WEBVTT - Rerun:  Is Carbon Dating on the way out?

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<v Speaker 1>Welcome to tech Stuff, a production from my Heart Radio.

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<v Speaker 1>Hey there, and welcome to tex Stuff. I'm your host,

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<v Speaker 1>Jonathan Strickland. I'm an executive producer with I Heart Radio,

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<v Speaker 1>and I love all things tech and typically I would

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<v Speaker 1>have a news episode for you on today, which is Thursday,

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<v Speaker 1>April twenty one, but this week got away from the

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<v Speaker 1>big time. On the bright side, we have a really

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<v Speaker 1>cool thing coming up early next month that um tech

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<v Speaker 1>Stuff is taking part in that I think you guys

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<v Speaker 1>are really gonna dig. But that doesn't help me today,

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<v Speaker 1>does it. So instead of a news episode, we're going

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<v Speaker 1>to have a little bit of a classic episode here.

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<v Speaker 1>I thought, because I'm feeling so very old as I

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<v Speaker 1>try to to make sure I have these episodes ready

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<v Speaker 1>for you guys, it would be good to kind of

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<v Speaker 1>take stock. And by that I mean we're going to

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<v Speaker 1>listen to a classic episode called is carbon Dating on

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<v Speaker 1>the Way Out? This episode originally published on August two

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<v Speaker 1>thousand and fifteen. I hope you enjoy. This comes from

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<v Speaker 1>nikkil Cardale, and I do apologize that I'm sure I

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<v Speaker 1>mispronounced your name. The request was, could you do an

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<v Speaker 1>episode explaining this carbon dating is pretty useful, So this

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<v Speaker 1>effect seems relevant and uh Cardale actually uh commented on

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<v Speaker 1>and and included another tweet from real scientists that included

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<v Speaker 1>an article titled will our fossil use ruin our ability

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<v Speaker 1>to use carbon dating as a scientific tool? This is

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<v Speaker 1>really fascinating the idea of using carbon dating, uh, and

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<v Speaker 1>how that that method might be in jeopardy because the

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<v Speaker 1>use of fossil fuels. So I thought I would go

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<v Speaker 1>into that explain what carbon dating is and why it

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<v Speaker 1>might not be an accurate means of telling how old

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<v Speaker 1>something is after too long. So going into the article,

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<v Speaker 1>it's about how the enormous amount of carbon emissions we

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<v Speaker 1>generate could make carbon dating and unreliable means to determine

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<v Speaker 1>the age of certain types of materials. But to understand

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<v Speaker 1>how that's possible, we need to know how carbon dating

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<v Speaker 1>works first, So we're gonna do a carbon dating one

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<v Speaker 1>oh one. Now, the first thing that we have to

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<v Speaker 1>talk about is carbon fourteen. So the fourteen in carbon

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<v Speaker 1>fourteen tells us it's an isotope of carbon. This particular

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<v Speaker 1>isotope must have eight neutrons because carbon has six protons.

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<v Speaker 1>You can change the number of neutrons in an atom.

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<v Speaker 1>That's the different types of isotopes atoms may have. But

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<v Speaker 1>you can't change the number of protons and atom has

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<v Speaker 1>without changing that element. So carbon had six protons, and

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<v Speaker 1>if you change that number of protons, you change the

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<v Speaker 1>element itself. It acts reacts differently in chemical operations, and

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<v Speaker 1>uh is no longer carbon. So carbon twelve is the

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<v Speaker 1>most common form of carbon that we find. It has

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<v Speaker 1>six protons and six neutrons. Then you have carbon thirteen,

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<v Speaker 1>which is six protons and seven neutrons, and both of

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<v Speaker 1>those are stable forms of carbon. That means they don't decay.

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<v Speaker 1>So if you have carbon twelve or carbon thirteen, you

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<v Speaker 1>put it in a box and you leave for I

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<v Speaker 1>don't know, two billion years, and you come back, you're

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<v Speaker 1>still gonna have carbon twelve or carbon thirteen because they

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<v Speaker 1>remain stable. They do not decay. But carbon fourteen is different.

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<v Speaker 1>It is a radio isotope. Radioisotopes are also known as

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<v Speaker 1>radio nucleides, and these are isotopes of a particular atom

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<v Speaker 1>that have an unstable nucleus. These isotopes undergo what we

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<v Speaker 1>call nuclear decay, and in that process they release some

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<v Speaker 1>excess energy in the form of stuff like gamma rays

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<v Speaker 1>and or subatomic particles. Carbon fourteen undergoes what is called

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<v Speaker 1>beta decay. So when it decays, one of the neutrons

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<v Speaker 1>in the nucleus spontaneously changes into a proton, an electron,

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<v Speaker 1>and an anti neutrino. The nucleus gives the boot to

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<v Speaker 1>the electron and the anti neutrino, but the proton stays behind,

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<v Speaker 1>which means the atom no longer is a carbon atom.

