  We present spatially resolved mass outflow rate measurements ($\dot M_{out}$)
for the narrow line region of Markarian 34, the nearest Compton-thick type 2
quasar (QSO2). Spectra obtained with the Hubble Space Telescope and at Apache
Point Observatory reveal complex kinematics, with distinct signatures of
outflow and rotation within 2 kpc of the nucleus. Using multi-component
photoionization models, we find that the outflow contains a total ionized gas
mass of $M \approx 1.6 \times 10^6 M_{\odot}$. Combining this with the
kinematics yields a peak outflow rate of $\dot M_{out} \approx 2.0 \pm
0.4~M_{\odot}$ yr$^{-1}$ at a distance of 470 pc from the nucleus, with a
spatially integrated kinetic energy of $E \approx 1.4 \times 10^{55}$ erg.
These outflows are more energetic than those observed in Mrk 573 and NGC 4151,
supporting a correlation between luminosity and outflow strength even though
they have similar peak outflow rates. The mix of rotational and outflowing
components suggests that spatially resolved observations are required to
determine accurate outflow parameters in systems with complex kinematics. (See
appended erratum for updated values.)
