 1>and listen. Ice is back with a brand new invention.

0:38:54.239 --> 0:38:56.879
<v Speaker 1>Al Right, guys, that wraps up this topic. Thank you,

0:38:57.320 --> 0:39:00.000
<v Speaker 1>thank you. It's time to go solo. No, not really,

0:39:00.200 --> 0:39:03.400
<v Speaker 1>not really. Alright, guys, if you enjoyed this episode, or

0:39:03.480 --> 0:39:06.239
<v Speaker 1>maybe you have something you want to add to the discussion,

0:39:06.280 --> 0:39:09.919
<v Speaker 1>perhaps about particle physics, or maybe it's just that there's

0:39:09.920 --> 0:39:12.360
<v Speaker 1>another related topic you've always wanted to hear about, or

0:39:12.400 --> 0:39:15.480
<v Speaker 1>maybe it's something we just never ever mentioned right to us.

0:39:15.560 --> 0:39:18.120
<v Speaker 1>Let us know what you think. Text stuff at Discovery

0:39:18.200 --> 0:39:21.160
<v Speaker 1>dot com is our email address, and you can also

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<v Speaker 1>let us know on Facebook, Twitter, or tumbler. We are

0:39:24.719 --> 0:39:27.319
<v Speaker 1>a tech stuff hs W at all three of those,

0:39:27.680 --> 0:39:29.960
<v Speaker 1>and Lauren and I will talk to you again really

0:39:30.000 --> 0:39:36.760
<v Speaker 1>soon for more on this and thousands of other topics.

0:39:36.840 --> 0:39:44.000
<v Speaker 1>Does it has stuff works dot com