Numerical Integration of Orbits

Solar System Barycentre

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This integration shows the Solar System but starts off with a close-up of the Sun. Instead of holding the Sun static in the centre of the screen it is free to move around as in fact it does naturally. The centre of the screen is the Solar System Barycentre (centre of mass and momentum of the Solar System). Notice how the Sun moves round the Barycentre in response to the gravity of the planets.

Zoom out until you can see the orbits of the inner planets. Notice how the tracks they follow are slightly uneven showing how the entire orbits of these planets follow the Sun's movements quite closely.   This is much less noticeable with the outer planets.

This integration includes all the major bodies of the Solar System plus Halley's comet and Sedna. Integration steps are variable.  Integration method is Yoshida 6th Order. The Solar System barycentre is held static as the central point. 

 

 

 


Tony Evans 2004-2011

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