Step 1: Recall the eccentricity vector formula.
For an orbit around a body with gravitational parameter $\mu$, the eccentricity vector is
\[
\vec{e} = \frac{1}{\mu}\left[\left(v^2 - \frac{\mu}{r}\right)\vec{r} - (\vec{r}\cdot\vec{v})\vec{v}\right]
\]
and the magnitude of this vector is the orbit eccentricity. An eccentricity below 1 means an ellipse, exactly 1 means a parabola, and above 1 means a hyperbola.
Step 2: Work out the scalar quantities needed.
$r^2 = 8000^2+9000^2 = 145000000$, so $r \approx 12041.6$ km.
$v^2 = (-6)^2+6^2 = 72$ km$^2$/s$^2$.
$\vec{r}\cdot\vec{v} = (8000)(-6)+(9000)(6) = -48000+54000 = 6000$ km$^2$/s.
$v^2 - \mu/r = 72 - 398600/12041.6 = 72 - 33.10 = 38.90$
Step 3: Build the eccentricity vector.
\[
\vec{e} = \frac{1}{398600}\Big[38.90(8000,9000) - 6000(-6,6)\Big]
\]
\[
= \frac{1}{398600}\big[(311200,350100) - (-36000,36000)\big] = \frac{1}{398600}(347200,314100)
\]
\[
\vec{e} = (0.871,\ 0.788)
\]
Step 4: Find the eccentricity and read off the orbit type.
\[
e = \sqrt{0.871^2+0.788^2} = \sqrt{0.759+0.621} = \sqrt{1.380} \approx 1.175
\]
Since $e \approx 1.175 > 1$, the orbit is open and unbound. This matches what the energy check gives, and confirms the trajectory is hyperbolic, not an ellipse, circle, parabola or straight line.
\[
\boxed{e \approx 1.175 > 1 \Rightarrow \text{Hyperbola}}
\]