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<v Speaker 1>Since again we mentioned that atoms depend upon the number

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<v Speaker 1>of protons and the nucleus, so the carbon fourteen decays

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<v Speaker 1>into nitrogen fourteen, and nitrogen fourteen has seven protons and

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<v Speaker 1>seven neutrons. Also, by the way, one of the few

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<v Speaker 1>stable elements that has both an odd number of protons

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<v Speaker 1>and an odd number of neutrons uh, and nitrogen fourteen

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<v Speaker 1>is stable. It makes up the vast majority of the

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<v Speaker 1>nitrogen found naturally under Earth, More than of the nitrogen

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<v Speaker 1>found on Earth is nitrogen fourteen. So radioactive decay occurs

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<v Speaker 1>naturally within these isotopes, and it's a spontaneous occurrence. That's

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<v Speaker 1>really important to remember. Carbon fourteen has a radioactive half

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<v Speaker 1>life of about five thousand, seven hundred years. There's some

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<v Speaker 1>confusion about what that means. I find in day to

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<v Speaker 1>day conversations with people who haven't had science in a while.

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<v Speaker 1>You guys who have recently had this in science class,

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<v Speaker 1>you're rolling your eyes right now. But for adults who

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<v Speaker 1>have not taken a science class in a long time,

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<v Speaker 1>this might require some some refreshing. So, half life of

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<v Speaker 1>five thousand, seven hundred years, what does that mean? It

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<v Speaker 1>means if you have a given amount of carbon fourteen,

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<v Speaker 1>after five thousand, seven hundred years or so, you'll have

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<v Speaker 1>only half of that carbon fourteen remaining, the other half

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<v Speaker 1>having undergone decay, radioactive decay and turning into nitrogen. Now,

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<v Speaker 1>this doesn't mean that all the carbon four team will

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<v Speaker 1>be gone after another five thousand, seven hundred years, nor

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<v Speaker 1>doesn't mean that carbon fourteen has a full life of

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<v Speaker 1>eleven thousand, four hundred years or anything like that. In fact,

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<v Speaker 1>what it really means is that after another five thousand,

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<v Speaker 1>seven hundred years, half of the remaining sample will have decayed,

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<v Speaker 1>leaving you with about a quarter of what you started with.

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<v Speaker 1>And another five thousand, seven hundred years if that means

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<v Speaker 1>you be left with about an eighth of that sample,

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<v Speaker 1>and so on. Carbon fourteen exists naturally on Earth in

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<v Speaker 1>trace amounts. Before the nineteen forties, the carbon fourteen on

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<v Speaker 1>Earth was created through a natural process. Once in a while,

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<v Speaker 1>cosmic rays, these very high energy particles in outer space,

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<v Speaker 1>would collide with an atom in our atmosphere or upper atmosphere,

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<v Speaker 1>and this collision would end up emitting a high energy

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<v Speaker 1>neutron that then could collide with nitrogen atoms that are

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<v Speaker 1>also way up there in our atmosphere. Now, cosmic rays

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<v Speaker 1>are high energy sub atomic particles. They originate outside of

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<v Speaker 1>our solar system, usually are admitted by supernova of massive stars,

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<v Speaker 1>and these sub atomic particles are primarily atomic nuclei and

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<v Speaker 1>high energy protons. So this collision of the high energy

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<v Speaker 1>neutron with the nitrogen forces a proton to leave the

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<v Speaker 1>nucleus and the in fourteen changes to C fourteen. So,

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<v Speaker 1>in other words, nitrogen fourteen turns to carbon fourteen. So

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<v Speaker 1>instead of having seven protons and seven neutrons, the new

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<v Speaker 1>atom has six protons and eight neutrons. The proton that

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<v Speaker 1>was broken off from the nucleus zooms off with an electron,

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<v Speaker 1>so you get one proton and one electron. That means

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<v Speaker 1>you have an atom of hydrogen. So again what's happening

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<v Speaker 1>is a high energy neutron collides with nitrogen fourteen, forces

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<v Speaker 1>out a proton. The proton and an electron high tail

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<v Speaker 1>it and honeymoon off as hydrogen and the incoming neutron

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<v Speaker 1>joins the party, and now you've got carbon fourteen. So

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<v Speaker 1>pre nineteen forties, carbon fourteen is rare because of two reasons.

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<v Speaker 1>It undergoes radioactive decay, so over time it disappears, and

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<v Speaker 1>it's produced by an event that's not super frequent, though

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<v Speaker 1>it's also not uncommon, so it does happen regularly enough

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<v Speaker 1>that carbon fourteen is replenished, but it's a very small

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<v Speaker 1>overall percentage of the carbon here on Earth. We've got

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<v Speaker 1>some more to say about carbon dating in just a second,

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<v Speaker 1>but first let's take a quick break for our sponsor. Now,

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<v Speaker 1>living things here on Earth absorb carbon through various means,

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<v Speaker 1>and some of that carbon is carbon fourteen. So it

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<v Speaker 1>maybe that you know, you eat a plant in that

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<v Speaker 1>plant has some of the carbon fourteen in it. Now

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<v Speaker 1>you have some of the carbon fourteen and you and

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<v Speaker 1>if we know the ratio of carbon fourteen to the

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<v Speaker 1>stable form of carbon twelve, we can look at materials

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<v Speaker 1>and analyze them to see how the ratio of carbon

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<v Speaker 1>fourteen to carbon twelve in the material stacks up to

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<v Speaker 1>the standard ratio. With living things, this becomes a matter

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<v Speaker 1>of looking at how much carbon fourteen is not there?

