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Ozone: Good Up High, Bad Nearby

Ozone is a gas that forms in the atmosphere when 3 atoms of oxygen are combined (03). It is not emitted directly into the air, but at ground level is created by a chemical reaction between oxides of nitrogen (NOx), and volatile organic compounds (VOC) in the presence of sunlight. Ozone has the same chemical structure whether it occurs high above ...

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Ozone
Geology

Haleakala Crater

Modern geology indicates that the Hawaiian Islands are situated near the middle of the Pacific Plate, one of a dozen thin, rigid structures covering our planet like the cracked shell of an egg. Though ... Continue reading

HaleakalaCrater
Mathematics

Leaps and Bounds

Leap years are years with 366 days, instead of the usual 365. Leap years are necessary because the actual length of a year is 365.242 days, not 365 days, as commonly stated. Basically, leap years ... Continue reading

LeapsandBounds
Science

Subrahmanyan Chandrasekhar

NASA's premier X-ray observatory was named the Chandra X-ray Observatory in honor of the late Indian-American Nobel laureate, Subrahmanyan Chandrasekhar (pronounced: su/bra/mon'/yon chandra/say/kar). ... Continue reading

SubrahmanyanChandrasekhar
Astronomy

The Constellations

The random arrangement of the stars visible to the naked eye has remained essentially unchanged since the time of the first written records. One of the earliest complete lists we have was compiled in ... Continue reading

TheConstellations

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.