Orbital Evolution Studies of O.D.A.S. Asteroids

In an attempt to investigate the dynamical evolution of NEOs numerical integration studies of the orbital history of selected asteroids will be presented here. The results might be updated or improved in course of more accurate orbital parameters will become avaiable, in particular for newly discovered objects. The findings shown in these pages therefore should be considered as rather preliminary.

Any information obtained from these pages may only be used if referenced properly as originated from the O.D.A.S. Webpages maintained by G. Hahn, Institute of Planetary Exploration, DLR, Berlin-Adlershof, Germany

For further information please contact Gerhard Hahn

Orbits studied so far: