You Need to Understand Radio-carbon Dating

Last week I read this in an Israeli newspaper:

“A massive tower that defended [Jerusalem’s] main water source – which was thought to have been built in the Middle Bronze Age, nearly 4,000 years ago – [Carbon dating results] have shown the structure likely dates back only to the ninth century B.C.E.”

Like it or not, you need to understand radio-carbon dating. Nearly every field of science relies on it. Archaeologists in particular count on carbon dating to help them determine the age of many of the artifacts they dig up.

What is it? How does it work?

At this moment, powerful cosmic particles from somewhere out in the Milky Way are striking Earth’s upper atmosphere. They combine with nitrogen atoms to form unstable Carbon 14 atoms – unstable in the sense that the C-14 atoms slowly decay back to nitrogen.

The C-14 and the more stable C-12 carbon atoms combine with oxygen atoms to form carbon dioxide. The ratio between the two types of carbon dioxide is - currently - one trillion to 1.

Both types of carbon dioxide are breathed in by living plants. Animals, of course, breathe in oxygen and breathe out carbon dioxide. However, animals collect C-12 and C-14 from the plants they eat. So animals and humans, like plants, are assumed to have the same one trillion to 1 ratio of C-12 to C-14. Obviously, rocks cannot be measured by a carbon clock.

(The archaeologists in Jerusalem had to have dated some piece of wood they found, not the stones the tower is built from. It was the piece of wood, or technically, the death of the tree the wood came from, that dated to David’s day, not the tower.)

When a plant or animal dies, it stops taking in carbon. It is assumed that the C-12 remains stable for the rest of eternity, but its C-14 decays.

It is assumed that all plants take in C-12 and C-14 in the same amounts and with the same ratio. It is further assumed that the ratio has remained constant; that is, that a plant living, say, 6000 years ago took up one C-14 atom to every one trillion C-12 atoms, just as plants do today.

The rate of decay – that is, the rate at which C-14 leeches away – is currently measured at one half every 5,700 years. And it is assumed that it has always been the same. So if you were to analyze a sample of 100 trillion carbon atoms from a modern plant, 100 of them would be C-14 atoms. If you looked at 100 trillion atoms of a 5,700 year-old plant you would only count fifty C-14 atoms – half the original amount. 100 trillion atoms from a plant 11,400 years old would have only twenty-five C-14 atoms, and so on.

Simple, right? The lower the amount of C-14, the older the sample. Given all that, any sample more than a few thousand years old will have a microscopically small amount of C-14... one might even say an "immeasurably small amount." And, of course, when you are measuring things in atoms, the samples (and the machinery) are subject to contamination.

According to radiocarbon.com, scientists use oxalic acid made from sugar beets known to have been harvested in 1955 to calibrate their tests. They also use wood from a tree known to have been cut in 1890, “unaffected by fossil fuel effects.”

Wait: What?

Yup. Turns out that changes to the atmosphere mess with the carbon levels. Scientists assume that, prior to the fossil fuel age there were no significant changes to the atmosphere. That explains that reference to the ‘1955 sugar beet oxalic acid,’ as well: atmospheric testing of hydrogen bombs in the fifties significantly altered the levels of C-12 and C-14 in the atmosphere.

Notice all the assumptions involved: For the carbon clock to be reliable, the amount of the mysterious cosmic rays striking the atmosphere from the unknown space source would have to remain constant over tens of thousands of years. Have they? Who knows? The scientists admit they know little about them.

In addition, cosmic rays are greatly affected by magnetic fields – both that of the earth and that of the sun. The magnetic fields, in fact, are the reason scientists can only say the cosmic rays come from 'somewhere in the galaxy' – because each magnetic field they pass on their way to Earth changes their direction and their intensity. 

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Earth's magnetic field fluctuates dramatically. The sun’s does as well.

Let’s take it a step further. For much of Earth's geologic history a dense shroud of water, dust or other debris covered the planet. Would this have affected cosmic rays striking the atmosphere? Absolutely. Would that have altered the relative amounts of nitrogen, oxygen, and carbon dioxide in the atmosphere? Again, yes.

Atmospheric oxygen is believed to have been as low as 15%, and as high as 35%, at various points in geologic history. The nitrogen level went down when oxygen went up, and vice versa. Carbon dioxide levels changed nearly every time a volcano erupted. When humans began cooking and heating with fire (6,000 years ago according to the Bible or 350,000 years ago according to science) carbon dioxide climbed. When we began using fossil fuels, CO2 really jumped. Atmospheric testing of nuclear weapons in the 1950s also greatly affected levels of C-14 in the atmosphere.

So how can anyone say that the ratio of C-14 to ordinary carbon in a plant living today is the same as the ratio in a plant that lived thousands of years ago?

The scientists themselves, who lean so heavily on the radiocarbon clock, need to read the work of other scientists:

• “A large and sudden increase in radiocarbon around AD 773 is documented in coral skeletons from the South China Sea…forming a spike of 45% in late spring, followed by two smaller spikes. The carbon anomalies coincide with an historic comet collision with the Earth's atmosphere on 17 January AD 773.” – Nature.com
• “We find [in annual rings of Japanese cedar trees] a rapid increase of about 12% in the C-14 content from a.d. 774 to 775, which is about 20 times larger than the change attributed to ordinary solar modulation.” – Nature, June 2012
• “The rate of carbon 14 radioactive decay may have been different in the past. The amount of carbon dioxide in the atmosphere may have been different in the past. The assumption of a constant ratio of C-14 to C-12 is invalid; equilibrium would require about 30,000 years, (or 50,000 years according to this mathematician) and the C-14/C-12 ratio appears to be increasing still.” – Tufts.edu

That last part there, about “equilibrium,” is important. If all the assumptions were true, 30,000-50,000 years after the C-14 process began, whenever that was, the atmosphere should have reached equilibrium… it should have reached a point where the C-14 decayed away at the same rate at which it is being generated. Otherwise, by now we’d be swimming in C-14.

But it is still increasing. Which can ONLY mean:

1. The C-14 process – cosmic rays reaching the atmosphere, the atmosphere containing the present-day levels of nitrogen, oxygen, and CO2, the C-14 being absorbed by plants then decaying out, etc. – that process began less than 30,000 years ago… or
2. The theory on which Carbon 14 dating is based, is just wrong…

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