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<v Speaker 1>All right, That's it's a little confusing. Let me explain. So,

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<v Speaker 1>when a living thing is still alive, it accumulates carbon

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<v Speaker 1>at about the same rate it loses carbon, so carbon

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<v Speaker 1>cosmic rays produced this carbon fourteen frequently enough that the

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<v Speaker 1>ratio between carbon fourteen and carbon twelve remains steady, So

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<v Speaker 1>the percentage of carbon fourteen to carbon twelve is fairly standardized.

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<v Speaker 1>But when a living thing stops being alive and turns

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<v Speaker 1>into a not living anymore thing, it stops accumulating carbon,

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<v Speaker 1>so it has the carbon that it has inside of

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<v Speaker 1>it stays. That's it. You're not losing anymore. You're not

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<v Speaker 1>gaining any more except for carbon fourteen because carbon fourteen

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<v Speaker 1>undergoes radioactive decay, so over time, some of that carbon

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<v Speaker 1>fourteen starts to convert to nitrogen. So that means if

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<v Speaker 1>you can look at the remains of a living thing

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<v Speaker 1>and detect the ratio of carbon fourteen to carbon twelve.

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<v Speaker 1>You can get an idea of how long ago it

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<v Speaker 1>was that it stopped taking in carbon, as in, how

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<v Speaker 1>long ago was it that this lip, once living thing died.

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<v Speaker 1>It gets a little more complicated than all that, but

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<v Speaker 1>here's the basic rule. If we want to be really precise,

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<v Speaker 1>here's the equation we use to determine the age of

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<v Speaker 1>a sample of material. You have an equation where you

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<v Speaker 1>take the natural logarithm of n F divided by n

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<v Speaker 1>o uh that in turn is divided by negative point

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<v Speaker 1>six nine three, and then you multiply it by t

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<v Speaker 1>uh one half, so one half t the natural logarithm

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<v Speaker 1>is a specific logarithm applied to this equation and other

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<v Speaker 1>things as well. N F divided and oh actually refers

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<v Speaker 1>to the percentage of carbon fourteen and the sample compared

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<v Speaker 1>to the amount found in living stuff today at times

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<v Speaker 1>one half is the half life of carbon, so that's

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<v Speaker 1>five thousand, seven hundred years. So it was a lot

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<v Speaker 1>easier to understand this if we take a specific example.

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<v Speaker 1>So let's say you've got a sample of some sort

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<v Speaker 1>of material and you have determined that there is five

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<v Speaker 1>percent of the amount of carbon fourteen in that material

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<v Speaker 1>compared to what you would find in something that is alive.

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<v Speaker 1>Right now, so you take a sample of a living thing,

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<v Speaker 1>and then you take the sample of the thing you're testing.

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<v Speaker 1>You see that the thing you're testing only has five

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<v Speaker 1>percent of the carbon fourteen you would find in living things.

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<v Speaker 1>That means you would fill out the equation with the

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<v Speaker 1>natural logarithm of point zero five divided by negative point

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<v Speaker 1>six nine three, and you multiply that that result to

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<v Speaker 1>with five thousand, seven hundred years. The natural lug ay

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<v Speaker 1>them at point zero five, by the way, in case

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<v Speaker 1>you don't want to whip out your calculator, is negative

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<v Speaker 1>two point nine nine five seven three to two seven

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<v Speaker 1>three five five. If you divide that by negative point

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<v Speaker 1>six nine three, you get four point three to two

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<v Speaker 1>eight four five. Don't dial that number. If you take

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<v Speaker 1>that number, the four point three, etcetera, and you multiply

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<v Speaker 1>that by five thousand, seven hundred years, you end up

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<v Speaker 1>with twenty four thousand, six hundred forty point two years.

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<v Speaker 1>I mean, the stuff you're looking at died somewhere around

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<v Speaker 1>that time frame, give or take thirty two hundred years,

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<v Speaker 1>So somewhere on twenty four thousand, six hundred forty years

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<v Speaker 1>ago is when that thing no longer breathed or lived,

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<v Speaker 1>or however you wanted to find it. By the way,

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<v Speaker 1>this approach does have a limitation. Anything older than sixty

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<v Speaker 1>thousand years is pretty much out of bounds. Carbon fourteen

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<v Speaker 1>just isn't a reliable means of dating that sort of material,

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<v Speaker 1>and we have to rely on other methods so and

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<v Speaker 1>fourteen because of the decay once against two very small amounts,

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<v Speaker 1>it's very difficult to narrow it down to a specific time,

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<v Speaker 1>and if it's long enough, there won't be any carbon

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<v Speaker 1>fourteen at all all the carbon fourteen will have decayed

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<v Speaker 1>by then. You can't use carbon dating if there's no

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<v Speaker 1>carbon fourteen left. So to actually test the carbon fourteen concentration,

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<v Speaker 1>you first have to take the sample, uh whatever object

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<v Speaker 1>it might be. You have to remove part of it,

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<v Speaker 1>and typically you would apply some chemicals to the material,

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<v Speaker 1>usually a very strong acid wash and a strong base wash.

