WEBVTT - TechStuff Classic: Is Carbon Dating on the way out?

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<v Speaker 1>Welcome to tech Stuff, a production from I Heart Radio.

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<v Speaker 1>Hey there, and welcome to tech 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 how the tech are you? It is time for

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<v Speaker 1>a tech Stuff classic episode. This episode originally aired on

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<v Speaker 1>August tenth, two thousand fifteen. It is titled is carbon

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<v Speaker 1>Dating on the Way out? This episode might need to

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<v Speaker 1>be carbon dated. Let's take a listen. 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, but uh, the request was could you

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<v Speaker 1>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 including 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'd 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 they're emitted by supernova of massive stars,

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<v Speaker 1>and these subatomic particles are primarily atomic nuclei and high

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<v Speaker 1>energy protons. So this collision of the high energy neutron

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<v Speaker 1>with the nitrogen forces a proton to leave the nucleus

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<v Speaker 1>and the IN fourteen changes to C fourteen, So in

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<v Speaker 1>other words, nitrogen fourteen turns to carbon fourteen. So instead

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<v Speaker 1>of having seven protons and seven neutrons, the new atom

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<v Speaker 1>has six protons and eight neutrons. The proton that was

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<v Speaker 1>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 hydrogen 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 nineties, 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'll be

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<v Speaker 1>back with more of this classic episode of tech stuff

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<v Speaker 1>after this quick break. Now, living things here on Earth

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<v Speaker 1>absorb carbon through various means, and some of that carbon

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<v Speaker 1>is carbon fort So it maybe that you know, you

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<v Speaker 1>eat a plant and that plant has some of the

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<v Speaker 1>carbon fourteen in it. Now you have some of the

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<v Speaker 1>carbon fourteen and you And if we know the ratio

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<v Speaker 1>of carbon fourteen to the stable form of carbon twelve,

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<v Speaker 1>we can look at materials and analyze them to see

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<v Speaker 1>how the ratio of carbon fourteen to carbon twelve in

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<v Speaker 1>the material stacks up to the standard ratio. With living things,

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<v Speaker 1>this becomes a matter of looking at how much carbon

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<v Speaker 1>fourteen is not there? All right, That's it's a little confusing.

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<v Speaker 1>Let me explain. So, when a living thing is still alive,

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<v Speaker 1>it accumulates carbon at about the same rate it loses carbon.

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<v Speaker 1>So carbon cosmic rays produced this carbon fourteen frequently enough

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<v Speaker 1>that the ratio between carbon fourteen and carbon twelve remains steady.

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<v Speaker 1>So the percentage of carbon fourteen to carbon twelve is

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<v Speaker 1>fairly standardized. But when a living thing stops being alive

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<v Speaker 1>and turns into a not living any more or thing,

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<v Speaker 1>it stops accumulating carbon, so it has the carbon that

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<v Speaker 1>it has inside of it stays. That's it. You're not

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<v Speaker 1>losing anymore. You're not gaining any more except for carbon

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<v Speaker 1>fourteen because carbon fourteen undergoes radioactive decay, so over time,

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<v Speaker 1>some of that carbon fourteen starts to convert to nitrogen.

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<v Speaker 1>So that means if you can look at the remains

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<v Speaker 1>of a living thing and detect the ratio of carbon

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<v Speaker 1>fourteen to carbon twelve, you can get an idea of

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<v Speaker 1>how long ago it was that it stopped taking in carbon,

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<v Speaker 1>as in, how long ago was it that this lip

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<v Speaker 1>once living thing died. It gets a little more complicated

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<v Speaker 1>than all that, but here's the basic rule. If we

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<v Speaker 1>want to be really precise, here's the equation we use

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<v Speaker 1>to determine the age of a sample of material. You

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<v Speaker 1>have an equation where you take the natural logarithm of

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<v Speaker 1>NF divided by n o uh that in turn is

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<v Speaker 1>divided by negative point six nine three, and then you

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<v Speaker 1>multiply it by t uh one half, so one half t.

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<v Speaker 1>The natural logarithm is a specific logarithm applied to this

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<v Speaker 1>equation and other things as well. NF divided way n

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<v Speaker 1>O actually refers to the percentage of carbon fourteen and

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<v Speaker 1>the sample compared to the amount found in living stuff today,

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<v Speaker 1>and T times one half is the half life of carbon.

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<v Speaker 1>So that's five thousand, seven hundred years. So it's a

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<v Speaker 1>lot 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 either the thing you're testing only

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<v Speaker 1>has five percent of the carbon fourteen you would find

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<v Speaker 1>in living things. That means you would fill out the

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<v Speaker 1>equation with the natural logarithm of point zero five divided

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<v Speaker 1>by negative point six nine three, and you multiply that

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<v Speaker 1>that result to with five thousand, seven hundred years the

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<v Speaker 1>natural logorithm at point zero five. By the way, in

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<v Speaker 1>case you don't want to whip out your calculator is

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<v Speaker 1>negative two point nine nine five seven three to two

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<v Speaker 1>seven three five five. If you divide that by negative

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<v Speaker 1>point six nine three, you get four point three to

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<v Speaker 1>two eight four five nine. Don't dial that number. If

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<v Speaker 1>you take that number, the four point three, etcetera, and

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<v Speaker 1>you multiply that by five thousand, seven hundred years, you

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<v Speaker 1>end up with twenty four thousand, six hundred forty point

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<v Speaker 1>two years, meaning the stuff you're looking at died somewhere

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<v Speaker 1>around 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 define 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>thou 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 carbon fourteen,

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<v Speaker 1>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

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<v Speaker 1>too much damage to to uh make on this item.

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<v Speaker 1>So certain items are considered very precious and there's a

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<v Speaker 1>big resistance to using carbon dating because by the definition,

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<v Speaker 1>you're going to be damaging the material. Now there's several

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<v Speaker 1>lines of research that are exploring possible non destructive means

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<v Speaker 1>of using radiocarbon dating. There's one that uses plasma oxidation

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<v Speaker 1>and the use of non destructive washes to clean samples

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<v Speaker 1>of those contaminating humic acids, which would lead to errors

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<v Speaker 1>if they remained behind, but those are still largely in

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<v Speaker 1>the testing phase and aren't the common means of using

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<v Speaker 1>carbon dating. Also, keep in mind that we use this

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<v Speaker 1>method to estimate the date of things made from organic materials,

0:14:20.960 --> 0:14:24.760
<v Speaker 1>like the Dead Sea scrolls, but this estimation is based

0:14:24.800 --> 0:14:27.880
<v Speaker 1>upon when the materials were harvested, so, in other words,

0:14:28.160 --> 0:14:30.920
<v Speaker 1>whenever the living thing that the materials came from stopped

0:14:30.920 --> 0:14:34.640
<v Speaker 1>being alive, it doesn't tell us the date of when

0:14:34.640 --> 0:14:37.880
<v Speaker 1>the artifact was actually produced. So it's possible that you

0:14:37.880 --> 0:14:41.440
<v Speaker 1>could come across an artifact like a scroll and you

0:14:41.560 --> 0:14:44.160
<v Speaker 1>use carbon dating on it and find out that the

0:14:44.320 --> 0:14:47.800
<v Speaker 1>scroll material is two thousand years old, meaning two thousand

0:14:47.920 --> 0:14:52.360
<v Speaker 1>years ago whatever the scroll was made out of stopped living,

0:14:53.040 --> 0:14:56.320
<v Speaker 1>but it doesn't tell you about the contents written in

0:14:56.360 --> 0:15:00.200
<v Speaker 1>the scroll. It's possible that the contents were at to

0:15:00.240 --> 0:15:04.280
<v Speaker 1>the scroll much after the living thing stopped being alive.

0:15:04.400 --> 0:15:07.320
<v Speaker 1>Still it's a pretty good bet that the two are

0:15:07.320 --> 0:15:10.360
<v Speaker 1>within the same neighborhood of time, rather than someone held

0:15:10.400 --> 0:15:13.720
<v Speaker 1>onto blank scrolls for a few centuries before finally jotting

0:15:13.760 --> 0:15:17.200
<v Speaker 1>something down. All Right, it's all this is cool, But

0:15:17.920 --> 0:15:21.360
<v Speaker 1>how did we even figure out radio carbon dating would

0:15:21.400 --> 0:15:25.560
<v Speaker 1>be a possible way of figuring out how old something is. Well.

0:15:25.560 --> 0:15:27.960
<v Speaker 1>Some early discoveries were made in the nineteen thirties at

0:15:27.960 --> 0:15:31.920
<v Speaker 1>the Lawrence Radiation Laboratory in Berkeley, and you probably remember

0:15:31.920 --> 0:15:34.360
<v Speaker 1>that if you've been listening to tech stuff. It factored

0:15:34.360 --> 0:15:36.760
<v Speaker 1>heavily into the discussion I had with Ben Bolan about

0:15:36.760 --> 0:15:42.840
<v Speaker 1>the Manhattan Project. So Franz Curry, an American physicist, observed

0:15:42.880 --> 0:15:46.080
<v Speaker 1>something really interesting when he irradiated a cloud of air

0:15:46.280 --> 0:15:50.360
<v Speaker 1>in a cloud chamber. He used neutrons to uh to

0:15:50.520 --> 0:15:55.040
<v Speaker 1>irradiate that cloud, and he saw proton recoil tracks that

0:15:55.080 --> 0:15:59.520
<v Speaker 1>indicated something was losing protons. So he concluded that the

0:15:59.600 --> 0:16:02.960
<v Speaker 1>neutral rons that he was using, we're colliding with nitrogen

0:16:03.040 --> 0:16:06.680
<v Speaker 1>fourteen and producing what was believed to be a form

0:16:06.720 --> 0:16:09.880
<v Speaker 1>of carbon as a result, with hydrogen being the other

0:16:09.920 --> 0:16:13.200
<v Speaker 1>product of this collision. His work was further explored by

0:16:13.240 --> 0:16:18.280
<v Speaker 1>physicists like Tom W. Bonner, W. M. Brubaker, W. J. Bircham,

0:16:18.560 --> 0:16:22.680
<v Speaker 1>and Maurice gold Hauber. Now collectively, this laid the foundation

0:16:22.760 --> 0:16:25.760
<v Speaker 1>for the simple equation of a high energy neutron plus

0:16:25.920 --> 0:16:31.040
<v Speaker 1>nitrogen fourteen produces one hydrogen atom and one carbon fourteen atom.

0:16:31.120 --> 0:16:33.920
<v Speaker 1>Then you had Enrico Fermi. We talked about him in

0:16:33.960 --> 0:16:37.240
<v Speaker 1>the Manhattan Project, and his work showed that the cross

0:16:37.280 --> 0:16:40.400
<v Speaker 1>section of a nitrogen fourteen atom was much larger than

0:16:40.400 --> 0:16:45.400
<v Speaker 1>other materials, and that suggested that neutron and nitrogen collisions

0:16:45.440 --> 0:16:48.440
<v Speaker 1>might happen fairly regularly in nature as long as there

0:16:48.480 --> 0:16:52.760
<v Speaker 1>were a supply of high energy neutrons. Stay tuned for

0:16:52.800 --> 0:16:56.760
<v Speaker 1>the exciting conclusion of this textuff classic episode right after

0:16:56.800 --> 0:17:08.600
<v Speaker 1>we take this break. Then you have a Serge Korf,

0:17:09.000 --> 0:17:11.439
<v Speaker 1>who was a physicist who was born in Finland and

0:17:11.440 --> 0:17:13.960
<v Speaker 1>whose family immigrated to the United States in the early

0:17:14.000 --> 0:17:18.880
<v Speaker 1>twentieth century. He discovered the phenomenon that cosmic rays interact

0:17:18.920 --> 0:17:22.399
<v Speaker 1>with atoms and produce high energy neutrons in the upper atmosphere.

0:17:22.680 --> 0:17:28.040
<v Speaker 1>So Pharem's prediction and corpse observation we're starting to kind

0:17:28.080 --> 0:17:31.960
<v Speaker 1>of coalesce here. The observations convinced scientists that the neutrons

0:17:32.000 --> 0:17:35.679
<v Speaker 1>themselves were not cosmic rays, because the neutrons had a

0:17:35.680 --> 0:17:40.080
<v Speaker 1>lifespan of just eighteen minutes, and therefore a neutron wouldn't

0:17:40.080 --> 0:17:42.560
<v Speaker 1>be able to survive the long trip through space. They

0:17:42.640 --> 0:17:45.720
<v Speaker 1>must have been something else first, so they said the

0:17:45.720 --> 0:17:49.280
<v Speaker 1>neutrons had to be a byproduct of another interaction. A

0:17:49.320 --> 0:17:52.480
<v Speaker 1>cosmic ray must be interacting with something in the atmosphere.

0:17:52.880 --> 0:17:56.280
<v Speaker 1>That interaction caused this high energy neutron to be emitted,

0:17:56.560 --> 0:17:59.480
<v Speaker 1>and Core hypothesized that these neutrons could then interact with

0:17:59.600 --> 0:18:04.440
<v Speaker 1>nitrogen and fourteen to produce carbon fourteen in the upper atmosphere. Now,

0:18:04.440 --> 0:18:06.639
<v Speaker 1>it was Willard F. Libby who came up with the

0:18:06.720 --> 0:18:09.760
<v Speaker 1>idea that since carbon fourteen is generated at a steady

0:18:09.880 --> 0:18:12.719
<v Speaker 1>rate due to cosmic ray interactions in our atmosphere, you

0:18:12.760 --> 0:18:16.000
<v Speaker 1>should be able to use it to measure how long

0:18:16.160 --> 0:18:19.200
<v Speaker 1>something has been dead. Libby would measure the value of

0:18:19.240 --> 0:18:22.800
<v Speaker 1>carbon fourteen's half life at five thousand, five hundred sixty

0:18:22.800 --> 0:18:25.840
<v Speaker 1>eight years, give or take thirty years, which became known

0:18:25.920 --> 0:18:29.000
<v Speaker 1>as the Libby half life, and Libby himself would be

0:18:29.000 --> 0:18:32.120
<v Speaker 1>awarded the Nobel Prize in nineteen sixty for his work

0:18:32.160 --> 0:18:35.800
<v Speaker 1>in radiocarbon dating. All right, So that's the history of

0:18:35.880 --> 0:18:39.920
<v Speaker 1>radiocarbon dating and generally how radiocarbon dating works. So why

0:18:40.040 --> 0:18:43.280
<v Speaker 1>is it in trouble or what could possibly be causing

0:18:43.320 --> 0:18:46.800
<v Speaker 1>confusion with radiocarbon dating. Well, there are two big things

0:18:46.800 --> 0:18:49.439
<v Speaker 1>we need to talk about, and one was one that

0:18:49.480 --> 0:18:51.720
<v Speaker 1>I've alluded to a couple of times. I mentioned that,

0:18:52.720 --> 0:18:56.119
<v Speaker 1>you know, pre nineteen forties, you had a certain level

0:18:56.240 --> 0:19:00.440
<v Speaker 1>of carbon fourteen that was pretty standard, but the nuclear

0:19:00.480 --> 0:19:04.119
<v Speaker 1>age really messed things up for us. They made carbon

0:19:04.160 --> 0:19:06.880
<v Speaker 1>fourteen dating a bit tricky. Starting in the nineteen forties,

0:19:06.920 --> 0:19:10.600
<v Speaker 1>we began testing nuclear bombs. Now, these bombs released a

0:19:10.600 --> 0:19:13.520
<v Speaker 1>lot of energy upon exploding, partly in the form of

0:19:13.600 --> 0:19:16.280
<v Speaker 1>high energy neutrons. You can probably see where this is going.

0:19:16.680 --> 0:19:19.760
<v Speaker 1>Some of those high energy neutrons ended up interacting with

0:19:19.920 --> 0:19:23.520
<v Speaker 1>nitrogen fourteen atoms, which meant that it produced carbon fourteen

0:19:23.560 --> 0:19:27.840
<v Speaker 1>atoms as a result. So the concentration of carbon fourteen

0:19:28.280 --> 0:19:33.040
<v Speaker 1>increased in the wake of nuclear bomb testing. So anything

0:19:33.080 --> 0:19:36.080
<v Speaker 1>that died after the nineteen forties actually has a higher

0:19:36.119 --> 0:19:39.800
<v Speaker 1>concentration of carbon fourteen than the stuff that died before

0:19:39.920 --> 0:19:43.440
<v Speaker 1>the nineteen forties did even know at the time of death.

