WEBVTT - Is Carbon Dating on the way out?

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<v Speaker 1>Get in Touch with Technology? What textfrom hofks dot com.

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<v Speaker 1>Hey there, and welcome to text UFF. I'm Jonathan Strickland,

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<v Speaker 1>your beloved host, and I'm on my own today. So uh,

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<v Speaker 1>I will not be throwing it over to anybody because

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<v Speaker 1>they won't be able to talk because they won't be here,

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<v Speaker 1>as opposed to the normal reason where I just talk

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<v Speaker 1>over them. So today I wanted to talk about something

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<v Speaker 1>that was sent in as a listener request. In fact,

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<v Speaker 1>this was sent in over Twitter, and uh, this comes

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<v Speaker 1>from nikkil Cardale, and I do apologize that I'm sure

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<v Speaker 1>I mispronounced your name, but uh, the request was could

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<v Speaker 1>you do an episode explaining this carbon dating is pretty useful?

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<v Speaker 1>So this effect seems relevant and uh Cardale actually uh

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<v Speaker 1>commented on and and included another tweet from real scientists

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<v Speaker 1>that included an article titled will our fossil use ruin

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<v Speaker 1>our ability to use carbon dating as a scientific tool?

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<v Speaker 1>This is really fascinating the idea of using carbon dating, uh,

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<v Speaker 1>and how that that method might be in jeopardy because

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<v Speaker 1>of the use of fossil fuels. So I thought I

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<v Speaker 1>would go into that explain what carbon dating is and

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<v Speaker 1>why it might not be an accurate means of telling

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<v Speaker 1>how old something is after too long. So going into

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<v Speaker 1>the article, it's about how the enormous amount of carbon

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<v Speaker 1>emissions we generate could make carbon dating and unreliable means

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<v Speaker 1>to determine the age of certain types of materials. But

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<v Speaker 1>to understand how that's possible, we need to know how

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<v Speaker 1>carbon dating works first, So we're gonna do a carbon

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<v Speaker 1>dating one oh one. Now, the first thing that we

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<v Speaker 1>have to talk about is carbon fourteen. So the fourteen

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<v Speaker 1>in carbon fourteen tells us it's an isotope of carbon.

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<v Speaker 1>This particular isotope must have eight neutrons because carbon has

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<v Speaker 1>six protons. You can change the number of neutrons in

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<v Speaker 1>an atom. That's the different types of isotopes atoms may have,

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<v Speaker 1>But you can't change the number of protons and atom

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<v Speaker 1>has without changing that element. So carbon has six protons,

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<v Speaker 1>and if you change that number of protons, you change

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<v Speaker 1>the element itself. It acts reacts differently in chemical operations,

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<v Speaker 1>and uh is no longer carbon. So carbon twelve is

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<v Speaker 1>the most common form of carbon that we find. It

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<v Speaker 1>has 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 unearthed, More than of the nitrogen found

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<v Speaker 1>on Earth is nitrogen fourteen. So radioactive decay occurs naturally

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<v Speaker 1>within these isotopes, and it's a spontaneous occurrence. That's really

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<v Speaker 1>important to remember. Carbon fourteen has a radioactive half life

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<v Speaker 1>of about five thousand, seven hundred years. There's some confusion

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<v Speaker 1>about what that means. I find in day to day

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<v Speaker 1>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 fourteen will be

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<v Speaker 1>gone after another five thousand, seven hundred years, nor does

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<v Speaker 1>it 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 collie 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 they're emitted 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 allignes 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. Now, living

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<v Speaker 1>things here on Earth absorb carbon through various means, and

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<v Speaker 1>some of that carbon is carbon fourteen. So it may

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<v Speaker 1>be that you know, you eat a plant and 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 way n O actually

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<v Speaker 1>refers to the percentage of carbon fourteen and the sample

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<v Speaker 1>compared to the amount found in living stuff today at

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<v Speaker 1>times one half is the half life of carbon, so

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<v Speaker 1>that's five thousand, seven hundred years. So it's 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