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<v Speaker 1>That's to remove all the contaminating materials that could end

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<v Speaker 1>up giving you false readings on carbon fourteen. Then you

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<v Speaker 1>would burn the sample within a glass container to capture

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<v Speaker 1>the carbon dioxide that is emitted when you burn the material.

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<v Speaker 1>And then you would analyze the carbon dioxide to find

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<v Speaker 1>out the concentration of carbon fourteen. So you can see

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<v Speaker 1>that this approach has a big drawback. It ends up

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<v Speaker 1>damaging whatever it is you are attempting to date in

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<v Speaker 1>the first place. And that's why some particularly high valued

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<v Speaker 1>items go without being tested, because the perception is that

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<v Speaker 1>even a small sample of that original piece would be

0:14:16.679 --> 0:14:21.240
<v Speaker 1>too much damage to to uh make on this item.

0:14:21.360 --> 0:14:25.040
<v Speaker 1>So certain items are considered very precious and there's a

0:14:25.080 --> 0:14:28.920
<v Speaker 1>big resistance to using carbon dating because by definition, you're

0:14:28.920 --> 0:14:32.040
<v Speaker 1>going to be damaging the material. Now, there's several lines

0:14:32.080 --> 0:14:35.960
<v Speaker 1>of research they're exploring possible non destructive means of using

0:14:36.080 --> 0:14:40.800
<v Speaker 1>radiocarbon dating. There's one that uses plasma oxidation and the

0:14:40.920 --> 0:14:44.600
<v Speaker 1>use of non destructive washes to clean samples of those

0:14:44.840 --> 0:14:48.840
<v Speaker 1>contaminating humic acids, which would lead to errors if they

0:14:48.840 --> 0:14:52.920
<v Speaker 1>remain behind. But those are still largely in the testing

0:14:52.960 --> 0:14:56.640
<v Speaker 1>phase and aren't the common means of using carbon dating. Also,

0:14:57.040 --> 0:14:59.600
<v Speaker 1>keep in mind that we use this method to estimate

0:14:59.640 --> 0:15:02.600
<v Speaker 1>the date of things made from organic materials, like the

0:15:02.640 --> 0:15:06.680
<v Speaker 1>Dead Sea scrolls, but this estimation is based upon when

0:15:06.720 --> 0:15:10.000
<v Speaker 1>the materials were harvested So, in other words, whenever the

0:15:10.080 --> 0:15:12.880
<v Speaker 1>living thing that the materials came from stopped being alive,

0:15:14.040 --> 0:15:16.640
<v Speaker 1>it doesn't tell us the date of when the artifact

0:15:16.720 --> 0:15:19.600
<v Speaker 1>was actually produced. So it's possible that you could come

0:15:19.640 --> 0:15:23.480
<v Speaker 1>across an artifact like a scroll, and you use carbon

0:15:23.560 --> 0:15:26.600
<v Speaker 1>dating on it and find out that the scroll material

0:15:27.240 --> 0:15:29.760
<v Speaker 1>is two thousand years old, meaning two thousand years ago

0:15:30.480 --> 0:15:34.480
<v Speaker 1>whatever the scroll was made out of stopped living, But

0:15:34.520 --> 0:15:38.360
<v Speaker 1>it doesn't tell you about the contents written in the scroll.

0:15:38.480 --> 0:15:42.080
<v Speaker 1>It's possible that the contents were added to the scroll

0:15:42.360 --> 0:15:46.920
<v Speaker 1>much after the living thing stopped being alive. Still, it's

0:15:46.920 --> 0:15:49.080
<v Speaker 1>a pretty good bet that the two are within the

0:15:49.120 --> 0:15:52.520
<v Speaker 1>same neighborhood of time, rather than someone held onto blank

0:15:52.600 --> 0:15:55.800
<v Speaker 1>scrolls for a few centuries before finally jotting something down.

0:15:57.280 --> 0:15:59.680
<v Speaker 1>All right, it's all this is cool, But how did

0:15:59.680 --> 0:16:03.000
<v Speaker 1>we even figure out radio Carbon dating would be a

0:16:03.040 --> 0:16:06.920
<v Speaker 1>possible way of figuring out how old something is. Well,

0:16:06.960 --> 0:16:09.360
<v Speaker 1>some early discoveries were made in the nineteen thirties at

0:16:09.360 --> 0:16:13.280
<v Speaker 1>the Lawrence Radiation Laboratory in Berkeley, and you probably remember

0:16:13.320 --> 0:16:15.720
<v Speaker 1>that if you've been listening to tech stuff. It factored

0:16:15.760 --> 0:16:18.120
<v Speaker 1>heavily into the discussion I had with Ben Boland about

0:16:18.160 --> 0:16:24.200
<v Speaker 1>the Manhattan Project. So Franz Curry, an American physicist, observed

0:16:24.240 --> 0:16:27.520
<v Speaker 1>something really interesting when he irradiated a cloud of air

0:16:27.640 --> 0:16:31.760
<v Speaker 1>in a cloud chamber. He used neutrons to UH to

0:16:31.920 --> 0:16:36.400
<v Speaker 1>irradiate that cloud, and he saw proton recoil tracks that

0:16:36.480 --> 0:16:40.920
<v Speaker 1>indicated something was losing protons. So he concluded that the

0:16:41.000 --> 0:16:44.880
<v Speaker 1>neutrons that he was using were colliding with nitrogen fourteen

0:16:45.440 --> 0:16:48.240
<v Speaker 1>and producing what was believed to be a form of

0:16:48.280 --> 0:16:51.720
<v Speaker 1>carbon as a result, with hydrogen being the other product

0:16:51.760 --> 0:16:55.320
<v Speaker 1>of this collision. His work was further explored by physicists

0:16:55.360 --> 0:16:59.640
<v Speaker 1>like Tom W. Bonner, W. M. Brubaker, W. J. Burcham,

0:17:00.000 --> 0:17:04.080
<v Speaker 1>and Maurice gold Hauber. Now collectively, this laid the foundation

0:17:04.119 --> 0:17:07.160
<v Speaker 1>for the simple equation of a high energy neutron plus

0:17:07.280 --> 0:17:12.400
<v Speaker 1>nitrogen fourteen produces one hydrogen atom and one carbon fourteen atom.

0:17:12.520 --> 0:17:15.280
<v Speaker 1>Then you had Narrico Fermi. We talked about him in

0:17:15.320 --> 0:17:18.639
<v Speaker 1>the Manhattan Project, and his work showed that the cross

0:17:18.640 --> 0:17:21.760
<v Speaker 1>section of a nitrogen fourteen atom was much larger than

0:17:21.800 --> 0:17:26.760
<v Speaker 1>other materials, and that suggested that neutron and nitrogen collisions

0:17:26.840 --> 0:17:29.800
<v Speaker 1>might happen fairly regularly in nature as long as there

0:17:29.840 --> 0:17:33.480
<v Speaker 1>were a supply of high energy neutrons. All right, we

0:17:33.600 --> 0:17:36.160
<v Speaker 1>got a little bit more about carbon dating, and then

0:17:36.840 --> 0:17:47.440
<v Speaker 1>what's It's back to reality for me? I guess so

0:17:47.880 --> 0:17:50.320
<v Speaker 1>Sage Korff, who was a physicist who was born in

0:17:50.359 --> 0:17:53.399
<v Speaker 1>Finland and whose family immigrated to the United States in

0:17:53.400 --> 0:17:57.560
<v Speaker 1>the early twentieth century, he discovered the phenomenon that cosmic

0:17:57.680 --> 0:18:01.199
<v Speaker 1>rays interact with atoms and produce high energy neutrons in

0:18:01.240 --> 0:18:06.440
<v Speaker 1>the upper atmosphere. So Pharem's prediction and course observation, we're

0:18:06.480 --> 0:18:11.120
<v Speaker 1>starting to kind of coalesce here. The observations convinced scientists

0:18:11.160 --> 0:18:14.879
<v Speaker 1>that the neutrons themselves were not cosmic rays, because the

0:18:14.880 --> 0:18:18.400
<v Speaker 1>neutrons had a lifespan of just eighteen minutes, and therefore

0:18:19.000 --> 0:18:21.560
<v Speaker 1>a neutron wouldn't be able to survive the long trip

0:18:21.600 --> 0:18:25.120
<v Speaker 1>through space. They must have been something else first, so

0:18:25.160 --> 0:18:27.720
<v Speaker 1>they said the neutrons had to be a byproduct of

0:18:27.760 --> 0:18:31.439
<v Speaker 1>another interaction. A cosmic ray must be interacting with something

0:18:31.440 --> 0:18:35.440
<v Speaker 1>in the atmosphere. That interaction caused this high energy neutron

0:18:35.480 --> 0:18:38.600
<v Speaker 1>to be emitted, and Quarter hypothesized that these neutrons could

0:18:38.640 --> 0:18:41.919
<v Speaker 1>then interact with nitrogen fourteen to produce carbon fourteen in

0:18:41.960 --> 0:18:45.879
<v Speaker 1>the upper atmosphere. Now, it was Willard F. Libby who

0:18:45.960 --> 0:18:48.480
<v Speaker 1>came up with the idea that since carbon fourteen is

0:18:48.560 --> 0:18:51.280
<v Speaker 1>generated at a steady rate due to cosmic ray interactions

0:18:51.280 --> 0:18:54.640
<v Speaker 1>in our atmosphere, you should be able to use it

0:18:54.680 --> 0:18:58.280
<v Speaker 1>to measure how long something has been dead. Libby would

0:18:58.320 --> 0:19:01.520
<v Speaker 1>measure the value of carbon fourteen's half life at five thousand,

0:19:01.640 --> 0:19:04.480
<v Speaker 1>five hundred sixty eight years, give or take thirty years,

0:19:04.840 --> 0:19:08.000
<v Speaker 1>which became known as the Libby half life. And Libby

0:19:08.080 --> 0:19:11.359
<v Speaker 1>himself would be awarded the Nobel Prize in nineteen sixty

0:19:11.440 --> 0:19:15.160
<v Speaker 1>for his work in radiocarbon dating. All right, so that's

0:19:15.200 --> 0:19:18.560
<v Speaker 1>the history of radiocarbon dating and generally how radiocarbon dating works.

