ScienceIQ.com

Does The Sun Go A Bit Wobbly?

Our Sun may seem an enduring, unwavering beacon in the sky, but in truth it has a 'heartbeat' of sorts--a pulsation between dimmer and brighter phases so slow that it only 'beats' 9 times each century! It's understandable that you might not have noticed. The pulsing is not only slow, it's also subtle. The total energy coming from the Sun only ...

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WobblySun
Astronomy

Black Hole Sound Waves

Astronomers using NASA's Chandra X-ray Observatory have found, for the first time, sound waves from a supermassive black hole. The 'note' is the deepest ever detected from any object in our Universe. ... Continue reading

BlackHoleSoundWaves
Geology

Pointing North

The needle of a compass is a small magnet, one that is allowed to pivot in the horizontal plane. The needle experiences a torque from the ambient magnetic field of the Earth. The reaction to this ... Continue reading

PointingNorth
Geology

A Undersea View of Our Earth's Geography

The ocean bottom is divided into three major areas: the continental shelf, the continental slope, and the deep ocean basin. The continental shelf extends underwater from each of the major land masses ... Continue reading

UnderseaEarthsGeography
Chemistry

Chemical Burning

Chemical burns are the result of very normal reactions that can occur between the offending material and living tissue components. People generally tend to regard their bodies as things outside of the ... Continue reading

ChemicalBurning

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.