The satellite's orbit has perigee and apogee distances of 9000 km and 11000 km from the center of the Earth, respectively, when adding Earth's radius (6500 km) to their heights above the surface. The semi-major axis (a) can be computed as the average of these distances:
\[a=\frac{9000\text{ km}+11000\text{ km}}{2}=10000\text{ km}\]
The eccentricity (e) of the orbit is defined as:
\[e=\frac{\text{apogee distance}-\text{perigee distance}}{\text{apogee distance}+\text{perigee distance}}\]
Substituting the distance values:
\[e=\frac{11000-9000}{11000+9000}=\frac{2000}{20000}=0.1\]