0:19:18.920 --> 0:19:22.000
<v Speaker 1>So why is it in trouble or what could possibly

0:19:22.200 --> 0:19:26.120
<v Speaker 1>be causing confusion with radiocarbon dating. Well, there are two

0:19:26.119 --> 0:19:28.840
<v Speaker 1>big things we need to talk about, and one was

0:19:28.960 --> 0:19:30.840
<v Speaker 1>one that I've alluded to a couple of times. I

0:19:30.920 --> 0:19:35.119
<v Speaker 1>mentioned that, you know, pre nineteen forties, you had a

0:19:35.160 --> 0:19:39.520
<v Speaker 1>certain level of carbon fourteen that was pretty standard, but

0:19:39.640 --> 0:19:43.119
<v Speaker 1>the nuclear age really messed things up for us. They

0:19:43.160 --> 0:19:45.879
<v Speaker 1>made carbon fourteen dating a bit tricky. Starting in the

0:19:45.960 --> 0:19:50.000
<v Speaker 1>nineteen forties, we began testing nuclear bombs. Now, these bombs

0:19:50.000 --> 0:19:52.840
<v Speaker 1>released a lot of energy upon exploding, partly in the

0:19:52.880 --> 0:19:55.600
<v Speaker 1>form of high energy neutrons. You could probably see where

0:19:55.600 --> 0:19:58.680
<v Speaker 1>this is going. Some of those high energy neutrons ended

0:19:58.760 --> 0:20:01.719
<v Speaker 1>up interacting with night jan fourteen atoms, which meant that

0:20:01.840 --> 0:20:05.600
<v Speaker 1>it produced carbon fourteen atoms as a result. So the

0:20:05.720 --> 0:20:10.960
<v Speaker 1>concentration of carbon fourteen increased in the wake of nuclear

0:20:11.000 --> 0:20:14.720
<v Speaker 1>bomb testing. So anything that died after the nineteen forties

0:20:14.760 --> 0:20:18.159
<v Speaker 1>actually has a higher concentration of carbon fourteen than the

0:20:18.200 --> 0:20:22.520
<v Speaker 1>stuff that died before the nineteen forties did even at

0:20:22.520 --> 0:20:25.960
<v Speaker 1>the time of death. According to Professor Nalini nod Karnie

0:20:26.080 --> 0:20:29.119
<v Speaker 1>of the Evergreen State College, the nineteen fifties saw a

0:20:29.240 --> 0:20:34.080
<v Speaker 1>one hundred percent spike in carbon fourteen coming into the atmosphere.

0:20:34.800 --> 0:20:38.080
<v Speaker 1>In nineteen sixty three, the United States and Russia agreed

0:20:38.119 --> 0:20:41.359
<v Speaker 1>to stop above ground nuclear testing, and the levels of

0:20:41.359 --> 0:20:44.160
<v Speaker 1>carbon fourteen in the atmosphere gradually dropped down to their

0:20:44.200 --> 0:20:47.119
<v Speaker 1>normal levels. But that means there's a blip in the

0:20:47.160 --> 0:20:51.320
<v Speaker 1>carbon fourteen radar between the nineteen forties and nineteen sixty three.

0:20:51.520 --> 0:20:53.159
<v Speaker 1>So if you put yourself in the shoes of a

0:20:53.280 --> 0:20:58.240
<v Speaker 1>future archaeologist. Radio carbon dating becomes unreliable because the levels

0:20:58.240 --> 0:21:00.920
<v Speaker 1>of carbon fourteen could be decept tip. If the thing

0:21:00.920 --> 0:21:04.520
<v Speaker 1>you're measuring died during the era of nuclear testing, it

0:21:04.600 --> 0:21:07.800
<v Speaker 1>might appear to be younger than you thought because there's

0:21:07.800 --> 0:21:11.480
<v Speaker 1>a higher concentration of carbon fourteen in its sample than

0:21:11.600 --> 0:21:14.840
<v Speaker 1>you otherwise would have expected. So it may seem that

0:21:14.960 --> 0:21:20.000
<v Speaker 1>something died in twenty fifteen as opposed to nineteen sixty three.

0:21:20.680 --> 0:21:24.040
<v Speaker 1>That's just an example. Now to the article that prompted

0:21:24.040 --> 0:21:27.040
<v Speaker 1>this episode in the first place, that's a different case.

