Fig. 5
Nine orbital solutions of the binary asteroid system (22) Kalliope are displayed in the equatorial J2000 reference plane. They represent the solutions for which fp < 18 mas (see Fig. 3) and the Keplerian solution. This 3D-representation of the orbits spanned over 10 years shows that they are very close in shape due to the low eccentricity and inclination of the orbits.
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