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1816 - The Year Without A Summer

Most global temperature change occurs over a long period of time, centuries rather than years, and in small increments. But in 1816, the Northeastern part of the United State and Northern Europe were hit with successive cold fronts that brought snow and ice, and dropped temperatures almost to the freezing point. Spring started out cold, but by June ...

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1816YearSummer
Chemistry

Table Salt - It's All In The Ions

All elements are defined by their individual atoms, which are in turn identified by the number of protons in the nucleus of each atom. Since protons are carriers of positive electrical charge, there ... Continue reading

TableSaltItsAllInTheIons
Biology

The Art of Hunting

Most of us have seen a praying mantis. Two thousand species of praying mantis are scattered throughout the world, ranging in size from less than half an inch (1.27 cm) to more than five inches (12.7 ... Continue reading

PrayingMantis
Biology

Wise As An Owl

Are owls the smartest birds? According to trainers that work with them, not by a long shot. Parrots are easy to train and can have extensive vocabularies. Hawks can be taught to retrieve objects. Even ... Continue reading

WiseAsAnOwl
Physics

Poincare's Chaos

Over two hundred years after Newton published his laws of planetary motion the King Oscar II of Sweden and Norway sponsored a most unusual competition that would discover a whole new science. ... Continue reading

PoincaresChaos

Ultraviolet Light

UltravioletLightUltraviolet light is a form of radiation which is not visible to the human eye. It's in an invisible part of the 'electromagnetic spectrum'. Radiated energy, or radiation, is given off by many objects: a light bulb, a crackling fire, and stars are some examples of objects which emit radiation. The type of radiation being emitted depends on the temperature of the object. A coal glowing red in a barbecue is cooler than our Sun, which appears yellow, which is cooler still than some stars which appear bright white.

If a prism is used to break-up the radiated light from an object into its component colors, the 'visible light' which our eyes can see makes up only a small part of the total spectrum. Visible light runs from the familiar blue to green to yellow to orange to red. Red light is the least energetic of the colors of visible light, and blue is the most energetic. Beyond the red end of the visible part of the spectrum lies the infrared and radio radiation. Infrared 'light' is familiar to us as heat, while radio waves are used for TV and radio broadcasts.

Beyond the blue end of the visible spectrum lies ultraviolet light, X-rays and gamma-rays. All of the X-rays, gamma-rays and ultraviolet light emitted by stars are absorbed by the Earth's atmosphere. That is why we need to send our telescopes into space (such as Astro-2 !) in order to measure the ultraviolet light from stars and galaxies. Many scientists are interested in studying the invisible universe of ultraviolet light, since the hottest and most active objects in the universe give off large amounts of ultraviolet energy.