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<v Speaker 1>alive right now, So you take a sample of a

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<v Speaker 1>living thing, and then you take the sample of the

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<v Speaker 1>thing you're testing. You see that the thing you're testing

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<v Speaker 1>only has five percent of the carbon fourteen you would

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<v Speaker 1>find in living things. That means you would fill out

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<v Speaker 1>the equation with the natural logarithm of point zero five

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<v Speaker 1>divided by negative point six nine three, and you multiply

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<v Speaker 1>that that result to with five thousand, seven hundred years

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<v Speaker 1>the natural logorithm at point zero five. By the way,

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<v Speaker 1>in case you don't want to whip out your calculator

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<v Speaker 1>is negative two point nine nine five seven three to

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<v Speaker 1>two seven three five five. If you divide that by

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<v Speaker 1>negative point six nine three, you get four point three

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<v Speaker 1>to two eight four five night. Don't dial that number.

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<v Speaker 1>If you take that number, the four point three, etcetera,

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<v Speaker 1>and you multiply that by five thousand, seven hundred years,

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<v Speaker 1>you end up with twenty four thousand, six hundred forty

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<v Speaker 1>point two years, meaning the stuff you're looking at died

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<v Speaker 1>somewhere around that time frame, give or take thirty two

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<v Speaker 1>hundred years. So somewhere on twenty four thousand, six hundred

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<v Speaker 1>forty years ago is when that thing no longer breathed

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<v Speaker 1>or lived, or however you wanted to find it. By

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<v Speaker 1>the way, this approach does have a limitation. Anything older

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<v Speaker 1>than sixty thousand years is pretty much out of bounds.

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<v Speaker 1>Carbon fourteen just isn't a reliable means of dating that

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<v Speaker 1>sort of material, and we have to rely on other methods.

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<v Speaker 1>So carbon fourteen, because of the decay once against two

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<v Speaker 1>very small amounts, it's very difficult to narrow it down

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<v Speaker 1>to a specific time, and if it's long enough, there

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<v Speaker 1>won't be any carbon fourteen in at all. All the

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<v Speaker 1>carbon fourteen will have decayed by then you can't use

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<v Speaker 1>carbon dating if there's no carbon fourteen left. So to

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<v Speaker 1>actually test the carbon fourteen concentration, you first have to

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<v Speaker 1>take the sample, uh whatever object it might be. You

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<v Speaker 1>have to remove part of it, and typically you would

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<v Speaker 1>apply some chemicals to the material, usually a very strong

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<v Speaker 1>acid wash and a strong base wash. That's to remove

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<v Speaker 1>all the contaminating materials that could end up giving you

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<v Speaker 1>false readings on carbon fourteen. Then you would burn the

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<v Speaker 1>sample within a glass container to capture the carbon dioxide

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<v Speaker 1>that is emitted when you burn the material, and then

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<v Speaker 1>you would end allize the carbon dioxide to find out

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<v Speaker 1>the concentration of carbon fourteen. So you can see that

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<v Speaker 1>this approach has a big drawback. It ends up damaging

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<v Speaker 1>whatever it is you are attempting to date in the

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<v Speaker 1>first place. And that's why some particularly high valued items

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<v Speaker 1>go without being tested, because the perception is that even

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<v Speaker 1>a small sample of that original piece would be too

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<v Speaker 1>much damage to to uh make on this item. So

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<v Speaker 1>certain items are considered very precious and there's a big

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<v Speaker 1>resistance to using carbon dating because by the definition, you're

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<v Speaker 1>going to be damaging the material. Now there's several lines

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<v Speaker 1>of research they are exploring possible non destructive means of

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<v Speaker 1>using radiocarbon dating. There's one that uses plasma oxidation and

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<v Speaker 1>the use of non destructive washes to clean samples of

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<v Speaker 1>those contaminating humic acids, which would lead to errors if

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<v Speaker 1>they remain behind, but those are still largely in the

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<v Speaker 1>testing phase and aren't the common means of using carbon dating. Also,

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<v Speaker 1>keep in mind that we use this method to estimate

0:14:05.480 --> 0:14:08.400
<v Speaker 1>the date of things made from organic materials, like the

0:14:08.440 --> 0:14:12.520
<v Speaker 1>Dead Sea scrolls, but this estimation is based upon when

0:14:12.559 --> 0:14:15.840
<v Speaker 1>the materials were harvested, so, in other words, whenever the

0:14:15.880 --> 0:14:18.720
<v Speaker 1>living thing that the materials came from stopped being alive,

0:14:19.880 --> 0:14:22.480
<v Speaker 1>it doesn't tell us the date of when the artifact

0:14:22.520 --> 0:14:25.440
<v Speaker 1>was actually produced. So it's possible that you could come

0:14:25.480 --> 0:14:29.320
<v Speaker 1>across an artifact like a scroll and you use carbon

0:14:29.400 --> 0:14:32.440
<v Speaker 1>dating on it and find out that the scroll material

0:14:33.080 --> 0:14:35.600
<v Speaker 1>is two thousand years old, meaning two thousand years ago

0:14:36.320 --> 0:14:40.320
<v Speaker 1>whatever the scroll was made out of stopped living, but

0:14:40.360 --> 0:14:44.160
<v Speaker 1>it doesn't tell you about the contents written in the scroll.

0:14:44.320 --> 0:14:47.920
<v Speaker 1>It's possible that the contents were added to the scroll

0:14:48.200 --> 0:14:52.760
<v Speaker 1>much after the living thing stopped being alive. Still, it's

0:14:52.760 --> 0:14:54.920
<v Speaker 1>a pretty good bet that the two are within the

0:14:54.960 --> 0:14:58.360
<v Speaker 1>same neighborhood of time, rather than someone held onto blank

0:14:58.400 --> 0:15:01.640
<v Speaker 1>scrolls for a few centuries before or finally jotting something down.

0:15:03.120 --> 0:15:05.520
<v Speaker 1>All right, it's all this is cool, But how did

0:15:05.560 --> 0:15:08.800
<v Speaker 1>we even figure out? Radio carbon dating would be a

0:15:08.880 --> 0:15:12.760
<v Speaker 1>possible way of figuring out how old something is. Well.

0:15:12.800 --> 0:15:15.160
<v Speaker 1>Some early discoveries were made in the nineteen thirties at

0:15:15.200 --> 0:15:19.120
<v Speaker 1>the Lawrence Radiation Laboratory in Berkeley, and you probably remember

0:15:19.160 --> 0:15:21.560
<v Speaker 1>that if you've been listening to tech stuff. It factored

0:15:21.560 --> 0:15:23.960
<v Speaker 1>heavily into the discussion I had with Ben Bolan about

0:15:23.960 --> 0:15:30.040
<v Speaker 1>the Manhattan Project. So Franz Curry, an American physicist, observed

0:15:30.080 --> 0:15:33.280
<v Speaker 1>something really interesting when he irradiated a cloud of air

0:15:33.480 --> 0:15:37.600
<v Speaker 1>in a cloud chamber. He used neutrons to uh to

0:15:37.720 --> 0:15:42.240
<v Speaker 1>irradiate that cloud, and he saw proton recoil tracks that

0:15:42.280 --> 0:15:46.760
<v Speaker 1>indicated something was losing protons. So he concluded that the

0:15:46.840 --> 0:15:50.720
<v Speaker 1>neutrons that he was using were colliding with nitrogen fourteen

0:15:51.280 --> 0:15:54.040
<v Speaker 1>and producing what was believed to be a form of

0:15:54.080 --> 0:15:57.520
<v Speaker 1>carbon as a result. With hydrogen being the other product

0:15:57.560 --> 0:16:00.440
<v Speaker 1>of this collision, his work was further expo or by

0:16:00.440 --> 0:16:05.480
<v Speaker 1>physicists like Tom W. Bonner, W. M. Brubaker, W. J. Burcham,

0:16:05.760 --> 0:16:09.880
<v Speaker 1>and Maurice gold Hauber. Now collectively, this laid the foundation

0:16:09.960 --> 0:16:12.960
<v Speaker 1>for the simple equation of a high energy neutron plus

0:16:13.120 --> 0:16:18.240
<v Speaker 1>nitrogen fourteen produces one hydrogen atom and one carbon fourteen atom.

0:16:18.360 --> 0:16:21.120
<v Speaker 1>Then you had Enrico Fermi. We talked about him in

0:16:21.160 --> 0:16:24.440
<v Speaker 1>the Manhattan Project, and his work showed that the cross

0:16:24.480 --> 0:16:27.600
<v Speaker 1>section of a nitrogen fourteen atom was much larger than

0:16:27.600 --> 0:16:32.600
<v Speaker 1>other materials, and that suggested that neutron and nitrogen collisions

0:16:32.640 --> 0:16:35.640
<v Speaker 1>might happen fairly regularly in nature as long as there

0:16:35.680 --> 0:16:39.040
<v Speaker 1>were a supply of high energy neutrons. Then you have

0:16:39.120 --> 0:16:41.880
<v Speaker 1>a Serge Korf, who was a physicist who was born

0:16:41.880 --> 0:16:44.960
<v Speaker 1>in Finland and whose family immigrated to the United States

0:16:45.000 --> 0:16:48.480
<v Speaker 1>in the early twentieth century. He discovered the phenomenon that

0:16:48.720 --> 0:16:52.760
<v Speaker 1>cosmic rays interact with atoms and produce high energy neutrons

0:16:52.800 --> 0:16:57.840
<v Speaker 1>in the upper atmosphere. So Faremi's prediction and corpse observation

0:16:57.960 --> 0:17:02.400
<v Speaker 1>we're starting to kind of coalesce here. The observations convinced

0:17:02.400 --> 0:17:06.440
<v Speaker 1>scientists that the neutrons themselves were not cosmic rays, because

0:17:06.480 --> 0:17:09.560
<v Speaker 1>the neutrons had a lifespan of just eighteen minutes, and

0:17:09.600 --> 0:17:12.840
<v Speaker 1>therefore a neutron wouldn't be able to survive the long

0:17:12.920 --> 0:17:15.760
<v Speaker 1>trip through space. They must have been something else first,

0:17:16.640 --> 0:17:18.880
<v Speaker 1>So they said the neutrons had to be a byproduct

0:17:19.320 --> 0:17:22.639
<v Speaker 1>of another interaction. A cosmic ray must be interacting with

0:17:22.760 --> 0:17:26.680
<v Speaker 1>something in the atmosphere. That interaction caused this high energy

0:17:26.720 --> 0:17:30.040
<v Speaker 1>neutron to be omitted, and Core hypothesized that these neutrons

0:17:30.080 --> 0:17:33.440
<v Speaker 1>could then interact with nitrogen fourteen to produce carbon fourteen

0:17:33.520 --> 0:17:37.399
<v Speaker 1>in the upper atmosphere. Now, it was Willard F. Libby

0:17:37.440 --> 0:17:40.000
<v Speaker 1>who came up with the idea that since carbon fourteen

0:17:40.119 --> 0:17:42.439
<v Speaker 1>is generated at a steady rate due to cosmic ray

0:17:42.480 --> 0:17:46.120
<v Speaker 1>interactions in our atmosphere, you should be able to use

0:17:46.160 --> 0:17:49.760
<v Speaker 1>it to measure how long something has been dead. Libby

0:17:49.760 --> 0:17:52.360
<v Speaker 1>would measure the value of carbon fourteen's half life at

0:17:52.440 --> 0:17:55.360
<v Speaker 1>five thousand, five hundred sixty eight years, give or take

0:17:55.440 --> 0:17:58.879
<v Speaker 1>thirty years, which became known as the Libby half life,

0:17:59.160 --> 0:18:02.000
<v Speaker 1>and Libby, him off, would be awarded the Nobel Prize

