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Jumping Starlight

'Twinkle, twinkle, little star, how I wonder what you are,' says the song by Jane Taylor. But stars don’t really twinkle; their light reaches the earth in a steady way. Why then do we see them flickering around in the sky? The answer is in the atmosphere. ...

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JumpingStarlight
Biology

Nematodes Are Everywhere

Nematodes are simple worms consisting of an elongate stomach and reproduction system inside a resistant outer cuticle (outer skin). Most nematodes are so small, between 400 micrometers to 5 mm long, ... Continue reading

NematodesAreEverywhere
Engineering

The Motion of An Aircraft

We live in a world that is defined by three spatial dimensions and one time dimension. Objects move within this domain in two ways. An object translates, or changes location, from one point to ... Continue reading

TheMotionofAnAircraft
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
Geology

What is Geodesy?

Geodesy is the science of measuring and monitoring the size and shape of the Earth. Geodesists basically assign addresses to points all over the Earth. If you were to stick pins in a model of the ... Continue reading

WhatisGeodesy

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.