Asteroid 3040 Kozai

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Kozai Mechanism

In 1962 Yoshihide Kozai published a paper describing how a small body, with a high orbital inclination relative to a large body, could undergo long term variations of eccentricity and inclination. The theory indicates that the body must have an inclination more than 39.2 degrees. In 1979 an asteroid with an inclination of 47 degrees was discovered and named 3040 Kozai.

3040 Kozai

In this integration I attempt to show the Kozai mechanism in action. As it is a long term effect do not expect anything dramatic. Watch the orbit of the asteroid (green). A rapid rate of precession is clear quite quickly. The variation of eccentricity is less easy to see. Use the rotate and tilt controls to try and gain an impression of how the asteroid's orbit compares to Earth and Mars. Up to ~10000 years its orbit seems to become more circular and is all beyond Mars. Then it starts to get more eccentric and by 30000 has become quite eccentric passing into the region between Earth and Mars.

This integration includes Earth, Mars, Jupiter and Saturn (no orbit drawn) and 3040 Kozai. Mercury and Venus and the outer planets are excluded to maximise running speed as they would make little difference to the effect. The integration step is fixed at 2 days and the display step 1000 days. The method is Yoshida 6th order. The speed of the integration will depend very much on the speed of your computer. I am getting about 8000 years per minute on a 2.4Gh machine.

 

 

 


Tony Evans 2004-2009

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