0:18:02.000 --> 0:18:06.159
<v Speaker 1>in nineteen sixty for his work in radiocarbon dating. All right,

0:18:06.560 --> 0:18:08.919
<v Speaker 1>so that's the history of radiocarbon dating and generally how

0:18:09.040 --> 0:18:12.640
<v Speaker 1>radiocarbon dating works. So why is it in trouble or

0:18:12.680 --> 0:18:17.280
<v Speaker 1>what could possibly be causing confusion with radiocarbon dating. Well,

0:18:17.320 --> 0:18:19.280
<v Speaker 1>there are two big things we need to talk about,

0:18:19.840 --> 0:18:22.040
<v Speaker 1>and one was one that I've alluded to a couple

0:18:22.040 --> 0:18:25.920
<v Speaker 1>of times. I mentioned that, you know, pre nineteen forties

0:18:26.320 --> 0:18:29.000
<v Speaker 1>you had a certain level of carbon fourteen that was

0:18:29.080 --> 0:18:33.840
<v Speaker 1>pretty standard. But the nuclear age really messed things up

0:18:33.840 --> 0:18:37.040
<v Speaker 1>for us. They made carbon fourteen dating a bit tricky.

0:18:37.119 --> 0:18:41.080
<v Speaker 1>Starting in the nineteen forties, we began testing nuclear bombs. Now,

0:18:41.119 --> 0:18:44.320
<v Speaker 1>these bombs released a lot of energy upon exploding, partly

0:18:44.320 --> 0:18:46.879
<v Speaker 1>in the form of high energy neutrons. You can probably

0:18:46.880 --> 0:18:49.240
<v Speaker 1>see where this is going. Some of those high energy

0:18:49.240 --> 0:18:53.240
<v Speaker 1>neutrons ended up interacting with nitrogen fourteen atoms, which meant

0:18:53.240 --> 0:18:57.040
<v Speaker 1>that it produced carbon fourteen atoms as a result. So

0:18:57.119 --> 0:19:01.399
<v Speaker 1>the concentration of carbon fourteen in priest in the wake

0:19:01.880 --> 0:19:05.520
<v Speaker 1>of nuclear bomb testing. So anything that died after the

0:19:05.600 --> 0:19:09.280
<v Speaker 1>nineteen forties actually has a higher concentration of carbon fourteen

0:19:09.560 --> 0:19:12.760
<v Speaker 1>than the stuff that died before the nineteen forties did

0:19:13.280 --> 0:19:16.720
<v Speaker 1>even know at the time of death. According to Professor Nalini,

0:19:16.880 --> 0:19:20.439
<v Speaker 1>not Khannie of the Evergreen State College. The nineteen fifties

0:19:20.440 --> 0:19:24.879
<v Speaker 1>saw a one hundred percent spike in carbon fourteen coming

0:19:24.880 --> 0:19:28.720
<v Speaker 1>into the atmosphere. In nineteen sixty three, the United States

0:19:28.760 --> 0:19:32.480
<v Speaker 1>and Russia agreed to stop above ground nuclear testing, and

0:19:32.520 --> 0:19:35.280
<v Speaker 1>the levels of carbon fourteen in the atmosphere gradually dropped

0:19:35.280 --> 0:19:37.800
<v Speaker 1>down to their normal levels. But that means there's a

0:19:37.880 --> 0:19:41.480
<v Speaker 1>blip in the carbon fourteen radar between the nineteen forties

0:19:41.520 --> 0:19:44.119
<v Speaker 1>and nineteen sixty three. So if you put yourself in

0:19:44.119 --> 0:19:48.399
<v Speaker 1>the shoes of a future archaeologist, radio carbon dating becomes

0:19:48.480 --> 0:19:51.879
<v Speaker 1>unreliable because the levels of carbon fourteen could be deceptive.