0:19:43.640 --> 0:19:47.840
<v Speaker 1>According to Professor Nalini no Khannie of the Evergreen State College,

0:19:48.040 --> 0:19:51.919
<v Speaker 1>the nineteen fifties saw a one hundred percent spike in

0:19:52.040 --> 0:19:56.160
<v Speaker 1>carbon fourteen coming into the atmosphere. In nineteen sixty three,

0:19:56.560 --> 0:19:59.600
<v Speaker 1>the United States and Russia agreed to stop above ground

0:19:59.720 --> 0:20:02.280
<v Speaker 1>nucle you're testing, and the levels of carbon fourteen in

0:20:02.280 --> 0:20:05.560
<v Speaker 1>the atmosphere gradually dropped down to their normal levels. But

0:20:05.640 --> 0:20:08.679
<v Speaker 1>that means there's a blip in the carbon fourteen radar

0:20:08.760 --> 0:20:11.919
<v Speaker 1>between the nineteen forties and nineteen sixty three. So if

0:20:11.920 --> 0:20:14.720
<v Speaker 1>you put yourself in the shoes of a future archaeologist,

0:20:15.240 --> 0:20:19.320
<v Speaker 1>radiocarbon dating becomes unreliable because the levels of carbon fourteen

0:20:19.400 --> 0:20:22.679
<v Speaker 1>could be deceptive. If the thing you're measuring died during

0:20:22.720 --> 0:20:25.600
<v Speaker 1>the era of nuclear testing, it might appear to be

0:20:25.760 --> 0:20:29.040
<v Speaker 1>younger than you thought because there's a higher concentration of

0:20:29.119 --> 0:20:33.520
<v Speaker 1>carbon fourteen in its sample than you otherwise would have expected.

0:20:33.840 --> 0:20:38.160
<v Speaker 1>So it may seem that something died in twenty fifteen

0:20:38.200 --> 0:20:41.879
<v Speaker 1>as opposed to nineteen sixty three. That's just an example.

0:20:42.440 --> 0:20:44.840
<v Speaker 1>Now to the article that prompted this episode in the

0:20:44.880 --> 0:20:49.040
<v Speaker 1>first place, that's a different case. Researchers published a study

0:20:49.040 --> 0:20:51.960
<v Speaker 1>in the Proceedings of the National Academy of Sciences about

0:20:52.000 --> 0:20:55.639
<v Speaker 1>how the use of fossil fuels is further making radiocarbon

0:20:55.720 --> 0:20:59.560
<v Speaker 1>dating less reliable, and this time it's not an excess

0:20:59.600 --> 0:21:03.000
<v Speaker 1>of carbon and fourteen. It's actually the opposite problem. Fossil

0:21:03.040 --> 0:21:07.120
<v Speaker 1>fuels have no carbon fourteen in them because they are

0:21:07.200 --> 0:21:12.000
<v Speaker 1>fossil fuels. This is billions of years old, so they're

0:21:12.000 --> 0:21:14.679
<v Speaker 1>far too old for any carbon fourteen to remain. Remember

0:21:14.680 --> 0:21:18.720
<v Speaker 1>that carbon fourteen is decaying over time and turning into nitrogen,

0:21:18.840 --> 0:21:23.600
<v Speaker 1>so eventually all of those carbon fourteen atoms decay. So

0:21:23.640 --> 0:21:27.360
<v Speaker 1>burning a fossil fuel releases carbon dioxide, and the carbon

0:21:27.520 --> 0:21:30.120
<v Speaker 1>in that CEO two has no carbon fourteen and it's

0:21:30.160 --> 0:21:33.840
<v Speaker 1>all carbon toolver carbon thirteen. So the more fossil fuels

0:21:33.880 --> 0:21:37.480
<v Speaker 1>we burn, the more we dilute the concentration of carbon

0:21:37.520 --> 0:21:40.800
<v Speaker 1>fourteen that's in the atmosphere. So stuff from the nuclear

0:21:40.840 --> 0:21:44.040
<v Speaker 1>age tends to look younger than it really is because

