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Weathering, Erosion, and Deposition

Weathering, erosion, and deposition are processes continually at work on or near earth's surface. Over time, these processes result in the formation of sedimentary rocks. Weathering occurs when rocks are broken down into smaller particles but not moved. Mechanical weathering is the breaking of rocks by expansion and contraction. This can be as a ...

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WeatheringErosionDeposition
Geology

A Big, Big Wave

A tsunami (pronounced 'soo-nah-mee') is a series of waves of extremely long wave length and long period generated in a body of water by an impulsive disturbance that vertically displaces the water. ... Continue reading

ABigBigWave
Medicine

Mother Nature's Own Brand of Bioterror

We've been hearing a lot about smallpox lately, as a possible bioterror attack. But Mother Nature has her own brand of bioterror. Smallpox has been with us for about ten thousand years, since the ... Continue reading

Bioterror
Physics

When Do We Encounter Ionizing Radiation In Our Daily Lives?

Everyone who lives on this planet is constantly exposed to naturally occurring ionizing radiation (background radiation). This has been true since the dawn of time. The average effective dose ... Continue reading

IonizingRadiation
Chemistry

What Is Arsenic?

Arsenic is a naturally occurring element widely distributed in the earth's crust. In the environment, arsenic is combined with oxygen, chlorine, and sulfur to form inorganic arsenic compounds. Arsenic ... Continue reading

WhatIsArsenic

Poincare's Chaos

PoincaresChaosOver 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.

Competition promised a cash prize to a scientist that would answer this question: ‘How Stable is the Solar System?’. Contestants would basically have to use Newton’s laws of gravitation to mathematically show the stability of our solar system. Applying Newton’s equations was easy for two bodies, say the Sun and Earth, however as soon as one added a third body, say the Moon, the problem would become so complicated that even the best physicists and mathematicians of the time were not able to compute anything. They were not even able to predict the three bodies’ trajectories of motion. This so called ‘three-body problem’ was therefore at the heart of this competition.

The prize was awarded ultimately to Jules Henri Poincare, one of the France’s leading mathematical physicists, even though he did not completely solve the problem and furthermore he showed what everybody was expecting the least. With his elegant math he showed that the three-body system behaved in a complex and totally unpredictable way. The Solar System, or at least his three-body approximation, was not stable at all, it was chaotic! Small changes in the initial conditions (such as planets positions and initial velocities) produced huge and unpredictable outcomes. His findings were ground stones for what we today know as chaos theory.