0:19:52.119 --> 0:19:54.760
<v Speaker 1>If the thing you're measuring died during the era of

0:19:54.840 --> 0:19:58.399
<v Speaker 1>nuclear testing, it might appear to be younger than you

0:19:58.480 --> 0:20:01.800
<v Speaker 1>thought because there's a higher concentration of carbon fourteen in

0:20:01.880 --> 0:20:05.639
<v Speaker 1>its sample then you otherwise would have expected. So it

0:20:05.720 --> 0:20:10.240
<v Speaker 1>may seem that something died in twenty fifteen as opposed

0:20:10.240 --> 0:20:14.480
<v Speaker 1>to nineteen sixty three. That's just an example. Now to

0:20:14.560 --> 0:20:17.000
<v Speaker 1>the article that prompted this episode in the first place,

0:20:17.440 --> 0:20:20.720
<v Speaker 1>that's a different case. Researchers published a study in the

0:20:20.720 --> 0:20:23.760
<v Speaker 1>Proceedings of the National Academy of Sciences about how the

0:20:23.840 --> 0:20:28.520
<v Speaker 1>use of fossil fuels is further making radiocarbon dating less reliable.

0:20:29.080 --> 0:20:32.080
<v Speaker 1>And this time it's not an excess of carbon fourteen.

0:20:32.119 --> 0:20:36.280
<v Speaker 1>It's actually the opposite problem. Fossil fuels have no carbon

0:20:36.359 --> 0:20:40.439
<v Speaker 1>fourteen in them because they are fossil fuels. This is

0:20:40.840 --> 0:20:44.280
<v Speaker 1>billions of years old, so they're far too old for

0:20:44.320 --> 0:20:47.320
<v Speaker 1>any carbon fourteen to remain. Remember that carbon fourteen is

0:20:47.400 --> 0:20:52.000
<v Speaker 1>decaying over time and turning into nitrogen, so eventually all

0:20:52.040 --> 0:20:56.000
<v Speaker 1>of those carbon fourteen atoms decay. So burning a fossil

0:20:56.040 --> 0:20:59.280
<v Speaker 1>fuel create releases carbon dioxide, and the carbon in that

0:20:59.359 --> 0:21:02.119
<v Speaker 1>CEO two has no carbon fourteen and it's all carbon

0:21:02.160 --> 0:21:05.800
<v Speaker 1>twolve carbon thirteen. So the more fossil fuels we burn,

0:21:06.240 --> 0:21:09.720
<v Speaker 1>the more we dilute the concentration of carbon fourteen that's

0:21:09.720 --> 0:21:13.280
<v Speaker 1>in the atmosphere. So stuff from the nuclear age tends

0:21:13.320 --> 0:21:15.680
<v Speaker 1>to look younger than it really is because of the

0:21:15.760 --> 0:21:19.400
<v Speaker 1>higher concentration of carbon fourteen. Stuff from the later ages

0:21:19.520 --> 0:21:22.960
<v Speaker 1>of fossil fuel use will look older than they really

0:21:23.000 --> 0:21:26.480
<v Speaker 1>are because carbon fourteen has been deluded. So, according to

0:21:26.520 --> 0:21:30.520
<v Speaker 1>the study, fresh organic material in twenty fifty would contain

0:21:30.560 --> 0:21:33.760
<v Speaker 1>the same amount of carbon fourteen relative to carbon twelve

0:21:34.240 --> 0:21:38.320
<v Speaker 1>as something dating from ten fifty, So you have a

0:21:38.440 --> 0:21:43.560
<v Speaker 1>thousand years of doubt in any radio carbon dated samples.

0:21:44.560 --> 0:21:46.919
<v Speaker 1>You would look at the two samples if you if

0:21:47.040 --> 0:21:50.480
<v Speaker 1>all you had were miniscule samples of two things and

0:21:50.560 --> 0:21:53.600
<v Speaker 1>one of them was a T shirt that was made

0:21:53.640 --> 0:21:57.040
<v Speaker 1>in twenty fifty, and another was a piece of cloth

0:21:57.280 --> 0:22:00.159
<v Speaker 1>that dated from ten fifty, and you did do you

0:22:00.240 --> 0:22:04.199
<v Speaker 1>carbon dating, you'd get the same result. This is not