0:21:44.040 --> 0:21:47.080
<v Speaker 1>of the higher concentration of carbon fourteen. Stuff from the

0:21:47.160 --> 0:21:51.000
<v Speaker 1>later ages of fossil fuel use will look older than

0:21:51.040 --> 0:21:54.439
<v Speaker 1>they really are because carbon fourteen has been diluted So

0:21:54.480 --> 0:21:58.159
<v Speaker 1>according to the study, fresh organic material in twenty fifty

0:21:58.440 --> 0:22:01.280
<v Speaker 1>would contain the same amount of AREB and fourteen relative

0:22:01.359 --> 0:22:06.359
<v Speaker 1>to carbon twelve as something dating from ten fifty. So

0:22:06.480 --> 0:22:11.000
<v Speaker 1>you have a thousand years of doubt in any radiocarbon

0:22:11.119 --> 0:22:14.960
<v Speaker 1>dated samples. You would be look at the two samples

0:22:14.960 --> 0:22:18.280
<v Speaker 1>if you if all you had were miniscule samples of

0:22:18.359 --> 0:22:20.520
<v Speaker 1>two things and one of them was a T shirt

0:22:21.080 --> 0:22:24.119
<v Speaker 1>that was made in twenty fifty, and another was a

0:22:24.160 --> 0:22:28.080
<v Speaker 1>piece of cloth that dated from ten fifty, and you

0:22:28.119 --> 0:22:32.560
<v Speaker 1>did radiocarbon dating, you'd get the same result. This is

0:22:32.560 --> 0:22:35.160
<v Speaker 1>not good if you are trying to figure out how

0:22:35.240 --> 0:22:39.840
<v Speaker 1>old something is. Heather Graven, who authored the study on

0:22:39.880 --> 0:22:43.080
<v Speaker 1>fossil fuel emissions and the effect on radiocarbon dating, says

0:22:43.119 --> 0:22:47.280
<v Speaker 1>that if we were to reduce carbon dioxide emissions drastically

0:22:47.359 --> 0:22:50.919
<v Speaker 1>in the very near future, the effect on future radiocarbon

0:22:51.000 --> 0:22:54.359
<v Speaker 1>dating would be equivalent to inserting a one year error

0:22:54.440 --> 0:22:59.440
<v Speaker 1>on top of any estimation. If we don't drastically reduce emissions,

0:22:59.480 --> 0:23:03.160
<v Speaker 1>that error age will continue to grow over time. One

0:23:03.200 --> 0:23:06.000
<v Speaker 1>thing that the concentration of carbon fourteen tells us is

0:23:06.000 --> 0:23:08.520
<v Speaker 1>how much carbon dioxide in the atmosphere comes from the

0:23:08.520 --> 0:23:12.440
<v Speaker 1>burning of fossil fuels, So as we see the concentration decrease,

0:23:12.760 --> 0:23:16.240
<v Speaker 1>we know that's because proportionally more carbon twelve is being

0:23:16.280 --> 0:23:19.720
<v Speaker 1>released into the atmosphere, diluting the already tiny concentration of

0:23:19.760 --> 0:23:22.639
<v Speaker 1>carbon fourteen. So that's useful for scientists who are studying

0:23:22.680 --> 0:23:27.280
<v Speaker 1>climate change and pollution. But that's not exactly a happy story,

0:23:27.400 --> 0:23:32.000
<v Speaker 1>is it. So what are our options if carbon dating

0:23:32.160 --> 0:23:36.040
<v Speaker 1>becomes unreliable. Well, that depends on what you're trying to analyze.

