Calculating the trajectories of two gravitating bodies is straightforward mathematics. But introducing even just one more variable into an orbital system can make its long-term trajectory impossible to predict. In 2009, two researchers at the University of California, Santa Cruz investigated just how difficult this mathematical phenomenon – known as the ‘N-body problem’ – makes forecasting the eventual fate of our own corner of space. The team ran 2,000 simulations of the solar system’s trajectory up to 5 billion years into the future, with the only variable being less than a millimetre difference in the distance between Mercury and the Sun. The simulations yielded a stunning array of results, including the possibility of Mercury careening into the Sun, colliding with Venus and destablising the entire inner solar system. This animation from TED-Ed breaks down the N-body problem with rich visuals and methodical clarity, and concludes with scientists’ efforts to minimise N-body unpredictability as humans press further into space.
videoMathematics
After centuries of trying, we’ve yet to arrive at a perfect way to map colour
20 minutes
videoMusic
A riveting audiovisual dive into what makes sounds harmonious, or not
28 minutes
videoMathematics
Spiral into the ‘golden ratio’ – and separate the myths from the maths
4 minutes
videoHistory of science
How we came to know the size of the Universe – and what mysteries remain
26 minutes
videoOceans and water
A stunning visualisation explores the intricate circulatory system of our oceans
5 minutes
videoHistory of science
Ideas ‘of pure genius’ – how astronomers have measured the Universe across history
29 minutes
videoComputing and artificial intelligence
A future in which ‘artificial scientists’ make discoveries may not be far away
9 minutes
videoBiology
Butterflies become unrecognisable landscapes when viewed under electron microscopes
4 minutes
videoMetaphysics
What do past, present and future mean to a philosopher of time?
55 minutes