0:22:04.320 --> 0:22:07.080
<v Speaker 1>good if you are trying to figure out how old

0:22:07.320 --> 0:22:11.760
<v Speaker 1>something is. Heather Graven, who authored the study on fossil

0:22:11.800 --> 0:22:14.719
<v Speaker 1>fuel emissions and the effect on radiocarbon dating, says that

0:22:14.760 --> 0:22:18.919
<v Speaker 1>if we were to reduce carbon dioxide emissions drastically in

0:22:18.960 --> 0:22:22.720
<v Speaker 1>the very near future, the effect on future radiocarbon dating

0:22:22.720 --> 0:22:26.040
<v Speaker 1>would be equivalent to inserting a one year error on

0:22:26.119 --> 0:22:30.960
<v Speaker 1>top of any estimation. If we don't drastically reduce emissions,

0:22:31.000 --> 0:22:34.680
<v Speaker 1>that error range will continue to grow over time. One

0:22:34.720 --> 0:22:37.480
<v Speaker 1>thing that the concentration of carbon fourteen tells us is

0:22:37.520 --> 0:22:40.040
<v Speaker 1>how much carbon dioxide in the atmosphere comes from the

0:22:40.040 --> 0:22:43.960
<v Speaker 1>burning of fossil fuels. So as we see the concentration decrease,

0:22:44.280 --> 0:22:47.760
<v Speaker 1>we know that's because proportionally more carbon twelve is being

0:22:47.760 --> 0:22:51.240
<v Speaker 1>released into the atmosphere, diluting the already tiny concentration of

0:22:51.240 --> 0:22:54.159
<v Speaker 1>carbon fourteen. So that's useful for scientists who are studying

0:22:54.160 --> 0:22:58.760
<v Speaker 1>climate change and pollution. But that's not exactly a happy story,

0:22:58.880 --> 0:23:03.480
<v Speaker 1>is it. So what are our options if carbon dating

0:23:03.680 --> 0:23:07.560
<v Speaker 1>becomes unreliable. Well, that depends on what you're trying to analyze.

0:23:07.880 --> 0:23:11.120
<v Speaker 1>If you're looking at inorganic stuff like rocks, you don't

0:23:11.160 --> 0:23:13.119
<v Speaker 1>need to use carbon fourteen in the first place. That

0:23:13.160 --> 0:23:16.000
<v Speaker 1>would be pretty much useless. You would use something else

0:23:16.040 --> 0:23:19.560
<v Speaker 1>like potassium argon dating, which is useful to estimate the

0:23:19.560 --> 0:23:21.920
<v Speaker 1>age of rocks that are a hundred thousand years old

0:23:22.000 --> 0:23:24.440
<v Speaker 1>or younger. And if that's not a big enough range,

0:23:24.480 --> 0:23:27.720
<v Speaker 1>you can actually use uranium lead dating and that will

0:23:27.760 --> 0:23:30.840
<v Speaker 1>let you estimate rocks between one point four and five

0:23:31.000 --> 0:23:34.480
<v Speaker 1>million years old. There's a lot of different options if

0:23:34.520 --> 0:23:37.359
<v Speaker 1>you're trying to date stuff. When it comes to organic materials, however,

0:23:37.400 --> 0:23:40.639
<v Speaker 1>it's a lot more tricky. Radio carbon was a great tool,

0:23:41.600 --> 0:23:44.960
<v Speaker 1>but if it becomes unreliable, we're gonna have to use

0:23:45.000 --> 0:23:50.200
<v Speaker 1>other methods like contextual clues and other items that are

0:23:50.680 --> 0:23:55.480
<v Speaker 1>helping us connect things to dates. So this is a

0:23:55.520 --> 0:23:59.400
<v Speaker 1>big problem. I guess you could argue that's a big

0:23:59.440 --> 0:24:03.320
<v Speaker 1>problem for future generations. And perhaps the records we leave

0:24:03.359 --> 0:24:11.280
<v Speaker 1>behind now are so uh so complete, they're so voluminous,