0:21:27.400 --> 0:21:30.360
<v Speaker 1>Researchers published a study in the Proceedings of the National

0:21:30.359 --> 0:21:33.320
<v Speaker 1>Academy of Sciences about how the use of fossil fuels

0:21:33.880 --> 0:21:38.000
<v Speaker 1>is further making radiocarbon dating less reliable, and this time

0:21:38.040 --> 0:21:41.040
<v Speaker 1>it's not an excess of carbon fourteen. It's actually the

0:21:41.040 --> 0:21:45.880
<v Speaker 1>opposite problem. Fossil fuels have no carbon fourteen in them

0:21:46.119 --> 0:21:50.800
<v Speaker 1>because they are fossil fuels. This is billions of years old,

0:21:51.440 --> 0:21:54.080
<v Speaker 1>so they're far too old for any carbon fourteen to remain.

0:21:54.160 --> 0:21:57.800
<v Speaker 1>Remember that carbon fourteen is decaying over time and turning

0:21:57.800 --> 0:22:03.200
<v Speaker 1>into nitrogen, so eventually all of those carbon fourteen atoms decay.

0:22:03.320 --> 0:22:06.639
<v Speaker 1>So burning a fossil fuel create releases carbon dioxide, and

0:22:06.680 --> 0:22:09.640
<v Speaker 1>the carbon in that CEO two has no carbon fourteen

0:22:09.640 --> 0:22:13.000
<v Speaker 1>and it's all carbon twolve carbon thirteen. So the more

0:22:13.040 --> 0:22:16.840
<v Speaker 1>fossil fuels we burn, the more we dilute the concentration

0:22:16.840 --> 0:22:20.119
<v Speaker 1>of carbon fourteen that's in the atmosphere. So stuff from

0:22:20.119 --> 0:22:23.080
<v Speaker 1>the nuclear age tends to look younger than it really

0:22:23.160 --> 0:22:26.359
<v Speaker 1>is because of the higher concentration of carbon fourteen. Stuff

0:22:26.440 --> 0:22:29.920
<v Speaker 1>from the later ages of fossil fuel use will look

0:22:30.119 --> 0:22:34.280
<v Speaker 1>older than they really are because carbon fourteen has been diluted. So,

0:22:34.280 --> 0:22:38.000
<v Speaker 1>according to the study, fresh organic material in twenty fifty

0:22:38.280 --> 0:22:41.280
<v Speaker 1>would contain the same amount of carbon fourteen relative to

0:22:41.320 --> 0:22:46.359
<v Speaker 1>carbon twelve as something dating from ten fifty. So you

0:22:46.400 --> 0:22:50.840
<v Speaker 1>have a thousand years of doubt in any radio carbon

0:22:50.920 --> 0:22:54.919
<v Speaker 1>dated samples. You would look at the two samples if

0:22:54.960 --> 0:22:58.400
<v Speaker 1>you if all you had were miniscule samples of two

0:22:58.440 --> 0:23:01.000
<v Speaker 1>things and one of them was a T shirt that

0:23:01.359 --> 0:23:05.400
<v Speaker 1>was made in and another was a piece of cloth

0:23:05.600 --> 0:23:09.280
<v Speaker 1>that dated from ten fifty, and you did radiocarbon dating,

0:23:10.000 --> 0:23:13.280
<v Speaker 1>you'd get the same result. This is not good if

0:23:13.320 --> 0:23:16.280
<v Speaker 1>you are trying to figure out how old something is

0:23:17.520 --> 0:23:20.880
<v Speaker 1>Heather Graven, who authored the study on fossil fuel emissions

0:23:20.920 --> 0:23:23.399
<v Speaker 1>and the effect on radiocarbon dating, says that if we

0:23:23.400 --> 0:23:27.680
<v Speaker 1>were to reduce carbon dioxide emissions drastically in the very

0:23:27.680 --> 0:23:31.359
<v Speaker 1>near future, the effect on future radiocarbon dating would be

0:23:31.359 --> 0:23:34.800
<v Speaker 1>equivalent to inserting a one year error on top of

0:23:34.840 --> 0:23:39.720
<v Speaker 1>any estimation. If we don't drastically reduce emissions, that error

0:23:39.840 --> 0:23:43.320
<v Speaker 1>range will continue to grow over time. One thing that

0:23:43.359 --> 0:23:46.240
<v Speaker 1>the concentration of carbon fourteen tells us is how much

0:23:46.280 --> 0:23:48.760
<v Speaker 1>carbon dioxide in the atmosphere comes from the burning of

0:23:48.800 --> 0:23:52.679
<v Speaker 1>fossil fuels. So as we see the concentration decrease, we

0:23:52.760 --> 0:23:56.439
<v Speaker 1>know that's because proportionally more carbon twelve is being released

0:23:56.440 --> 0:24:00.320
<v Speaker 1>into the atmosphere, diluting the already tiny concentration of carbon fourteen.

0:24:00.600 --> 0:24:03.320
<v Speaker 1>So that's useful for scientists who are studying climate change

0:24:03.320 --> 0:24:07.359
<v Speaker 1>and pollution. That's not exactly a happy story, is it.

