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Oil Viscosity

Everybody recognizes 'oil' as a word for liquid materials that do not behave like water. They have a 'thickness' and self-cohesive character (autocohesion) that enables them to form a film on a surface. Oils have a characteristic feel when rubbed between one's thumb and forefinger. They are often compounds that have a high degree of hydrocarbon ...

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OilViscosity
Astronomy

The Oldest Light in the Universe

A NASA satellite has captured the sharpest-ever picture of the afterglow of the big bang. The image contains such stunning detail that it may be one of the most important scientific results of recent ... Continue reading

OldestLightUniverse
Medicine

How a Horse Can Save Your Life?

Most people who have been vaccinated with the smallpox vaccine never really question what exactly was injected into their body. If they did, they might be surprised, and maybe thank a horse or two. ... Continue reading

HorseLife
Astronomy

The Sun’s Corona

The White-Light Corona - The Corona is the Sun's outer atmosphere. It is visible during total eclipses of the Sun as a pearly white crown surrounding the Sun. The corona displays a variety of features ... Continue reading

TheSunCorona
Astronomy

Near-Earth Supernovas

Supernovas near Earth are rare today, but during the Pliocene era of Australopithecus supernovas happened more often. Their source was an interstellar cloud called 'Sco-Cen' that was slowly gliding by ... Continue reading

Supernovas

Carbon Dating From The Skies

CarbonDatingFromTheSkiesDetermining the age of relatively recent fossils, those of plants and animals that lived tens of thousands of years ago, is not a guessing game but an exact science. By using carbon dating we can determine their age to within few years. Carbon dating is a technique where by measuring the residual carbon-14 concentration of the fossil and comparing it to that from samples that recently died, one can accurately estimate the date when the plant or animal in question died.

Naturally, carbon occurs in three isotopes or forms: C12, C13 and C14. The number after the letter 'C' denotes the different number of neutrons in the nucleus. The C12 and C13 are both stable and therefore useless in carbon dating. The C14 is unstable and undergoes radioactive decay with a half-life of about 5,568 years. If you leave 100 atoms of C14 on the shelf today, in about 5,568 years you will have 50 atoms of C14 left. The remaining 50 will have decayed into nitrogen plus some electrons as byproducts. After 11,136 years, you will have 25 atoms of C14 and 75 atoms of nitrogen and so on. The important question is: How do you know how many C14 atoms you started with? Also, how does this radioactive carbon get into living things?

It all starts high up in the skies. Nitrogen from the air is constantly bombarded by cosmic ray neutrons. Infrequently, one of these neutrons manages to penetrate deep into the nitrogen nucleus and converts it to carbon-14. This C14 then gets oxygenated into carbon-14-dioxide which plants absorb through photosynthesis and which gets into animals through the food-chain. The day the plant or animal dies, it stops absorbing C14. From then on, this fixed number of C14 atoms only gets depleted as the years go by. The number of these C14 atoms at the time of death is approximately constant for any given type of plant or animal regardless of whether it died today or 10,000 years ago. Almost all of the radioactive C14 gets depleted in about 60,000 years, so this technique becomes useless for older fossils.