0:24:11.359 --> 0:24:14.640
<v Speaker 1>I guess is the best word, that future generations will

0:24:14.640 --> 0:24:18.320
<v Speaker 1>likely have more than enough material to determine when something

0:24:18.800 --> 0:24:23.560
<v Speaker 1>originated from our time versus earlier times. But the point

0:24:23.600 --> 0:24:27.639
<v Speaker 1>being that the way we're interacting with our world is

0:24:27.760 --> 0:24:33.320
<v Speaker 1>changing this fundamental ratio of carbon fourteen to carbon twelve,

0:24:34.080 --> 0:24:38.440
<v Speaker 1>and that means that a really brilliant means of determining

0:24:38.440 --> 0:24:41.760
<v Speaker 1>how old something is is not really going to be

0:24:42.320 --> 0:24:46.159
<v Speaker 1>an accurate measure for very much longer. So it's kind

0:24:46.200 --> 0:24:50.200
<v Speaker 1>of a bummer obviously for things that are much much

0:24:50.240 --> 0:24:53.240
<v Speaker 1>much older. Uh, it'll at least in the short term,

0:24:53.640 --> 0:24:55.879
<v Speaker 1>not be that big of a deal, especially if we

0:24:55.920 --> 0:24:59.600
<v Speaker 1>can relate it to other items that we we already

0:24:59.640 --> 0:25:02.639
<v Speaker 1>know the age of those items. It won't be as

0:25:02.760 --> 0:25:06.600
<v Speaker 1>destructive as saying we can never use radio carbon dating again.

0:25:06.880 --> 0:25:11.399
<v Speaker 1>We just have to keep that changing uh ratio of

0:25:11.480 --> 0:25:14.159
<v Speaker 1>carbon protein to carbon twelve in mind so that we

0:25:14.240 --> 0:25:17.560
<v Speaker 1>make sure we're making accurate measurements. So thank you so

0:25:17.640 --> 0:25:20.560
<v Speaker 1>much for the request. It was fun to go into that,

0:25:21.000 --> 0:25:23.480
<v Speaker 1>and obviously there's a lot more we could talk about

0:25:23.480 --> 0:25:27.920
<v Speaker 1>with various means of dating materials. So if you want

0:25:27.920 --> 0:25:30.920
<v Speaker 1>to hear more about that, I could probably get one

0:25:30.960 --> 0:25:33.520
<v Speaker 1>of the stuff you missed in history class hosts to

0:25:33.640 --> 0:25:38.359
<v Speaker 1>join me for an episode about how people determine the

0:25:38.520 --> 0:25:42.120
<v Speaker 1>age of things, especially organic materials, and we can maybe

0:25:42.160 --> 0:25:44.199
<v Speaker 1>do a full episode if that would be of interest

0:25:44.240 --> 0:25:46.280
<v Speaker 1>to you. I could probably also grab some of the

0:25:46.320 --> 0:25:49.280
<v Speaker 1>stuff to blow your mind folks to talk about this

0:25:49.400 --> 0:25:52.960
<v Speaker 1>as well. Let me know if you have any other suggestions.

0:25:53.000 --> 0:25:56.159
<v Speaker 1>You can of course write me. The email address to

0:25:56.240 --> 0:26:00.000
<v Speaker 1>contact me is tech stuff at how stuff works dot com,

0:26:00.119 --> 0:26:03.240
<v Speaker 1>or you can write me on Twitter or Facebook or tumbler,

0:26:03.600 --> 0:26:05.879
<v Speaker 1>and I used the handle tech stuff hs W at

0:26:05.920 --> 0:26:08.080
<v Speaker 1>all three. I look forward to hearing from you, and

0:26:08.080 --> 0:26:16.359
<v Speaker 1>you'll hear from me again really soon for more on

0:26:16.400 --> 0:26:18.760
<v Speaker 1>this and bousands of other topics, because it has to

0:26:18.760 --> 0:26:28.520
<v Speaker 1>have work dot Com