Radiocarbon Dating
Carbon-14 serves as an atomic clock capable of determining the age of archeological artifacts up to about 50,000 years old. It is used to date objects such as bone, cloth, wood and plant fibers.
 

Innovator
As a member of the Manhattan Project (1941-45), Willard Frank Libby (1908-1980) helped develop method for separating uranium isotopes--an essential step in the creation of the atomic bomb. In 1946 he showed that tritium, the heaviest isotope of hydrogen, was produced by cosmic radiation. The following year he developed the carbon-14 dating technique. This technique is used to date material derived from former living organisms as old as 50,000 years. It measures small amounts of radioactivity from the carbon-14 in organic or carbon-containing materials and is able to identify older objects as those having less radioactivity. Awarded the 1960 Nobel Prize in Chemistry for radiocarbon dating, the nominating committee offered the following in praise of Libby:

"Seldom has a single discovery in chemistry had such an impact on the thinking of so many fields of human endeavor. Seldom has a single discovery generated such wide public interest."
 
 
 

Producing Carbon-14
Cosmic rays collide with atoms in the upper atmosphere producing energetic neutrons. When these neutrons collide with nitrogen (7 protons/7 neutrons), carbon-14 (6 protons/8 neutrons) is produced:

Being radioactive, carbon-14 eventually decays to form nitrogen-14 and a  beta particle (high speed electron).

While one can’t predict exactly when a particular C-14 atom will emit an electron and turn into N-14, the statistics are very
predictable. Given a large number of C-14 atoms, we can say with a high degree of confidence that half of them will turn into
N-14 in 5,730 years. This is called the “half-life” because half of the C-14 will turn into N-14. Half of the remaining C-14 turns into N-14 in another 5,730 years. The half-life is a convenient concept for getting a general feel for how fast radioactive elements decay, but it isn't very convenient for calculating the amount left after an arbitrary period of time. For example, how much will be left in 2,000 years?  An equation is needed to predict how much is left at any particular time, not just multiples of the half-life.
 

Equation
Carbon-14 atoms combine with oxygen to form carbon dioxide; the ratio of normal carbon (C-12) to C-14 in the air and in all living things at any given time is nearly constant (about one in a trillion carbon atoms are C-14). Although C-14 atoms are always decaying, they are replaced by new C-14 atoms at a constant rate. At this moment, your body has the same percentage of C-14 as all living plants and animals. However, when a living organism dies, it stops taking in new carbon and the ratio of C-14 to C-12 decreases (C-14 decays with a half-life of 5,730 years while stable C12 remains constant). By measuring the ratio of C-12 to C-14, it is possible to determine the age of a formerly living object.

Decay of C-14 follows first-order kinetics:
ln (A0/At) = kt           k = 0.693/t1/2      (t1/2 = 5,730 yr)
where A0/At is ratio of C-14 in currently living objects compared to C-14 in sample
Substituting 0.693/t1/2 for k gives:
ln (A0/At) = (0.693)t/t1/2      or      t = (t1/2)[ln(A0/At)]/0.0693

For example,  an object with 1/10 C-14 content compared to a living sample would be about 19,000 years old:
t = [5,730 yr][ ln (10)/(0.693)] = 19,000 yr

To determine how much C-14 is left in an object and therefore how old it is, we count the number of beta radiations given off per minute per gram of carbon. Modern C-14 emits about 15 beta radiations per minute per gram while objects 5730 years old emit half that amount per minute. So if a sample taken from an object emits 7.5 radiations per minute per gram, the organism must be 5730 years old. The accuracy of radiocarbon dating was tested on objects with dates that were already known through historical records such as parts of the dead sea scrolls and some wood from an Egyptian tomb. Analysis showed that C-14 agreed very closely with the historical information.
 
 
 
 

Dead Sea Scrolls
Between 1947 and 1956 thousands of fragments of biblical and early Jewish documents were discovered in eleven caves near the site of Khirbet Qumran on the shores of the Dead Sea. Carbon-14 dating of samples taken from ragged edges of manuscript margins determined the ages of the scrolls to range from the third century B.C. to 68 A.D. These dates support earlier paleographic research, which estimated the ages of the scrolls by analyzing the handwriting styles, materials, and formatting of the manuscripts.
 
 

Limitations


 

Martian Meteorite
The principle of carbon-14 dating applies to other isotopes including:

The 5-pound  meteorite shown above was found in Antarctica (1984) covered with black glass. This black glass, called fusion crust, forms on all meteorites as they burn entering Earth's atmosphere. The meteorite formed originally from molten lava about 4 billion years ago on Mars--the strongest evidence is traces of trapped gas just like the martian atmosphere. But to get off Mars, the meteorite needed an escape velocity of about 11,000 mph. The only known natural process capable of generating such a velocity is meteorite impact; a meteorite hits Mars and rocks on surface blast up faster than the escape velocity. After leaving Mars, the meteorite began orbiting the Sun. Gravity from planets (especially Jupiter) slowly changed the orbit and by chance, the meteorite collided with the Earth about 13,000 years ago. Analysis reveals that  the meteorite was in space and exposed to cosmic rays for about 16 million years before colliding with Earth.