0:23:36.400 --> 0:23:39.640
<v Speaker 1>If you're looking at inorganic stuff like rocks, you don't

0:23:39.640 --> 0:23:41.639
<v Speaker 1>need to use carbon fourteen in the first place. That

0:23:41.640 --> 0:23:44.520
<v Speaker 1>would be pretty much useless. You would use something else

0:23:44.520 --> 0:23:48.040
<v Speaker 1>like potassium argon dating, which is useful to estimate the

0:23:48.040 --> 0:23:50.400
<v Speaker 1>age of rocks that are a hundred thousand years old

0:23:50.520 --> 0:23:52.920
<v Speaker 1>or younger. And if that's not a big enough range,

0:23:52.960 --> 0:23:56.200
<v Speaker 1>you can actually use uranium lead dating and that will

0:23:56.280 --> 0:23:59.320
<v Speaker 1>let you estimate rocks between one point four and five

0:23:59.480 --> 0:24:03.000
<v Speaker 1>million years old. There's a lot of different options if

0:24:03.000 --> 0:24:05.840
<v Speaker 1>you're trying to date stuff. When it comes to organic materials, however,

0:24:05.880 --> 0:24:09.159
<v Speaker 1>it's a lot more tricky. Radio carbon was a great tool,

0:24:10.119 --> 0:24:13.440
<v Speaker 1>but if it becomes unreliable. We're gonna have to use

0:24:13.520 --> 0:24:19.160
<v Speaker 1>other methods like contextual clues and other items that are

0:24:19.160 --> 0:24:23.960
<v Speaker 1>helping us connect things to dates. So this is a

0:24:24.000 --> 0:24:27.880
<v Speaker 1>big problem. I guess you could argue that's a big

0:24:27.920 --> 0:24:31.800
<v Speaker 1>problem for future generations. And perhaps the records we leave

0:24:31.880 --> 0:24:39.840
<v Speaker 1>behind now are so uh so complete, they're so voluminous,

0:24:39.880 --> 0:24:43.120
<v Speaker 1>I guess is the best word that future generations will

0:24:43.160 --> 0:24:46.840
<v Speaker 1>likely have more than enough material to determine when something

0:24:47.280 --> 0:24:52.040
<v Speaker 1>originated from our time versus earlier times. But the point

0:24:52.080 --> 0:24:56.119
<v Speaker 1>being that the way we're interacting with our world is

0:24:56.240 --> 0:25:01.800
<v Speaker 1>changing this fundamental ratio of carbon fourteen to carbon twelve,

0:25:02.560 --> 0:25:06.920
<v Speaker 1>and that means that a really brilliant means of determining

0:25:06.920 --> 0:25:10.280
<v Speaker 1>how old something is is not really going to be

0:25:10.800 --> 0:25:14.679
<v Speaker 1>an accurate measure for very much longer. So it's kind

0:25:14.680 --> 0:25:18.680
<v Speaker 1>of a bummer. Obviously, for things that are much, much

0:25:18.760 --> 0:25:22.280
<v Speaker 1>much older, it'll at least in the short term, not

0:25:22.440 --> 0:25:24.600
<v Speaker 1>be that big of a deal, especially if we can

0:25:24.680 --> 0:25:28.239
<v Speaker 1>relate it to other items that we we already know

0:25:28.440 --> 0:25:31.880
<v Speaker 1>the age of those items. It won't be as destructive

0:25:31.960 --> 0:25:35.080
<v Speaker 1>as saying we can never use radio carbon dating again.

0:25:35.400 --> 0:25:39.919
<v Speaker 1>We just have to keep that changing, uh ratio of

0:25:39.960 --> 0:25:42.639
<v Speaker 1>carbon fourteen to carbon twelve in mind, so that we

0:25:42.720 --> 0:25:46.560
<v Speaker 1>make sure we're making accurate measurements. I hope you enjoyed

0:25:46.600 --> 0:25:50.080
<v Speaker 1>that classic episode of tech Stuff about carbon dating. If

0:25:50.080 --> 0:25:52.919
<v Speaker 1>you have suggestions for topics I should cover in future

0:25:53.000 --> 0:25:56.119
<v Speaker 1>episodes of tech Stuff, please reach out to me on Twitter.

0:25:56.440 --> 0:25:58.840
<v Speaker 1>The handle for the show is text Stuff H s

0:25:59.040 --> 0:26:04.280
<v Speaker 1>W and I talked to you again really soon. Yes.

0:26:08.440 --> 0:26:11.440
<v Speaker 1>Text Stuff is an I Heart Radio production. For more

0:26:11.520 --> 0:26:14.920
<v Speaker 1>podcasts from I Heart Radio, visit the I Heart Radio app,

0:26:15.040 --> 0:26:18.200
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