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3rd Austrian Hungarian Workshop
Birgit Priebe
Escapes and Collisions in the inner Solar System
Our solar system seems to be stable, but the
work of Jaques Laskar (1996) showed the chaotic features of our
planetary system. For our calculations, we used a presumed stable model - the inner solar system with Jupiter and Saturn.
We calculated the orbit of Mercury over a period of 10 million years with different initial conditions for
its eccentricity.
We found several close encounters between Mercury and Venus; additionally collisions of this two planets were found for values of e larger than 0.5.
This result verifies Laskars work where he also
proposes chaotic behavior of Mercury at rather low values of
its eccentricity.
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