0:24:08.520 --> 0:24:13.920
<v Speaker 1>So what are our options if carbon dating becomes unreliable, Well,

0:24:13.960 --> 0:24:16.560
<v Speaker 1>that depends on what you're trying to analyze. If you're

0:24:16.560 --> 0:24:19.680
<v Speaker 1>looking at inorganic stuff like rocks, you don't need to

0:24:19.760 --> 0:24:22.040
<v Speaker 1>use carbon fourteen in the first place. That would be

0:24:22.160 --> 0:24:25.160
<v Speaker 1>pretty much useless. You would use something else like potassium

0:24:25.320 --> 0:24:28.159
<v Speaker 1>argon dating, which is useful to estimate the age of

0:24:28.280 --> 0:24:30.840
<v Speaker 1>rocks that are a hundred thousand years old or younger.

0:24:31.400 --> 0:24:32.959
<v Speaker 1>And if that's not a big enough range, you can

0:24:33.000 --> 0:24:36.320
<v Speaker 1>actually use uranium lead dating, and that will let you

0:24:36.440 --> 0:24:40.560
<v Speaker 1>estimate rocks between one point four and five million years old.

0:24:41.240 --> 0:24:43.240
<v Speaker 1>There's a lot of different options if you're trying to

0:24:43.320 --> 0:24:45.880
<v Speaker 1>date stuff. When it comes to organic materials, however, it's

0:24:45.880 --> 0:24:49.000
<v Speaker 1>a lot more tricky. Radio carbon was a great tool,

0:24:49.960 --> 0:24:53.280
<v Speaker 1>but if it becomes unreliable, we're gonna have to use

0:24:53.359 --> 0:24:58.520
<v Speaker 1>other methods like contextual clues and other items that are

0:24:59.000 --> 0:25:03.800
<v Speaker 1>helping us connect things to dates. So this is a

0:25:03.840 --> 0:25:07.720
<v Speaker 1>big problem. I guess you could argue that's a big

0:25:07.760 --> 0:25:11.640
<v Speaker 1>problem for future generations and perhaps the records we leave

0:25:11.720 --> 0:25:19.640
<v Speaker 1>behind now are so uh so complete, they're so voluminous,

0:25:19.680 --> 0:25:22.960
<v Speaker 1>I guess is the best word. That future generations will

0:25:23.000 --> 0:25:26.640
<v Speaker 1>likely have more than enough material to determine when something

0:25:27.119 --> 0:25:31.879
<v Speaker 1>originated from our time versus earlier times. But the point

0:25:31.920 --> 0:25:36.639
<v Speaker 1>being that the way we're interacting with our world is changing.

0:25:36.680 --> 0:25:42.720
<v Speaker 1>This fundamental ratio of carbon fourteen to carbon twelve, and

0:25:43.200 --> 0:25:46.920
<v Speaker 1>that means that a really brilliant means of determining how

0:25:46.960 --> 0:25:50.800
<v Speaker 1>old something is is not really going to be an

0:25:50.840 --> 0:25:54.560
<v Speaker 1>accurate measure for very much longer. So it's kind of

0:25:54.600 --> 0:25:59.240
<v Speaker 1>a bummer. Obviously for things that are much much much older.

0:25:59.640 --> 0:26:02.359
<v Speaker 1>UH will at least in the short term, not be

0:26:02.560 --> 0:26:04.879
<v Speaker 1>that big of a deal, especially if we can relate

0:26:04.920 --> 0:26:08.400
<v Speaker 1>it to other items that we we already know the

0:26:08.440 --> 0:26:11.960
<v Speaker 1>age of those items. It won't be as destructive as

0:26:11.960 --> 0:26:15.320
<v Speaker 1>saying we can never use radio carbon dating again. We

0:26:15.400 --> 0:26:20.479
<v Speaker 1>just have to keep that changing ratio of carbon fourteen

0:26:20.480 --> 0:26:22.960
<v Speaker 1>to carbon twelve in mind so that we make sure

0:26:23.040 --> 0:26:26.680
<v Speaker 1>we're making accurate measurements. I hope you enjoyed that classic

0:26:26.720 --> 0:26:29.919
<v Speaker 1>episode of tech Stuff. Again, my apologies. I've got a

0:26:29.920 --> 0:26:31.760
<v Speaker 1>lot of things I wish I could have talked about,

0:26:31.920 --> 0:26:35.800
<v Speaker 1>like the fact that there's now a patent for a

0:26:35.840 --> 0:26:40.800
<v Speaker 1>retractable lightsaber blade thing. I really want to talk more

0:26:40.840 --> 0:26:44.440
<v Speaker 1>about that, so maybe next week. But in the meantime,

0:26:44.560 --> 0:26:47.399
<v Speaker 1>if you have any suggestions for topics I should tackle

0:26:47.480 --> 0:26:50.159
<v Speaker 1>on tech Stuff, let me know. Send me a message

0:26:50.200 --> 0:26:53.240
<v Speaker 1>on Twitter. The handle is text stuff h s W.

0:26:54.000 --> 0:27:02.400
<v Speaker 1>I'll talk to you again really soon. Yeah. Text stuff

0:27:02.440 --> 0:27:05.640
<v Speaker 1>is an I heart radio production For more podcasts from

0:27:05.640 --> 0:27:09.400
<v Speaker 1>I heart Radio, visit the i heart Radio app, Apple podcasts,

0:27:09.520 --> 0:27:11.520
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